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10.1371_journal.pcbi.1011775.pdf
|
Data Availability Statement: The software
“ImportRisk-v1.0.0” to compute the import risk is
available under the Zenodo repository https://doi.
org/10.5281/zenodo.7852476.
|
The software 'ImportRisk-v1.0.0' to compute the import risk is available under the Zenodo repository https://doi. org/10.5281/zenodo.7852476 .
|
RESEARCH ARTICLE
Inferring country-specific import risk of
diseases from the world air transportation
network
Pascal P. KlamserID
Clara Jongen1,2, Frank Schlosser1,2, Dirk BrockmannID
1,2, Adrian ZachariaeID
1,2, Benjamin F. MaierID
1,2,7*
1,2,3,4, Olga Baranov5,6,
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
OPEN ACCESS
Citation: Klamser PP, Zachariae A, Maier BF,
Baranov O, Jongen C, Schlosser F, et al. (2024)
Inferring country-specific import risk of diseases
from the world air transportation network. PLoS
Comput Biol 20(1): e1011775. https://doi.org/
10.1371/journal.pcbi.1011775
Editor: Yamir Moreno, University of Zaragoza:
Universidad de Zaragoza, SPAIN
Received: May 3, 2023
Accepted: December 21, 2023
Published: January 24, 2024
Peer Review History: PLOS recognizes the
benefits of transparency in the peer review
process; therefore, we enable the publication of
all of the content of peer review and author
responses alongside final, published articles. The
editorial history of this article is available here:
https://doi.org/10.1371/journal.pcbi.1011775
Copyright: © 2024 Klamser et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: The software
“ImportRisk-v1.0.0” to compute the import risk is
available under the Zenodo repository https://doi.
org/10.5281/zenodo.7852476.
1 Department of Biology, Institute for Theoretical Biology, Humboldt-Universita¨t zu Berlin, Berlin, Germany,
2 Robert Koch Institute, Berlin, Germany, 3 DTU Compute, Technical University of Denmark, Kongens
Lyngby, Denmark, 4 Copenhagen Center for Social Data Science, University of Copenhagen, Copenhagen,
Denmark, 5 Division of Infectious Diseases and Tropical Medicine, University Hospital, LMU Munich, Munich,
Germany, 6 German Center for Infection Research (DZIF), Partner Site Munich, Munich, Germany, 7 Center
Synergy of Systems (SynoSys), Center for Interdisciplinary Digital Sciences, Technische Universita¨t
Dresden, Dresden, Germany
* [email protected]
Abstract
Disease propagation between countries strongly depends on their effective distance, a mea-
sure derived from the world air transportation network (WAN). It reduces the complex
spreading patterns of a pandemic to a wave-like propagation from the outbreak country,
establishing a linear relationship to the arrival time of the unmitigated spread of a disease.
However, in the early stages of an outbreak, what concerns decision-makers in countries is
understanding the relative risk of active cases arriving in their country—essentially, the likeli-
hood that an active case boarding an airplane at the outbreak location will reach them.
While there are data-fitted models available to estimate these risks, accurate mechanistic,
parameter-free models are still lacking. Therefore, we introduce the ‘import risk’ model in
this study, which defines import probabilities using the effective-distance framework. The
model assumes that airline passengers are distributed along the shortest path tree that
starts at the outbreak’s origin. In combination with a random walk, we account for all possible
paths, thus inferring predominant connecting flights. Our model outperforms other mobility
models, such as the radiation and gravity model with varying distance types, and it improves
further if additional geographic information is included. The import risk model’s precision
increases for countries with stronger connections within the WAN, and it reveals a geo-
graphic distance dependence that implies a pull- rather than a push-dynamic in the distribu-
tion process.
Author summary
For the spread of a contagious disease, human mobility puts distant places in proximity
and geographically closer targets may be effectively much further away. The worldwide
flight network is crucial for long distance travels and the previously proposed ‘effective
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Funding: B.F.M received funding through Grant
CF20-0044, HOPE: How Democracies Cope with
Covid-19, from the Carlsberg Foundation and was
supported as an Add-On Fellow for Interdisciplinary
Life Science by the Joachim Herz Stiftung. P.P.K,
A.Z, F.S received funding through Grant D81870,
COVID-19 Lockdown-Monitor, from Germany’s
Federal Ministry of Health. The funders had no role
in study design, data collection and analysis,
decision to publish, or preparation of the
manuscript.
Competing interests: The authors declare no
competing interests.
distance’ translates this mobility into a distance measure that correlates with the disease
arrival time. We use the effective distance to generate a bottom-up and thus parameter-
free distribution process of passengers on the flight network, which takes into account all
possible flight routes. This allows us to determine the import probability of a disease. Our
‘import risk’ model outperforms or matches established mobility models, some of which
require calibration with scarce or costly data. In contrast, our approach relies on minimal
flight network data, that is the number of planes between airports and their passenger
capacities, but not on passenger data. Its bottom-up approach enables future studies on
country-specific measures for controlling and containing infected passengers, a challenge
with existing models. Thus, the ‘import risk’ model’s strength lies in its data simplicity,
this relevance to pandemics, and parameter-free design.
Introduction
The recent decades have seen a considerable increase in mobility: The worldwide number of
passenger cars in use increased by an average of about 4% each year between 2006 and 2015,
reaching approximately 1 billion in 2015 [1]. This growth is comparable to the yearly increase
in the number of sea containers shipped [2], and the global scheduled air passenger count also
experienced an annual growth of about 6% between 2004 and 2019 [3] In essence, the world is
becoming increasingly interconnected in terms of passenger mobility, both on a small scale
(cars) and a large scale (air traffic), as well as in the import and export of goods. This height-
ened connectivity facilitates the distribution of goods and people, as demonstrated by the dis-
tribution of over 400 invasive species through agricultural imports, which is best predicted by
the global trade network [4]. A prime example of unwanted side effects of well-connected
regions is the potential for pandemics, accompanied by death, economic damage and the
potential stigmatization of survivors, migrants and minorities [5–7]. Already the first plague
pandemic that started AD 541 in the Nile Delta of Egypt spread in 8 years across the territories
(Mediterranean, Northern Europe and Near East) of 2 affected empires because of the intense
commerce in the Roman Empire [6]. Nowadays, the intensified exchange reduces the time
until a pandemic reaches all parts of the world to months as for the 2009 H1N1 virus that
spread from Mexico in 5 months to all continents [8, 9] or the recent COVID-19 pandemic
whose variants spread within a few months across the globe [10–13].
The connection strength between world regions is only partly explained by their geographic
proximity. Instead, due to historic geopolitical relations [14, 15] pandemics spread rather
along an effective distance that is derived from the world air transportation network (WAN)
[16–19], or, if applied on a smaller scale, also from other means of transportation [16, 20].
According to the effective distance, region B is closest to region A if the passenger flow from A
to B is greater than to other destinations. An intriguing extension is the multipath effective dis-
tance, which enhances the prediction of disease arrival times by considering all paths taken by
a random walker on the WAN [17]. The effective distance is regularly used to analyze the
impact of mobility on the spread of diseases, as for example for MERS [21], Ebola [22], Zika
[23] and most recently COVID-19 [20, 24–26]. While it enables a qualitative estimation of dis-
ease arrival times, its applicability is severely restricted when it comes to describing the impor-
tation of infected passengers from a specific source to a target. However, these import events
are highly relevant for political decision-makers and to enable modeling predictions.
In this work, we describe these import events via the “import probability” p(B|A), which is
equivalent to the origin-destination (OD) matrix whose element TBA represents the number of
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
trips from A to B, with the difference that the probability is normalized by all trips starting in
A, i.e. p(B|A) = TBA/TA. There are mobility models that fit the OD matrix, requiring a reference
OD matrix as seen in the gravity model [27–31]. Additionally, some models integrate OD
matrix-fitted models on a smaller scale with the OD matrix of the global air transportation net-
work, creating a multiscale mobility network to represent all modes of transportation [32, 33].
Note that the multiscale mobility model has been successfully employed to analyze past pan-
demics [34–36]. Yet, it can be extremely difficult to obtain the OD matrix and most often it is
estimated by small surveys [37] or alongside a census [38]. Even for the air transportation net-
work derived from a booking system, the OD is only an approximation since passengers
increasingly book directly at the airlines (in 2015 30% of all Lufthansa flights were booked
directly which increased to 52% in 2018 [39]) and not via the big GDS (global distribution sys-
tems) from which most OD-estimates are derived [40, 41]. This means that to exactly compute
the air transportation OD matrix, bookings of all GDSs and about 900 airlines must be pur-
chased/estimated and combined. Thus, models that do not rely on an existing reference OD
matrix are important and those either assume an underlying decision process without integrat-
ing traffic information as the radiation model [42, 43] or they apply a maximum entropy
approach to distribute the unknown OD trips along possible routes of a known traffic network
[30, 44, 45]. However, none of the above approaches use the effective distance with its qualita-
tive link to disease propagation and none is based on a mechanistic distribution process on a
traffic network. To our understanding, a mechanistic process mimics the detailed movement
behavior of the passengers on the traffic network, and neither uses only quantities of and
between the locations (gravity and radiation model) nor relies on principles of system in ther-
modynamic equilibrium (maximum entropy model), in other words it is a bottom-up
approach. This approach grants us a mechanistic understanding of the observed patterns,
enabling us to investigate how modifications impact passenger distribution. For instance, we
can analyze how containment interventions along distribution routes reduce the import prob-
ability of infected passengers.
In this work, we introduce the import risk model, based on a distribution process following
the shortest path tree of the WAN based on effective distance. This process is combined with a
random walker that explores all potential paths within the WAN. We are using WAN data
from the year 2014 and compare it to the Global Transnational Mobility Dataset from 2014
[40], as a ground truth baseline. Additionally, we investigate the discrepancy to the import risk
and alternative mobility models as the gravity [27, 31] and radiation model [43] through multi-
ple comparison measures. We find that the import risk model outperforms the alternative
models and improves only slightly when it includes not only WAN information but also the
geodetic distance between airports. Lastly, we evaluate the quality of import probability estima-
tion for specific countries and assess if and how the geodesic distance is encoded in the import
risk estimate.
Results
Relating the WAN, OD-probability and the effective distance
In this work, we introduce the import risk, which estimates the probability of a passenger
departing from airport A to conclude their journey at any airport worldwide, even those not
directly connected to the origin airport. The estimation is based on the traffic flow of airplanes
and the respective maximal passenger capacity between airports, a.k.a. the world air transpor-
tation network (WAN), provided by the Official Airline Guide (OAG) [46]. This inference-
problem is intriguing because it is much easier to monitor the origin and destination of air-
planes, than of passengers with possibly multiple connecting flights until their final
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
destination. In our study, we use the WAN from 2014 (Fig 1A) and compare the derived
import probabilities to a reference dataset. The reference import probability is based on the
Global Transnational Mobility Dataset (GTN) from 2014 [40, 47], which combines an origin-
final-destination dataset from a major global distribution system (GDS) with a tourism dataset
from the World Tourism Organization (Fig 1B, see Material and methods for more details on
the data). Before introducing the import risk model, we contrast the two datasets, introduce
the effective distance [16] and quantify its potential as the base metric for our proposed model.
By comparing the world air transportation network (WAN) with the country-specific refer-
ence import probability from the GTN (compare Fig 1A and 1B), we see that the airports con-
nected via direct links belong to countries that also have a high import probability.
Nevertheless, due to physical constraints and logistical optimization, not all countries with
non-zero import probabilities are directly connected to airports in the source country; instead,
they are reached via connecting flights. In the context of import probability, estimates based
on geodesic distance and the population of the target country are useful but exhibit limitations
in certain scenarios. For instance, the import probability for Italy is approximately 1.4 times
greater than that for Germany, even though Germany is geographically closer to Canada and
Fig 1. The relation between WAN, OD-probability, SPT and effective distance. A: The world air transportation network (WAN) represents the direct flight
connections and maximal seat capacities between airports in 2014, here shown for flights starting from five selected countries. It is based on flight-schedule-data. The
lines are bundled and do not represent the specific flight route, but illustrate the links to airports abroad. B: The reference import probability from Canada to all
countries, based on the OD matrix (Origin-Destination) of the Global Transnational Mobility Data set [40, 47] in 2014. It combines origin and final-destination trips
between countries from the SABRE and the World Tourism Organization (UNWTO). The lines illustrate the connection to the common source country. C: Based on
the effective distance deff = d0 − ln(p) a shortest path tree (SPT) is constructed with the largest Canadian airport as source (YYZ: Toronto Pearson International
Airport). The link color and thickness shows the hop distance, i.e. number of connecting flights. D: exponential decay of the reference import probability (as in B but
for all countries as source) with the effective distance deff (derived from the SPT (C) of the WAN (A)). Each dot represents a country-country link, the lines are
medians including either all source countries or only from a specific continent. Maps are created with geopandas [48].
https://doi.org/10.1371/journal.pcbi.1011775.g001
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
has a larger population. The effective distance is an alternative network-based distance mea-
sure that does not rely solely on direct connections and geographic information [16–19].
Instead, it is based on the passenger flow Fij from j to i and its relationship to the outflow Fj
through the transition probability Pij = Fij/Fj. Together with a constant distance offset d0, the
effective distance between directly connected airports is
deffðij jÞ ¼ d0 (cid:0)
lnðPijÞ :
ð1Þ
The effective distance between airports without direct connection is the cumulative distance
along the shortest path tree (SPT) derived from deff, as illustrated for the largest Canadian air-
port (Toronto Pearson Airport, YYZ) in Fig 1C. Note that a distance offset of d0 = 0 would
make two routes indistinguishable as long as the product of the transition probabilities along
each route is the same, but with d0 > 0 the one route with fewer connecting flights is effectively
shorter. Previous studies have demonstrated that the arrival time of diseases in countries
exhibits a linear dependence on their effective distance [16–19]. We show that the import
probability also correlates with deff (Fig 1D), whereby the correlation is higher than for other
distance measures (see Fig A in S1 Text). In fact, the import probability decays exponentially
with effective distance (linear decay on a semi-log scale in Fig 1D) which can be reproduced in
a simplified model for a passenger that travels at a constant effective speed and has a constant
exit rate. Therefore, the effective distance seems to be a good representation of the underlying
distribution process, and is a promising candidate for the base of our proposed import risk
model, to directly estimate the import probability.
Import risk model
The idea behind the import risk model is a combination of two elements: (i) a random walk
with an exit probability of the walker to finish its travel at the current node and (ii) a distribu-
tion mechanism derived from the deff SPT (Fig 2). The use of a random walk is motivated by
Iannelli et al. [17] who could improve the arrival-order prediction of deff by including all possi-
ble paths. The exit probability enables us to combine the random walk with a distribution
mechanism that assigns the likelihood of each node being the final destination, as explained in
detail in the second step. In the first step, we use the transition network representation of the
WAN and let a random walker start at source n0 and after each step it either exits at the current
node i with exit probability qi or continues to walk. Let us define the walker’s probability to
continue walking to node n given it was at node n − 1 before and originally started in n0 by
Sn;n(cid:0) 1ðn0Þ ¼ Pn;n(cid:0) 1ð1 (cid:0) qn(cid:0) 1ðn0ÞÞ ;
ð2Þ
with Pn,n−1 as the transition probability from n − 1 to n. Now the probability to walk along a
path Γ starting at n0 and exiting at n is the probability to continue walking Si,j along each link
(i, j) that is part of the path times the exit probability of the final node
pðGÞ ¼ qn
Y
ði;jÞ2G
Si;j ;
ð3Þ
where we omitted the explicit dependence on the source n0. Our goal is to describe all possible
paths the walker can take from n0 to n. We will use the matrix S, whose elements are the proba-
bilities to continue walking Si,j. The element (i, j) of the product of the matrix with itself
S � S = S2 sums over all paths of length l = 2 that end at i and start at j. Next, we can define the
probability of a walker to exit at n after traversing all paths of length l as
plðnjn0Þ ¼ qnðSlÞn;n0
:
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Fig 2. Import risk scheme. Starting from the transition network (left) the shortest path tree is computed based on the
effective distance (center bottom). Based on the shortest path tree, the exit probabilities q� = q(�|?) are computed. In
the formula, the geometric symbols represent the estimated population of the respective node, which can also be
distance-weighted (depending on the exact model). A random walk-process with exit probability is defined (top): at
each step, the walker either exits the node with prob. q� = q(�|?), or continues walking with prob. (1 − q�). The import
risk p1(�|?) (right) is the probability of a walker to exit at node � given it started at node ? under consideration of all
possible paths.
https://doi.org/10.1371/journal.pcbi.1011775.g002
Finally, the import risk is the probability to exit at n given all paths of all lengths
p1ðnjn0Þ ¼ qn
!
X1
Sl
l¼1
n;n0
¼ qnððI (cid:0) SÞ(cid:0) 1 (cid:0) IÞn;n0
;
ð5Þ
where we used the convergence of the geometric series with identity matrix I.
In the second step, we approximate the exit probability qi(n0) that we used above, but did
not specify yet. Thereby, we assume that passengers start at source airport n0, travel along the
SPT and exit at node i with an exit-probability
qiðn0Þ ¼
NðiÞ
NðiÞ þ NðOðijn0ÞÞ
ð6Þ
with N(i) as the population at airport i and O(i|n) as the set of all offspring nodes downstream
of i on the SPT centered at source n0. Hence, the exit probability at node i is determined by the
ratio of the population at node i to the combined populations of all downstream nodes of i on
the SPT, inclusive of node i.
We estimate the population at airport i using its outflow on the WAN, denoted as N(i) = Fi.
To aggregate the import probabilities at the country level, we sum the targets and apply a
weighted average to the source airports, with population serving as the weighting factor.
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Infer import risk from the WAN
To elucidate how additional information about the geographic distance between nodes
influences p1, we explore two variations of the import risk model: In the variation with “geo-
desic distance weighted” exit probability the populations in Eq 6 are substituted with
^N ðijn0Þ ¼ NðiÞ=di;n0
is the geodesic distance between i and n0. To control for
increasing model complexity, we study the “effective distance weighted” exit probability,
where ^N ðijn0Þ ¼ NðiÞ=deffðijn0Þ, i.e. no geographic information is used, but the model struc-
ture is equivalent.
, where di;n0
Alternative models. Numerous alternative models estimate the OD-matrix, from which
the import probability can be derived [30, 31, 42, 43, 49–52]. Among those, the gravity [27]
and the intervening opportunity [42, 43] model are most widely used. A recent variant of the
latter is the radiation model [43]. Although past studies have found that the gravity model out-
performs the radiation model at small scale [38, 53, 54], especially the radiation model’s good
performance at the large scale [38, 54] makes it an interesting model for mobility on the WAN.
It was originally conceptualized for commuter flows [43] where the surrounding populations
serve as a proxy for possible job opportunities. By estimating an airport’s population based on
its outflow, we adjust the concept from job opportunities to tourism opportunities. Its deriva-
tion from a mechanistic decision process makes it parameter free, and therefore similar and a
good comparison to our model. However, it only requires information on the population den-
sity and does not integrate flight data.
We compare our model to the gravity model with an exponential and power-law distance
dependence and the radiation model (see Material and methods for definitions). These models
solely rely on the outflow data from the WAN to estimate the node’s population and the geo-
graphic locations. To incorporate structural information of the WAN [55], the alternative mod-
els are also implemented with the geodesic path distance (the geodesic distance along the SPT)
and the effective distance, i.e. there are in total nine alternative models: the radiation model,
the gravity model with exponential and with power-law distance decaying function, and each
implemented with geodesic, geodesic path and effective distance. The exponents of the six grav-
ity models are fitted to the reference import probability by assigning the best fitting exponent
to each of the six comparison measures (Pearson correlation, root-mean-square error, common
part of commuters, Kendalls rank correlation and the correlation and RMSE of the logarithmic
measures, all defined in Material and methods) and taking their mean value (see Figs B and C
in S1 Text). As comparison measures, we have chosen three measures that are related to the
absolute error and three that are related to the relative error between estimate and reference.
Symmetry by returning visitors. Each of the twelve models provides an estimate for the
import probability p(i|n0), which is used to compute the OD-matrix T through multiplication
with the corresponding source population N(n0). By comparing the symmetry of T with the
reference OD-matrix ^T, we find a much higher and qualitatively different symmetry in the ref-
erence data (see Supplementary Note B, Fig D in S1 Text). The high symmetry is likely due to
visitors (family, business, tourism, etc.) that dominate the international travel. They return to
their home-location after a limited period [56] and only the minority of the travelers are
migrants, i.e. stay permanently at the destination. Interestingly, the import risk model has the
highest symmetry, but is still less symmetric than the reference data by a factor of 4. Therefore,
before conducting a detailed comparison of the estimates, we rectify the import probability
estimates by symmetrizing their OD-matrix (by extracting the symmetric part and recalculat-
ing the import probability; for further details, refer to Material and methods and Supplemen-
tary Note B in S1 Text). This correction can be seen as an alternative version of a doubly
constrained model where normally the constraints on in- and out-flow are ensured by an itera-
tive proportionate fitting [31].
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Model comparison
In the subsequent analysis, we evaluate the import probability estimates against the reference
data through four approaches: (i) a direct comparison and assessment of their medians to
identify potential systematic errors, (ii) the application of six distinct goodness-of-fit metrics
to assess the individual model’s rank and relative performance, (iii) a classification task identi-
fying countries with the highest import risk, particularly relevant in the context of a pandemic
and (iv) a correlation study of the arrival time of 20 diseases and SARS-CoV-2 variants.
Qualitative comparison.
In Fig 3 the import probability estimate p(i|n0) of each model is
compared to the reference import probability ^pðijn0Þ. The gravity models exhibit the closest
agreement with the reference data when the effective distance is employed, as indicated by the
medians (Fig 3, first and second columns). In contrast, the median values of the radiation and
import risk models are relatively stable and less influenced by variations in distance metrics or
their associated weighting (third and fourth columns). All models overestimate the lowest
median import probability (leftmost orange dot in Fig 3), since the estimated import probabil-
ity is always nonzero, but a large proportion of the lowest reference import probabilities are
zero due to the limited observation period and/or an insufficient number of departing passen-
gers. The overestimation of the median import probability is observed up to p(i|n0) � 10−4 for
both the gravity and import risk models. However, this overestimation is notably absent in the
case of the gravity model with an exponential distance decaying function and the effective
Fig 3. Estimates of import probability by the gravity model with exponentially (1st column) and power law (2nd column)
decaying distance function, the radiation model (3rd. column) and by the import risk model (4th column). The first three
models (1st-3rd column) use as distance the geodesic (1st row), geodesic path (2nd row) and the effective (3rd row) distance. The
import risk model is computed from the WAN with the geodesic distance (D) or the effective distance (L) as a weight for the exit
probabilities or without weighting (H), i.e. in the last two cases (H, D) only WAN information is used. The orange line depicts the
median and the gray line is y = x and illustrates perfect mapping.
https://doi.org/10.1371/journal.pcbi.1011775.g003
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
distance metric (Fig 3I), where the median demonstrates the closest alignment with the refer-
ence data. The radiation models (third column) systematically overestimates the highest import
probabilities (p(i|n0) >� 10−1) and consequently underestimates the lower import probabilities.
Goodness of fit by multiple measures. We compared each model with the reference
import probability via the Pearson correlation, the root-mean-square error (RMSE), and the
common part of commuters. These measures are more sensitive to strong links, i.e. large
import probabilities, which is important when the emphasis is placed on the countries that are
most likely to import passengers. However, if the focus is to get a fair comparison including all
links, logarithmic versions of the above measures or rank correlations are more appropriate.
Thus, we also quantify the agreement by the correlation and the RMSE of the logarithm of the
measures and by Kendall’s rank correlation. The three import risk model variations outper-
form the other models in all but one measure, whereby the variation employing the geodesic
Fig 4. Rank and relative performance of import risk estimation models. The different import probability models are
compared via their rank (A) and relative performance (B), with the highest values representing the best approach. The
rank and relative performance are shown for each (black dots) of the six comparison measures (corr, logcorr, RMSE,
logRMSE, cpc, τKendall) the box illustrates the interquartile range, the horizontal line the median and the red triangle
the mean. The colors of the boxes illustrate the different distance measures in use. The outlier measure of the import
risk models (I.R.) is the logRMSE, where the gravity models with effective distance are performing best. See Material
and methods for definitions of comparison measures and Figs E, F in S1 Text for absolute and detailed relative
performance.
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
distance weighted exit probability performs best (Fig 4A). Following the import risk models,
the two gravity models based on effective distance also exhibit strong rankings. In contrast, the
remaining models lack consistent high rankings across all six measures and are more evenly
distributed within the lower half. This model categorization also holds for the relative perfor-
mance of the models (Fig 4B), with linear scaling of values in between (see Eq 22). In contrast
to the rankings, the median relative performance shows a notable improvement when the
gravity models incorporate effective distance. However, among the import risk models, the dif-
ference in median relative performance remains marginal.
The only measure where the import risk models are outperformed by the gravity models
with effective distance is the logRMSE (Figs E, F in S1 Text). It is expected from the gravity
models’ good agreement in median import probability with the reference data over wide
ranges and the overestimation of low import probability by the import risk model. This overes-
timation can be reduced by model-modifications that introduce parameters favoring the exit
at nodes with large-populations (for details, see Supplementary Note C and Figs G, H in S1
Text). However, we refrain from adding complexity to the model, since its generic nature is its
key aspect.
Classification of ten top risk countries.
In a pandemic context, it is of specific interest to
identify the countries with the highest import probability. We analyzed how well the twelve
proxy models can classify, if a country is among the ten countries with the highest import
probability. Again, the import risk models outperform the other models and the one with geo-
desic distance-weighted exit probabilities is the top predictor with a sensitivity of 71.1% (Fig
5D). All effective distance-based models have a high sensitivity (>� 65%), including the radia-
tion model with 66.8% that had the lowest relative performance and second-lowest mean rank
(Fig 5I–5K). For these high import probabilities, the import risk models now outperform the
Fig 5. Classification of the 10 countries with the highest import probability by the gravity model with
exponentially (1st column) and power law decaying (2nd column) distance function, the radiation model (3rd.
column) and by the import risk model (4th column). A true or false positive (T. Pos. or F. Pos.) means that the country
is or is not among the 10 countries with the highest reference import probability ^p. A false negative (F. Neg.) means
that it belongs to the reference set but was not detected by the respective model. The pie chart illustrates the sensitivity
of the models.
https://doi.org/10.1371/journal.pcbi.1011775.g005
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Fig 6. Correlation analysis: Disease arrival time vs. the effective model distance. Each model’s import probability is converted to
an effective distance dM(i|n0) = −ln(p(i|n0)) with n0 as the outbreak country of the respective disease. The correlation results C(tA, dM)
with the arrival time tA(i) of the disease in the target country i are grouped by model (A) and by the disease (B). As comparison
distances, the correlation of the geodesic, geodesic path (on the effective shortest path tree) and the effective distance with tA are
shown. Each dot represents a correlation result of the 21 considered outbreaks (H1N1 in 2009, COVID-19 in 2020 and the spread of
18 of its variants in the years 2020–2022).
https://doi.org/10.1371/journal.pcbi.1011775.g006
other models also in terms of RMSE and logRMSE, i.e. the 10 countries at highest risk are not
only classified best by the import risk model, but also quantitatively assessed best.
Disease arrival time.
In our final comparison, we evaluate the correlation between disease
arrival times and the estimated import probability from the outbreak country of the disease.
Note that the effective distance, which is the base of the import risk model, already has the
clear relation to disease arrival times and the import risk model is developed to extend this
qualitative relation to a quantitative number of passengers imported, as done in a recent study
on the pandemic potential of SARS-CoV-2 variants [11]. However, a qualitative comparison to
arrival time is of course possible via the negative logarithm of the import probability for each
model, which we refer to as effective model distance, which linearly relates [16, 19] to the arrival
time tA(i|j) of a disease
dMðijjÞ ¼ (cid:0)
lnðpijÞ / tAðijjÞ
ð7Þ
with j as the disease outbreak country. The arrival time tA(i|j) is the number of days between
the disease outbreak and the day the first case is reported in the target country i. We evaluated
the correlation C(tA, dM) for the H1N1 pandemic starting 2009 [8], the COVID-19 pandemic
starting 2019 [57] and 18 of its variants. Additional to the import probability models, the cor-
relations of the geodesic, geodesic path and effective distance with tA are included. Our analysis
reveals that models employing the effective distance as the distance measure consistently out-
perform those relying on the geodesic or geodesic path distance (Fig 6A). Interestingly, the
gravity model with a power-law decaying distance function consistently performs well, regard-
less of the specific distance measure employed. We do not observe a specific model that excels
exclusively for certain diseases. Instead, we observe similar correlation values for the same dis-
ease across models (Fig 6B), which suggests that there is considerable noise on the arrival time
tA that varies between diseases. The noise could be related to the disease specific spreading
speed: our assumption, that the outbreak country is the sole source, gets increasingly violated
the slower the disease spreads, because other countries become secondary sources. A simple
linear regression of the mean correlation hC(tA, dM)i and the mean arrival time htai supports
this hypothesis (r = −0.44, p = 0.055, Fig K in S1 Text).
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Import risk of countries and regions
Having quantified the performance of the import risk model, we now focus on (i) country spe-
cific differences in its prediction quality, (ii) possible limitations due to no concept of adminis-
trative units (e.g. countries) whose airports are more interconnected and (iii) how the geodesic
distance is encoded in the import risk model, i.e. how a distance dependence emerges from
WAN information only.
Country specific performance.
In the import risk approach, we assume minimal knowl-
edge of the system, i.e. only the WAN is known. Consequently, we differentiate countries only
via their network properties, one of which is the degree of a node, or more precisely the node
strength, since the WAN is a weighted network. It is the simplest metric that is also easily
adjustable for the country-level perspective. At the country level, the node strength corre-
sponds directly to the flow out of country C
FC ¼
X
X
n2C
m=2C
Fmn :
ð8Þ
This country-specific characteristic signifies a country’s potential to influence the network’s
structure, since flows from small-outflow countries are diluted by large-outflow countries.
From an ecological point of view, the outflow is strongly correlated with the gross domestic
product of a country (Fig N in S1 Text). The correlation (logcorr) between the logarithms of
the import risk p1 and the reference import probability ^p1 improves with the outflow of the
source country (Fig 7), as illustrated by Great Britain (GB) as the country with the largest out-
flow in the WAN and Eritrea (ER) as one of the countries with the lowest outflow. The predic-
tion improvement with the country’s outflow suggests that the WAN is dominated by large-
outflow countries and therefore predictions worsen for countries with lower WAN outflow.
However, the prediction improvement is also present in model alternatives that do not use
WAN information at all (e.g. gravity with geodesic distance, Fig M in S1 Text). We rule the
explanation out that the alternative models show this improvement due to preferential fitting
of strong links—and therefore of large-outflow countries—since the models are fitted to the
reference data by their import probabilities, which ensures equal weighting among countries.
It rather suggests that the mobility behavior in low outflow regions is different, also supported
by the sudden performance saturation for countries with a WAN outflow of FC >� 106 (Fig 7
and Fig M in S1 Text). Possibly, their passenger distribution is constrained by additional fac-
tors and is limited to the regions in proximity.
There are clear exceptions where the import risk estimation is worse compared to outbreak
countries with a similar WAN outflow, as Australia (AU), Israel (IL) and Macao (MO). These
countries are connected due to historical relations to specific regions that are either not in
their direct neighborhood (European countries for AU and IL) or that are more important
than the bare neighborhood would suggest, as Macao that is a special administrative region of
China. For Macao the import risk to China is underestimated, which consequently overesti-
mates the import to other countries, and for AU and IL Europe is underestimated which over-
estimates other regions (Fig 7). AU, IL, and MO serve as examples illustrating that the WAN
may not fully encapsulate all relevant information accessible to the import risk model. Another
concept that is missing in our methodological approach is the idea of a country or another
administrative unit. Instead, it treats airport pairs uniformly, disregarding their country affilia-
tions. Since we know the international flights leaving a specific country from the WAN, we
can run a self-consistency analysis, i.e. without the need of reference import probability data.
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Fig 7. Source countries’ prediction quality and WAN outflow. The correlation between the logarithm of the import
risk and the reference import probability logcorr ¼ corrðlogðp1Þ; logð^pÞÞ improves with the outflow of the respective
source country (top). Examples of source countries with particularly low (ER, Eritrea) and high (GB, Great Britain)
outflow and log_corr are shown with their import risk and reference import risk to target countries (middle row).
Countries with exceptionally low log_corr measures compared to source countries with a comparable outflow are
either historically linked to specific regions as Australia (AU) and Israel (IL) to European countries (lower right panel)
or politically as Macao (MO) as a special administrative region of China.
https://doi.org/10.1371/journal.pcbi.1011775.g007
We can estimate the outflow leaving the country C by the import risk model by
X
X
TC ¼
p1ðmjnÞNn :
n2C
m=2C
ð9Þ
If we compare it to FC the WAN flow out of country C (see Eq 8), it turns out that the import
risk model systematically overestimates the flow out of a country (Fig I panel A in S1 Text). In
fact, the relative error increases with the number of airports belonging to the country (Fig I
panel B in S1 Text). Possible explanations for this overestimation include the absence of a
country-specific concept within the import risk model and the unintentional inclusion of tran-
sit passengers in the population count of airport catchment areas (since we use the outflow as a
proxy for the population). However, we can easily correct for this overestimation on country-
level analysis, by normalizing the airport population such that the WAN country outflow is
recovered.
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Fig 8. Import risk aggregated on regional level “to target” vs. “from source” and its geodesic distance dependence. The geodesic distance between regions predicts
the import risk p1 to a single target from all sources (A, B) better than from a single source to all targets (D, E) as can be seen by the p-values (C) of the power law fit
p1(d) = c�d−α that is illustrated for each selected examples by a grey line (A, B, D, E). The fitted exponent α of the import risk to a single target decreases with the
respective regional WAN flow out of the target region (F), i.e. the more connected a region, the weaker the import risk decays with distance. The dashed horizontal
lines show the average import risk of a single target (A, B) or a single source (D, E). The color of the dots corresponds to the depicted world regions (right). Maps are
created with geopandas [48].
https://doi.org/10.1371/journal.pcbi.1011775.g008
Geodesic distance dependence. The import risk model estimates import probabilities
without explicit geodesic-distance information (excluding the variant with distance weighted
exit probability). Since classical models have proven distance to be a good predictor for human
mobility, we assume that it is encoded in the WAN structure and by consequence in the
import risk estimate [58]. To enhance clarity, we aggregate the import risk data across twenty-
two world regions. We observe that the import risks to individual targets decrease in a manner
resembling a power-law as the geodesic distance to the sources increases (Fig 8A and 8B and
Fig L in S1 Text). When we change our perspective and examine the distance-dependence
from a single source to all target regions (Fig 8D and 8E), the observed dependence is less con-
sistent with a power-law fit of the form p1 ¼ c � d(cid:0) a
import risk is computed via a source-centric view (by computing the exit probability from the
shortest path tree originating at each source), which suggests that the distance dependence
should be best from one source to its possible targets. A possible explanation is that each target
possesses its own attractiveness independent of the source region. This suggests that the distri-
bution dynamics may resemble a pull mechanism rather than a push mechanism. Indeed, we
find that the fitted exponent α from the power-law fit decreases as the WAN flow out of the
target region increases, which can serve as a proxy for the attractiveness of a region (Fig 8F). In
other words, the more attractive a region, the larger the import risks from more distant source
regions. The fitted exponent c has a high rank correlation with α (τKendall = 0.89), i.e. also the
coefficient is dependent on the attractiveness of the region.
(Fig 8C). This is surprising, since the
ij
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Discussion and conclusion
Motivated by the import probability’s strong dependence on the effective distance, we imple-
mented the import risk model based on the effective distance shortest path tree’s exit probabil-
ity in combination with a random walk on the WAN. As a result, we can infer the passenger
trip distribution within the traffic network of their transport vehicle (WAN). When we com-
pare our parameter-free model to variations of established mobility models, we observe that it
surpasses the alternatives in most comparison measures. The only exception is where the two
parameter-fitted gravity models with effective distance perform the best. The import risk
model is the most accurate in determining countries with the highest import probability and is
one of the models that correlate best with the time of arrival of 20 diseases, showcasing its
importance for epidemic-related problems. However, it systematically overestimates low
import probabilities and its performance worsens for countries with a passenger outflow
below a million per year. Despite the lack of any explicit geodesic distance information, the
import risk model recovers a geodesic distance dependence. This distinction is more promi-
nent when considering all sources to a single target compared to the reverse scenario. We attri-
bute this phenomenon to a target’s specific attractiveness, which we estimate using its node
strength, i.e. the target’s passenger outflow.
The only measure where the gravity models with effective distance outperform the import
risk models is the logRMSE. This is likely due to their good agreement over wide ranges of the
import probability (Fig 3I and 3J). The import risk model performs poorly with respect to the
logRMSE due to its systematic overestimation of low import probabilities. Note, that the sec-
ond parameter free model, the radiation model, systematically underestimates low import
probabilities in the same way as the import risk model does. This is expected, since deviation
from the assumptions cannot be corrected by any parameter adjustment. We identified several
ways to reduce the import risk’s overestimation of low import probabilities by introducing an
additional parameter that scales the population of the respective airport, changes the exit prob-
ability along the shortest path tree or only the exit probability of specific nodes (for details, see
Supplementary Note C and Figs G, H in S1 Text). In conclusion, we find that introducing
modifications that enhance the probability of exiting at airports or nodes with large popula-
tions mitigates the issue of overestimation. However, we leave this as a possible extension of
our model and highlight that it outperformed the other models in all correlation measures,
illustrating its high potential.
The radiation model’s poor performance can likely be attributed to its initial design, which
focused on small-scale commuter flows driven by work opportunities [43], which shows that
bottom-up approaches are often limited to their specific use case but can be adapted, such as
the extended radiation model [59], which is no longer parameter-free and has similar perfor-
mance to the gravity model [54]. Interestingly, the radiation model is the only one that does
not improve with inclusion of flight network information via the geodesic path or the effective
distance (Fig 4). The radiation model’s insensitivity to network information can be attributed
to the fact that it only extracts rank information from the distance data, resulting in a signifi-
cant loss of information. The rank representation has the problem that airports that directly
follow in their rank with respect to a source airport could be separated by a mountain range or
ocean, i.e. the rank difference is minimal but the actual distance immense. This argument
holds for any distance information.
We corrected the import probability by the symmetrization of the respective OD-matrices
which corresponds to a specific form of a doubly-constrained model. Normally, the constraints
only ensure that the out- and inflow of each location corresponds to the observations [31, 52,
54], in contrast, we assume that both equal each other because of returning visitors. We
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
repeated the model comparison without the correction: it reduced the agreement with the ref-
erence data for all but five of the seventy-two model-measure combinations (Fig F in S1 Text),
which is in agreement with previous studies that report a better performance of doubly con-
strained models [54]. Importantly, the import risk model still outperforms the other models if
the import probability estimates are not corrected (compare Fig 4 with Fig J in S1 Text). It’s
crucial to note that the assumption of returning visitors is applicable when visitors and tourists
dominate while migrants can be disregarded. However, this assumption may not hold for links
between low- and high-income countries or conflict regions.
In the disease arrival time analysis, all models that use the effective distance perform simi-
larly well, including all gravity models with power-law distance decay. The disease arrival time
tA correlates with the logarithm of the estimated import probabilities, i.e. the results should be
in agreement with the logcorr goodness of fit results. The models with effective distance vary
only by maximal 0.07 in their logcorr measures and these are based on 183 countries as poten-
tial source (Fig J in S1 Text). However, the 20 diseases in the arrival time analysis have only 10
unique outbreak countries. Additionally, due to factors like varying testing rates between
countries, the uncertainty in arrival times, and other factors, the sample size is likely insuffi-
cient to recover the logcorr results. In order to decrease the noise on tA, we repeated the analy-
sis by extrapolating the arrival time via a logarithmic fit on the early cases, i.e. assuming an
initial exponential growth (see Supplementary Note D in S1 Text). As a result of this proce-
dure, some countries with insufficient data for extrapolation had to be excluded, which in turn
led to the exclusion of more diseases. Nevertheless, the results are consistent with the tA esti-
mation by 1st count (compare Fig 6 and Fig P in S1 Text).
We found that without providing any geodesic distance information to the import risk
model, a distance dependence is recovered that is stronger for import probabilities to a single
target, than from a single source, even if the import probability is computed from a source-
centric view. Since the WAN is spatially embedded and has a network dimension of three [58],
its connections reflect up to a certain degree the characteristics of the embedding space. This
explains the import risk model’s ability to capture distance dependence in general. That dis-
tance is a better predictor in the target-centric view aligns well with a previous study in which
a target-specific human-mobility model collapses mobility data to multiple targets by assigning
each target a specific attractiveness that is proportional to the target’s population [51].
The import risk model predictions worsen for countries with a small outflow on the WAN,
and since the country’s WAN outflow is proportional to its gross domestic product, the model
performs less good for countries with a lower GDP, i.e. small population and/or low to middle
income countries. This is unfortunate, as our model derives Origin-Destination (OD) infor-
mation (costly to directly monitor) from cost-effective traffic flow monitoring, making it par-
ticularly valuable for regions with limited resources. However, we find that the model
alternatives (gravity, radiation) also perform poorly for low-outflow countries and that the pas-
senger distribution of the latter is most likely constrained by the GDP and thus limited to the
target-regions in effective proximity. To circumvent this problem, one could aggregate neigh-
boring low-outflow countries until the conglomerate crosses the outflow threshold of FC = 106
above which we observe a performance saturation (Fig 7 and Fig M in S1 Text). Of course, this
compromise comes with a lower spatial resolution and we emphasize the need for future
research in this direction.
While we have assessed the model’s performance on the world air transportation network,
its applicability extends to other modes of transportation such as subway systems, cars, buses,
and trains. Future research will explore the specific conditions under which this model can be
effectively applied. Furthermore, there is room for improvement in the basic estimation of the
traveling population within an airport’s catchment area based solely on its outflow. This
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
estimation does not currently account for the significant role of hubs and the missing informa-
tion about transit passengers. The simple framework that only relies on the traffic network is
appealing, but in certain scenarios its prediction can be refined by using information about the
GDP, Gini-coefficient or population density.
Our comparison focused on the parameter-free radiation model and the fitted gravity
model, but we acknowledge the existence of promising variations and alternative models that
were not included in this study [30, 31, 54, 59]. However, the gravity model is widely applied
and has been shown to perform equally well [59] or better than alternatives [54]. There are
exceptions, e.g. an iterative computation of a gravity-like model outperforms the common
gravity model in cases where the complete mobility network is not available [29]. Additionally,
the radiation model outperforms the gravity model for long-distance connections [38, 54].
Still, the simplicity of the gravity model and its adaptability by parameter adjustment make it a
strong counterpart. The model alternatives make use of the WAN-structure information by
using the effective distance as done in e.g. Ren et al. [60] where the radiation model with time-
distance was better than the travel-distance on the road network to predict the traffic on each
link. Similarly, we observed that the effective distance, which is related to the arrival time of
diseases, outperforms geodesic path-distance in predicting import probabilities.
The import risk model is fundamentally different from classic approaches that estimate OD
trips from traffic data, because the latter find the OD trips that best reproduce the traffic data
[28, 30, 44, 45], while our model runs a distribution process on the traffic data network. Thus,
our model is a mechanistic bottom-up approach, while the classic approaches either fit and
require the knowledge of the reference trip data [28, 30] or are based on the assumption that
the trip distribution across the links follows the maximum entropy principle, i.e. the OD trips
are considered as most likely that can be realized by the largest number of microstates [44, 45].
Note that maximum entropy approaches require an estimation of routes and their alternatives
between each OD pair, while we allow all routes to be taken by the random walker. To the best
of our knowledge, our model stands as unique in its mechanistic nature, enabling the study of
modifications to its underlying distribution process. This includes strategies for containment
aimed at slowing or restricting a pandemic, for instance. A straight forward implementation
could be the testing of a fraction of passengers Ci � 1 at every transit airport i, which corre-
sponds to reducing the probability to continue walking of an infected passenger (Eq 2) to
~Sn;n(cid:0) 1ðn0; CÞ ¼ ð1 (cid:0) Cn(cid:0) 1Þ � Pn;n(cid:0) 1ð1 (cid:0) qn(cid:0) 1ðn0ÞÞ :
With C = [C1, C2, . . .] one could allow for a varying testing capacity between the airports.
Material and methods
Data sources
The WAN provided by OAG (Official Airline Guide) [46] contains the number of flights and
the respective maximum seat capacity Fi,j between airports i and j aggregated for the year 2014.
The reference import probability ^pðmjnÞ ¼ ^T mn= ^T n is based on the “Global Transnational
Mobility Dataset” [40, 47] that assigns the number of trips in 2014 ^T mn from country n to m
worldwide by combining the world air transportation origin-final-destination data set from
the company SABRE, and cross-boarder visits with an overnight stay from the UNWTO
(World Tourism Organization). Thus, ^pðmjnÞ represents not only the mobility via air travel
but also via other means (sea, road, rail). However, air travel dominates long distance trips
which makes it a fair reference set of the air transportation origin-final-destination matrix. For
details on how the data sets were combined, see Supplementary Note A in S1 Text.
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Alternative models
The gravity model states that the number of trips between regions n and m increase with their
population sizes (Nn and Nm) and decrease with distance dnm
Tmn ¼ On
Nn Nm
f ðdnmÞ
;
ð10Þ
with f(d) as a function that grows monotonically with distance d, most often chosen as either a
power-law f(d) = dγ or an exponential f(dnm) = eγd.
In the radiation model, the trips from n to m depend on their respective population sizes
Nn, Nm (or other measures as job opportunities) and on the number of people smn that are in a
circle with radius rmn centered around location n including Nn and Nm:
Tmn ¼ On
Nn Nm
ðsmn (cid:0) NmÞsmn
:
ð11Þ
The import probability of both models is computed by normalizing the trips with respect to
the source-region
pðmjnÞ ¼
TmnP
jTjn
¼
Tmn
Tn
:
ð12Þ
Trip-symmetrization
We correct the import probability via symmetrizing the OD-matrix by (i) compute the esti-
mated OD-matrix
m;n ¼ pð0ÞðmjnÞNn
Tð0Þ
from the import probability estimate, (ii) correct it by computing its symmetric part
S ¼ ðT þ T>Þ=2
and (iii) compute the corresponding corrected import probability via
pð1ÞðAjBÞ ¼ SAB=SB :
ð13Þ
ð14Þ
ð15Þ
By going through these steps, the asymmetry is reduced heavily but still persists. Thus, we
repeat steps (i) till (iii) until p(3)(A|B), which returns for all models a comparable asymmetry in
mean and median to the reference data (see Supplementary Note B in S1 Text for details).
Comparison measures
We compare the import probability models with the reference data via the Pearson correlation
corrðx; yÞ ¼
E½ðx (cid:0) �xÞðy (cid:0) �yÞ�
sxsy
;
with E½x� � �x as average, the root-mean-square error
RMSEðx; yÞ ¼
q
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
E½ðx (cid:0) yÞ2�
;
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ð17Þ
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PLOS COMPUTATIONAL BIOLOGYthe common part of commuters [59]
cpcðx; yÞ ¼
P
2
P
ij minðxij; yijÞ
P
ijxij þ
ijyij
Infer import risk from the WAN
;
ð18Þ
which is 1 if all links are identical and 0 if none of them agrees. All the above measures are
more sensitive to strong links, i.e. large import probabilities. However, if the focus is to get a
fair comparison including all links, we are more interested in logarithmic versions of the
above measures or rank correlations. Thus, we compare the logarithm of the import probabili-
ties via correlation
logcorrðx; yÞ ¼ corrðlogðxÞ; logðyÞÞ ;
root-mean-square error
logRMSEðx; yÞ ¼ RMSEðlogðxÞ; logðyÞÞ ;
and use the Kendall rank correlation coefficient
tKendall ¼
q
C (cid:0) D
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
ðC þ D þ TxÞðC þ D þ TyÞ
;
ð19Þ
ð20Þ
ð21Þ
with C and D as the number of concordant and discordant pairs and Tx and Ty as ties only in x
and y, respectively.
To simplify and generalize the comparison we combine the six above defined measures by
computing the mean rank of each model, i.e. the best correlating model has the highest (12)
and the worst the lowest (0) rank and the mean rank of one model is the average of all six
ranks.
To quantify the mean difference between the models we define the relative performance of
one model M as
rel:perf:ðf ðxM; yÞÞ ¼
f ðxMÞ (cid:0) worstðf ðxkÞ; kÞ
bestðf ðxkÞ; kÞ (cid:0) worstðf ðxkÞ; kÞ
;
ð22Þ
with f(xM) = f(xM, y) as the specific comparison function and best( f (xk), k) and worst( f (xk), k)
as the best and worst performing value of all models using this comparison function. Note,
that best(. . .) = max(. . .) apart for the rmse-measures, where it is min(. . .) (analog for worst
(. . .)).
Disease arrival times
The disease arrival time tA(i) in country i is estimated by the date of the first reported case for
H1N1 and SARS-CoV-2. For the SARS-CoV-2 variants we use the first sequenced sample in
this country. However, for certain variants some sequenced samples appear in the statistics
month before the outbreak date declared by the WHO [61], which we treat as misclassifica-
tions, discard them and use instead the first sample after the WHO listed outbreak for the
respective country (see Supplementary Note D for details and Fig O in S1 Text). For each of
the diseases/variants we used the WAN that we have access to and that is closest to the respec-
tive outbreak date (see Table B in S1 Text) and as outbreak country we used the one listed by
the WHO as first country with first sequenced sample of the respective variant [61]. For the
H1N1 outbreak in 2009 we used the case data provided by FluNet [62, 63] (the column
AH1N12009), for the COVID-19 cases we use the WHO COVID-19 dashboard [64] accessed
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
through ourworldindata.org, the number of sequenced samples was accessed through GISAID
[65–67] using the file gisaid_variants_statistics.json.
Supporting information
S1 Text. Supplementary Note A: Origin-destination data (“Global Transnational Mobility
Dataset”). Supplementary Note B: Symmetrized flows. Supplementary Note C: On the overes-
timation of low import probabilities. Supplementary Note D: Disease arrival time analysis.
Table A. Filtering criteria for the log-cases fit to extrapolate the arrival times tA. A country is
excluded if (C0:) the detection is too sparse before peak-0 (less than 6 weeks of data), (C1:) the
number of cases at peak-0 is below 30 (otherwise the signal is too noisy), (C2:) the extrapolated
arrival time is before the WHO-outbreak date. N is the number of countries for which case
data could be generated. NC0 and NC1 are the countries that pass criteria C0 and C1. NC0 & C1
and NC0 & C1 & C2 are the numbers of countries that pass multiple criteria. Table B. Disease
and SARS-CoV-2 Variant outbreak information and WAN date. For each disease/variant
the outbreak country and the date of the WAN used to compute the import probability esti-
mates with the different models is displayed. Note that we only have the WAN from the years
2014 and 2019 in a yearly resolution and from 2020–2022 in monthly resolution. We repeated
the analysis for COVID with the WAN from the month 2020–01-01, instead of using the yearly
WAN from 2019, which gave comparable results. Fig A. Import probability dependence on
the geographic distance (A), the effective distance (B) and the geographic path distance (C).
The orange line represents the median and C(x, y) is the correlation between the two measures
either log-transformed or not. The geographic distance between countries is averaged over all
airport pairs. The geographic path distance is the geographic distance along the shortest path
derived from the WAN using deff, i.e. it is a combination of geographic and network informa-
tion. The axis scale corresponds to the one with the highest correlation, i.e. log-log for distance
and path distance (A, C) and y-log for the effective distance (B). Fig B. Gravity model scans.
Parameter dependence of measures that compare the model estimated import probability with
the reference import risk ^pðijn0Þ. Thereby is “corr” the correlation, “cpc” the common part of
commuters, “log_corr” the correlation on log-scale, “rmse” the root mean squared error and
“kendalltau” the rank correlation via Kendalls tau. Two versions of the gravity model are
shown with an exponentially decaying distance function f(d) = e−γd (left column: A, C, E), and
a power law decaying distance function f(d) = d−β (right column: B, D, F). As distance the geo-
desic distance (first row: A, B), the geodesic path distance (second row: C, D) and the effective
distance (third row: E, F) are used. The dotted horizontal lines show the comparison measure
with the import risk as model and have the same respective color. Fig C. Mean optimal
parameters for gravity models. For each gravity model with exponentially and power law
decaying distance function and with one of the three different distance measures (geodesic dis-
tance, geodesic path distance and effective distance), the exponent γ or β that results in the
best fit to the reference import risk is shown. The comparison is quantified via the correlation
(corr), correlation between the log-transformed import risks (log_corr), root mean square
error (rmse), root mean square error of the log-transformed import risks (log_rmse), Kendall
rank correlation (kendalltau) and the common part of commuters (cpc). The mean optimal
parameter for each model is marked by a horizontal line and their values are γ = [6.71, 6.41] *
10−4 for geographic and geo. path distance and γ = 0.84 for the effective distance, and β =
[1.90, 1, 95, 5.10] for geo., geo. path, and effective distance, respectively. Fig D. Symmetry
check for OD-matrix. Each dot represents the number of passengers that travel between 2
countries and back. The OD-matrix is computed by the radiation model (1st. column), gravity
model with exponentially (2nd column) and power law decaying (3rd column) distance
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
function and by the import risk model (4th column). The OD-matrix of the models is com-
puted by multiplying the import probability with the source-outflow. The reference trips and
return trips have the highest symmetry (5th column, M). The orange line depicts the median
and the gray line is y = x and illustrates perfect symmetry. The mean (AVG(asym)) and median
(MED(asym)) asymmetry of the flows, computed according to Eq. C in S1 Text., are shown in
each panel. The reference trips (M) show the lowest asymmetry, especially for large passenger
flows. Fig E. Relative comparison measures for the import probability estimates. The rank
(A) and the relative performance (B) for the different import probability estimation models.
The model that agrees best (worst) with the reference import risk according a specific measure
has the highest (lowest) rank and a relative performance of one (zero). The relative perfor-
mance is then a linear interpolation between the best and worst model. The comparison mea-
sures are the correlation (corr), correlation between the log-transformed import risks
(log_corr), Root-mean-square error (rmse), Root-mean-square error of the log-transformed
import risks (log_rmse), Kendall rank correlation (kendalltau) and the common part of com-
muters (cpc). As exponents of the gravity models the mean optimal parameter is used (hori-
zontal lines in Fig C in S1 Text.). Fig F. Absolute comparison measures for the import
probability estimates. The comparison measures are the correlation (corr), correlation
between the log-transformed import risks (log_corr), Root-mean-square error (rmse), Root-
mean-square error of the log-transformed import risks (log_rmse), Kendall rank correlation
(kendalltau) and the common part of commuters (cpc). As exponents of the gravity models
the mean optimal parameter is used (horizontal lines in Fig C in S1 Text.). The colors depict
the 4 different models. The solid circles are the models with corrected import probability by
symmetrizing their OD-matrix, and the transparent squares are the non-corrected import
probabilities of the respective model. Fig G. Import risk comparison and its deviation from
a linear relation. Scatter plot (left) and only median and IQR with an exponential fit (right).
Fig H. Variations of the import risk model to investigate how additional parameters influ-
ence the relation between the import risk and the reference import risk. A: the flow scaling
exponent ν that estimates the travelling population N(i) of the airport i depending on its WAN
outflow Fi via NðiÞ ¼ Fn
i (default: ν = 1). B: the effective distance offset d0 that penalizes larger
hop-distances in the effective distance deff(i|n0) = d0 − ln(Pij) when creating the shortest path
tree (default: d0 = 1). C: the descendant fraction introduced in the shortest path exit probabil-
ity, where 0.5 is the default value and values larger than 0.5 mean that the exiting at the descen-
dant (or offspring) nodes compared to the current node becomes more likely. D: different
weight options introduced for the shortest path tree exit probability. Per default, the node pop-
ulations are not weighted. The weight is the inverse of either the geodesic or the effective dis-
tance. E: manually set shortest path exit probability of leaf nodes (dead-end nodes). Per
default, the exit probability is 1. A decrease to 0.9 or 0.8 does not visually change the median.
Fig I. Country outflow reconstruction by import risk. The flow in the WAN leaving a coun-
try FC is estimated by the import risk model by TC = ∑n2C ∑m=2C p1(m|n)Nn. Both measures are
directly compared (A) and the relative error is computed depending on the number of airports
in the respective country Narpts (B). The import risk model does not include the concept of a
country which partly explains the overestimation for larger airports. Another explanation is
the overestimation of the respective airport population Nn = Fn by the WAN outflow for the
import risk model (the true population is smaller because of the transit passengers that need to
be excluded). Note that the WAN is used here, i.e. we check for self-consistency of the model
and no reference data is included. Fig J. Uncorrected models: rank and relative performance.
Same analysis as in the main text in Fig 4), however, here the uncorrected model predictions
are used, i.e. without symmetrizing the OD-matrix. Fig K. Mean correlation between arrival
time and effective model distance vs. the speed of the disease estimated by the mean arrival
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
time htA(C)iC, averaged over all countries C. The correlation C(tA, dM) between arrival time tA
and effective model distance dM is averaged over all models. The size of the datapoints illus-
trates the number of countries that were reached by the disease. Fig L. Import risk between
world regions to a specific target region. In contrast to its derivation the import risk is dis-
played in a target-centric view, i.e. each panel displays the import probability to a single target
region from all source regions. The distance between world regions is the mean distance
between their airport locations. The grey line represents a power-law fit p1 = c � d−α. The
mean import risk is marked for each world region by a horizontal dashed line. The 22 target-
world-regions are sorted according to their mean import risk. Maps are created with geopan-
das [48]. Fig M. Source countries prediction quality and WAN outflow for two gravity
models. Same model-result representation as in Fig 7 but here instead of the import risk
model, the gravity model with power-law distance decaying function using the geodesic dgeo
(left) or effective deff (right) distance is applied. Also for these models the logcorr between
import probability estimates p(i|n0) and the reference data ^pðijn0Þ improves for countries with
a larger outflow in the WAN. Fig N. WAN flow out of countries vs. population and GDP
The WAN flow out of a country is best mapped by its gross domestic product (GDP, C) com-
pared to its population (A) or per capita GDP (B). The linear double-logarithmic regression
results are shown in the lower part of each panel (r- and p-value). The size of each country cor-
responds to its population (A) and the color codes its continent. GDP is taken from the World
Bank Dataset for the year 2014 [69]. Fig O. Variant outbreak detection and fraction of
sequenced samples for each of the considered variants. To illustrate the spread of the variant
and how often it occurs worlwide the fraction of the variant in all sequenced probes is plotted,
i.e. if it reaches 1, all sequenced probes are the respective variant. The official WHO outbreak
date [61] is highlighted as red dotted vertical line. We estimated an outbreak date by 45 days
before the fraction of sequenced samples reached 2.5% of its world-wide peak. The orange ver-
tical lines (lower row of lines) show for each country the arrival of the variant, estimated by the
first sequenced probe (“count1”). The black vertical lines (upper row of lines) show the arrival
times after the outbreak which are used in the main text. Fig P. Correlation analysis with log-
cases estimated arrival time. Each model’s import probability is converted to an effective dis-
tance dM(i|n0) = −ln(p(i|n0)) with n0 as the outbreak country of the respective disease. The cor-
relation results C(tA, dM) with the arrival time tA(i) of the disease in the target country i are
grouped by model (A) and by the disease (B). As comparison distances, the correlation of the
geodesic, geodesic path (on the effective shortest path tree) and the effective distance with tA
are shown. Each dot represents a correlation result of the 10 considered outbreaks (H1N1 in
2009, COVID-19 in 2020 and the spread of 8 of its variants in the years 2020–2022). For the
analysis only those diseases/variants were used with more than 10 datapoints (see Table A in
S1 Text.). Fig Q. New case numbers of the Alpha variant for countries that passed the selec-
tion criteria for the log-cases fit to extrapolate the arrival time tA in the attempt to reduce
noise. The vertical dashed line marks the outbreak as listed by the WHO [61], the yellow star is
the extrapolated arrival time from the log-cases fit that is illustrated by a yellow line. To deter-
mine the peak-0 (marked by a vertical line) we used a difference analysis on the smoothed
new-cases data. Fig R. New case numbers of the Alpha variant for countries that failed the
selection criteria for the log-cases fit to extrapolate the arrival time tA in the attempt to reduce
noise. The vertical dashed line marks the outbreak as listed by the WHO [61]. Those countries
that passed the criteria C0 and C1 (see Table A in S1 Text. for details) show the log-cases fit.
Note that the latter have an extrapolated tA before the outbreak date listed by the WHO. To
determine the peak-0 (marked by a vertical line) we used a difference analysis on the smoothed
new-cases data.
(PDF)
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PLOS COMPUTATIONAL BIOLOGYInfer import risk from the WAN
Acknowledgments
We acknowledge Marc Wiedermann for insightful comments.
Author Contributions
Conceptualization: Pascal P. Klamser, Dirk Brockmann.
Data curation: Pascal P. Klamser, Adrian Zachariae, Benjamin F. Maier, Olga Baranov, Clara
Jongen, Frank Schlosser.
Formal analysis: Pascal P. Klamser, Adrian Zachariae, Benjamin F. Maier.
Funding acquisition: Dirk Brockmann.
Methodology: Pascal P. Klamser, Benjamin F. Maier, Frank Schlosser, Dirk Brockmann.
Software: Pascal P. Klamser, Adrian Zachariae, Benjamin F. Maier.
Visualization: Pascal P. Klamser.
Writing – original draft: Pascal P. Klamser.
Writing – review & editing: Pascal P. Klamser, Adrian Zachariae, Olga Baranov, Clara Jon-
gen, Dirk Brockmann.
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PLOS COMPUTATIONAL BIOLOGY
| null |
10.1167_jov.23.6.7.pdf
|
The configurations and codes for
this experiment are available in: Github
github.com/Znasif/ColorCalibration, Google
Colab colab.research.google.com/drive/
1eHDXJPRn3HaeAqcdGbOKHVJSiNBXBCMv.
| null |
Journal of Vision (2023) 23(6):7, 1–20
1
Calibration of head mounted displays for vision research with
virtual reality
Nasif Zaman
Prithul Sarker
Alireza Tavakkoli
Department of Computer Science and Engineering,
University of Nevada, Reno, NV, USA
Department of Computer Science and Engineering,
University of Nevada, Reno, NV, USA
Department of Computer Science and Engineering,
University of Nevada, Reno, NV, USA
Immersion in virtual environments is an important
analog for scientists. Situations that cannot be safely
organized in the real world are being simulated virtually
to observe, evaluate, and train aspects of human
behavior for psychology, therapy, and assessment.
However, creating an immersive environment using
traditional graphics practices may create conflict with a
researcher’s goal of evaluating user response to
well-defined visual stimuli. Standard computer monitors
may display color-accurate stimuli, but it is generally
viewed from a seating position, where the participant
can see real-world visual context. In this article, we
propose a novel means to allow vision scientists to exert
finer control over the participants visual stimuli and
context. We propose and verify a device-agnostic
approach to color calibration by analyzing display
properties such as luminance, spectral distribution, and
chromaticity. We evaluated five different head-mounted
displays from different manufacturers and showed how
our approach produces conforming visual outputs.
Introduction
Recent advances in virtual reality (VR) head-
mounted displays (HMD) have enabled wide adoption
of the technology in diverse research areas. High-acuity
screen resolution (Varjo XR-3, 2022), a wider field
of view (Pimax 8k, 2022), higly affordable wireless
VR (Oculus Rift, 2022), all-inclusive AR, VR, and
eye-tracking capabilities (Vive Pro Eye, 2020) showcase
how different commercial products have varied
usefulness for research on fields such as vision science
(Li et al., 2022), psychology (Ventura, Baños, Botella,
& Mohamudally, 2018), therapeutics (Emmelkamp
& Meyerbröker, 2021; Hilty et al., 2020), training
(Kaplan et al., 2021; Lee, Park, & Park, 2019) and
simulation (Stock, Erler, & Stork, 2018). Increasingly,
researchers are adopting game engines such as Unreal
Engine and unity to design and present immersive
environments and stimuli to their subjects. Some of
these applications require precise color specifications
and display. However, no standard procedure exists that
help researchers calibrate these HMDs and specify a
color in their chosen color space for visualization.
Increasingly, VR technology is replacing traditional
displays for more immersive experiments and
assessments. For example, virtual simulation of ocular
pathologies such as color vision deficiency (Cwierz,
Díaz-Barrancas, Llinás, & Pardo, 2021), cataracts
(Krösl et al., 2019; Krösl et al., 2020), and macular
degeneration (Zaman, Tavakkoli, & Zuckerbrod,
2020) are helping researchers to quantify the effects
of these diseases on quality of life. Additionally,
VR-based visual assessments are being used to diagnose
glaucoma (Skalicky & Kong, 2019), age-related
macular degeneration (Zaman et al., 2020). Binocular
compensation available in AR displays are being
used to correct neuronal loss in experimental settings.
Traditional optics may soon be replaced digital
spectacles that manipulate the camera feed for recovery
of visual function loss. However, such solutions in the
fields of assessment, simulation, and rehabilitation
would entail a module that can be easily calibrated for
accurate color representation that is common for most
medical usage of color displays.
Several lines of work exist that characterize the
chromatic properties of different VR headsets and
compare the perceptual performance with more
traditional displays (Toscani et al., 2019), physical
objective tests (Díaz-Barrancas, Cwierz, Pardo, Pérez,
& Suero, 2020; Gil Rodríguez et al., 2022; Cwierz et al.,
2021), and so on. In Diaz-Barrancas, Cwierz, Pardo,
Perez, and Suero (2020), Díaz-Barrancas et al. (2020),
Citation: Zaman, N., Sarker, P., & Tavakkoli, A. (2023). Calibration of head mounted displays for vision research with virtual reality.
Journal of Vision, 23(6):7, 1–20, https://doi.org/10.1167/jov.23.6.7.
https://doi.org/10.1167/jov.23.6.7
Received December 13, 2022; published June 14, 2023
ISSN 1534-7362 Copyright 2023 The Authors
This work is licensed under a Creative Commons Attribution 4.0 International License.
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
2
and; Cwierz et al. (2021), the authors have implemented
a way to reconstruct hyperspectral representation
of physical scenes from multispectral images using
CS-2000 tele-spectroradiometer. The reconstructed
virtual scenes were Color-checker box, Ishihara test
and Farnsworth-Munsell 100 Hue test. Although such
a line of work is focused on creating an accurate virtual
representation of captured scene components, in a
separate line of work Kim, Cheng, Beams, and Badano
(2021) and Toscani et al. (2019) have identified complex
behavior in VR renders with Unity and Unreal Engine
4 (UE4), respectively, that invalidate standard color
calibration practices. In Kim et al. (2021), the authors
experimented with different render configurations
to find the most perceptually correct representation
for medical applications. In Toscani et al. (2019), the
authors have disabled this behavior and formulated
how to accurately control color and luminance in
HTC Vive Pro Eye with Unreal Engine. However, their
solution involved disabling system-wide tonemapping
that is set by default in Unreal. Although this procedure
causes clipped linear gamma behavior per channel and
normal luminance additivity, it changes the behavior
of many built-in shaders and materials, compromising
the realistic effects default to Unreal Engine levels.
Therefore, if researchers require fine-grained control
over the behaviors of specific shaders without altering
the appearance of the rest of the scene, a modular
approach is necessary. More detailed differences
between this work and ours will be discussed in the
next section. In their subsequent work (Gil Rodríguez
et al., 2022), the researchers showed the application
of such a system to a real-world scenario, establishing
the color constancy of a virtual scene calibrated using
their approach. However, disabling the postprocessing
routine means that the scene appears brighter and the
light sources are clipped, contrary to the more realistic
postprocess-enabled pathway. In Murray, Patel, and
Wiedenmann (2022), the authors use look-up tables
and color grading built into Unity to calibrate the
luminance of VR headsets. Their procedure does not
include color correction.
In this work, we present a framework for UE4 that
calibrates and shows any viable color expressed in xyY,
Luv, or Lab color spaces to the displays of a VR HMD
in a modular manner. The main contribution of our
proposed approach is the ability to present the scene
such that parts of the view preserve default properties
while specific stimuli behave according to specified
chromaticity. Our packaged abstraction would allow
researchers to create and render realistic stimuli without
requiring extensive knowledge of the specific HMD
device, spectrophotometer, or color representation
in UE4. Furthermore, unlike Toscani et al. (2019),
the proposed work would allow for a greater number
of researchers to use VR technology for their
workflow.
Our contributions in this work include measuring
and comparing spectral distributions of major
commercial HMDs including HTC Vive Pro Eye,
Oculus Rift, Pimax, Fove and Varjo XR-3 using the
i1 Pro 2 spectrophotometer (i1Pro, 2022). We build
a novel UE4 camera asset that, when placed in any
map, allows the scene to be processed along two
different graphic pipelines. One pathway allows default
Unreal rendering behavior to persist, so that objects
in the scene appear realistic and provide a sense of
immersion. The second pathway objects in the scene
to display color-correct properties that are imperative
for verifiable and reproducible vision research. This
is achieved by modifying the postprocess material so
that every object in the scene would go through the
first pathway or if given a certain custom-depth stencil
value would be processed along the second pathway.
Furthermore, it works alongside i1Pro 2 to calibrate and
preserve parameters of conversion for a specific HMD
with regards to CIE xy, CIE Luv, and RGB. Finally, we
validate whether the predicted and measured values of
random color space coordinates match up closely.
Materials and methods
Standard color calibration practices make some
assumptions about the properties of the display. Similar
to Toscani et al. (2019), we characterize the properties
of the HMDs to apply the appropriate calibration
protocol. Suppose, we define default postprocess
tonemapping as a function of input emissive FLinear
Color RGB values τ (RGB). FLinear Color is an
Unreal Engine object that defines color within a range
of [0,1]. This is distinct from the reflectance values
considered in Toscani et al. (2019), where the scene
objects were either illuminants or Default Lit shading
materials and, therefore, depended on illumination and
viewing conditions.Then, disabling tonemapping has
the following effect on input emissive values:
Lxyview = ˜τ (RGB),
(1)
where ˜τ is a composite postprocess that includes all
other postprocess operations except for tonemapping
τ . In our setup, we use self-emitting virtual surfaces
and we do not disable system wide tonemapping, and
instead, use a mapping function α(RGB) that converts
stimuli RGB values so that, for the output chromaticity,
Lxystimuli
= ˜τ (τ (α(RGB)))
(2)
has the same effect as ˜τ , while the rest of the scene
behaves as default:
Lxyscene = ˜τ (τ (RGB))
(3)
Scene objects are any part of the three-dimensional
environment that is rendered using the Default
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
3
Lit shading model and, therefore, is influenced by
external lighting, shadow, tonemapping, and other
postprocesses. Stimuli are objects that have no inherent
chromaticity and obtain their color value from
prescribed Lxy values that are calibrated to display
exact chromaticity output to the HMD screen.
and the output luminance Y. These relations were
established for three different scenarios:
• Conventional postprocessing.
• Postprocess tonemapping disabled.
• Selective correction.
Experimental setup
Our experimental setups include a handheld
spectrophotometer for recording HMD display outputs.
The spectrophotometer is controlled using MATLAB
script and the HMDs are controlled using Unreal
Engine. We placed the spectrophotometer against the
right display of the HMDs. The device was held in
place so that it pointed to the center of the display.
As we did not have access to wide field colorimeters
such as the I29 used by Gil Rodríguez et al. (2022), this
may have resulted in off-axis measurements. We make
comparisons between the characteristics of the separate
HMDs and between the left and right ocular displays to
help establish reliable color and luminance calibration
procedures.
Calibration process
For calibration, two sets of data were collected
for each headset. The first set involved measuring
luminance and chromaticities of ten linearly spaced
points in the R = RGB(x, 0, 0), G = RGB(0, x, 0),
and B = RGB(0, 0, x) channels as well as a combined
channel (x, x, x) where x(cid:4){0, 1}. The latter set involved
measuring spectral distributions (Sp), chromaticities
(x, y), and luminance (Y) from red, green and blue
primaries alongside the white point.
Using the first set of measurements we modeled
the gamma correction, relation between input RGB to
the emissive property of the shaders in Unreal Engine
With the second set of measurements we verified the
established relation between the input RGB and the
chromaticity of the output (x, y).
Considerations before rendering in unreal
engine
Rendering in Unreal Engine entails several
considerations that help to avoid unintended color
effects. A scene in Unreal Engine consists of two
types of objects: illumination sources and reflective
objects. Unlit shaders behave the same way under
any lighting condition and can be considered as a
self-emissive surface material. Emissive attribute is
the only component that produces chromaticity and
luminosity in unlit shaders. Default-lit materials, in
contrast, are affected by lighting conditions. Figure 1
demonstrates these differences. After a main shading
pass, which applies lighting and specular properties to
objects in default-lit mode and only emissive property
in unlit mode, the scene is passed through a series
of post processing steps that introduce effects like
tonemapping, motion blur, flare, and bloom. Selecting
unlit shader model does not have any impact on these
postprocess steps because these attributes are not
influenced by external lighting conditions, but by their
own properties of self-emission. Therefore, to correct
any tonemapping and color grading, a method can
either be setup by placing an unbounded postprocess
volume in the scene that impacts every scene object
within render view (Toscani et al., 2019) or by changing
the postprocess material of the scene camera. We chose
Figure 1. Comparison between different shading models and attributes.
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
4
Figure 2. Comparison between (Toscani et al., 2019) and our approach.
to create a blueprint ready object (PostCamera) that
inherits from the Camera object in Unreal Engine and
is modified to disable all postprocessing steps solely
through camera settings when placed within a scene
and used as target view. Additionally, for rendering and
measuring stimuli properties, we chose to disable all
illumination sources except for the stimuli. The stimuli
material has lambertian surface parameters enabled
with emissive (RGB) values set to be visible to the scene
camera. This material is applied to a square plane
directly in front of the scene camera. Moreover, our
approach allows users to visually represent two kinds of
materials at once: i) material displaying conventional
photorealistic properties and ii) material displaying
color-correct properties. By assigning selected specific
values to the custom depth pass for each object in the
scene, photorealism-specific graphics routines are not
applied to them. This means illumination, shadow,
exposure, and so on, have no effect on the colorcorrect
material rendered to the corresponding final HMD
pixel output due to its separate graphics pipeline.
In some classical approaches, the light source of the
scene is manipulated to change the reflectance value
of materials for the desired HMD output. Generally,
this approach would be ineffectual in Unreal Engine
rendering pipeline as the postprocess routines would
still alter the chromaticity and luminance intensity
of the scene objects. To make this classical approach
work, Toscani et al. (2019) disabled the complete
postprocess routines. However, this approach still has
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
5
Rendered field of
view (horizontal
in degrees)
HTC Vive Pro Eye
Oculus Rift
Fove 0
Pimax 5k Plus
Varjo VR-3
107
88
90
160
115
Table 1. Specifications of VR headsets.
Pixel density
(pixel per
degrees)
13.45
12.27
14.2
16
70 (central) 30
(peripheral)
Display type
AMOLED
OLED
OLED
LCD
uOLED (center)
LCD
(peripheral)
See-through
camera
Native eye
tracking
Yes
No
No
No
Yes
Yes
No
Yes
No
Yes
some limitations. First, after calibration with a certain
illumination, the scene illumination needs to remain
same for all scenes that use the calibrated reflectance
values. Instead, in our approach, we leverage the
postprocess pathway in such a manner that objects with
custom depth pass assigned to them will behave not
as default lit shader materials, but as self-illuminants.
By leveraging emissive property and the postprocess
pathway, we ensure that the rendering results are
final and independent of scene illumination. Thereby,
calibration process does not need to be repeated if the
scene illumination changes. Figure 2 summarizes the
important differences between Toscani et al. (2019) and
our work.
Equipment
For measuring display outputs we use the i1Pro
2 (i1Pro, 2022) spectrophotometer. We measure the
HMDs mentioned in Table 1. The data in Table 1 are
taken through independent measurements (Murphy,
Maraj, & Hurter, 2018; Hmd geometry database,
2021) or manufacturer reports (Hmd comparison,
2022). Most VR devices have masked diagonal regions,
decreasing the diagonal visible area from those reported
by manufacturers. Therefore, the pixel densities were
calculated by dividing horizontal resolution with
horizontal field of view.
The HTC Vive Pro Eye is widely used for its all-round
functionalities which include a moderate resolution,
field of view, eye tracking and video see-through camera
(480 p). Oculus Rift has lower resolution (1,440 vs.
1,080 horizontal per eye) and field of view, but is a
good choice for commercial therapeutics because of the
affordability of the Oculus headsets. Pimax 5k Plus has
a considerably wider field of view and resolution (2560
horizontal per eye). Fove 0 is a compact alternative to
the HTC Vive Pro Eye. It has a limited field of view
and resolution (1,280 horizontal per eye). However, its
eye tracking api allows vision researchers to monitor
external ocular properties in real time. The Varjo VR-3
is a considerable improvement over all the other HMDs
discussed so far. It has the highest resolution displays
(central 27 degrees 1,920 and peripheral 88 degrees
2,880 horizontal per eye), and cameras (1,080 p). It has
an eye tracking api that gives functional access similar
to Fove. However, its cost may make it unsuitable
for some research and commercial assessment and
therapeutics. These devices vary in display types
(AMOLED: HTC Vive Pro, OLED: Fove 0, Oculus
Rift, LCD: Pimax 5k and mixed: Varjo VR-3). The
mixture of two different display types in Varjo VR-3 of
uOLED (central 27°) and LCD (peripheral) requires
additional consideration before application in color
vision research. The applications were rendered in a
computer with a 4.2-GHz Intel Core i7 processor and a
Nvidia GeForce RTX 2080 graphics card.
Rendering with conventional
postprocessing
This is the default behavior in UE4.27. In these set
of experiments, all camera and postprocessing settings
were left to default behavior.
Relationship between input intensity and
luminance
In Unreal Engine, instances of light sources such
as point light, and directional light have intensity
values (cd and lux respectively) associated with them.
However, physically based lighting may have unintended
effects on stimuli color perception. Therefore, we
chose to use the emissive values (RGB) of the stimuli
material to reproduce the intended luminance (Y).
This procedure allows stimuli chromaticityperception
to be independent of scene illumination and context
although stimuli perception will still be affected.
Figure 3 shows the luminance (cd/m2) corresponding
to the input R = RGB(x, 0, 0), G = RGB(0, x,
0) and B = RGB(0, 0, x) emissive for the HMDs.
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
6
Figure 3. Default configuration. The X axis shows emissive values x in scene material: RGB(x, 0, 0) for red, RGB(0, x, 0) for green,
RGB(0, 0, x) for blue, and RGB(x, x, x) for white. The Y axis shows luminance in cd/m2.
HTC Vive
Oculus
Fove
Pimax
Varjo
Red channel
Green channel
Blue channel
mX
8.9
255.6
18.3
t
17.5
44.15
3.36
mX
54.6
319.8
41.3
t
22.7
53.1
6.75
mX
1.5
29.8
0.6
t
5.5
12.6
1.93
mX
7.8
73.4
18.7
t
5.4
16.5
2.9
mX
57.6
379.7
65.2
t
12.5
45.6
8.1
Table 2. Default configuration: Slope and threshold for modeled relationship between luminance and emissive value.
The figures demonstrate how for different HMDs
the luminous intensities are different for the same
emissive values. LED LCD displays can be brighter
than variants of OLED displays. However, this is
not evident in the results shown in Figure 3. As we
shall see in the other variants of this experiments,
Unreal Engine’s postprocess routines play a role in
the diminished brightness of LED LCD displays.
Furthermore, the default camera exposure lead to the
intensity of emissive materials in the scene to saturate
quickly. Here, our observations differ dramatically from
the ones reported by Toscani et al. (2019) because they
simply used default shaded materials and reflectance
values, whereas we used emissive materials. Default
emissive materials behave like light sources and reach
a predefined intensity to emulate light exposure. For
this reason, in subsequent methods, we disabled the
autoexposure property. Further, in Figure 3, we see that
green has higher luminance than white, which is also a
result of this autoexposure property of self-emitting
surface materials.
All the displays now exhibit properties of a clipped
linear function. The relationship is modeled as follows:
(cid:2)
x · mX (cid:4)[R,G,B], x · mX < t
otherwise
t,
L =
(4)
where L is the luminance, mX is the slope
corresponding with a specific channel, and t is the
threshold beyond which the luminance does not vary
with change in x. Table 2 shows the corresponding
values of mX, t for each HMD.
Table 2 shows that highest exposure effect is
displayed by Varjo for green colors. Varjo is also the
brightest in this default configuration, while Fove is
the dimmest. Therefore, vision research that involves
scotopic stimuli, with realistic rendering still enabled,
can make use of Fove for their research. In contrast, for
simulation of real-world performance, Varjo is ideal,
because it exhibits the highest dynamic range (signified
by the steep slope). However, HTC Vive can be a good
alternative if affordability is a concern.
All displays show a spike and saturation at the
start, which is caused by the saturation due to camera
exposure. Pimax and Varjo HMDs show a secondary
spike. In Varjo, white is the brightest, whereas in all
other displays, green is the brightest. The OLED
displays (Oculus and Fove) show equal spread between
the luminance of these colors. Fove and Pimax have
considerably dimmer brightness compared to the
other HMDs. As default gamma correction is enabled,
displays show piece-wise linear behavior.
Luminance additivity
For standard displays, summation of R, G, and B
channel intensities give grayscale intensities:
L(RGB(x, x, x)) = L(RGB(x, 0, 0))
+L(RGB(0, x, 0)) + L(RGB(0, 0, x))
(5)
demonstrating additive property. However, when
postprocess tonemapping is enabled, as is default for
UE4, such behavior is not visible (Figure 4). Instead,
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
7
Figure 4. Default configuration. The X axis shows emissive values x and the Y axis shows the ratio (LR + LG + LB)/LW.
HTC Vive Oculus
Fove
Pimax
Varjo
HTC Vive
Oculus
Fove
Pimax
Varjo
(LR + LG + LB)/LW
2.74
2.27
2.07
1.78
1.39
Table 3. Default configuration: Average luminance ratios for ten
shades within x(cid:4)[0.1, 1.0].
cred
cgreen
cblue
0.001
0.02
0.04
0.002
0.007
0.006
0.002
0.003
0.002
0.002
0.002
0.005
0.005
0.017
0.023
Table 4. Channel constancy scaling error mse(c ∗ φX
0.1
, φX
x ).
subadditive property is observed for all HMDs. This
shows considerably more subadditivity (approximately
200%) compared with the one observed by Toscani
et al. (2019) because of our choice of self-emitting
surfaces. Here, we can see that Fove is the only device
that shows near constancy across x values. All other
devices show an upfront increase in ratio (caused by
exposure) and a dip at the tail (for x = 1, LW transitions
from grey to white). For different devices, the ratio of
predicted (sum of individual channels) and measured
luminance are shown in Table 3. It further shows that
Varjo is closest to displaying luminance additivity while
HTC Vive is the farthest. It means, for HTC Vive, white
is significantly less bright than the summation of the
primaries.
Channel constancy
Channel constancy is maintained when scaling
emissive values (RGB values) linearly also scales the
spectral outputs by the same factor. Channel constancy
means that scaling the channels independently would
not change the chromaticity and only impact luminance.
To determine whether color constancy is preserved for
all HMDs, we carry out the following experiment. We
measure the spectral output (φ(RGB)) for x = 0.1 in R
= RGB(x, 0, 0), G = RGB(0, x, 0), and B = RGB(0, 0,
x) channels separately. Next, we obtain spectral outputs
sr·m2 ) for x(cid:4)[0.1, 1.0] for all the channels. If
(Radiance W
the spectral outputs are a linear scaling of x, such that:
of display (Varjo with uOLED and LCD), the channels
show multiple peaks for the primaries (Figure 6).
The local peaks indicate multiple wavelengths are
dominantly present in the composition of the primaries.
For the rest of the HMDs the channels show a single
peak. Moreover, the channels have the same scaling
factor of 1 for all the devices except for Varjo. This
means only Varjo violates channel constancy. Using
the scaling factor (c) of the peak of each shade and 0.1
shade we calculate the mean error in Table 4. The error,
e is calculated by taking the mean square error of all
c ∗ φX
channel constancy for all other devices. For Varjo the
constancy error is still small, as we used the peak ratio
x This negligible error demonstrates good
0.1 and φX
However, this may simply be caused by auto exposure
transforming intermediate brightness levels to the
primary brightness level. Further violations of channel
constancy is demonstrated in Figure 5. Only the Varjo
HMD primaries fall inside the chromaticity coordinates
while displaying a slight drift in the shades. For all
the rest of the HMDs, the calibration process creates
a calibration matrix that when applied to original
primary RGB values in R = RGB(1, 0, 0), G = RGB(0,
1, 0), and B = RGB(0, 0, 1) output chromaticity values
that fall outside the gamut. This means the calibration
process based on autoexposure peak values is faulty We
will further investigate the calibration process in the
following subsection.
φX
x=[0.1,1.0]
= c · φX
0.1; where X (cid:4)[R, G, B],
(6)
Calibration test
then it can be said that the HMDs maintain channel
constancy. For the only HMD with more than one type
For standard color calibration to be applicable,
luminance additivity and channel constancy must
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
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Figure 5. Default configuration. CIE 1931 Chromaticity diagram with ‘x’ denoting actual device output for different shades (0.1
through 0.9) of the primaries. ‘o’ denotes the theoretical position of the actual primaries using the calibration matrix.
be preserved (Brainard, 1989). However, as we have
seen in the preceding sections, these properties are
not demonstrated by any of the VR devices while
Unreal Engine’s default postprocess tonemapping is
enabled. This is further demonstrated when we try to
use standard calibration practices to this system. We
record the primaries and using the least square method
find an M that minimizes the euclidean distance XYZ
− M · RGBT. Original XYZ are obtained from the
spectroradiometer measurements of the primaries by
converting xyY to XYZ:
X = x ∗ Y/y
Y = Y/100
Z = (1 − x − y) ∗ Y.
(8)
(7)
(9)
To verify if the calibration was successful, we display
eight different emissive values. These emissive values
correspond to the eight corners of two cubes such that
one corner of the bigger cube is located at RGB(0.2, 0.2,
0.2) and the other corner at RGB(0.8,0.8,0.8) and one
corner of the smaller cube is located at RGB(0.4,0.4,0.4)
and the other corner at RGB(0.6,0.6,0.6). Essentially,
these combination of colors are selected simply because
of their spread in both RGB and chromaticity space
(Figure 7) which facilitates verification of the calibration
process. Next, we measure the Lxy values with the
spectroradiometer. Let us represent the corresponding
CIE xy chromaticity values as Lxymeasured. Using the
conversion matrix from the primaries, let us now obtain
the calibrated position of the cube corners:
Lxypredicted = Lxy(M · RGBT
cube)
(10)
Figure 7 shows how the plotted Lxymeasured and
Lxypredicted deviate, confirming that standard calibration
is not effective. The theoretical coordinates of the cube
points vary significantly between devices owing to the
variation in the chromaticity of the primaries measured
with the spectroradiometer. This is because we use those
values to construct the conversion matrix M. Because
the Varjo device had the primaries most closely situated
with the theoretical position, the mapped cube points
also are quite near to the actual device measurement.
In the following sections we will demonstrate two
methods to calibrate and display nominal values by
1) disabling tonemapping and 2) computationally
correcting for tonemapping.
Rendering with postprocess
tonemapping disabled
As we saw in the earlier section, the standard
camera in Unreal Engine had auto exposure enabled by
default which was responsible for the discrepancy with
luminance additivity, and channel constancy properties
needed for accurate color calibration. These effects
were not present in Toscani et al. (2019) as their objects
were reflective instead of self-illuminant. We therefore
supplanted the standard camera with our PostCamera
object. Our PostCamera object inherits from the
camera actor object in Unreal Engine. It is setup to
partially disable tonemapping at begin play. Disabling
tonemapping entails overriding the autoexposure,
bloom, motion blur, grain jitter, scene fringe, and
graining. Additionally, we applied a postprocess
material that altered the blendable location to Before
Tonemapping. In Unreal Engine, blendables are sets
of parameters such as base color, opacity, and so on
that are passed on to graphics pipeline for rendering.
Different stages of the rendering pipeline read and
write to different blendables. When set to Before
Tonemapping, PostProcessInput0 in the postprocess
material editor provides access to scene color with all
lighting HDR. Therefore, we use it to only counter the
effects of tonemapping using a single pipeline for both
stimuli and scene objects. Figure 8 shows the rendering
pipeline and how the input emissive or chromaticity
values are interpreted to render accurate pixels to the
HMD. Now with these altered settings, we repeated the
previous experiments.
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
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Figure 6. Default configuration. Per channel spectral distribution graph. The X axis denotes the wavelength in nanometers and the Y
axis denotes the spectral output at that wavelength. The spectral distribution of different shades of red, green, blue, and white (from
left to right) are shown for each device (top to bottom).
Relationship between input intensity and
luminance
Figure 9 shows the luminance (cd/m2) corre-
sponding to the input R, G and B channels. The
figures demonstrate how different HMDs react to
disabling postprocess tonemapping. As the auto
exposure is now disabled, the piece-wise-linear
relation is not present. Instead, we can see that
disabling the tonemapping has disabled gamma
correction as well. This is unlike the relationship
found by Toscani et al. (2019) where they found
Journal of Vision (2023) 23(6):7, 1–20
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Figure 7. Default configuration. CIE 1931 Chromaticity diagram with ‘x’ denoting actual device output for different points on the cubes
discussed earlier.‘o’ denotes the theoretical position of the actual RGB values using the calibration matrix.
Figure 8. Demonstration of rendering pipelines for scene object and stimuli object.
Figure 9. Disabled tonemapping. The X axis shows emissive values x in RGB(x, 0, 0) for red, RGB(0, x, 0) for green, RGB(0, 0, x) for blue,
and RGB(x, x, x) for white. The Y axis shows luminance in cd/m2.
piecewise-linear relationship restored by the same
setting. It is possible that their settings included
additional routines to enable gamma correction.
Otherwise, the luminance groups are conserved
so that Fove and Pimax are still dimmer than
the rest. Instead of the tail spike that was visible
for Varjo with default settings, now the opposite
can be seen. The primaries seem to be dimmer
compared with a portion of the shades of the
primaries.
This also illustrates a significant limitation of the
normal settings in Unreal Engine. If a stimulus required
precise luminance control, that cannot be attained as
auto exposure maps most intensities over a threshold
to saturation. Using this disabled tonemapping state,
intermediate luminance levels can be reached.
Journal of Vision (2023) 23(6):7, 1–20
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Figure 10. Disabled tonemapping. The X axis shows emissive values x, while the Y axis shows the ratio (LR + LG + LB)/LW.
HTC Vive Oculus
Fove
Pimax
Varjo
HTC Vive
Oculus
Fove
Pimax
Varjo
(LR + LG + LB)/LW
1.04
1.14
1.39
1.01
1.02
Table 5. Disabled tonemapping: Average luminance ratios for
ten shades within x(cid:4)[0.1, 1.0].
cred
cgreen
cblue
0.017
0.019
0.012
0.028
0.018
0.013
0.069
0.058
0.056
0.01
0.017
0.007
0.078
0.047
0.052
Table 6. Disabled tonemapping: Channel constancy scaling error.
Luminance additivity
Figure 10 shows the luminance additivity property
discussed earlier. The dashed lines represent predicted
luminance (summation of channel luminance) and
the circles represent actual grayscale luminance. As
the predicted and measured luminance values align,
we can say that the luminance additivity property is
preserved. For different devices, the ratio of predicted
(sum of individual channels) and measured luminance
are shown in Table 5.
The ratios are now much closer to 1.0. However, the
OLED display (Oculus and Fove) ratios are slightly
higher. Additionally, Fove HMD shows the same drop
it exhibited in the normal settings.
Channel constancy
As with the earlier channel constancy experiment,
here we determine whether spectral distributions at
higher emissive values are some constant multiples of
the φ(x = 0.1) distributions.
Compared with single spectral distributions for
single type displays, the new distributions have separate
distributions for each shade of the primary colors
(Figure 12). This is a direct result of turning off
auto exposure, as now different shades have different
brightness and therefore different peaks in their spectral
distribution. Furthermore, the scaling factors c seem
to denote multiplicative spectral profile and channel
constancy. Using the same methods of the earlier
section we calculate the mean squared error with the
scaling factors shown in Table 6.
Because auto exposure is now disabled, we can
more easily visualize the difference in luminance for
each shade. Preservation of channel constancy is also
demonstrated in Figure 11. Fove shows significant
drift in measured chromaticity for shades of the
red, green, and blue colors. Other HMDs show
negligible shift in chromaticity. This slight drift is
caused solely by uncorrected gamma. Color gamut
Figure 11. Disabled tonemapping. CIE 1931 Chromaticity diagram with ‘x’ denoting actual device output for different shades (0.1
through 0.9) of the primaries. ‘o’ denotes the theoretical position of the actual primaries using the calibration matrix.
Journal of Vision (2023) 23(6):7, 1–20
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Figure 12. Disabled tonemapping. Per channel spectral distribution graph. The X axis denotes the wavelength in nanometers and the Y
axis denotes the spectral output at that wavelength. The spectral distribution of different shades of red, green, blue, and white (from
left to right) are shown for each device (top to bottom).
for Pimax and Varjo are also within the boundary of
the coordinate system. Demonstrating that disabling
tonemapping is a much better solution for visual
stimuli presentation in VR-based vision science
products.
Color calibration test
We record the new primaries and using the least
square method find an M that minimizes the euclidean
distance XYZ − M · RGBT. New XYZ are obtained
Journal of Vision (2023) 23(6):7, 1–20
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Figure 13. Disabled tonemapping. CIE 1931 Chromaticity diagram with ‘x’ denoting actual device output for different points on the
cubes discussed earlier.‘o’ denotes the theoretical position of the actual RGB values using the calibration matrix. The top row shows
uncorrected thoretical positions of the cube RGBs, while the bottom row shows gamma corrected positions.
from the spectroradiometer measurements of the
primaries by converting xyY to XYZ.
Figure 13 shows the positions of the cube corners
in CIE XY space for predicted and measured xyY
values with the spectroradiometer. Let us represent
the corresponding CIE xy chromaticity values as
Lxymeasured. Using the conversion matrix from the
primaries, let us now obtain the calibrated position of
the cube corners:
Lxypredicted = Lxy(M · RGBT
cube).
(11)
Figure 13 shows how the plotted Lxymeasured and
Lxypredicted do not align perfectly, confirming that
standard calibration is affected by the absence of
gamma correction. We, therefore, designed the following
scheme to apply gamma correction in the XYZ space
using α(RGB) that converts emissive values to produce
the same effect as disabling tonemapping. We apply a
function ˜α(xyY ) on xyY after converting the predicted
XYZ = Mcorrected · RGBT to xyY using the following
equation:
R = X + Y + Z
(12)
x = X/R
(13)
y = Y/R
(14)
Y = Y.
(15)
For an input xyYscene and white point xyYw, we use
the function ˜α(xyY ) defined as:
˜α(xyscene) = xyw + xyscene − xyw
(1 + B|xyscene−xyw|)
˜α(Yscene) =
(cid:2)
x · mX (cid:4)[R,G,B], x · mX < t
otherwise
t,
(16)
.
(17)
This correction is formulated by examining the
relative positions of the predicted and measured
chromaticities. The predicted positions are radially
spread more outwards compared with the measured
values. Our ˜α(xyY ) function revises the predicted
values further inward radially. Figure 20 shows how the
function now maps the predicted values very close to
the measured ones for B = 0.01.
The correction shown in Figure 20 is necessary
because of the gamma correction being withheld by
completely disabling tonemapping and postprocess
settings. Essentially, our function is a gamma correction
in the chromaticity space.
Rendering with selective color
correction
We repeated the measures and analyses presented in
the previous section after re-enabling the tonemapping.
However, we still do it with our PostCamera
substitution of standard camera. However, we disable
all the overrides we made in the previous section,
basically reinstating tonemapping. To correct all the
effects of tonemapping, we rely solely on the postprocess
material now. Instead of using the blendable mode that
Journal of Vision (2023) 23(6):7, 1–20
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Figure 14. Difference between the two rendering pipelines: i) tonemapping disabled and ii) tonemapping and LDR enabled, gamma
corrected.
before tonemapping, we now use after tonemapping so
that the material output is now the final render phase.
To selectively use custom processing on only the stimuli
and leave the rest of the scene with Unreal Engine’s
default realistic rendering, we make use of custom
render depth pass. This property allows the postprocess
material to selectively only apply counter-tonemapping
to the stimuli target. In the postprocess material, we
use scene texture: PostProcessInput2, which is the
scene texture before the tonemapping pass but without
gamma correction. We simply correct gamma and it has
the intended corrective effect, as will be demonstrated in
the following subsections. The differences with previous
method is summarized in Figure 14.
Relationship between input intensity and
luminance
Figure 15 shows the luminance (cd/m2)
corresponding with the input R, G and B channels. The
figures demonstrate how our postprocessing material
alone alters different HMDs rendering, without
changing other postprocess routines. All the displays
now exhibit properties of a clipped linear function as
the input emissive values. However, one distinction
from the clipped linear function of Figure 3 is that now
the saturation does not occur immediately. This is due
to the proxy shutdown of auto exposure through post
process materials. Now, the relationship between input
Journal of Vision (2023) 23(6):7, 1–20
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Figure 15. Tonemapping countered. The X axis shows emissive values x in : RGB(x, 0, 0) for red, RGB(0, x, 0) for green, RGB(0, 0, x) for
blue, RGB(x, x, x) for white. The Y axis shows luminance in cd/m2.
HTC Vive Oculus
Fove
Pimax
Varjo
HTC Vive Oculus
Fove
Pimax
Varjo
(LR + LG + LB)/LW
1.04
1.11
1.12
0.95
0.97
mX
t mX
t mX
t mX
t mX
t
Table 7. Tonemapping countered: Luminance ratios.
intensity and luminance is similar to when the works of
Toscani et al. (2019) disabled postprocessing.
Vive, Oculus, and Pimax show complete linearity in
the given emissive ranges in Figure 15. This means that
vision experimenters can smoothly change the emissive
values to increase the display brightness. Fove and Varjo
show slight clipping, showing that the experiments
would need to be mindful of the brightness beyond
the threshold and either restrict the protocols within
the cutoff brightness or account for the two different
gradients for luminance variation. Interestingly, Varjo
primaries are again a little dimmer compared to the 0.9
shade. Although Fove primaries are not dimmer, the
rate of change is diminished.
Luminance additivity
When postprocess tonemapping is enabled and our
α(RGB) function is applied to counteract tonemapping
for stimuli, luminance additivity is reinstated (Figure 4).
For different devices, the ratio of predicted (sum of
individual channels) and measured luminance are
shown in Table 7. Table 7 and Figure 16 demonstrate
that all the displays are now showing almost perfect
15.5 15.5 24
Red channel
Green channel 40 40.2 67.2 70.5 87.8 85 37 38.5 67
8
7
Blue channel
30 30 8.7 8.8 17.3 15.4
57
7
7.3 7.8 5
2.5 2.5
24
5
7
Table 8. Tonemapping countered: Slope and threshold for
modeled relationship between luminance and emissive values.
additivity, whereas OLED displays are very slightly off.
Table 8 shows the corresponding values of mX, t for
each HMD.
Whereas Fove used to be the dimmest display in
the previous settings, now Fove is one of the brightest
displays. It is now seven times as bright as before.
Brightness of all HMDs have increased in the current
settings, while the dimmest point has remained similar.
This results in the overall increase in dynamic range
of the system. Transforming Fove from one of the
worst devices to render HDR images to one of the best
HMDs for that purpose. However, the difference would
be more indicative of true potential with auto exposure
disabled in the normal camera settings.
Channel constancy
By applying our corrective material, the new
distributions have a higher peak corresponding
Figure 16. Tonemapping countered. The X axis shows emissive values x while the Y axis shows the ratio (LR + LG + LB)/LW.
Journal of Vision (2023) 23(6):7, 1–20
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Figure 17. Tonemapping countered. Per channel spectral distribution graph. The X axis denotes the wavelength in nanometers and
the Y axis denotes the spectral output at that wavelength. The spectral distribution of different shades of red, green, blue, and white
(from left to right) are shown for each device (top to bottom).
with the overall increase in luminance (Figure 17).
Moreover, constant scaling factors c across channels
of a device represent multiplicative spectral profile and
channel constancy. Table 9 shows the least squared
error is consistent with our expectations of channel
constancy.
HTC Vive
Oculus
Fove
Pimax
Varjo
cred
cgreen
cblue
0.012
0.013
0.009
0.028
0.026
0.019
0.052
0.046
0.041
0.021
0.021
0.024
0.028
0.012
0.026
Table 9. Tonemapping countered: Channel constancy scaling.
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Figure 18. Tonemapping countered. CIE 1931 Chromaticity diagram with ‘x’ denoting actual device output for different shades (0.1
through 0.9) of the primaries. ‘o’ denotes the theoretical position of the actual primaries using the calibration matrix.
Figure 19. Demonstration of parallel rendering pipelines. (i) Default-lit and (ii) gamma-corrected and unlit.
In Figure 18, we see that the drift in Fove HMD for
Calibration test
the chromaticity coordinates of intermediate shades
of the whites and primaries is still present. All the
primaries theoretical positions now reside within
the chromaticity diagram and except for Fove, agree
perfectly with measurements.
With the postprocessing routines re-enabled and
application of corrective material, the HMDs now
conform to standard calibration procedure. Again,
we tested its accuracy by rendering the cube corners.
Figure 20. Tonemapping countered. CIE 1931 Chromaticity diagram with ‘x’ denoting actual device output for different points on the
cubes discussed earlier.‘o’ denotes the theoretical position of the actual RGB values using the calibration matrix.
Journal of Vision (2023) 23(6):7, 1–20
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We used the newly calibrated Mcorrected to compute the
nominal values X Y Z = M · RGBT
cubes and converting
to Lxy space. In Figure 20, we see how the measured
values and nominal values are very close, indicating
that it is possible to control the color of the emitted
light with our strategy. Figure 8 shows the rendering
pipeline and how the input emissive or chromaticity
values are interpreted to render accurate pixels to
the HMD
Discussion
We have established that it is not necessary to disable
level wide tonemapping and postprocess settings for
color accuracy. Using our hybrid approach permits
vision scientists to show color accurate stimuli in
real-world settings. This ensures that components
of default behavior of Unreal Engine such as auto
exposure, high dynamic range, tonemapping etc can
be retained for real-world objects while assigning
objects of interest with separate graphics render path
for color accuracy. This is further demonstrated in
the Figure 21 where the primaries of all the HMDs
align to the ideal red, green and blue. In the normal
settings, the primaries appear more washed out and the
whites appear darker for all HMDs. In the settings with
tonemapping disabled, the colors appear closer to ideal
but slightly off due to absence of gamma correction.
HTC Vive
Oculus
Fove
Pimax
Varjo
λred
λgreen
λblue
610
520
450
620
520
460
620
530
460
610–620
540
450
630
540
450
Table 10. Wavelength in nanometer of the peak spectral
distribution for each primaries.
The results are even more apparent when we look at the
visualization of the cube RGBs in Figure 22 described
earlier. The normal settings clearly appear washed out.
Although Varjo still shows washed out effect in the
tonemap disabled settings, the rest of the HMDs only
have a slightly elevated brightness owing to uncorrected
gamma.
Table 10 shows how different the peaks of the
spectral distributions are for each of the HMDs, which
contribute to the overall change in the appearance
and chromaticity coordinates of the primaries. Finally,
in Figure 23, we can see the (cid:7)E (Brainard, 2003)
perceived color difference for each of the discussed
approaches for the cube colors. Our approach clearly
shows significantly lower (cid:7)E. Values less than 1.0 is
imperceptible to human eyes, and Vive shows the least
perceptible difference in our approach, closely followed
by Pimax. Values between 1 and 2 indicate differences
perceptible through close observation between 2 and 10
are perceptible at a glance. This indicates that for most
of the colors, close observation is required to perceive
Figure 21. Approximate visualization of the primaries.
Figure 22. (From left to right: Vive, Oculus, Fove, Pimax and Varjo.) Cube sRGB representation where the top rows are normal settings,
middle rows are tonemapping disabled setting and the bottom rows are postprocess corrected settings.
Journal of Vision (2023) 23(6):7, 1–20
Zaman, Sarker, & Tavakkoli
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Figure 23. Perceived error. (From left to right Standard postprocessing, disabled tonemapping, and our selective correction approach).
The X axis shows index of the cube colors and the Y axis shows the corresponding (cid:7)E perceived error.
differences when VR devices are calibrated using our
approach. Indices 7 and 15 show white and gray points,
which are brought closer together when postprocessing
is disabled, compared with standard. Overall, the line
graph shows that standard postprocessing has an easily
perceptible color difference compared with input and
the variability between devices is high. However, when
the postprocessing routines are disabled, the interdevice
variability reduces while the perceived errors converge.
Conclusion
Future studies that leverage different rendering
pathways laid out in this current work should reveal
how this impacts results of color vision research with
VR-HMDs. Furthermore, this should help researchers
pick the ideal HMD for their particular application.
Their are still limitations to the brightness and color
gamut achievable by any particular HMD, but with
careful consideration of display properties and graphics
rendering pipeline, most relevant stimuli can be
generated with some of the cheaper HMDs. However,
using the two different calibration processes laid out
in this work, a wide range of virtual studies can be
conducted without requiring the express knowledge of
underlying display properties.
Keywords: virtual reality, color calibration, color
vision
Acknowledgments
Supported in part by National Institute of General
Medical Sciences of the National Institutes of Health
under grant numbers [P30 GM145646], the Department
of Defense by grant number [FA9550-21-1-0207], and
by the National Science Foundation by grant number
[OAC-2201599].
The configurations and codes for
this experiment are available in: Github
github.com/Znasif/ColorCalibration, Google
Colab colab.research.google.com/drive/
1eHDXJPRn3HaeAqcdGbOKHVJSiNBXBCMv.
Commercial relationships: none.
Corresponding author: Nasif Zaman.
Email: [email protected].
Address: 1664 North Virginia Street (M.S. 171) Reno,
NV 89557, USA.
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10.1371_journal.pmed.1003998.pdf
| null |
Data will be available to successful applications for clearly specified research projects following /our-research/other-research- policy/data-sharing/ Discussion with the trial team is encouraged to determine whether the relevant data to support the application are available. .
|
RESEARCH ARTICLE
Radiotherapy to the prostate for men with
metastatic prostate cancer in the UK and
Switzerland: Long-term results from the
STAMPEDE randomised controlled trial
2, Noel W. Clarke3,4,
2, Silke GillessenID
1, Christopher D. BrawleyID
9,10, Alex Hoyle3,4, Rob J. JonesID
7, David P. Dearnaley1, Hassan Douis8, Duncan C. GilbertID
Chris C. Parker1*, Nicholas D. JamesID
Adnan Ali3, Claire L. Amos2, Gerhardt Attard5, Simon Chowdhury6, Adrian CookID
William CrossID
Clare GilsonID
Zafar I. Malik12, Malcolm D. Mason13, David MathesonID
Mary RauchenbergerID
Amit Bahl15, Alison BirtleID
Joanna GaleID
Anna LydonID
Delia PudneyID
Jacob TanguayID
Trial Collaborative Group¶
2,6, J Martin RussellID
16,17, Lisa Capaldi18, Omar Din19, Daniel Ford8,
23,
3,22, Mohammed KagziID
26, Omi ParikhID
12, Narayanan Nair SrihariID
20, Ann HenryID
24, Joe M. O’Sullivan25, Sangeeta A. PaiseyID
28, Vijay RamaniID
31, Mahesh K. B. ParmarID
2☯, Matthew R. SydesID
3,29, Peter RobsonID
21, Peter HoskinID
14, Robin Millman2,
2, Hannah RushID
27,
2,
11, Hannah Sweeney2,
30,
2,
11, Ruth E. LangleyID
2,
2☯*, for the STAMPEDE
1 The Institute of Cancer Research and Royal Marsden NHS Foundation Trust, London, United Kingdom,
2 MRC Clinical Trials Unit at UCL, UCL, London, United Kingdom, 3 The Christie Hospital, Manchester,
United Kingdom, 4 Salford Royal Hospitals, Manchester, United Kingdom, 5 UCL Cancer Institute, UCL,
London, United Kingdom, 6 Guys and St Thomas’s NHS Foundation Trust, London, United Kingdom, 7 St
James’s University Hospital, Leeds, United Kingdom, 8 University Hospitals Birmingham NHS Foundation
Trust, Birmingham, United Kingdom, 9 Istituto Oncologico della Svizzera Italiana, EOC, Bellinzona,
Switzerland, 10 Università della Svizzera Italiana, Lugano, Switzerland, 11 Institute of Cancer Sciences,
University of Glasgow, Glasgow, United Kingdom, 12 Clatterbridge Cancer Centre, Liverpool, United
Kingdom, 13 Cardiff University, Cardiff, United Kingdom, 14 University of Wolverhampton, Wolverhampton,
United Kingdom, 15 University Hospitals Bristol NHS Trust, Bristol, United Kingdom, 16 Rosemere Cancer
Centre, Lancs Teaching Hospitals, University of Manchester, Manchester, United Kingdom, 17 UCLan,
Lanchashire, United Kingdom, 18 Worcestershire Acute Hospitals NHS Trust, Worcester, United Kingdom,
19 Weston Park Cancer Centre, Sheffield, United Kingdom, 20 Queen Alexandra Hospital, Portsmouth,
United Kingdom, 21 University of Leeds, Leeds, United Kingdom, 22 Mount Vernon Cancer Centre,
Northwood, United Kingdom, 23 The James Cook University Hospital, Middlesbrough, United Kingdom,
24 Torbay and South Devon NHS Trust, Torbay, United Kingdom, 25 Patrick G Johnston Centre for Cancer
Research, Queen’s University Belfast, United Kingdom, 26 Hampshire Hospitals NHS Foundation Trust,
Hampshire, United Kingdom, 27 Royal Preston Hospital, Preston, United Kingdom, 28 South West Wales
Cancer Centre, Swansea, United Kingdom, 29 Manchester University Hospitals NHS Trust, Manchester,
United Kingdom, 30 Shrewsbury & Telford Hospitals NHS Trust, Shrewsbury, United Kingdom, 31 Velindre
Cancer Centre, Cardiff, United Kingdom
☯ These authors contributed equally to this work.
¶ Membership of the STAMPEDE Trial Collaborative Group is listed in S4 Text.
* [email protected] (CCP); [email protected] (MRS)
Abstract
Background
STAMPEDE has previously reported that radiotherapy (RT) to the prostate improved overall
survival (OS) for patients with newly diagnosed prostate cancer with low metastatic burden,
but not those with high-burden disease. In this final analysis, we report long-term findings on
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OPEN ACCESS
Citation: Parker CC, James ND, Brawley CD, Clarke
NW, Ali A, Amos CL, et al. (2022) Radiotherapy to
the prostate for men with metastatic prostate
cancer in the UK and Switzerland: Long-term
results from the STAMPEDE randomised controlled
trial. PLoS Med 19(6): e1003998. https://doi.org/
10.1371/journal.pmed.1003998
Academic Editor: James Derek Brenton, University
of Cambridge, UNITED KINGDOM
Received: January 4, 2022
Accepted: April 22, 2022
Published: June 7, 2022
Peer Review History: PLOS recognizes the
benefits of transparency in the peer review
process; therefore, we enable the publication of
all of the content of peer review and author
responses alongside final, published articles. The
editorial history of this article is available here:
https://doi.org/10.1371/journal.pmed.1003998
Copyright: © 2022 Parker et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: Data will be available
to successful applications for clearly specified
research projects following the MRC CTU at UCL
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
1 / 20
PLOS MEDICINEstandard data sharing processes: https://www.
mrcctu.ucl.ac.uk/our-research/other-research-
policy/data-sharing/ Discussion with the trial team
is encouraged to determine whether the relevant
data to support the application are available. Email
to: [email protected].
Funding: Research support for this comparison
and other comparisons in the STAMPEDE protocol
was awarded by Cancer Research UK
(CRUK_A12459) www.cancerresearchuk.org (for
this comparison, co-authors CCP, DPD, MDM,
MKBP, MR, MRS, NDJ; and additionally for other
comparisons DG, DM, GA, REL, RM, WC); Medical
Research Council (MRC_MC_UU_12023/25,
MC_UU_00004/01 and MC_UU_00004/02) www.
ukri.org/councils/mrc (to authors MKBP, MRS,
REL); and Swiss Group for Clinical Cancer
Research, www.sakk.ch (to co-author SG). Other
research support for the STAMPEDE protocol was
awarded by Astellas www.astellas.com, Clovis
Oncology www.clovisoncology.com, Janssen
www.janssen.com, Novartis www.novartis.com,
Pfizer www.pfizer.com, Sanofi-Aventis www.sanofi.
com. CCP, DPD and NDJ are supported by the
National Institute for Health Research (NIHR)
Biomedical Research Centre at The Royal Marsden
NHS Foundation Trust and the Institute of Cancer
Research, London. The funders had no role in
study design, data collection and analysis, decision
to publish, or preparation of the manuscript.
Competing interests: I have read the journal’s
policy and the authors of this manuscript have the
following competing interests: CCP reports
personal fees from Bayer, personal fees from
Janssen, personal fees from Clarity
Pharmaceuticals, personal fees from Myovant,
personal fees from ITM Oncologics, outside the
submitted work NDJ received research funding to
the institution from Astellas, Astra Zeneca
&Janssen; receipt of honoraria/fees on the
advisory board for Astra Zenenca, Clovis, Janssen,
Merck, Novartis & Sanofi; received fees as a
speaker for Bayer & Novartis NWC received
honoraria from Astellas & Janssen; took a
consulting/advisory role for Astellas, Janssen,
Ferring, Bayer & Sanofi; was paid speakers fees b
Janssen & Astellas; received funding for the
institution from Astra Zeneca; received meeting
and travel expenses from Janssen, Astellas, Sanofi,
Astra Zeneca, Ferring & Ipsen GA reports personal
fees from Sanofi Aventis, during the conduct of the
study; personal fees and non-financial support
from Astellas, personal fees and non-financial
support from Medivation, personal fees from
Novartis, personal fees from Millennium
Pharmaceuticals, personal fees and non-financial
Radiotherapy to the prostate for metastatic disease
the primary outcome measure of OS and on the secondary outcome measures of symptom-
atic local events, RT toxicity events, and quality of life (QoL).
Methods and findings
Patients were randomised at secondary care sites in the United Kingdom and Switzerland
between January 2013 and September 2016, with 1:1 stratified allocation: 1,029 to standard
of care (SOC) and 1,032 to SOC+RT. No masking of the treatment allocation was
employed. A total of 1,939 had metastatic burden classifiable, with 42% low burden and
58% high burden, balanced by treatment allocation. Intention-to-treat (ITT) analyses used
Cox regression and flexible parametric models (FPMs), adjusted for stratification factors
age, nodal involvement, the World Health Organization (WHO) performance status, regular
aspirin or nonsteroidal anti-inflammatory drug (NSAID) use, and planned docetaxel use.
QoL in the first 2 years on trial was assessed using prospectively collected patient
responses to QLQ-30 questionnaire.
Patients were followed for a median of 61.3 months. Prostate RT improved OS in patients
with low, but not high, metastatic burden (respectively: 202 deaths in SOC versus 156 in
SOC+RT, hazard ratio (HR) = 0�64, 95% CI 0.52, 0.79, p < 0.001; 375 SOC versus 386
SOC+RT, HR = 1.11, 95% CI 0.96, 1.28, p = 0�164; interaction p < 0.001). No evidence of
difference in time to symptomatic local events was found. There was no evidence of differ-
ence in Global QoL or QLQ-30 Summary Score. Long-term urinary toxicity of grade 3 or
worse was reported for 10 SOC and 10 SOC+RT; long-term bowel toxicity of grade 3 or
worse was reported for 15 and 11, respectively.
Conclusions
Prostate RT improves OS, without detriment in QoL, in men with low-burden, newly diag-
nosed, metastatic prostate cancer, indicating that it should be recommended as a SOC.
Trial registration
ClinicalTrials.gov NCT00268476, ISRCTN.com ISRCTN78818544.
Author summary
Why was this study done?
• Prostate cancer is the most common cancer in males.
• Radiotherapy (RT) to the prostate is widely used as a radical treatment for nonmeta-
static prostate cancer.
• A comparison was added to the STAMPEDE protocol to assess whether RT to the pros-
tate would also be helpful for males with metastatic prostate cancer. A benefit in survival
was targeted.
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
2 / 20
PLOS MEDICINEsupport from Abbott Laboratories, personal fees
and non-financial support from Essa
Pharmaceuticals, personal fees and non-financial
support from Bayer Healthcare Pharmaceuticals,
personal fees from Takeda, grants from
AstraZeneca, grants from Arno Therapeutics,
grants from Innocrin Pharma, grants, personal fees
and non-financial support from Janssen, personal
fees from Veridex, personal fees and non-financial
support from Roche/Ventana, personal fees and
non-financial support from Pfizer, personal fees
from The Institute of Cancer Research (ICR),
outside the submitted work; and The Institute of
Cancer Research (ICR) receives royalty income
from abiraterone I receive a share of this income
through the ICR’s Rewards to Discoverers Scheme
SC received consulting fees from Telix, remedy &
Huma; received payment for speaker fees and/or
manuscript writing and/or educational events from
Astra Zeneca, Novartis/AAA, Clovis, Janssen,
Bayer, Pfizer, Beigene & Astellas; they were a
member of the data safety monitoring/advisory
board for Astra Zeneca, Novartis/AAA, Clovis,
Janssen, Bayer, Pfizer, Beigene & Astellas DPD
received payment to the institution from C33589/
A19727 Advances in Physics for Precision
Radiotherapy; previous employer, The Institute of
Cancer Research receives loyalty income from
abiraterone, receives personal share of this income
through ICR’s Rewards to Discoverer’s Scheme;
honoraria for consultancy from Janssen;
EP1933709B1 – Location and Stabilisation Device.,
European patent issued, Pending in Canada and
India SG reports personal fees from Orion,
personal fees from Janssen Cilag, personal fees
from ProteoMedix, personal fees from Amgen,
personal fees from MSD, other from Tolero
Pharmaceuticals, other from Astellas Pharma,
other from Janssen, other from MSD Merck
Sharp&Dome, other from Bayer, other from
Roche, other from Pfizer, other from Telixpharma,
other from Amgen, other from Bristol-Myers
Squibb, other from AAA International SA, other
from Orion, other from Silvio Grasso Consulting,
from Tolremo, outside the submitted work; In
addition, Gillessen has a patent WO2009138392
issued and Menarini Silicon Biosystems (Advisory
Board 2019) - not compensated Aranda (Advisory
Board 2019) - not compensated RJJ received
research funding to the institution from Bayer,
Astellas & Pfizer; received honoraria on the
advisory board for Janssen, Astellas, Bayer, Pfizer;
received speaker fees from Janssen, Astellas,
Bayer & Pfizer REL received an institutional grant
from the MRC CG received research funding to the
institution from Janssen, Clovis Oncology, Sanofi,
Astellas, Medical Research Council & Cancer
Radiotherapy to the prostate for metastatic disease
• The trial previously reported a clinically relevant, statistically significant overall survival
(OS) benefit for patients with a low metastatic burden but not for men with a high meta-
static burden.
• This long-term analysis assesses survival with substantially longer follow-up and more
events and looked also at complications of local disease.
What did the researchers do and find?
• A randomised controlled trial of adding RT to the prostate to standard of care (SOC)
was incorporated into the STAMPEDE protocol.
• More than 2,000 patients joined the comparison between 2013 and 2016.
• The data set was frozen in 2021 and analysed using standard methods.
• There was a clear improvement in survival with prostate RT in the low metastatic bur-
den group.
• There was no improvement in survival with prostate RT in the high metastatic burden
group.
• Symptomatic local progression and the need for later local intervention were improved
with RT in the low metastatic burden group.
• In the low metastatic burden group, the improvement with RT was similar whether the
RT was given with a daily schedule (over 4.5 weeks) or a weekly schedule (over 6
weeks).
• The adverse effects of RT were manageable without any impact on long-term quality of
life (QoL).
What do these findings mean?
• Prostate RT is a relatively cheap, widely accessible, and well-tolerated treatment.
• Prostate RT is indicated in patients with newly diagnosed prostate cancer with a low
metastatic burden.
• RT to the prostate is not routinely indicated for patients with a high metastatic burden.
Introduction
Prostate radiotherapy (RT) is recommended for men with newly diagnosed, low-burden, met-
astatic prostate cancer, but not for men with high-burden disease [1]. This recommendation is
based largely on the initial results of the STAMPEDE trial, reported in 2018 [2]. In this rando-
mised controlled trial of 2,061 men with newly diagnosed metastatic prostate cancer, prostate
RT improved overall survival (OS) for men with low metastatic burden (hazard ratio [HR]
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
3 / 20
PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Research UK DF received speaker fees and/or
manuscript writing and/or educational events from
BMS, IPSEN, EUSA, Pfizer, ESAI; they received
travel expenses from Janssen & IPSEN MDM is an
advisory board member for Endocyte & Clovis AB
received payment for lecture/presentation/speaker
bureau/manuscript writing or educational event
from Boston Scientific AJB received speaker fees
and travel support from Janssen DF received
payment for lectures for Janssen, Pfizer & BMS;
support for attending conferences/meetings from
Genisiscare & BMS AMH received research grants
from CRUK and NIHR; support attending meetings
from the European Association of Urologists; is a
member of the European Association of Urologists
& the Prostate Cancer Guidelines Group MK
received travel, accommodation and conference
fees as expenses from Bayer, travel and
accommodation fees for Prostate cancer summits
from Janssen AL received expenses for attending
meetings and/or travel from Astellas, Bayer, BMS
& MSD JMOS received speaker fees from AAA,
Astellas, Bayer, Janssen, Novartis, Sanofi and
participated as an advisory board member and/or
member of the data safety monitoring board for
AAA, Astellas, Bayer, Janssen, Novartis & Sanofi
NNS received travel/meeting payments from
Janssen JT received support for conference
attendance from Janssen, Roche & Bayer;
participated on the advisory board for Astra
Zeneca, Astellas & Bayer MKBP received research
funding to the Unit he directs from Acoria Pvt Ltd,
Akagera, Amgen, Aspirin Foundation, Astellas,
AstraZeneca, Baxter, Bayer, BMS US, Bri-Bio,
Cepheid, Cipla, Clovis Inc, CSL Behring, Eli-Lilly,
Emergent Biosolutions, Gilead Sciences,
GlaxoSmithKline, Grifols, Janssen Products LP,
Janssen-Cilag, Johnson & Johnson, Micronoma,
Modus Theraputics, Mylan, Novartis, Pfizer, Sanofi,
Serum Institute of India, Shionogi, Synteny
Biotechnology, Takeda, Tibotec, Transgene, ViiV
Healthcare, Virco and Xenothera MRS received
research funding to the institution from Astellas,
Clovis, Janssen, Novartis, Pfizer, Sanofi-Aventis;
received speaker fees from Lilly Oncology &
Janssen; independent member of data monitoring
committees. All other authors have nothing to
declare.
Abbreviations: ADT, androgen deprivation therapy;
AE, adverse event; CONSORT, Consolidated
Standards of Reporting Trials; CTCAE, Common
Terminology Criteria for Adverse Events; FPM,
flexible parametric model; GnRH, gonadotrophin-
releasing hormone; HR, hazard ratio; IQR,
interquartile range; ITT, intention-to-treat; LIFS,
local intervention–free survival; NSAID,
nonsteroidal anti-inflammatory drug; OS, overall
0.68, 95% CI 0.52 to 0.90; p = 0.007), with no evidence of a meaningful effect on survival in
men with high metastatic burden (HR 1.07, 95% CI 0.90 to 1.28; p = 0.420). That initial analy-
sis, triggered by a preplanned number of events, was done after a median follow-up of 37
months and was based on 761 events. Here, we report the final analysis of OS, with an addi-
tional 2 years follow-up.
We hypothesised that prostate RT would reduce the complications of local disease progres-
sion, such as urinary or bowel obstruction. If so, this could benefit men with metastatic disease,
regardless of disease burden. Here, we report data on freedom from local interventions (e.g.,
urinary catheter, ureteric stents, nephrostomies, and colostomy).
Any benefits of prostate RT need to be weighed against the risk of treatment-related adverse
events (AEs). We report, for the first time, data from the trial on quality of life (QoL).
The trial was stratified according to the choice of 1 of 2 RT dose-fractionation schedules,
nominated prior to randomisation; 36 Gy in 6 fractions over 6 weeks, or 55 Gy in 20 fractions
over 4 weeks. The 2 schedules were chosen in the expectation that they would be similarly
effective. With the benefit of additional follow-up, and more events in the final analysis, we
have tested for any differential impact on OS by choice of RT schedule.
Methods
Study participants
Eligible patients had prostate cancer that was newly diagnosed, with no previous radical treat-
ment, had metastatic disease confirmed on a bone scintigraphic scan and soft tissue imaging,
and were within 12 weeks after starting androgen deprivation therapy (ADT). Patients were
required to have no contraindications to RT and no clinically significant cardiovascular his-
tory. Participants were recruited at secondary care sites in the UK and Switzerland.
The trial was registered as NCT00268476 (ClinicalTrials.gov) and ISRCTN78818544
(ISRCTN.com). The trial was done in accordance with Good Clinical Practice guidelines and
the Declaration of Helsinki and had relevant ethics (West Midlands–Edgbaston Research Eth-
ics Committee) and regulatory approvals. All patients gave written informed consent. The
rationale and design, including sample size calculations, have been described previously [2,3].
Full details are in the protocol at www.stampedetrial.org.
Procedures
All patients received lifelong hormone therapy as gonadotrophin-releasing hormones
(GnRHs) agonists or antagonists or orchidectomy. In addition, docetaxel was permitted after
it became available for this setting in the UK. Docetaxel, when used, was given as six 3 weekly
cycles of 75mg/m2 with or without prednisolone 10 mg daily.
External beam RT to the prostate was given as 1 of 2 schedules nominated prior to rando-
misation: 36 Gy in 6 consecutive weekly fractions of 6 Gy or 55 Gy in 20 daily fractions of
2.75 Gy over 4 weeks. Treatment was given with the patient supine, with a full bladder and an
empty rectum. The planning target volume consisted of the prostate only with an 8-mm mar-
gin posteriorly and a 10-mm margin elsewhere. RT was to commence as soon as practicable
after randomisation, and, if the patient was having docetaxel as part of standard of care (SOC),
within 3 to 4 weeks after the last docetaxel dose.
Patients were followed up 6 weekly until 6 months after randomisation, 12 weekly to 2
years, 6 monthly to 5 years, and then annually. Toxicities and symptoms were reported at regu-
lar follow-up visits or when an AE was categorised as “serious.” These were graded with Com-
mon Terminology Criteria for Adverse Events (CTCAE) v4�0. Separately, bowel and bladder
adverse effects during RT and long-term possible RT effects were recorded using the RTOG
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
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PLOS MEDICINEsurvival; PH, proportional hazard; QoL, quality of
life; RMST, restricted mean event-free (“survival”)
time; RT, radiotherapy; SLEFS, symptomatic local
event-free survival; SOC, standard of care; WHO,
World Health Organization.
Radiotherapy to the prostate for metastatic disease
scale [4]. Participants were asked to complete the EORTC QLQ-C30 at each scheduled follow-
up appointment.
Metastatic burden at randomisation was evaluated retrospectively through central imaging
review of whole body scintigraphy and computerized tomography (CT) or MRI staging scans.
Metastatic burden was classified according to the definition used in the CHAARTED trial [5]
as either high (polymetastatic; �4 bone metastases with �1 outside the vertebral bodies or pel-
vis and/or visceral metastases) or low (oligometastatic). Patients with only lymph node metas-
tases, in the absence of bone or visceral disease, were therefore classified as low metastatic
burden regardless of the number of nodal metastases.
Randomisation and masking
Patients were randomised centrally using a computerised algorithm, developed and main-
tained by the trials unit. Minimisation with a random element of 20% was used (80% probably
of allocation to a minimising treatment), stratifying for hospital, age at randomisation (<70
versus �70 years), nodal involvement (negative versus positive versus indeterminate), the
World Health Organization (WHO) performance status (0 versus 1 or 2), planned form of
ADT (orchidectomy versus LHRH (leuteinising hormone-releasing hormone) agonist versus
LHRH antagonist versus dual androgen blockade), and regular aspirin or nonsteroidal anti-
inflammatory drug (NSAID) use (yes or no). Planned docetaxel use was added as a stratifica-
tion factor after use was permitted as part of SOC. Allocation was 1:1 to SOC only or SOC+RT.
There was no blinding to treatment allocation.
Primary and secondary outcomes
The primary efficacy outcome measure was OS, defined as time from randomisation to death
from any cause. Secondary outcomes for this long-term efficacy analysis included local inter-
vention–free survival (LIFS)—consisting of time from randomisation to the first report on
case report forms of TURP, ureteric stent, surgery for bowel obstruction, urinary catheter,
nephrostomy, colostomy, death from prostate cancer—and symptomatic local event-free sur-
vival (SLEFS), comprising any of these LIFS events or acute kidney injury, urinary tract infec-
tion, or urinary tract obstruction. Cause of death was determined by the site investigator, with
some cases reclassified as prostate cancer death according to predefined criteria which sug-
gested this to be the likely cause. Patients without the event of interest were censored at the
time last known to be event free. QoL analyses focused on Global QoL % and QLQ-30 Sum-
mary Score %, as derived from patient reports at scheduled assessment time points in the first
2 years after randomisation (see S2 Text).
Statistical analysis
The primary outcome measure, OS, was assessed across all patients and separately within
patient subgroups characterised by baseline metastatic burden (low versus high) and nomi-
nated RT schedule (daily versus weekly).
Standard survival analysis methods were used to analyse time-to-event data in Stata v16.1
(College Station, Texas, United States of America). A nonparametric stratified log-rank test
was used to assess any difference in survival between treatment groups; this was stratified
across the minimisation factors used at randomisation (except hospital and planned form of
hormone therapy) plus protocol-specific time periods defined by other arms recruiting to
STAMPEDE or changes to SOC which could affect the population being randomised. Cox
proportional hazards (PHs) regression models adjusting for the same stratification factors and
stratified by time period were used to estimate relative treatment effect; a HR less than 1�00
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
favoured the research arm. Unadjusted estimates of treatment effect are also presented. Flexi-
ble parametric models (FPMs) were fitted with degrees of freedom (5.5) and adjusted for strati-
fication factors and time periods [6]. Medians and 5-year survival estimates are presented
from the FPM fitted to the data. Kaplan–Meier curves, using the KMunicate format [7], show
estimated survival over time. Following the fitting of Cox models, the PHs assumption was
tested using a global Grambsch–Therneau test with log-transformed time; restricted mean
event-free (“survival”) time (RMST) was emphasised in the presence of nonproportionality,
using a t-star of 91 months as determined by the Royston and Parmar method [6]. Cox and
Fine and Gray regression models [8] were used for cause-specific and competing risk analyses,
respectively; competing risks were non-prostate cancer–related death for prostate cancer–spe-
cific survival and death from any cause for SLEFS and LIFS. Evidence for different treatment
effect across subgroups was assessed using the likelihood ratio p-value for an interaction term
added to the relevant adjusted Cox/FPM model, or Wald test p-value from Fine and Gray
model. Sensitivity analyses of local event outcomes examined the impact of excluding death
from prostate cancer and a competing risks approach with death from any cause specified as a
competing event. All tests are presented as 2 sided, with 95% CIs and the relevant p-value.
Median follow-up was estimated using the Kaplan–Meier method with reverse censoring
on death. All patients were included in the efficacy and QoL analyses according to allocated
treatment on an intention-to-treat (ITT) basis; sensitivity analyses exclude patients who did
not explicitly fulfill all of the eligibility criteria. AE data are shown for the safety population, in
patients with at least 1 follow-up assessment and analysed according to whether RT was
received within 1 year of randomisation (SOC+RT) or not (SOC).
Analyses of the QoL outcomes included partly conditional and composite approaches, build-
ing on the approaches previously used in the trial [9]. For the former, missing values were mul-
tiply imputed using observed data using chained equations. Imputed values for assessments
dating after a patient had died were restored to missing. Generalised estimating equations with
an independence correlation matrix were used to estimate the expected value of the outcome
for each treatment arm at each assessment time point. For the composite approach, observa-
tions following the death of a patient were set to 0% (corresponding to the lowest possible QoL
state). Mixed linear regression with random intercept and slope (with unstructured correlation
specification) was used to model the outcome. Additional cross-sectional analyses estimated the
difference in average QoL associated with treatment allocation in patients alive and with data
available at a given assessment time point, controlling for baseline state.
This trial is reported per the Consolidated Standards of Reporting Trials (CONSORT; see
S3 Text).
Results
Patients
Between January 22, 2013 and September 2, 2016, 2,061 patients were randomised from 117
hospitals in UK and Switzerland: 1,029 to SOC and 1,032 to SOC+RT. The data set was frozen
on March 17, 2021 and included information up to November 30, 2020. Fig 1 shows the CON-
SORT flow diagram for analyses presented in this paper. Table 1 shows baseline characteristics
balanced across the allocated treatment groups. Table A in S1 Text shows baseline characteris-
tics in 1,939 (94%) patients who were evaluable for disease burden, 819 (40%) with low- and
1,120 (54%) with high-burden disease.
Median duration of follow-up was 61.3 months (interquartile range [IQR] = 53.8 to 73.1)
and was similar in both treatment groups: SOC 61.0 (IQR = 53.8 to 72.6) and SOC+RT 61.6
(IQR = 53.8 to 73.1).
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Fig 1. CONSORT diagram. AE, adverse event; CONSORT, Consolidated Standards of Reporting Trials; RT,
radiotherapy to the prostate, SOC, standard of care. �Alive, no withdrawal of permission for continued data collection.
https://doi.org/10.1371/journal.pmed.1003998.g001
OS by allocated treatment and metastatic burden
A total of 1,183 deaths were reported, 609 in patients allocated to SOC and 574 in those allo-
cated to SOC+RT (Fig 2, Table 2).
In the low metastatic burden group, 358 had died: 202/409 SOC and 156/410 SOC+RT.
Median survival was 63.6 months for SOC and 85.5 months for SOC+RT (5-year survival 53%
versus 65%); adjusted HR = 0.64 (95% CI 0.52 to 0.79; p < 0.001 [p = 0.00004]) (Fig 3,
Table 2). There was no evidence of non-PHs.
In the high-burden disease group, 761 had died: 375/567 SOC and 386/553 SOC+RT.
Median survival was 41.2 months in SOC and 38.8 months in SOC+RT (5-year survival 35%
versus 30%): adjusted HR = 1.11 (95% CI 0.96 to 1.28; p = 0.164) (Fig 4, Table 2). There was
no evidence of non-PHs.
There was clear evidence of differential treatment effect according to metastatic burden:
interaction test p < 0.001 [p = 0.00005].
Similar results were obtained from cause-specific and competing risk analyses (Table 2). A
participant audit found 36 (<2%) patients with baseline data or documented protocol devia-
tion inconsistent with the comparison’s full eligibility criteria. Sensitivity analyses found no
impact from excluding these patients (Tables B and C in S1 Text). Analysis of time from ran-
domisation to reported second-line treatments indicates no confounding of RT treatment
effect on OS by postprogression abiraterone or enzalutamide therapy (S10 and S11 Figs).
Exploration of OS by elected RT schedule
In 980 patients nominated prior to randomisation for weekly RT, 575 had died: 282/482
SOC and 293/498 SOC+RT. Median survival was 52.2 months for SOC and 49.9 months for
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PLOS MEDICINETable 1. Baseline characteristics of all patients in the comparison.
Characteristic
Age at randomisation (years)
Median (IQR)
SOC (n = 1,029)
68 (63 to 73)
SOC+RT (n = 1,032)
68 (63 to 73)
Radiotherapy to the prostate for metastatic disease
WHO performance status
Pain from prostate cancer
Previous notable health issues
T-category at randomisation
N-category at randomisation
Metastatic burden
Sites of metastases
Gleason sum score
PSA pre-ADT (ng/ml)
Time from diagnosis (days)
Days from starting hormones
Planned for SOC docetaxel
Nominated RT schedule
Range
0
1 to 2
Absent
Present
Missing
Myocardial infarction
Cerebrovascular disease
Congestive heart failure
Angina
Hypertension
T0
T1
T2
T3
T4
TX
N0
N+
NX
Low metastatic burden�
High metastatic burden
Not classified
Bone
Liver
Lung
Distant lymph nodes
Other
< = 7
8 to 10
Unknown
Median (IQR)
Range
Median (IQR)
Missing
Median (IQR)
Range
Missing
No
Yes
36 Gy/6 f over 6 weeks
55 Gy/20 f over 4 weeks
37 to 86
732 (71%)
297 (29%)
826 (81%)
198 (19%)
5
67 (7%)
29 (3%)
5 (<1%)
46 (4%)
408 (40%)
0 (0%)
12 (1%)
84 (9%)
585 (62%)
260 (28%)
88
345 (36%)
620 (64%)
64
409 (42%)
567 (58%)
53
919 (89%)
23 (2%)
42 (4%)
295 (29%)
35 (3%)
173 (17%)
826 (83%)
30
98 (30 to 316)
1 to 20,590
73 (55 to 94)
1
53 (35 to 70)
-3 to 84
17
845 (82%)
184 (18%)
482 (47%)
547 (53%)
45 to 87
734 (71%)
298 (29%)
855 (83%)
172 (17%)
5
58 (6%)
32 (3%)
8 (1%)
52 (5%)
444 (43%)
1 (<1%)
12 (1%)
89 (9%)
603 (63%)
247 (26%)
80
344 (36%)
620 (64%)
68
410 (43%)
553 (57%)
69
917 (89%)
19 (2%)
48 (5%)
304 (29%)
32 (3%)
175 (18%)
820 (82%)
37
97 (33 to 313)
1 to 11,156
73 (55 to 93)
2
55 (34 to 70)
0 to 86
13
849 (82%)
183 (18%)
498 (48%)
534 (52%)
�Note: One patient classified with low-burden disease was subsequently restaged as nonmetastatic by the randomising site. They remain in the low metastatic burden
subgroup for this analysis.
ADT, androgen deprivation therapy; IQR, interquartile range; PSA, prostate specific antigen; RT, radiotherapy to the prostate; SOC, standard of care; WHO, World
Health Organization.
https://doi.org/10.1371/journal.pmed.1003998.t001
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Fig 2. OS in all patients. Adjusted HR = 0.90 (95% CI 0.81 to 1.01; p = 0.081). HR, hazard ratio; OS, overall survival;
RT, radiotherapy to the prostate; SOC, standard of care.
https://doi.org/10.1371/journal.pmed.1003998.g002
SOC+RT (5-year survival: 44% versus 42%); adjusted HR = 1.00 (95% CI 0.85 to 1.18);
p = 0.974 (Fig 5, Table 2). In 1,081 patients nominated prior to randomisation for daily RT,
608 died: 327/547 SOC and 281/534 SOC+RT. Median survival was 47.8 months in SOC and
55.5 months in SOC+RT (5-year survival 41% versus 47%); adjusted HR = 0.83 (95% CI 0.71
to 0.97; p = 0.022) (Fig 6, Table 2). There was no good evidence of interaction in the treatment
effect by RT schedule: interaction p = 0.088.
Given that RT improved OS in the low metastatic burden patients, RT schedule was further
explored in this subgroup. In 360 patients nominated for weekly RT, 162 had died: 94/190
SOC and 68/170 SOC+RT; adjusted HR = 0.67 (95% CI 0.49 to 0.93; p = 0.015 [p = 0.0155]). In
459 patients nominated for daily RT, 196 had died: 108/219 SOC and 88/240 SOC+RT;
adjusted HR = 0.62 (95% CI 0.47–0.83; p = 0.001 [p = 0.00112]). There was no good evidence
of interaction in the treatment effect by RT schedule: interaction p = 0.732.
SLEFS by allocated treatment
A total of 1,209 (59%) patients were reported as experiencing at least 1 symptomatic local
event: 608 SOC and 601 SOC+RT. In 789 cases (400 SOC and 389 SOC+RT), death from pros-
tate cancer was the only event recorded. Table 3 summarises the reported incidence of each
type of event. There was no evidence of a difference in time to first reported event by treatment
arm: adjusted HR = 1.00 (95% CI 0.90 to 1.13; p = 0.931); median symptomatic local event–
free survival 43.8 months SOC, 43.3 months SOC+RT (5-year SLEFS survival 39% versus 40%)
(S1 Fig, Table 2).
A total of 1,086 (53%) patients had 1 or more local intervention events reported, 556 SOC
and 530 SOC+RT, of which death from prostate cancer was the only event in 78% and 81% of
cases. Median local intervention event–free survival was 51.1 months in SOC and 53.6 months
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Table 2. Summary of estimated treatment effect for main outcome measures: all patients and metastatic burden subgroups.
Outcome measure
Patient group
Adjusted HR~
Unadjusted HR^
OS
All patients
0.90 (0.81 to 1.01)
0.90 (0.81 to 1.01)
Low metastatic burden
0.64 (0.52 to 0.79)
0.66 (0.54 to 0.82)
High metastatic burden
1.11 (0.96 to 1.28)
1.08 (0.94 to 1.25)
Weekly RT (36 Gy/6 f)
1.00 (0.85 to 1.18)
1.01 (0.86 to 1.19)
(Low metastatic burden)
0.67 (0.49 to 0.93)
0.71 (0.52 to 0.97)
(High metastatic burden)
1.22 (0.99 to 1.50)
1.19 (0.97 to 1.46)
Daily RT (55 Gy/20 f)
0.83 (0.71 to 0.97)
0.81 (0.69 to 0.95)
(Low metastatic burden)
0.62 (0.47 to 0.83)
0.63 (0.48 to 0.84)
(High metastatic burden)
1.02 (0.83 to 1.25)
0.99 (0.81 to 1.21)
Prostate cancer–specific survival
�
All patients
0.92 (0.81 to 1.04)
0.92 (0.81 to 1.04)
SLEFS#
LIFS#
Low metastatic burden
0.62 (0.49 to 0.79)
0.64 (0.50 to 0.81)
High metastatic burden
1.12 (0.96 to 1.31)
1.10 (0.94 to 1.28)
All patients
1.00 (0.90 to 1.13)
1.00 (0.90 to 1.12)
Low metastatic burden
0.72 (0.59 to 0.88)
0.73 (0.60 to 0.90)
High metastatic burden
1.23 (1.06 to 1.42)
1.21 (1.05 to 1.40)
All patients
0.94 (0.83 to 1.06)
0.93 (0.83 to 1.05)
Low metastatic burden
0.62 (0.49 to 0.77)
0.63 (0.50 to 0.78)
High metastatic burden
1.18 (1.01 to 1.37)
1.16 (1.00 to 1.34)
Event free at 5
years+
SOC
SOC
+RT
RMST+
SOC
SOC+RT
Difference
42%
53%
35%
44%
54%
37%
41%
52%
33%
49%
62%
41%
39%
46%
33%
44%
54%
38%
45%
65%
30%
42%
64%
29%
47%
66%
32%
51%
72%
35%
40%
58%
26%
47%
67%
32%
52.9
60.6
47.7
53.9
61.3
48.9
52.2
59.9
46.8
57.6
65.7
51.8
49.2
54.5
45.1
53.5
59.7
49.0
55.5
69.0
45.5
53.6
68.2
44.5
57.2
69.5
46.6
59.5
73.7
49.0
48.9
61.8
39.4
55.1
69.1
44.7
2.5 (−0.2 to 5.2)
8.4 (4.5 to 12.2)
−2.2 (−5.7 to 1.2)
−0.3 (−3.4 to 2.8)
6.9 (0.6 to 13.2)
−4.3 (−9.6 to 0.9)
5.0 (1.1 to 8.9)
9.6 (4.0 to 15.2)
−0.2 (−4.5 to 4.0)
1.9 (−1.1 to 5.0)
8.0 (4.0 to 12.0)
−2.8 (−6.6 to 1.0)
−0.3 (−3.5 to 2.8)
7.2 (2.5 to 11.9)
−5.8 (−9.7 to −1.9)
1.6 (−1.5 to 4.7)
9.5 (5.2 to 13.8)
−4.4 (−8.4 to −0.4)
Note: HR and RMST difference are for SOC+RT relative to SOC.
�Cause-specific treatment × metastatic burden interaction test p < 0.001 [p = 0.0000977]. Competing risks analysis: overall adjusted sub-HR = 0.93 (95% CI 0.82 to 1.05;
p = 0.260); low-burden adjusted sub-HR = 0.66 (95% CI 0.52 to 0.83; p = 0.001); high-burden adjusted sub-HR = 1.11 (95% CI 0.95 to 1.29; p = 0.189);
treatment × metastatic burden interaction test p < 0.001 [p = 0.000350].
#SLEFS: treatment × metastatic burden interaction test p < 0.001 [p = 0.0000314]. LIFS interaction p < 0.001 [p = 2.53 × 10−6].
~Estimates from Cox models adjusting for age, nodal involvement, WHO performance status, regular aspirin or NSAID use, and planned SOC docetaxel at
randomisation, stratified by randomisation time period.
^Estimates from unadjusted, unstratified Cox models.
+Survival probabilities and RMST estimates are taken from FPMs with t-star = 91 months.
HR, hazard ratio; LIFS, local intervention–free survival; NSAID, nonsteroidal anti-inflammatory drug; RMST, restricted mean event-free (“survival”) time; RT,
radiotherapy to the prostate; SLEFS, symptomatic local event–free survival; SOC, standard of care; WHO, World Health Organization.
https://doi.org/10.1371/journal.pmed.1003998.t002
in SOC+RT (5-year survival 44% versus 47%); adjusted HR = 0.94 (95% CI 0.83 to 1.06;
p = 0.286) (S2 Fig, Table 2, Table D in S1 Text). Table E in S1 Text presents the results of sen-
sitivity analyses.
AEs by allocated treatment
Urinary-related late AEs of grade 3 were reported for 20 (2%) patients who received RT within
1 year after randomisation; 10 (2%) were planned for weekly and 10 (2%) for daily treatment;
no grade 4 or 5 urinary-related events were reported. Bowel-related late AEs of grade 3 or 4
were reported for 26 (3%) patients, 15 (3%) planned for weekly and 11 (2%) daily treatment
(Table 4, Table F in S1 Text). For 610 patients with data available at 2 years, grade 3 urinary
AEs were reported for 3 (0.5%) and grade 3 bowel AEs for 6 (1%) (Table G in S1 Text). At 4
years, 2/467 (0.4%) patients had grade 3 or 4 bowel toxicity (Table H in S1 Text).
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Fig 3. OS in patients in the low-burden metastatic disease group. Adjusted HR = 0.64 (95% CI 0.52 to 0.79;
p < 0.001 [p = 0.00004]). HR, hazard ratio; OS, overall survival; RT, radiotherapy to the prostate; SOC, standard of
care.
https://doi.org/10.1371/journal.pmed.1003998.g003
Fig 4. OS in patients in the high-burden metastatic disease group. Adjusted HR = 1.11 (95% CI 0.96 to 1.28;
p = 0.164). HR, hazard ratio; OS, overall survival; RT, radiotherapy to the prostate; SOC, standard of care.
https://doi.org/10.1371/journal.pmed.1003998.g004
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Fig 5. OS in patients nominated for weekly RT (36 Gy/6 f) prior to randomisation. Adjusted HR = 1.00 (95% CI
0.85 to 1.18; p = 0.974). HR, hazard ratio; OS, overall survival; RT, radiotherapy to the prostate; SOC, standard of care.
https://doi.org/10.1371/journal.pmed.1003998.g005
Fig 6. OS in patients nominated for daily RT (55 Gy/20 f) prior to randomisation. Adjusted HR = 0.83 (95% CI
0.71 to 0.97; p = 0.022). HR, hazard ratio; OS, overall survival; RT, radiotherapy to the prostate; SOC, standard of care.
https://doi.org/10.1371/journal.pmed.1003998.g006
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Table 3. First symptomatic local event reported (patients with event reported).
Type of event
Urinary tract infection
Urinary catheter
Acute kidney injury
TURP
Urinary tract obstruction
Ureteric stent
Nephrostomy
Colostomy
Surgery for bowel obstruction
PCa death
SOC (n = 608)
57 (9%)
SOC+RT (n = 601)
80 (13%)
52 (9%)
33 (5%)
24 (4%)
15 (2%)
19 (3%)
5 (1%)
3 (<1%)
0 (0%)
400 (66%)
44 (7%)
34 (6%)
24 (4%)
15 (3%)
8 (1%)
2 (<1%)
3 (1%)
2 (<1%)
389 (65%)
PCa, prostate cancer; RT, radiotherapy to the prostate; SOC, standard of care; TURP, transurethral resection of the
prostate.
https://doi.org/10.1371/journal.pmed.1003998.t003
Over the entire reported follow-up period, at least 1 grade 3 to 5 AE was reported for 458
(44%) of SOC and 451 (45%) SOC+RT patients. Areas of focus for this long-term analysis
were endocrine disorders: 160/1,052 (15%) SOC versus 155/992 (16%) SOC+RT; musculoskel-
etal disorders: 112/1,052 (11%) SOC, 104/992 (10%) SOC+RT; blood and bone marrow disor-
ders: 56/1,052 (5%) SOC, 49/992 (5%) SOC+RT; cardiovascular disorders: 46/1,052 (4%) SOC,
56/992 (6%) SOC+RT; renal disorders: 50/1,052 (5%) SOC, 52/992 (5%) SOC+RT; general dis-
orders: 57/1,052 (5%) SOC, 43/992 (4%) SOC+RT; gastrointestinal disorders: 47/1,052 (4%)
SOC, 52/992 (5%) SOC+RT; lab abnormalities: 49/1,052 (5%) SOC, 48/992 (5%) SOC+RT
(Table I in S1 Text, S7 Fig). At 2 years, of 715 patients with data available, a grade 3 to 5 AE
was reported for 52/320 (16%) SOC and 54/395 (14%) SOC+RT (Table J in S1 Text, S8 Fig).
At 4 years, based on 358 patients, this was 12/133 (9%) SOC versus 29/225 (13%) SOC+RT
(Table K in S1 Text, S9 Fig).
Table 4. Patients with grade 3/4 worst late RT toxicity score reported over entire time on trial.
Toxicity area
SOC+RT
Urinary
Hematuria
Urethral stricture
Cystitis
Bowel
Proctitis
Diarrhea
Rectal–anal stricture
Rectal ulcer
Bowel obstruction
Weekly,
36 Gy/6 f
(n = 473)
10 (2%)
4 (1%)
3 (1%)
3 (1%)
15 (3%)
9 (2%)
6 (1%)
0 (0%)
0 (0%)
1 (<1%)
Daily,
55 Gy/20 f
(n = 517)
10 (2%)
4 (1%)
4 (1%)
4 (1%)
11 (2%)
5 (1%)
6 (1%)
0 (0%)
1 (<1%)
1 (<1%)
Note: SOC+RT in safety population (RTOG scale; patients with RT started within 1 year of randomisation). There
were no reported grade 5 late RT toxicity events.
RT, radiotherapy to the prostate; SOC, standard of care.
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Table 5. Summary of QoL analyses.
Outcome measure
Analysis
Average over first 2 years on trial
Difference (95% CI)
Global QoL (%)
QLQ-30 Summary Score (%)
Partly conditional
Composite outcome
Cross-sectional: 12 weeks
Cross-sectional: 24 weeks
Cross-sectional: 60 weeks
Cross-sectional: 104 weeks
Partly conditional
Composite outcome
Cross-sectional: 12 weeks
Cross-sectional: 24 weeks
Cross-sectional: 60 weeks
Cross-sectional: 104 weeks
SOC
73.2%
60.3%
n/a
n/a
n/a
n/a
85.4%
70.6%
n/a
n/a
n/a
n/a
SOC+RT
72.4%
61.6%
n/a
n/a
n/a
n/a
84.2%
71.7%
n/a
n/a
n/a
n/a
−0.8% (−2.5% to 0.9%)
1.3% (−1.1% to 3.8%)
−2.9% (−4.8% to −1.0%)
−0.9% (−3.1% to 1.3%)
−1.4% (−4.1% to 1.3%)
1.8% (−2.4% to 6.0%)
−1.2% (−2.4% to 0.0%)
1.2% (−1.3% to 3.6%)
−2.0% (−3.2% to −0.8%)
−1.0% (−2.3% to 0.4%)
−1.0% (−2.8% to 0.7%)
0.9% (−1.8% to 3.6%)
Note: Partly conditional estimates are based on observed and multiply imputed data from patients alive at scheduled assessments within the first 2 years since
randomisation. Composite outcome estimates are based on observed data and implied imputation of missing data from scheduled assessments when a patient was alive,
and the assumption of a patient’s Global QoL/QLQ-30 Summary Score being 0% at all scheduled assessments after they have died. Cross-sectional analyses estimate the
difference in average Global Qol/QLQ-30 Summary Score between SOC+RT and SOC treatment groups at the specified scheduled assessment, controlling for response
at baseline, in complete cases only (i.e., in patients with outcome data provided at baseline and who have survived and for who outcome data is available at the specified
scheduled assessment).
QoL, quality of life; RT, radiotherapy to the prostate; SOC, standard of care.
https://doi.org/10.1371/journal.pmed.1003998.t005
QoL
There was no evidence of a difference in QoL scores over time between the allocated treatment
groups. Average Global QoL in the first 2 years after randomisation across all patients was
73.2% SOC and 72.4% SOC+RT; absolute difference −0.8% (95% CI −2.5% to 0.9%), p = 0.349
(partly conditional analysis) (Table 5, S3 Fig). When including patients who had died prior to
an assessment as having a Global QoL score of 0% at that assessment, average Global QoL was
60.3% SOC versus 61.6% SOC+RT; absolute difference 1.3% (95% CI -1.1% to 3.8%), p = 0.287
(composite outcome analysis) (Table 5, S4 Fig).
Average QLQ-30 Summary Score in the first 2 years across all patients was 85.4% SOC and
84.2% SOC+RT; absolute difference −1.2% (95% CI −2.4% to 0.0%), p = 0.050 (partly condi-
tional analysis) (Table 5, S5 Fig). When assuming a value of 0% for assessments after a patient
had died, average Summary Score was 70.6% SOC and 71.7% SOC+RT; absolute difference
1.2% (95% CI −1.3% to 3.6%), p = 0.365 (composite outcome analysis) (Table 5, S6 Fig).
Cross-sectional analyses of both Global QoL and QLQ-30 Summary Score indicated evi-
dence of poorer QoL at week 12 after randomisation for patients allocated to SOC+RT—
Global QoL absolute difference −2.9% (95% CI −4.8% to −1.0%, p = 0.003); Summary Score
absolute difference −2.0% (95% CI −3.2% to −0.8%, p = 0.001)—but not at other assessments
(Table 5).
Discussion
This final analysis has confirmed that prostate RT improves OS in men with newly diagnosed,
low-burden metastatic prostate cancer, but not in men with high-burden disease. The magni-
tude of the survival benefit is substantial and clinically relevant, particularly given that prostate
RT is a relatively cheap, widely accessible, and well-tolerated treatment.
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
These results of the final analysis confirm the findings from the initial analysis. The addi-
tional 2 years of follow-up, and the subsequent increase in the number of events for analysis,
has reduced the CIs around the point estimate of the HR of the OS benefit for prostate RT.
However, the point estimate itself has changed very little, improving from 0.68 to 0.64 for men
in the low metastatic disease risk group. This result is consistent with that from the smaller
HORRAD trial [10]. Our new data strongly support those guidelines already recommending
the use of prostate RT in men with low-burden metastatic disease. We have not found any ben-
efit for prostate RT in men with high-burden disease, either in OS or in preventing interven-
tions for local disease progression.
We found no compelling evidence of a difference in efficacy or toxicity between the 2 RT
dose-schedules tested. The weekly schedule of 36 Gy in 6 fractions over 6 weeks has an obvious
practical advantage in terms of convenience and may be preferred for that reason. A daily
schedule might be preferred if pelvic nodal RT were to be used in addition or if RT dose escala-
tion was thought to be appropriate. Prostate RT did not have any long-term impact on QoL
either in this trial, or in the HORRAD trial [11]. The risk of toxicity from prostate RT,
although low, could be further reduced by the use of more contemporary intensity modulated
techniques [12].
The criteria used in the trial to classify cases as low or high burden were taken from those
used in the CHAARTED trial [5]. These criteria are based on the presence or absence of vis-
ceral disease on CT scan, together with the number and the location of bone metastases on
bone scan. Patients with only lymph node metastases have low-burden disease, regardless of
the extent of nodal disease. There is no good reason to think that these criteria are optimal for
identifying those patients with metastatic disease who stand to benefit from prostate RT. The
initial analysis of STAMPEDE suggested that the survival benefit from prostate RT gradually
decreased in magnitude as the number of bone metastases visible on a baseline bone scan
increased [13]. One could decide to identify patients suitable for prostate RT based solely on
the number of bone metastases visible on baseline bone scan, regardless of location. A count-
of-metastases approach would be simpler to use in the clinic than the CHAARTED definition
and would likely increase the number of men considered suitable for prostate RT.
The trial has several strengths, including the randomised design, the large number of events
for analysis, and recruitment from over 100 centres, which adds to the generalisability of the
results. The main limitations of the study are the changes in clinical practice since the trial
started, particularly with regard to imaging techniques and systemic treatment. The trial
recruited between 2013 and 2016 and, while this has the benefit of long follow-up, it also
means that newer imaging techniques, such as PSMA (Prostate-specific membrane antigen)
PET and whole body MRI, were unavailable. It is important to note that low-burden disease in
the trial was defined according to bone scan and CT scan. There is no agreed definition of met-
astatic disease burden based solely on PSMA PET or on whole body MRI. In patients without
visceral disease but who have more than 4 bone metastases on PET or MRI, a bone scan may
be required in addition, in order to determine suitability for prostate RT. If this is not practica-
ble, and there remains uncertainty as to whether a patient has high- or low-burden disease,
there is a strong argument for using prostate RT.
The systemic treatment of metastatic prostate cancer has changed since the trial recruited.
Standard treatment for men with low-burden metastatic disease now includes one of the
newer hormone agents (abiraterone or apalutamide or enzalutamide) in addition to ADT. The
effect of these agents on the survival benefit of prostate RT is unknown. Similarly, the effect of
prostate RT on the survival benefit of the newer hormonal agents is also unknown. Based on
current evidence, it is reasonable to assume that both prostate RT and one of the newer hor-
monal agents should be considered SOC for low-burden metastatic disease, in addition to
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
ADT. The PEACE-1 Trial is testing the use of prostate RT in men receiving ADT
+ abiraterone.
In summary, this final analysis confirms that prostate RT improves OS in men with low-
burden, newly diagnosed, metastatic prostate cancer, indicating that it should be recom-
mended as a SOC.
Supporting information
S1 Fig. SLEFS in all patients. Adjusted HR = 1.00 (95% CI 0.90 to 1.13; p = 0.931). HR, hazard
ratio; RT, radiotherapy to the prostate; SLE, symptomatic local event; SOC, standard of care.
(TIF)
S2 Fig. LIFS in all patients. Adjusted HR = 0.94 (95% CI 0.83 to 1.06; p = 0.286). HR, hazard
ratio; LI, local intervention; RT, radiotherapy to the prostate; SOC, standard of care.
(TIF)
S3 Fig. Model-estimated Global QoL (partly conditional analysis in all patients). Difference
in weighted average: −0.8% (95% CI −2.5% to 0.9%; p = 0.349). QoL, quality of life; RT, radio-
therapy to the prostate; SOC, standard of care.
(TIF)
S4 Fig. Model-estimated Global QoL (composite outcome analysis in all patients). Differ-
ence in weighted average: 1.3% (95% CI −1.1% to 3.8%; p = 0.287). QoL, quality of life; RT,
radiotherapy to the prostate; SOC, standard of care.
(TIF)
S5 Fig. Model-estimated QLQ-30 Summary Score (partly conditional analysis in all
patients). Difference in weighted average: −1.2% (95% CI −2.4% to 0.0%; p = 0.050). RT,
radiotherapy to the prostate; SOC, standard of care.
(TIF)
S6 Fig. Model-estimated QLQ-30 Summary Score (composite outcome analysis in all
patients). Difference in weighted average: 1.2% (95% CI −1.3% to 3.6%; p = 0.365). RT, radio-
therapy to the prostate; SOC, standard of care.
(TIF)
S7 Fig. Highest grade AE reported over entire time on trial (CTCAE v4.0, all patients). AE,
adverse event; CTCAE, Common Terminology Criteria for Adverse Events; RT, radiotherapy
to the prostate; SOC, standard of care.
(TIF)
S8 Fig. Highest grade AE reported at 2 years in patients prior to disease progression
(CTCAE v4.0). AE, adverse event; CTCAE, Common Terminology Criteria for Adverse
Events; RT, radiotherapy to the prostate; SOC, standard of care.
(TIF)
S9 Fig. Highest Grade AE reported at 4 years in patients prior to disease progression
(CTCAE v4.0). AE, adverse event; CTCAE, Common Terminology Criteria for Adverse
Events; RT, radiotherapy to the prostate; SOC, standard of care.
(TIF)
S10 Fig. Time to reported initiation of abiraterone or enzalutamide from randomisation.
RT, radiotherapy to the prostate; SOC, standard of care.
(TIF)
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
S11 Fig. Time to reported initiation of abiraterone or enzalutamide from FFS event. FFS,
failure-free survival; RT, radiotherapy to the prostate; SOC, standard of care.
(TIF)
S1 Text. Table A in S1 Text. Baseline characteristics for metastatic volume analyses. ADT,
androgen deprivation therapy; IQR, interquartile range; PSA, prostate specific antigen; RT, radio-
therapy to the prostate; SOC, standard of care; WHO, World Health Organization. Table B in S1
Text. Eligibility status following participant audit. RT, radiotherapy to the prostate; SOC, stan-
dard of care. Table C in S1 Text. Sensitivity analyses on OS based on explicit eligibility. ITT,
intention-to-treat; OS, overall survival; RT, radiotherapy to the prostate; SOC, standard of care.
Table D in S1 Text. First local intervention event reported (patients with event reported).
PCa, prostate cancer; RT, radiotherapy to the prostate; SOC, standard of care; TURP, transure-
thral resection of the prostate. Table E in S1 Text. Summary of analyses of time to local event
outcomes. �Subdistribution HR for competing risks models. ^Cox model, adjusting for age, nodal
involvement, WHO performance status, regular aspirin or NSAID use and planned SOC doce-
taxel at randomisation, stratified by randomisation time period. +Fine and Gray model with out-
come excluding PCa death and death from any cause as competing risk. NSAID, nonsteroidal
anti-inflammatory drug; PCa, prostate cancer; SOC, standard of care; WHO, World Health Orga-
nization. Table F in S1 Text. Grade 3 to 5 late RT toxicities reported over entire time on trial
(RTOG). Note: Treatment arms correspond to safety population; patients with �1 Follow-Up
CRF returned. RT, radiotherapy to the prostate; RTOG, Radiation Therapy Oncology Group;
SOC, standard of care. Table G in S1 Text. Grade 3 to 5 late RT toxicities reported at 2 years
(RTOG). Note: Treatment arms correspond to safety population; patients with �1 Follow-Up
CRF returned and no reported progression at 2 years. RT, radiotherapy to the prostate; RTOG,
Radiation Therapy Oncology Group; SOC, standard of care. Table H in S1 Text. Grade 3 to 5
late RT toxicities reported at 4 years (RTOG). Note: Treatment arms correspond to safety popu-
lation; patients with �1 Follow-Up CRF returned and no reported progression at 4 years. RT,
radiotherapy to the prostate; RTOG, Radiation Therapy Oncology Group; SOC, standard of care.
Table I in S1 Text. Grade 3 to 5 AEs reported over entire time on trial, overall and for selected
body systems (CTCAE). Note: Treatment arms correspond to safety population; patients with
�1 Follow-Up/SAE CRF returned. AE, adverse event; RT, radiotherapy to the prostate; RTOG,
Radiation Therapy Oncology Group; SOC, standard of care. Table J in S1 Text. Grade 3 to 5
AEs reported at 2 years, overall and for selected body systems (CTCAE). Note: Treatment
arms correspond to safety population; patients with �1 Follow-Up/SAE CRF returned and no
reported progression at 2 years. AE, adverse event; CTCAE, Common Terminology Criteria for
Adverse Events; RT, radiotherapy to the prostate; SOC, standard of care. Table K in S1 Text.
Grade 3 to 5 AEs reported at 4 years, overall and for selected body systems (CTCAE). Note:
Treatment arms correspond to safety population; patients with �1 Follow-Up/SAE CRF returned
and no reported progression at 4 years. AE, adverse event; CTCAE, Common Terminology Crite-
ria for Adverse Events; RT, radiotherapy to the prostate; SOC, standard of care.
(DOCX)
S2 Text. Statistical analysis plan.
(PDF)
S3 Text. CONSORT checklist. CONSORT, Consolidated Standards of Reporting Trials.
(PDF)
S4 Text. List of investigators, oversight committees, and contributors.
(PDF)
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1003998 June 7, 2022
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Acknowledgments
Large-scale trials do not happen without huge collaborations. Thanks to all central and site
staff who have made the STAMPEDE trial happen. See S4 Text for full list of investigators,
oversight committees, and contributors. In particular, thanks to all the people who have cho-
sen to participate in STAMPEDE and their families and friends who have supported them.
The views expressed are those of the authors and not necessarily those of the NIHR or the
Department of Health and Social Care.
Investigators and collaborators
See Credit List included as S4 Text and on the STAMPEDE trial website: http://www.
stampedetrial.org/media-section/presentation-repository/trial-recognition.
Author Contributions
Conceptualization: Chris C. Parker, Nicholas D. James, Noel W. Clarke, Peter Robson,
Mahesh K. B. Parmar, Matthew R. Sydes.
Data curation: Chris C. Parker, Nicholas D. James, Christopher D. Brawley, Noel W. Clarke,
Adnan Ali, Claire L. Amos, Gerhardt Attard, Simon Chowdhury, Adrian Cook, William
Cross, David P. Dearnaley, Duncan C. Gilbert, Clare Gilson, Silke Gillessen, Alex Hoyle,
Rob J. Jones, Ruth E. Langley, Zafar I. Malik, Malcolm D. Mason, David Matheson, Robin
Millman, Mary Rauchenberger, Hannah Rush, J Martin Russell, Hannah Sweeney, Amit
Bahl, Alison Birtle, Lisa Capaldi, Omar Din, Daniel Ford, Joanna Gale, Ann Henry, Peter
Hoskin, Mohammed Kagzi, Anna Lydon, Joe M. O’Sullivan, Sangeeta A. Paisey, Omi
Parikh, Delia Pudney, Vijay Ramani, Peter Robson, Narayanan Nair Srihari, Jacob
Tanguay, Mahesh K. B. Parmar, Matthew R. Sydes.
Formal analysis: Christopher D. Brawley, Adrian Cook, Matthew R. Sydes.
Funding acquisition: Chris C. Parker, Noel W. Clarke, David P. Dearnaley, Malcolm D.
Mason, Mahesh K. B. Parmar, Matthew R. Sydes.
Investigation: Chris C. Parker, Nicholas D. James, Christopher D. Brawley, Noel W. Clarke,
Adnan Ali, Claire L. Amos, Gerhardt Attard, Adrian Cook, William Cross, David P.
Dearnaley, Hassan Douis, Duncan C. Gilbert, Clare Gilson, Silke Gillessen, Alex Hoyle,
Rob J. Jones, Ruth E. Langley, Zafar I. Malik, Malcolm D. Mason, David Matheson, Robin
Millman, Mary Rauchenberger, Hannah Rush, J Martin Russell, Hannah Sweeney, Amit
Bahl, Alison Birtle, Lisa Capaldi, Omar Din, Daniel Ford, Joanna Gale, Ann Henry, Peter
Hoskin, Mohammed Kagzi, Anna Lydon, Joe M. O’Sullivan, Sangeeta A. Paisey, Omi
Parikh, Delia Pudney, Vijay Ramani, Peter Robson, Narayanan Nair Srihari, Jacob
Tanguay, Mahesh K. B. Parmar, Matthew R. Sydes.
Methodology: Chris C. Parker, Nicholas D. James, Noel W. Clarke, Malcolm D. Mason,
Mahesh K. B. Parmar, Matthew R. Sydes.
Project administration: Chris C. Parker, Nicholas D. James, Christopher D. Brawley, Noel W.
Clarke, Adnan Ali, Claire L. Amos, Clare Gilson, Alex Hoyle, Hannah Rush, Hannah
Sweeney, Mahesh K. B. Parmar, Matthew R. Sydes.
Software: Mary Rauchenberger.
Supervision: Chris C. Parker, Nicholas D. James, Noel W. Clarke, Claire L. Amos, Gerhardt
Attard, Simon Chowdhury, Adrian Cook, William Cross, David P. Dearnaley, Duncan C.
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PLOS MEDICINERadiotherapy to the prostate for metastatic disease
Gilbert, Silke Gillessen, Rob J. Jones, Ruth E. Langley, Zafar I. Malik, David Matheson,
Robin Millman, J Martin Russell, Mahesh K. B. Parmar, Matthew R. Sydes.
Validation: Christopher D. Brawley, Noel W. Clarke, Adnan Ali, Adrian Cook, Alex Hoyle,
Matthew R. Sydes.
Visualization: Chris C. Parker, Christopher D. Brawley, Adrian Cook, Mahesh K. B. Parmar,
Matthew R. Sydes.
Writing – original draft: Chris C. Parker, Nicholas D. James, Christopher D. Brawley, Noel
W. Clarke, Adrian Cook, Matthew R. Sydes.
Writing – review & editing: Chris C. Parker, Nicholas D. James, Christopher D. Brawley,
Noel W. Clarke, Adnan Ali, Claire L. Amos, Gerhardt Attard, Simon Chowdhury, Adrian
Cook, William Cross, David P. Dearnaley, Duncan C. Gilbert, Clare Gilson, Silke Gillessen,
Alex Hoyle, Ruth E. Langley, Zafar I. Malik, Malcolm D. Mason, David Matheson, Robin
Millman, Mary Rauchenberger, Hannah Rush, J Martin Russell, Hannah Sweeney, Amit
Bahl, Alison Birtle, Lisa Capaldi, Omar Din, Daniel Ford, Joanna Gale, Ann Henry, Peter
Hoskin, Mohammed Kagzi, Anna Lydon, Joe M. O’Sullivan, Sangeeta A. Paisey, Omi
Parikh, Delia Pudney, Vijay Ramani, Peter Robson, Narayanan Nair Srihari, Jacob
Tanguay, Mahesh K. B. Parmar, Matthew R. Sydes.
References
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PMID: 26522334; PubMed Central PMCID: PMC4664817.
13. Ali A, Hoyle A, Haran AM, Brawley CD, Cook A, Amos C, et al. Association of Bone Metastatic Burden
With Survival Benefit From Prostate Radiotherapy in Patients With Newly Diagnosed Metastatic Pros-
tate Cancer: A Secondary Analysis of a Randomized Clinical Trial. JAMA Oncol. 2021; 7(4):555–63.
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Could not heal snippet
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10.7554_elife.86784.pdf
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Data availability
Cryo- EM maps and atomic coordinates for the GC- C- Hsp90- Cdc37 complex have been deposited
in the EMDB (EMD- 29523) and PDB (8FX4). Material availability: The plasmids used in this study are
uploaded in (Supplementary file 1).
|
Data availability Cryo-EM maps and atomic coordinates for the GC-C-Hsp90-Cdc37 complex have been deposited in the EMDB (EMD-29523) and PDB (8FX4). Material availability: The plasmids used in this study are uploaded in (Supplementary file 1). The following datasets were generated:
|
RESEARCH ARTICLE
Structural insight into guanylyl cyclase
receptor hijacking of the kinase–Hsp90
regulatory mechanism
Nathanael A Caveney1*, Naotaka Tsutsumi1,2†, K Christopher Garcia1,2*
1Departments of Molecular and Cellular Physiology, and Structural Biology, Stanford
University School of Medicine, Stanford, United States; 2Howard Hughes Medical
Institute, Stanford University School of Medicine, Stanford, United States
Abstract Membrane receptor guanylyl cyclases play a role in many important facets of human
physiology, from regulating blood pressure to intestinal fluid secretion. The structural mechanisms
which influence these important physiological processes have yet to be explored. We present the
3.9 Å resolution cryo- EM structure of the human membrane receptor guanylyl cyclase GC- C in
complex with Hsp90 and its co- chaperone Cdc37, providing insight into the mechanism of Cdc37
mediated binding of GC- C to the Hsp90 regulatory complex. As a membrane protein and non-
kinase client of Hsp90–Cdc37, this work shows the remarkable plasticity of Cdc37 to interact with
a broad array of clients with significant sequence variation. Furthermore, this work shows how
membrane receptor guanylyl cyclases hijack the regulatory mechanisms used for active kinases
to facilitate their regulation. Given the known druggability of Hsp90, these insights can guide the
further development of membrane receptor guanylyl cyclase- targeted therapeutics and lead to new
avenues to treat hypertension, inflammatory bowel disease, and other membrane receptor guanylyl
cyclase- related conditions.
eLife assessment
In this important study, the human membrane receptor guanyl cyclase GC- C was expressed in
hamster cells, co- purified in complex with endogenous HSP90 and CDC37 proteins, and the struc-
ture of the complex was determined by cryo- EM. The study shows that the pseudo- kinase domain of
GC- C associates with CDC37 and HSP90, similarly to how the bona fide protein kinases CDK4, CRAF
and BRAF have been shown to interact. The methodology used is state of the art and the evidence
presented is compelling.
Introduction
Cyclic guanosine monophosphate (cGMP) is an important second messenger for signaling in mamma-
lian physiology, with roles in platelet aggregation, neurotransmission, sexual arousal, gut peristalsis,
bone growth, intestinal fluid secretion, lipolysis, phototransduction, cardiac hypertrophy, oocyte
maturation, and blood pressure regulation (Potter, 2011). Largely, cGMP is produced in response to
the activation of guanylyl cyclases (GC), a class of receptors that contains both heteromeric soluble
receptors (α1, α2, β1, and β2 in humans) and five homomeric membrane receptors (GC- A, GC- B, GC- C,
GC- E, and GC- F in humans). Of note are the membrane receptor guanylyl cyclases (mGC) GC- A
and GC- B, also known as natriuretic peptide receptors A and B (NPR- A and NPR- B), respectively,
and GC- C, all of which have been a focus of therapeutic development. In the case of NPR- A and B,
their role in regulating blood pressure in response to natriuretic peptide hormones (ANP, BNP, and
*For correspondence:
[email protected] (NAC);
[email protected] (KCG)
Present address: †Graduate
School of Medicine, Dentistry
and Pharmaceutical Sciences,
Okayama University, Okayama,
Japan
Competing interest: The authors
declare that no competing
interests exist.
Funding: See page 9
Sent for Review
25 February 2023
Preprint posted
16 March 2023
Reviewed preprint posted
02 May 2023
Reviewed preprint revised
12 July 2023
Version of Record published
03 August 2023
Reviewing Editor: Mohamed
Trebak, University of Pittsburgh,
United States
Copyright Caveney et al. This
article is distributed under the
terms of the Creative Commons
Attribution License, which
permits unrestricted use and
redistribution provided that the
original author and source are
credited.
Caveney et al. eLife 2023;12:RP86784. DOI: https://doi.org/10.7554/eLife.86784
1 of 12
Research article
CNP) has led to the exploration of agonists for use in the treatment of cardiac failure (Kobayashi
et al., 2012). Meanwhile, GC- C is the target of clinically approved laxative agonists, linaclotide, and
plecanatide (Miner, 2020; Yu and Rao, 2014), which increase intestinal fluid secretion.
These membrane receptor GCs consist of an extracellular ligand binding domain (ECD), which
acts as a conformational switch to drive intracellular rearrangements to activate the receptor (He
et al., 2001) a transmembrane region (TM); a kinase homology domain or pseudokinase domain (PK);
a dimerization domain; and a GC domain, which acts to produce cGMP. The PK domain is largely
thought to be involved in scaffolding and physical transduction of the extracellular rearrangements
to the GC domain, in some respects similar to the role of the PK domain in the Janus kinases of the
cytokine signaling system (Glassman et al., 2022). In addition, the PK domains of mGCs are regulated
through phosphorylation (Potter and Garbers, 1992; Potter and Hunter, 1998; Vaandrager et al.,
1993) and via association with heat shock proteins (Hsp) (Kumar et al., 2001).
While the role of the phosphorylation state on mGC activity has been explored in relative detail,
how the heat shock protein 90 (Hsp90) is able to regulate mGC activity is largely unknown. It has
been shown that GC- A activity can be regulated through the association of Hsp90 and the co- chap-
erone Cdc37 (Kumar et al., 2001). The chaperone Cdc37 is known to assist in the Hsp90 regulation
of around 60% of active kinases, both in soluble and membrane receptor form (Taipale et al., 2012).
Given the sequence and structural similarities between the PK domains of mGCs and the active kinase
domains which Hsp90–Cdc37 regulates, it is possible that mGCs have evolved to hijack the regulatory
mechanisms that are more broadly deployed for active kinases.
Here, we report the 3.9 Å resolution structure of the GC- C–Hsp90–Cdc37 regulatory complex. In
this structure, the core dimer of Hsp90 forms its canonical closed conformation, while Cdc37 and the
C- lobe of the GC- C PK domain asymmetrically decorate the complex. The client (GC- C) is unfolded
into the channel formed at the interface between the Hsp90 dimers. To our knowledge, this is the first
structure of a membrane protein client of Hsp90 and the first structure of a non- kinase client of the
Hsp90–Cdc37 regulatory system. This work provides a pivotal understanding of the mechanism and
structural basis of kinase fold recruitment to the Hsp90–Cdc37 regulatory complex. This increased
understanding can guide the further development of mGC- targeted therapeutics and lead to new
avenues to treat hypertension, inflammatory bowel disease (IBD), and other mGC- related conditions.
In addition, the general insights into the recruitment of Hsp90–Cdc37 clients can guide the further
development of Hsp90 targeting therapeutics in cancer treatment.
Results
Structure of the GC-C–Hsp90–Cdc37 regulatory complex
Membrane receptor guanylyl cyclases have been largely recalcitrant to structural analysis by x- ray
crystallography and electron microscopy, apart from various crystal structures of both liganded and
unliganded ECDs (He et al., 2001; He et al., 2006; Ogawa et al., 2004; Ogawa et al., 2010; van
den Akker et al., 2000). Given the relative disparity of our structural understanding, we sought to
develop a stable construct to image and gain a crucial understanding of the regulatory and functional
aspects of mGCs which occur intracellularly. By replacing the ligand- responsive ECD with a homod-
imeric leucine zipper, we mimic the ligand- activated geometry of the ECD (He et al., 2001), while
reducing complexity of the imaged complex and increasing stability (Figure 1A). This complex was
recombinantly expressed in mammalian cells, purified with anti- FLAG affinity chromatography, and
vitrified on grids for cryo- EM analysis.
The purified sample had a substantial portion of imaged particles for which the native regulatory
heat shock protein, Hsp90, and its co- chaperone, Cdc37, are bound. The Cricetulus griseus HSP90β
and Cdc37 show remarkable sequence conservation in comparison to the human equivalents, at 99.7
and 94.2% identity, respectively. This native pulldown strategy contrasts with the structures of Hsp90–
Cdc37 in complex with soluble kinases (García- Alonso et al., 2022; Oberoi et al., 2022; Verba
et al., 2016), for which Hsp90 and Cdc37 had to be overexpressed to obtain complex suitable for
imaging. Three- dimensional reconstruction of our GC- C–Hsp90–Cdc37 particles generated a 3.9 Å
resolution map of the regulatory complex (Figure 1, Figure 1—figure supplements 1 and 2). A
second, unsharpened map from subsequent heterogeneous refinement resolves additional density
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A
ECD
TM
TM
PK
DD
GC
B
GC-C
Gn, Uro
zipper
zipper
Cdc37
Cdc37
TMTM
TM
TM
PK
PK
DD
DD
GC
GC
PK
PK
DD
DD
GC
GC
Hsp90
Hsp90
Hsp90
Hsp90
GTP cGMP
signal
C
GC-C
90Å
D
NTD
NTD
Cdc37
coiled-
coil
MD
Hsp90
Hsp90
Cdc37
coiled-
coiled-
coil
coil
MD
CTD
DDDD
PK
PK
C-lobe
C-lobe
E
NTD
NTD
Cdc37
coiled-
coil
MD
MD
GC-C
PK
C-lobe
CTD
90°
NTD
MD
MD
MD
GC-C
PK
PK
C-lobe
C-lobe
MD
90°
GC-C
PK
C-lobe
CTD
CTD
CTD
MD
CTD
Figure 1. Composition and cryo- EM structure of the GC- C–Hsp90–Cdc37 regulatory complex. (A) Cartoon
representation of the components of guanylyl cyclase C (GC- C) signaling and Hsp90–Cdc37 regulation and the
zippered and activated GC- C. GC- C is colored in red, guanylin/uroguanylin (Gn/Uro) in yellow, Hsp90 in blue and
teal, and Cdc37 in purple. Extracellular domains (ECD), transmembrane domain (TM), pseudokinase domain (PK),
dimerization domain (DD), and guanylyl cyclase domain (GC) are labeled. In the rightmost cartoon, the regions
unobserved in the cryo- EM density are in a lighter shade with a dashed outline. (B) The refined and sharpened
cryo- EM density map of GC- C–Hsp90–Cdc37, colored as in A, with a transparent overlay of an unsharpened map
with additional DD density resolved. Cdc37 coil- coiled and middle domain (MD) are labeled. (C) Reference- free
2D averages for the GC- C–Hsp90–Cdc37 complex. (D) The refined and sharpened cryo- EM density map of GC- C–
Hsp90–Cdc37, colored as in A and B, labeled with all domains as in A and B, with the addition of Hsp90 N- terminal
domain (NTD), middle domain (MD), and C- terminal domain (CTD). (E) Ribbon representation of a model of GC- C–
Hsp90–Cdc37 complex, colored and labeled as in A, B, and C.
The online version of this article includes the following figure supplement(s) for figure 1:
Figure 1 continued on next page
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Figure 1 continued
Figure supplement 1. GC- C–Hsp90–Cdc37 complex cryo- EM data processing.
Figure supplement 2. Representative density of GC- C–Hsp90–Cdc37.
for the dimerization domain, extending outward from the PK domain (Figure 1B, Figure 1—figure
supplement 1).
The resultant GC- C–Hsp90–Cdc37 complex is a hetero- tetramer formed by one resolved monomer
of the GC- C receptor bound to a dimer of Hsp90 and one Cdc37 co- chaperone (Figure 1D). As
observed with most Hsp90–client structures, the bulk of the complex is composed of the C2 pseudo-
symmetric, ATP bound, closed state Hsp90 dimer. Building on this dimeric core, the Cdc37 protrudes
outward from one side with its characteristic long, coiled- coil, α-hairpin. On one face of the Hsp90
dimer core, Cdc37 interacts with the PK domain of GC- C, while an extended β-sheet wraps around
to the other face, lying across and extending a β-sheet in the middle domain (MDHsp90) of one Hsp90
monomer. At the opposite face, the globular and α-helical Cdc37 middle domain (MDCdc37) is formed.
The C- lobe of the GC- C PK domain packs against the N- terminal region of Cdc37 on one face of the
dimeric Hsp90 core, with the N- lobe unfolding through the dimer core to interface with the MDCdc37
on the opposite face. N- terminal to the PK N- lobe is the TM region, the density for which was unob-
served in our reconstructions. C- terminal to the PK C- lobe, we observe some poorly resolved density
for the likely mobile dimerization domain in our unsharpened map. This would precede the GC
domain, which is not observed in the density of our reconstructions (Figure 1B). Together, we can use
our understanding of mGC topology and our reconstruction to orient the complex as it would sit on
a membrane (Figure 1B), providing insight into how Hsp90 is able to access and regulate membrane
protein clients. No density is observed for the second GC- C of the dimer, though it is sterically unlikely
that an additional regulatory complex is forming on the second GC- C in a concurrent fashion, given
the large size of the first Hsp90–Cdc37 and the requisite proximity of the second GC- C. In addi-
tion, this disruption of the native state of GC- C, as observed in our structure, would likely leave GC
domains out of each other’s proximity, precluding their catalytic activity while Hsp90 is bound.
Cdc37 mediated GC-C recruitment and Hsp90 loading
Despite the recognized plasticity of Cdc37 co- chaperone binding to approximately 60% of kinases
(Taipale et al., 2012), the importance of the Hsp90–Cdc37 complex for pseudokinase domain-
containing proteins in the human proteome is not well studied. Thus, the structural basis for how
Cdc37 can recruit GC- C to the Hsp90 regulatory complex is of particular interest. In our structures,
we see that Cdc37 is displacing the N- lobe of the pseudokinase domain of GC- C, binding to the
C- lobe at the N–C interface, and guiding the unfolded N- lobe into the Hsp90 dimer (Figure 2). The
Cdc37–GC- C interface is relatively modest in size, with a calculated mean surface area of 689 Å2 (as
calculated by PISA Krissinel and Henrick, 2007). This interface is partly driven to form via charge
complementarity, with positive contributions from a cluster of arginine residues on Cdc37 (R30, R32,
R39) at the periphery of the interaction interface interacting with D609 and the polar residues Y580
and T586 (Figure 2B). Beyond this, the interface is likely largely driven via shape- complementarity,
due to a minimal contribution from hydrogen bonding, salt- bridge formation, and aromatic packing
contributions – in line with the ability of Cdc37 to chaperone such a diverse array of clients and client
sequences.
As the unfolded PK N- lobe extends away from Cdc37, it enters the channel formed at the interface
between the dimer of Hsp90 (Figure 2C). Here, GC- C residues 528–544 (VKLDTMIFGVIEYCERG) lie
across the upper region of the Hsp90 CTDs, which form the floor of the channel. These CTDs form
the bulk of the interaction interface as the unfolded N- lobe passes through this channel, yet there are
minor contributions from the loop regions of the β-sheet from the MDHsp90 which extend downward
into this channel region. The unfolded region is relatively poorly resolved in the density, with some
reconstructions from earlier refinement having no resolvable density in this channel region – indicative
of the low stability and high mobility of the unfolded N- lobe as it passes through this region.
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A
Hsp90
Hsp90
NTD
Hsp90
NTD
Cdc37
coiled-
coil
B
Cdc37
R39
B
GC-C
PK
C-lobe
MD
C
MD
T586T586
L581
T608
Y580
K585
D609D609
W31W31
R30
R30
R32R32
L28L28
I23I23
E18E18
N22N22
H20H20
K606
V604V604
K576K576
GC-C
E
Y
C
EE
II
R
G544G544
GC-CGC-C
Hsp90
Hsp90
CTD
CTD
C
Hsp90
Hsp90
V528V528
D
TT
KK
LL
I
M
G
V
F
Figure 2. Cdc37 mediated guanylyl cyclase C (GC- C) recruitment and heat shock protein 90 (Hsp90) loading
interfaces. (A) Ribbon representation of a model of GC- C–Hsp90–Cdc37 complex. GC- C is colored in red, Hsp90 in
blue and teal, and Cdc37 in purple. Pseudokinase (PK), coil- coiled, middle (MD), C- terminal (CTD), and N- terminal
(NTD) domains are labeled. (B) The Cdc37–GC- C interface in ribbon representation, with interacting residues
drawn in sticks, colored as in A. (C) The unfolded N- lobe of GC- C PK domain as it passes between the Hsp90
dimer, in ribbon representation, with interacting residues drawn in sticks, colored as in A and B. This region’s
sequence is: VKLDTMIFGVIEYCERG.
The online version of this article includes the following figure supplement(s) for figure 2:
Figure supplement 1. Conservation of Cdc37 mediated heat shock protein 90 (Hsp90) regulation.
Figure supplement 2. Regulatory mechanisms for membrane receptor guanylyl cyclase (mGC) activity.
Conservation of Cdc37 mediated Hsp90 regulation
The core structural principles of Cdc37 mediated client recruitment to Hsp90 appear to remain
constant across its large range of client diversity. Across other clients–Hsp90–Cdc37 complexes with
canonical soluble kinase clients (Cdk4, RAF1, B- raf) (García- Alonso et al., 2022; Oberoi et al., 2022;
Verba et al., 2016), we see a conserved role for Cdc37 in client recruitment by associating with the
C- lobe at the N-, C- lobe interface (Figure 2—figure supplement 1A, B). In these complexes, we see
high levels of structural conservation for the Hsp90–Cdc37 (Cα RMSDs of 1.4–3.3 Å for Hsp90 and
1.5–2.5 Å for Cdc37), while the client is structurally most homogenous at the interface with Cdc37,
though less structurally conserved overall (Cα RMSDs of 3.5–11.6 Å). Perhaps unsurprisingly, GC- C is
one of the most divergent of these clients from a sequence perspective (Figure 2—figure supplement
1C), with sequence homology between the GC- C PK domain and the other client kinase domains
ranging from 19 to 25% identity and 31 to 41% homology. This highlights the plasticity required of
this system which can service such a vast array of clients across a broad range of sequence variations,
yet more restricted fold architecture.
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Discussion
The present cryo- EM structure of GC- C–Hsp90–Cdc37 resolves the loading of GC- C, via its PK domain
and interaction with Cdc37, to the Hsp90 core dimer (Figures 1 and 2). This complex shows signifi-
cant structural similarity to the mechanism that regulates soluble active kinases (García- Alonso et al.,
2022; Oberoi et al., 2022; Verba et al., 2016) and presumably membrane receptor kinases in the
human proteome. This structural and mechanistic conservation is largely driven by the co- chaperone
Cdc37, which serves as the central binding platform for these clients by associating to the fold of the
kinase (or pseudokinase in the case of mGC) domain, relatively independent of sequence identity.
A model whereby recruitment is largely driven by both the fold complementarity and the specific
stability properties of the kinase fold has been proposed previously (Taipale et al., 2012). In this
model, instability of a fully folded kinase domain results in partial unfolding of the C- lobe, leading
Cdc37 to bind the partially unfolded state. Given the lack of functional and sequence conservation for
GC- C as a client of Cdc37, our data largely fits with this model for client recruitment. It is likely that
the pseudokinase domains of mGC have largely evolved to facilitate regulatory mechanisms for these
receptors, both via their phosphorylation and by hijacking the regulatory mechanisms used by active
soluble and membrane receptor kinases.
In the case of GC- A, previous work has shown that it associates with the Hsp90–Cdc37 complex
to regulate GC activity (Kumar et al., 2001). The authors showed that adding geldanamycin, an
Hsp90 inhibitor, reduces the overall cGMP output of cells in response to ANP stimulation while also
reducing the association of the Hsp90 to GC- A. While this initially may seem counterintuitive, this data
fits with a model of ligand- induced activity potentiating the instability of the PK domain, which then
facilitates binding of the regulatory complex to ‘re- fold’ GC- A for further catalysis and cGMP produc-
tion – in a core regulatory complex structurally similar to that which we observe for GC- C in this work
(Figure 2—figure supplement 2). In the case of the Hsp90 inhibitor, this would release the Hsp90 and
only allow full catalytic activity for the receptor until the receptor falls into the partially unfolded state,
as the Hsp90 would no longer be able to re- engage at the C- lobe when inhibited (Figure 2—figure
supplement 2).
Interestingly there may be an additional layer of regulation involved, with crosstalk between
the phosphorylation and Hsp90 regulatory mechanisms of mGC. The phosphatase PP5 is known
to interact with the Hsp90–Cdc37 system and dephosphorylate Hsp90, Cdc37, and the system’s
kinase clients (Oberoi et al., 2022). PP5 has been implicated in this role for mGC (Chinkers,
1994), though this interaction was unable to be detected by a pull- down in a second study (Kumar
et al., 2001). In this way, mGC association with the Hsp90–Cdc37 complex could result in multiple
fates and resultant activity profiles for the receptor. When the PK of an activated mGC falls into
a destabilized state, this would result in the recruitment of the Hsp90–Cdc37. First, the regula-
tory complex could refold the receptor to maintain the activity of the receptor (Figure 2—figure
supplement 2i). In another scenario, the Hsp90–Cdc37 complex could additionally recruit PP5 to
dephosphorylate the mGC (Figure 2—figure supplement 2ii). Particularly in the case of GC- A
and GC- B, and to some extent GC- C (Potter and Garbers, 1992; Potter and Hunter, 1998;
Vaandrager et al., 1993), this would impair the signaling activity of the mGC, though this could
be rescued through the kinase re- association and phosphorylation. In a final scenario, the binding
of the Hsp90–Cdc37 complex could result in the association of ubiquitin E3 ligases (Schopf et al.,
2017; Figure 2—figure supplement 2iii), which would ubiquitinate the mGC client, leading to the
removal of the receptor.
The regulation of mGC is influenced by a network of factors working in harmony to ensure proper
signaling and physiological response for these important receptors. The structure of the core regu-
latory complex shown in this work is key to many facets of mGC regulation. We hope that the struc-
tural basis for the Hsp90 regulatory platform for mGC will drive renewed investigation into these
diverse mechanisms and lead to the therapeutic manipulation of these mechanisms to improve mGC
targeting therapies.
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Key resources table
Reagent type (species) or
resource
Methods
Designation
Source or reference
Identifiers
Additional information
Cell line (Cricetulus griseus)
Chinese hamster ovary kidney
cells
GIBCO
ExpiCHO
Recombinant DNA reagent
pD649- GCN4- TM- GC- C_ICD
(plasmid)
This paper
See: Methods - Cloning and protein
expression
Software, algorithm
Data collection software
SerialEM
SerialEM
Software, algorithm
Data processing software
Software, algorithm
Data sharpening software
Structura Biotechnology
Inc.
cryoSPARC
Sanchez- Garcia et al.,
2021
DeepEMhancer
Software, algorithm
Initial modeling software
Jumper et al., 2021
AlphaFold
Software, algorithm
Graphics software
Pettersen et al., 2021
UCSF ChimeraX
Software, algorithm
Software, algorithm
Modeling and refinement
software
Adams et al., 2010
Phenix
Modeling and refinement
software
Emsley and Cowtan,
2004
Coot
Software, algorithm
Model validation software
Chen et al., 2010
MolProbity
Cloning and protein expression
For cryo- EM studies, a construct containing an HA secretion signal (MKTIIALSYIFCLVFA), a FLAG
peptide (DYKDDDD), linker and 3 C cleavage site (KGSLEVLFQGPG), GCN4 homodimeric zipper
( RMKQ LEDK VEEL LSKN YHLE NEVA RLKK LVGER), human GC- C regions corresponding to the small
extracellular linker region, TM, and intracellular domains (residues 399–1,053), a second linker and
3 C cleavage site (AAALEVLFQGPGAA), a Protein C epitope tag (EDQVDPRLIDGK), and an 8 x His
tag were cloned into a pD649 mammalian expression vector. This construct contains all domains of
the native GC- C, with the exception of the ECD (Supplementary file 1). Protein was expressed using
ExpiCHO Expression System Kit (Thermo Fisher). Briefly, ExpiCHO cells were maintained in ExpiCHO
Expression Media at 37 °C with 5% CO2 and gentle agitation, and transiently transfected by the
expression construct and cultured according to the manufacturer’s protocol. Cells were pelleted and
stored at –80 °C.
Protein purification
Cells were resuspended in 20 mM HEPES- Na pH 8.0, 300 mM NaCl, 1 mM TCEP, protease inhibitor
cocktail (Sigma), and benzonase (Sigma). Cells were lysed by Dounce homogenizer and cellular debris
was pelleted by low- speed centrifugation at 500 × g. Membranes were collected by centrifugation at
46,000 × g and stored at –80 °C until use. Membranes were thawed and solubilized with the addition
of 1% n- dodecyl β-D- maltoside (DDM) and 0.1% cholesteryl hemisuccinate (CHS) (10:1) (Anatrace).
Debris and unsolubilized membranes were pelleted by centrifugation at 46,000 × g. The superna-
tant was subsequently used in FLAG affinity chromatography. The supernatant was applied to M1
anti- FLAG resin. The resin was washed with 20 bed volumes of 20 mM HEPES- Na pH 8.0, 300 mM
NaCl, 1 mM TCEP, 0.005% lauryl maltose neopentyl glycol (LMNG), 0.0005% CHS (10:1) (Anatrace),
and 5 mM ATP. The protein complex was eluted with the addition of 200 μg/mL of FLAG peptide
(DYKDDDD) (GenScript). Protein was subsequently concentrated to >2 mg/mL and used for cryo- EM
imaging.
Cryo-electron microscopy
Aliquots of 3 μL of complex were applied to glow- discharged 300 mesh UltrAuFoil (1.2/1.3) grids. The
grids were blotted for 3 s at 100% humidity with an offset of 3 and plunged frozen into liquid ethane
using a Vitrobot Mark IV (Thermo Fisher). Grid screening and dataset collection occurred at Stanford
cEMc on a 200 kV Glacios microscope (Thermo Fisher) equipped with a K3 camera (Gatan). Movies
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Table 1. Cryo- EM data collection, refinement, and validation statistics.
GC- C–Hsp90–Cdc37 complex
PDB 8FX4
EMD- 29523
GC- C–Hsp90–Cdc37
complex with DD
density
Data collection and processing
Nominal magnification
Acceleration voltage (kV)
Electron exposure (e-/Å2)
Defocus range (µm)
Pixel size (Å)
Symmetry imposed
Final particle images
165,635
Map resolution FSC threshold
Map resolution (Å)
3.9
Refinement
Initial model used (PDB)
5FWK, 7ZR5, AlphaFold
45,000
200
58.8
0.8–2.0
0.9273
C1
0.143
48,283
6.3
Model resolution FSC threshold (Å)
Model resolution (Å)
Model Composition
Non- hydrogen atoms
Protein residues
Ligands
B- factors (Å2)
Protein
Ligand
R.m.s. deviations
Bond lengths (Å)
Bond angles (°)
Validation
MolProbity score
Clashscore
Rotamer outliers (%)
Ramachandran plot
Favored (%)
Allowed (%)
Outliers (%)
0.5
4.2
13,478
1,654
2
119.49
102.85
0.004
0.914
2.14
13.88
0.67
92.0
7.6
0.4
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were collected at a magnification corresponding to a 0.9273 Å per physical pixel. The dose was set
to a total of 58.8 electrons per Å2. Automated data collection was carried out using SerialEM with a
nominal defocus range set from –0.8 to –2.0 μM.
Image processing
All processing was performed in cryoSPARC (Punjani et al., 2017) unless otherwise noted (Figure 1—
figure supplement 1). 8788 movies were motion- corrected using patch motion correction. The
contrast transfer functions (CTFs) of the flattened micrographs were determined using patch CTF and
an initial stack of particles was picked using Topaz picker (Bepler et al., 2019). Successive rounds of
reference- free 2D classification were performed to generate a particle stack of 165,635 particles. These
particles were then used in ab- initio reconstruction, followed by non- uniform refinement (Punjani
et al., 2020) and finally local refinement with a loose mask around the entire complex. This resulted in
a 3.9 Å reconstruction of the GC- C–Hsp90–Cdc37 complex which was sharpened with deepEMhancer
(Sanchez- Garcia et al., 2021). These particles were also used in a 4- class heterogeneous refinement
to pull out a volume containing some resolved density for the dimerization domain of GC- C.
Model building and refinement
The Cdk4–Hsp90β–Cdc37 (PDB 5FWK), PP5–B- Raf–Hsp90β–Cdc37 (PDB 7ZR5), and AlphaFold
models for GC- C (Jumper et al., 2021; Mirdita et al., 2022) were docked into the map using UCSF
Chimera X (Pettersen et al., 2021). A resultant hybrid model was then manually curated to contain
the correct Cricetulus griseus sequences for Hsp90β–Cdc37 and run through Namdinator (Kidmose
et al., 2019). This was followed by automated refinement using Phenix real space refine (Adams
et al., 2010) and manual building in Coot (Emsley and Cowtan, 2004). The final model produced a
favorable MolProbity score of 2.14 (Chen et al., 2010) with 0.4% Ramachandran outliers (Table 1).
Model building and refinement software was installed and configured by SBGrid (Morin et al., 2013).
Acknowledgements
We thank Liz Montabana and Stanford cEMc for microscope access for data collection. We thank Paul
LaPointe and Kevin Jude for their insightful discussion of the Hsp90 structure and regulatory mech-
anisms. NAC is a CIHR postdoctoral fellow. KCG is an investigator with the Howard Hughes Medical
Institute. KCG is supported by National Institutes of Health grant R01- AI51321, the Mathers Founda-
tion, and the Ludwig Foundation.
Additional information
Funding
Funder
Canadian Institutes of
Health Research
National Institutes of
Health
Mathers Foundation
Ludwig Foundation
Grant reference number Author
Postdoctoral Fellowship
Nathanael A Caveney
R01-AI51321
K Christopher Garcia
K Christopher Garcia
K Christopher Garcia
The funders had no role in study design, data collection and interpretation, or the
decision to submit the work for publication.
Author contributions
Nathanael A Caveney, Conceptualization, Formal analysis, Investigation, Methodology, Writing - orig-
inal draft, Writing – review and editing; Naotaka Tsutsumi, Formal analysis, Investigation, Writing
– review and editing; K Christopher Garcia, Supervision, Funding acquisition, Project administration,
Writing – review and editing
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Author ORCIDs
Nathanael A Caveney
Naotaka Tsutsumi
K Christopher Garcia
http://orcid.org/0000-0003-4828-3479
https://orcid.org/0000-0002-3617-7145
https://orcid.org/0000-0001-9273-0278
Peer review material
Reviewer #1 (Public Review): https://doi.org/10.7554/eLife.86784.3.sa1
Reviewer #2 (Public Review): https://doi.org/10.7554/eLife.86784.3.sa2
Reviewer #3 (Public Review): https://doi.org/10.7554/eLife.86784.3.sa3
Author Response https://doi.org/10.7554/eLife.86784.3.sa4
Additional files
Supplementary files
• MDAR checklist
• Supplementary file 1. Plasmids used in this study.
Data availability
Cryo- EM maps and atomic coordinates for the GC- C- Hsp90- Cdc37 complex have been deposited
in the EMDB (EMD- 29523) and PDB (8FX4). Material availability: The plasmids used in this study are
uploaded in (Supplementary file 1).
The following datasets were generated:
Author(s)
Caveney NA, Garcia
CK
Year
2023
Caveney NA, Garcia
KC
2023
Dataset title
Dataset URL
Database and Identifier
Cryo- EM maps and atomic
coordinates for the GC-
C- Hsp90- Cdc37 complex
have been deposited
Cryo- EM maps and atomic
coordinates for the GC-
C- Hsp90- Cdc37 complex
have been deposited
https://www. ebi. ac.
uk/ emdb/ EMD- 29523
EMDataResource, EMD-
29523
https://www. rcsb. org/
structure/ 8FX4
RCSB Protein Data Bank,
8FX4
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10.1038_s41467-022-32646-w.pdf
|
Data availability
The data that support the findings in this study are available from the
corresponding authors upon reasonable request. Source data are
provided with this paper.
Code availability
All code to reproduce the main simulation results can be found on
GitHub (https://github.com/babaf/motor-adaptation-local-vs-input.git).
|
Data availability The data that support the findings in this study are available from the corresponding authors upon reasonable request. Source data are provided with this paper. Code availability All code to reproduce the main simulation results can be found on GitHub ( https://github.com/babaf/motor-adaptation-local-vs-input.git ).
|
nature communications
Article
https://doi.org/10.1038/s41467-022-32646-w
Small, correlated changes in synaptic
connectivity may facilitate rapid
motor learning
Received: 28 October 2021
Accepted: 8 August 2022
Barbara Feulner
Lee E. Miller4,5,6, Juan A. Gallego 1,7 & Claudia Clopath 1,7
1, Matthew G. Perich 2, Raeed H. Chowdhury 3,
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Animals rapidly adapt their movements to external perturbations, a process
paralleled by changes in neural activity in the motor cortex. Experimental
studies suggest that these changes originate from altered inputs (Hinput) rather
than from changes in local connectivity (Hlocal), as neural covariance is largely
preserved during adaptation. Since measuring synaptic changes in vivo
remains very challenging, we used a modular recurrent neural network to
qualitatively test this interpretation. As expected, Hinput resulted in small
activity changes and largely preserved covariance. Surprisingly given the
presumed dependence of stable covariance on preserved circuit connectivity,
Hlocal led to only slightly larger changes in activity and covariance, still within
the range of experimental recordings. This similarity is due to Hlocal only
requiring small, correlated connectivity changes for successful adaptation.
Simulations of tasks that impose increasingly larger behavioural changes
revealed a growing difference between Hinput and Hlocal, which could be
exploited when designing future experiments.
Animals, particularly primates, can perform a great variety of beha-
viours, which they are able to adapt rapidly in the face of changing
conditions. Since behavioural adaptation can happen even after a
single failed attempt1, the neural populations driving this process must
be able to adapt equally fast. How this occurs remains unexplained2.
Rapid motor learning is typically studied using external perturbations
such as a visuomotor rotation (VR), which rotates the coordinates of
the visual feedback with respect to those of the movement. Both
humans and monkeys can learn to compensate for the resulting error
between actual and expected visual feedback in a few tens of trials3,4.
This behavioural adaptation is accompanied by changes in the
activity of neurons in primary motor cortex (M1)5, and the upstream
dorsal premotor cortex (PMd)3. It is unclear whether these neural
activity changes are mediated by synaptic weight changes within the
motor cortices or are driven by altered inputs from even further
upstream areas.
When learning a skill over many days, behavioural improvements
are paralleled by rewiring between M1 neurons6–9. This seems not to be
the case for rapid learning: throughout VR adaptation, the statistical
interactions across neural populations in both M1 and PMd remain
largely preserved10. These preserved interactions rule out any large
synaptic changes within the motor cortices, as they would cause these
models to degrade11,12. Instead, rapid VR adaptation may be driven by
the cerebellum13–16 and/or posterior parietal cortex17,18.
A pioneering Brain Computer Interface (BCI) study cast further
doubt that significant synaptic changes occurring within M1 are
necessary for rapid learning19,20. In that study, monkeys controlled a
computer cursor linked by a “decoder” to the activity of recorded M1
1Department of Bioengineering, Imperial College London, London, UK. 2Département de neurosciences, Université de Montréal, Montréal, QC, Canada.
3Department of Bioengineering, University of Pittsburgh, Pittsburgh, PA, USA. 4Department of Neuroscience, Northwestern University, Evanston, IL, USA.
5Department of Biomedical Engineering, Northwestern University, Evanston, IL, USA. 6Department of Physical Medicine and Rehabilitation, Northwestern
University, and Shirley Ryan Ability Lab, Chicago, IL, USA. 7These authors contributed equally: Juan A. Gallego, Claudia Clopath.
e-mail: [email protected]; [email protected]
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neurons. After learning to use a decoder that used the natural
“intrinsic” mapping of neural activity onto cursor movements, the
monkeys were exposed to one of two types of perturbations. When
faced with a new decoder that preserved the statistical interactions
(i.e., neural covariance) across M1 neurons, the monkeys could master
it within minutes. In stark contrast, if the new decoder required
changes in the neural covariance (an “out of manifold” perturbation),
they could not learn it within one session—in fact, it required a pro-
gressive training procedure spanning just over nine days on average21.
Recording large scale synaptic changes in vivo remains challen-
ging and has not been achieved during rapid motor learning. Alter-
natively, recurrent neural network (RNN) models offer an exciting yet
unexplored opportunity to test the effect of synaptic changes (in the
model) on simulated activity during motor learning. RNNs trained on
motor, cognitive and BCI tasks exhibit many striking similarities with
the activity of neural populations recorded in animal studies22–28,
suggesting a fundamental similarity between the two. Previous work
using RNNs to model the BCI experiment described above19 showed
that network covariance can be highly preserved even when learning is
happening through weight changes within the network29. Thus, con-
trary to intuition, functionally relevant synaptic weight changes may
not necessarily lead to measurable changes in statistical interactions
across neurons30. As a consequence, synaptic changes within PMd and
M1 during VR adaptation may be very hard to identify through the
analysis of neural population recordings.
Here, we used RNN models to test whether VR adaptation might
be mediated by synaptic changes within PMd and M1, yet with largely
preserved neural covariance within these areas. We addressed this
question by asking how adaptation based on connection weight
changes within PMd and M1 (Hlocal) alters network activity compared
to the corresponding activity changes if VR adaptation is based on
altered inputs from upstream areas (Hinput)10,13–18 (Fig. 1A). To validate
our modelling results, we compared our simulations to experimental
recordings from PMd and M1 populations during the same VR task10.
Under Hlocal, the changes in covariance following VR adaptation
only slightly exceeded those under Hinput and were comparable to
experimental observations. Thus, when using neural population
recordings alone, it may be more challenging to disentangle these two
hypotheses than previously thought. Moreover, for both Hinput and
Hlocal, the learned connectivity changes were small and highly coor-
dinated, which made them surprisingly robust to noise. To identify
additional differences between Hinput and Hlocal, we examined learning
during paradigms requiring larger behavioural changes. Covariance
changes were larger for these paradigms in both PMd and M1 under
Hinput, but only in M1 under Hlocal, thus providing a possible way to
distinguish between the two hypotheses in future experiments. Our
findings have implications for the interpretation of neural activity
changes observed during learning, and suggest that tasks eliciting
larger behavioural changes may be necessary to elucidate how neural
populations adapt their activity during rapid learning.
Results
To understand whether motor adaptation could be driven by synaptic
changes within PMd and M1, we simulated a VR adaptation task using a
modular RNN that modelled these two areas, and compared the
resulting changes in network activity to those of neural population
recordings from PMd and M1 during the same VR task10. We quantified
neural activity changes both in the experimental data and in the model
using two measures (Fig. 1B): (1) the relative change in trial-averaged
single neuron activity, and (2) the change in neural covariance
(“Methods”). Combined, they capture aspects of single neuron as well
as population-wide activity changes during adaptation.
Small but measurable changes in neural activity within PMd and
M1 during VR adaptation
Monkeys were trained to perform an instructed delay task, in which
they reached to one of eight visual targets using a planar manip-
ulandum to receive a reward (“Methods”). After performing a block of
Fig. 1 | Competing hypotheses to explain where learning happens during a
visuomotor rotation task. A To study the processes mediating motor cortical
activity changes during adaptation in a visuomotor rotation task, we analyze and
model the activity of neural populations within dorsal premotor cortex (PMd) and
primary motor cortex (M1). We compare two hypotheses: plasticity upstream of
PMd/M1 (Hinput) and plasticity within PMd/M1 (Hlocal). B Measures to quantify the
changes in neural activity following adaptation: (1) relative change in trial-averaged
single neuron activity; (2) change in neural covariance. Both measures compare
baseline trials to late adaptation trials, after monkeys had adapted to the task. Data
from a representative session from Monkey C.
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Fig. 2 | Small but measurable changes in neural activity within PMd and M1
during VR adaptation. A Hand trajectories during the first 30 trials of the base-
line, and the early adaptation epoch (first 150 adaptation trials), and the last 30
trials of the late adaptation epoch (last 150 adaptation trials). Trajectories are
colour-coded by target. Data from Monkey C. B Angular error of the hand trajec-
tories for the example session in A has the typical time course of adaptation.
C Change in trial-averaged activity following adaptation. Data pooled across all
sessions from the two monkeys for PMd and M1 separately (green markers, 11 ses-
sions, 5 Monkey C, 6 Monkey M). Control sessions during which no perturbation
was applied are shown for comparison (black markers, 3 sessions, 1 Monkey C, 2
Monkey M). Shaded area and horizontal bars, data distribution with mean and
extrema (n = 11 experimental sessions). D Change in covariance following adapta-
tion. Same format as (C). The monkey image was created by Carolina Massumoto
who gave permission to use it under CC-BY license.
unperturbed reaches (200–243 trials, depending on the session),
visual feedback about the position of the hand was rotated by 30°,
either clockwise or counterclockwise, depending on the session.
Monkeys adapted rapidly to these perturbations: the curved reaches
observed immediately after the perturbation onset became straighter
after tens of trials, with the hand trajectories in the second (late) half of
the adaptation block becoming more similar to the baseline trajec-
tories (Fig. 2A). The angular error quantifying the difference between
initial reach direction and target location decreased during adaptation
(Fig. 2B). This error curve followed a similar trend for clockwise and
counterclockwise perturbations, allowing us to analyze the different
perturbations together.
Behavioural adaptation was accompanied by changes in neural
activity within both PMd and M1 (Fig. 2C)10. These changes exceeded
those during control sessions, where no perturbation was applied
(Fig. 2C black; linear mixed model analysis: t = 4.4, P = 0.0017). The
amount of change was greater within PMd than M1 (t = 8.9, P < 0.0001).
We also found small but detectable changes in neural covariance
during VR perturbation, suggesting that the statistical interactions
among neurons change slightly during adaptation (Fig. 2D). Again,
these changes exceeded those of the control sessions (Fig. 2D black;
t = 2.6, P = 0.026).
A modular recurrent neural network model to study VR
adaptation
To test whether experimentally observed changes in motor cortical
activity could be driven by rapid synaptic plasticity9 within PMd and
M1, we trained a modular RNN model23,27 to perform the centre-out
reaching task that we studied experimentally. To mimic broadly the
hierarchical architecture of the motor cortical pathways, input signals
were sent to the PMd module which then projected to the M1 module
to produce the final output signal (Fig. 3A; “Methods”). After initial
training on the task, the model produced correct reaching trajectories
to each of the eight different targets (Fig. 3B and Supplementary Fig. 1).
These RNN-controlled movements had the same dynamics as those of
monkeys (Fig. 3C). Furthermore, Principal Component Analysis
revealed that the population activity of the PMd and M1 network
modules was similar to that of the corresponding recorded neural
populations (Fig. 3D, E). We used Procrustes analysis31 to quantify this
apparent similarity between model and experimental population
activity (Supplementary Fig. 2). This analysis confirmed that the
modular RNN captured the area-specific features in the neural data
accurately, as the PMd and M1 modules better explained neural data
from the respective brain area compared to a cross-area control
(Supplementary Fig. 2).
Motor adaptation through altered inputs matches neural
recordings
After having verified that our modular RNN recapitulates the key
aspects of PMd and M1 population activity during reaching, we simu-
lated the VR adaptation experiment. The model was retrained to pro-
duce trajectories rotated by 30°, replicating the perturbation monkeys
had to counteract. Having full control of the location of learning-
related changes, we first constrained it to happen upstream of PMd
(Hinput). As anticipated from previous modelling18 and experimental
work10, changes in areas upstream of the motor cortices can lead to
successful adaptation: the hand trajectories produced after learning
were correctly rotated by 30° to counteract the perturbation (Fig. 4A).
When examining the activity of each of the PMd and M1 modules,
the relative change in network activity was similar in magnitude to the
changes observed in the corresponding neural population recordings
(Fig. 4B and Supplementary Fig. 3). PMd activity changed slightly more
than M1 activity (Fig. 4B), indicating a relation between the two mod-
ules that was also present in the experimental data (Fig. 2C). With
respect to interactions between neurons, covariance within each
module was strongly preserved (Fig. 4C), as was the case for the
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Fig. 3 | A modular recurrent neural network model to study VR adaptation. A A
modular RNN that models key motor cortical areas to study adaptation.
B Simulated (top) and actual (bottom) hand trajectories during 30 reaches to each
target taken from one session from Monkey C. C Example simulated and actual
hand trajectories to one target. Note the similarity in kinematics between the model
and the experimental data. D Simulated PMd population activity recapitulates key
features of actual PMd population activity. Neural trajectories extend from 600 ms
before the go cue (black dots) to 600 ms after the go cue (coloured dots); go cue is
indicated with coloured crosses. Reaching targets are colour-coded as in B. E Same
as (D) for M1.
experimental data (Fig. 2D). VR adaptation through altered inputs to
the motor cortices thus is very similar to the neural activity changes
observed in vivo.
Learning through plastic changes within PMd and M1 modules
occurs despite preserved the covariance
Our simulation results so far are consistent with experimental10,13–15 and
modelling18 studies proposing that VR adaptation is mediated by
regions upstream of the motor cortices. But can our model rule out the
alternative that adaptation is instead implemented by recurrent con-
nectivity changes within PMd and M1 (Hlocal)?
To address this question, we implemented Hlocal by constrain-
ing learning to happen only within PMd and M1, a process which also
led to successful adaptation (Fig. 4D). Interestingly, the activity
changes produced under Hlocal differed both from those of Hinput
and the experimental data: there were larger changes in the M1
module than in the PMd module (Fig. 4E). However, learning based
on recurrent weight changes within PMd and M1 did not lead to
large changes in covariance, which was largely preserved (Fig. 4F),
virtually as much as when no local plasticity was allowed (Hinput)
(Fig. 4C). Thus, the intuition that preserved covariance should be
interpreted as a sign of stable underlying connectivity may be
misleading.
Small but coordinated connectivity changes enable motor
adaptation
We wished to understand how the model can adapt to the VR pertur-
bation by changing the recurrent connectivity within the PMd and
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Fig. 4 | Activity changes following learning upstream (Hinput) and within (Hlocal)
the motor cortices. A Hand trajectories after learning under Hinput (coloured tra-
ces; baseline trajectories are shown in grey). B Changes in trial-averaged activity
following adaptation under Hinput (green markers) for PMd and M1, and reference
mean experimental values (black stars; same data as presented in Fig. 2). Shaded
area and horizontal bars, data distribution with mean and extrema (n = 10 network
initializations). C Change in covariance following adaptation under Hinput, and
reference values for change in covariance following the initial de-novo training
(dashed lines). Data presented as in B. D Hand trajectories after learning under
Hlocal. E Change in trial-averaged activity following adaptation under Hlocal.
F Change in covariance following adaptation under Hlocal. Data in D–F are pre-
sented as in A–C.Source data.
M1 modules without altering their covariance. Interestingly, the con-
nectivity changes under both Hlocal and Hinput (Fig. 5A, B) were small
relative to experimentally observed synaptic changes32: an average
weight change of 1–2% was sufficient regardless of whether they hap-
pened upstream of (Fig. 5C and Supplementary Fig. 4) or within the
motor cortical modules (Fig. 5E and Supplementary Fig. 5). These
changes were smaller than those observed during initial training
(4–31%), when the model learned to perform the reaching task from
random connection weights (Supplementary Fig. 6). Thus, “functional
connectivity” within the PMd and M1 modules, as measured here by
their covariance, may be largely preserved after VR adaptation
under Hlocal because network connection weights change very little
(Supplementary Fig. 7).
We next studied how such small changes in connection weights
could nevertheless drive effective behavioural adaptation. Recent
studies seeking to relate RNN activity and connectivity have high-
lighted the importance of low-dimensional structures in connectivity,
showing their explanatory power for understanding how tasks are
solved33–36. Inspired by this work, we looked for low-dimensional
structure in the connectivity changes emerging in the model during
adaptation (“Methods”). Our analysis revealed that the connectivity
change patterns of all plastic modules were low-dimensional, inde-
pendent of where learning happened (Fig. 5B, D, F). We thus hypo-
thesized that the small changes were effective because they were low-
dimensional. To test this, we examined how random changes in the
connection weights (noise), which are inherently high-dimensional,
would affect the behaviour.
Low-dimensional connectivity changes are highly robust
to noise
For both Hlocal and Hinput, the learned connectivity changes in the
model were small and low-dimensional. When considering the biolo-
gical plausibility of our model, this observation raises the question of
how such small connectivity changes could compete with ongoing
synaptic fluctuation, which is a known challenge for actual brains37–40.
To test the hypothesis that the low-dimensionality of the learned
connectivity changes is what makes them highly effective, we tested
how adding synaptic fluctuations, which are inherently high-dimen-
sional, would affect motor output. Simulating synaptic fluctuations by
applying random perturbations to the learned connectivity changes
increased the dimensionality of the weight changes (Fig. 6B, G;
“Methods”), but did not lead to any observable change in reaching
kinematics (Fig. 6C) or network activity (Fig. 6D, E). This was the case
even though the applied random perturbations in connectivity were
ten times bigger in magnitude than the learned connectivity changes
(Fig. 6F), completely masking them (Fig. 6A, B). Therefore, our model
not only suggests that VR adaptation can be implemented based on
coordinated synaptic weight changes within PMd and M1, but also that
this type of learning would be highly effective due to its robustness to
synaptic fluctuation.
Larger visuomotor rotations allow for a clearer distinction
between Hinput and Hlocal
Although neural activity changes during VR adaptation were better
reproduced by a model in which learning happens upstream of the
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Fig. 5 | Small but coordinated connectivity changes enable motor adaptation.
A Example connection weights for the M1 module after initial training. Top: esti-
mated dimensionality. B Example changes in M1 connection weights following VR
adaptation under Hlocal. Same format as (A). C Change in connection weights fol-
lowing adaptation under Hinput. Each bar summarizes results for either one module
of the network or a set of cross-module connections; bars and error bars, mean and
s.d. (n = 10 network initializations). D Estimated dimensionality of connection
weight changes for each network module and cross-module connections; data
presented as in (C). E Change in connection weights following adaptation under
Hlocal. F Dimensionality of connection weight changes under Hlocal. Data in E, F are
presented as in C, D, respectively. Source data.
motor cortices (Hinput), activity changes following learning through
weight changes within the motor cortices (Hlocal) were also in good
agreement with the experimental data. To verify that the stable cov-
ariance (Fig. 4C, F) is not a general feature of the model but reflects
task-specific demands, we modelled tasks for which we would expect
larger changes.
We first asked the network to learn larger VRs of 60° and 90°
instead of the original 30° rotation (Fig. 7A). The model was able to
compensate for these larger perturbations under both Hinput and Hlocal
(Fig. 7B, E). As expected, larger perturbations led to changes in net-
work activity and covariance that increased with rotation angle
(Fig. 7B, C, F, G). For the 90° rotation, we found a clear difference
between Hinput and Hlocal: Hinput produced larger activity changes in
PMd compared to M1, opposite that under Hlocal (Fig. 7C, F). Larger
rotation angles also increased the learning-related difference in
covariance between Hinput and Hlocal. Under Hinput, the increase in
covariance was similar for the PMd and M1 modules as the rotation
increased (Fig. 7D). In contrast, under Hlocal, the M1 covariance chan-
ged more with increasing rotation angle than did that of PMd (Fig. 7G).
These model predictions could help differentiate between Hinput and
In fact, preliminary M1 population
Hlocal
recordings obtained during larger VRs (45° and 60°) seemed to match
the model predictions for the covariance change under Hinput (Fig. 7D
stars), but not Hlocal (Fig. 7G stars).
in future experiments.
A visuomotor reassociation task can differentiate between Hlocal
and learning through remapping of input signals
Although larger visuomotor rotations help differentiate between
upstream learning and learning within PMd and M1, we sought to
identify a task that would lead to an even clearer distinction. To this
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Fig. 6 | Low-dimensional connectivity changes are highly robust to noise.
A Example changes in M1 connection weights following VR adaptation. Same data
as in Fig. 5B. B Same connection weight changes as in A, but with random con-
nectivity changes added. Note the dramatic increase in the dimensionality of the
connection weight changes. C Root mean squared error between target and pro-
duced hand trajectories following adaptation in models with and without random
weight changes; bars and error bars, mean and s.d. (n = 10 network initializations),
as in all the panels in this figure. Dashed line, error under VR perturbation without
any learning. D Change in trial-averaged activity for PMd and M1 module, without
(solid) and with (empty) random weight changes. E Change in covariance. Same
format as (D). F Change in connection weights for each network module and cross-
module connections in models with (green bars) and without (dashed lines) noise
in connectivity. G Dimensionality of connection weight changes. Same format
as (F).
end, we implemented a reassociation task where the model had to
learn a new, random mapping between cues and reaching directions
(Fig. 8A; “Methods”). This task allowed us to test a very specific change
in the input signal to the motor cortices that could implement
adaptation20,41: instead of adjusting the connectivity in an upstream
network (Hinput), which allows for highly unconstrained modulation of
input signals, the target-related input signals were manually reordered
to compensate for the reassociation of cue-reaching direction pairs
(Fig. 8B). This “learning through input reassociation” resulted in large
changes in network activity (Fig. 8C), comparable in magnitude to
those under Hlocal (Fig. 8F). Nevertheless, it did not cause any change in
covariance (Fig. 8D), which clearly distinguished it from Hlocal (Fig. 8G)
and the standard Hinput (Supplementary Fig. 8). This was the case
because, in contrast to the standard Hinput during VR adaptation, the
input signals did not change per se, but were only reassigned to dif-
ferent targets, thereby entirely preserving the network activity
patterns.
Discussion
Rapid motor learning is associated with neural activity changes in the
motor cortices. The origin of these changes remains elusive, due to the
current challenge of measuring synaptic strength in vivo. Here, we
have used modular RNNs to simulate the motor cortices and to explore
whether learning to counteract a visuomotor rotation within tens of
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Fig. 7 | Larger visuomotor rotations allow for a better distinction between
Hinput and Hlocal. A To verify that the modelled perturbation does not always
produce small activity changes, we tested adaptation to larger VR perturbations
(60° and 90°). B Root mean squared error between target and produced hand
trajectories without (grey) and with learning (black) under Hinput. Dashed line, error
after initial training, with no perturbation applied; shaded area and horizontal bars,
data distribution with mean and extrema (n = 10 network initializations). Same data
presentation in all panels. C Change in trial-averaged activity for PMd and M1 under
Hinput. A few experimental sessions from Monkey C with larger rotations are shown
as comparison (stars). D Change in covariance following adaptation. Data are
presented as in C. A few experimental sessions from Monkey C with larger rotations
are again shown as comparison (stars). Note the similarity between PMd (light
green) and M1 (dark green) across all rotation angles. E Error without (grey) and
with learning (black) under Hlocal. Same format as (B). F Change in trial-averaged
activity for PMd and M1 under Hlocal. G Change in covariance following adaptation.
Data in E–G are presented as in B–D.
minutes could be mediated by local synaptic changes (Hlocal). By
comparing the modelled network activity changes under Hlocal to the
modelled changes observed during learning upstream of the motor
cortices (Hinput), we have shown how the two hypotheses could be
distinguished based on neural population recordings during beha-
viour. Critically, despite the intuition that learning through plastic
changes should lead to detectable changes in neural interactions
within and across PMd and M1 populations, both Hlocal and Hinput
(Fig. 4) largely preserved the covariance within these two regions,
closely matching experimental observations (Fig. 2). This likely hap-
pened because adaptation under Hlocal was achieved through small,
coordinated weight changes within the PMd and M1 network modules
(Fig. 5). Finally, using our model, we propose tasks for which we
anticipate a more dramatic difference between these contrasting
hypotheses (Figs. 7, 8) which can potentially help to interpret experi-
mental data in the future.
Electrophysiological10,13–15 and modelling studies18, as well as psy-
chophysical evidence1,42 suggest that VR adaptation is driven by areas
upstream of the motor cortices. Neurophysiological evidence is largely
based on the observation that the statistical interactions within PMd
and M1 populations remain preserved throughout adaptation10. This
conclusion is in good agreement with studies showing that learning to
generate neural activity patterns that preserve the covariance
structure only takes a few tens of minutes19. Our direct comparison
between Hinput and Hlocal lends further support to this observation.
However, it also paints the intriguing picture that small, globally
organized changes in synaptic weights could enable rapid learning
without changing the neural covariance, a result that was robust
across model initializations (Fig. 4), parameter settings (Supplemen-
tary Fig. 9 and Supplementary Fig. 10), architectural design choices
(Supplementary Fig. 11) and learning algorithms (Supplementary
Fig. 12). Even implementing the modular RNN as a spiking neural net-
work, bringing it closer to biology, did not change this result (Sup-
plementary Fig. 13). Our simulations thus robustly show that
covariance stability is not as directly linked to stable local connectivity
as previously thought, as changes in covariance were comparable
between Hinput and Hlocal for a 30° VR perturbation (Fig. 4). Instead, the
change in neural covariance seemed to be more related to the task
itself, as it correlated with the size of the perturbation: the larger the
initial error (e.g., caused by larger rotations), the larger the change in
covariance (Fig. 7). However, the relation between initial error and
change in covariance differed depending on where the learning hap-
pened (Hinput or Hlocal).
The main difference between the two learning hypotheses we
have examined is where in the hierarchical RNN model the connectivity
changes occur: within the motor cortices (Hlocal), or upstream of them
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Fig. 8 | A visuomotor reassociation task can clearly differentiate between Hlocal
and learning through reassociation of input signals. A We simulated a task in
which the network had to learn new associations between target locations and
reach directions (“Reassociation''). B Root mean squared error between target and
produced hand trajectories without (grey) and with learning (black) through input
reassociation. Dashed line indicates error during baseline trial. Shaded area and
horizontal bars, data distribution with mean and extrema (n = 10 network
initializations). Same data presentation in all panels. C Change in trial-averaged
activity for PMd and M1 under input reassociation. D Change in covariance fol-
lowing adaptation. Note that the covariance matrices do not change at all. E Root
mean squared error between target and produced hand trajectories without (grey)
and with learning (black) under Hlocal. F Change in trial-averaged activity for PMd
and M1 under Hlocal. G Change in covariance following adaptation. Data in E–G are
presented as in B–D.
(Hinput). Although neural covariance was preserved similarly by Hlocal
and Hinput, we found a key characteristic that distinguished the two.
When local connectivity was allowed to be plastic, the largest activity
changes happened within the M1 module, with only small changes in
the PMd module (Fig. 4E). In contrast, when learning occurred
upstream of the PMd and M1 modules, the activity changes were
similar in PMd and M1 (Fig. 4B), even if some learning was also allowed
within PMd and M1 (Supplementary Fig. 10 and Supplementary Fig. 14).
The experimental data, with larger activity changes in PMd than M1,
better matched the pattern produced by Hinput. This observation fur-
ther supports the hypothesis that VR adaptation is mediated by plas-
ticity upstream of the motor cortices.
A more arbitrary visuomotor reassociation task allowed us to test
an alternate way in which upstream learning could occur, with con-
straints against input signals changing but simply being reassigned to
different targets (Fig. 8). Comparing this learning to that mediated by
local connectivity changes revealed a clear distinction: learning under
Hlocal modified the covariance in both PMd and M1, whereas learning
through input reassociation preserved it20. Thus, future experiments
seeking to disentangle to which extent learning happens within the
motor cortices and/or upstream could study this task.
Studies of learning in RNNs have focused on how networks
implement de-novo training23,24,27,36,43–49. However, our brain does not
learn to perform any task from scratch; it has been “trained” over many
generations throughout evolution50. Here we studied how neural net-
works adapt a learned behaviour, as opposed to de-novo learning. Our
work raises the intriguing possibility that rapid learning following a few
tens of minutes of practice could be easily achieved through small but
specific changes in circuit connectivity. Thus, initial training seems to
provide a highly flexible backbone to adapt behaviour as needed51.
The fact that the connectivity changes during adaptation under
both Hlocal and Hinput were small and low-dimensional (Figs. 5, 6) sug-
gests that either one could mediate rapid learning. First, as every
synaptic change is costly52, we would expect a constraint on the total
amount of connectivity change in the brain. The VR task being solved
with only minor weight changes reflects this; in fact, they could be well
achieved through long-term potentiation or depression of existing
synapses, as experiments have shown that synaptic strength can
double within minutes32. Second, the low dimensionality of these
weight changes is also important with respect to solving “credit
assignment”, the problem of determining how each synapse should
change in order to restore the desired behaviour53–56. Although it is still
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unclear how this is achieved in the brain, one possibility is that synaptic
plasticity is guided by “teacher” signals57,58. Since neuromodulatory
signals can regulate synaptic plasticity59,60, they seem ideal candidates
to regulate biologically plausible learning41,61–63. The finding that the
connectivity changes needed to adapt to the VR perturbation are
“naturally” low-dimensional is promising, as it suggests that learning
could be controlled through relatively few neuromodulatory signals.
Such implementation would contrast dramatically with the daunting
challenge of learning to regulate every single synapse independently.
Lastly, the robustness against synaptic fluctuations conveyed by the
low-dimensional connectivity changes makes both Hlocal and Hinput
attractive in terms of ensuring memory stability. Given the fluctuating
nature of brain connectivity37,
it remains puzzling how animals
remember anything38–40,64. That low-dimensional weight changes,
much smaller than ongoing synaptic fluctuations, can achieve suc-
cessful behavioural adaptation provides a potential solution to this
problem.
Our model consistently underestimated the changes in trial-
averaged activity observed during VR adaptation, despite closely
matching the small covariance changes (Fig. 2,4). This is to be expec-
ted, as the model only captures changes due to the motor adaptation
process itself, whereas the actual neural activity contains signals rela-
ted to other processes such as “impulsivity”65 or “engagement”66. In
fact, the experimentally observed neural activity changes between the
early and late trials of control reaching sessions with no perturbation
were almost as large as the changes during adaptation in our model
(Fig. 2C, black dots). How these changes that are not related to learning
are combined with the learning-related changes studied here remains
unclear. Our modelling predictions for the learning-related changes
could help tackle this question in future studies.
A second potential reason why our model consistently under-
estimated the activity changes during adaptation could be the fact that
we did not include visual or proprioceptive feedback signals in our
modelling approach67–71. As those signals also change during adapta-
tion, they might cause additional changes in trial-averaged neural
activity, despite not being directly necessary to solve the motor
adaptation task. This could explain why our model could solve the task
with smaller changes in neural activity. On the other hand, feedback
signals could also actively contribute to the adaptation process. From
this view, we may presently overestimate the already small con-
nectivity changes underlying VR adaptation (Fig. 5), as part of the
learning process could have been instead driven by dynamic feedback
signals. Thus, when taking feedback into account, rapid learning of a
motor perturbation could potentially be realized with even smaller
changes in underlying connectivity, or maybe even without any con-
nectivity changes at all2. To this point, the concrete role of feedback for
rapid motor learning remains unclear and it could be interesting to use
our model to further investigate this question.
Our simulations were not designed to study trial-by-trial learning:
we were interested in the neural activity changes between the baseline
and late adaptation phases when the subjects had largely learned to
counteract the perturbation and reached stable behaviour (Fig. 2B).
Given that motor adaptation seems to be mediated by two processes
with different timescales72–74, our model mainly captures the slower of
the two. The neural activity changes underlying the early phase
adaptation may be driven by different processes10, which our model
currently does not test.
In conclusion, our comparison between the activity changes fol-
lowing VR adaptation through plastic changes within or upstream of
the motor cortices shows that local plasticity (Hlocal) leads to neural
signatures that are unexpectedly similar to those of upstream learning
(Hinput). Intriguingly, Hlocal not only largely preserved the covariance
within PMd and M1 but also resulted in connectivity changes that seem
biologically reasonable: they are small, make the network robust
against synaptic fluctuations, and can be controlled by relatively few
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teaching signals. Our simulations thus encourage caution when
drawing conclusions from the analysis of neural population recordings
during learning, and further suggest potential behavioural tasks that
could make it easier to identify where learning is happening within the
motor system.
Methods
Tasks
We studied motor adaptation using a visuomotor rotation (VR) para-
digm, previously described in Perich et al. 201810. Monkeys (macaca
mulatta) performed an instructed delay centre-out-reaching task in
which they had to reach to one of eight targets uniformly distributed
along a circle. All targets were 2 cm squares. The delay period was
variable and ranged between 500 and 1500 ms. For additional details
on the task, see10. During the adaptation phase, visual feedback was
rotated clockwise or counterclockwise by 30°, 45°, or 60°. All surgical
and experimental procedures were approved by the Institutional Ani-
mal Care and Use Committee (IACUC) of Northwestern University.
Using our modular RNN model, we simulated both this task and a
visuomotor reassociation task in which there was no consistent rota-
tion of the visual feedback; instead, each target required reaching to a
different direction, uniquely selected from the initial set of eight dif-
ferent targets.
Experimental recordings
We analyzed eleven sessions from two monkeys (five for Monkey C, six
for Monkey M) that were exposed to a clockwise or counterclockwise
30° rotation (data previously presented in10). In addition to these data,
we also analyzed three control sessions (one for Monkey C, two for
Monkey M) in which no perturbation was applied, as well as additional
sessions with larger VR angles from Monkey C where only M1 data was
collected (30°, nine sessions; 45°, two sessions; 60°, two ses-
sions) (Fig. 7).
The spiking activity of putative single neurons was binned into 10
ms bins and then smoothed using a Gaussian filter (s.d., 50 ms). Only
successful trials, where monkeys received a reward at the end, were
included in the analysis. We defined the early and late adaptation
epochs as the first and last 150 trials of the perturbation phase, when
the visuomotor rotation was applied, respectively.
RNN model
Architecture. The neural network contained three recurrent modules,
each consisting of 400 neurons, which we refer to as upstream, PMd
and M1, respectively (Fig. 3A). The PMd and the upstream modules
received an identical three-dimensional input signal, with the first two
dimensions signalling the x and y target location of that trial, and the
third dimension signalling go (1 until the go, and 0 from then on). The
upstream module connects to the PMd module and the PMd module
connects to the M1 module. The output is calculated as a linear readout
of the M1 module activity. Recurrent, as well as feedforward connec-
tions were all-to-all. The model dynamics are given by
t + 1 = xUP
xUP
t +
(cid:1)
dt
τ
(cid:1)xUP
t + WUP tanhðxUP
t
Þ + Win,UPst
(cid:3)
ð1Þ
t + 1 = xPMd
xPMd
t
+
(cid:1)
(cid:1)xPMd
t
dt
τ
+ WPMd tanhðxPMd
t
Þ + WUP-PMd tanhðxUP
t
Þ + Win,PMdst
(cid:3)
t + 1 = xM1
xM1
t +
(cid:1)
dt
τ
(cid:1)xM1
t + WM1 tanhðxM1
t
Þ + WPMd-M1 tanhðxPMd
t
(cid:3)
Þ
t = Wout tanhðxM1
xout
t
Þ + bout
ð2Þ
ð3Þ
ð4Þ
10
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where xUP describes the network activity in the upstream module, and
xPMd and xM1 the network activity in the PMd and M1 module respec-
tively. WUP, WPMd and WM1 define the recurrent connectivity matrix
within the upstream module, the PMd module and the M1 module,
respectively. WUP-PMd defines the connectivity matrix from the
upstream module to the PMd module, and WPMd-M1 defines the con-
nectivity matrix from the PMd module to the M1 module. The input
connectivity matrices for the upstream and the PMd module are given
by Win,UP and Win,PMd, respectively; st represents the three-dimensional
input signal described above. The two-dimensional output xout is
decoded from the M1 module activity via the output connectivity
matrix Wout and the bias term bout. The time constant is τ = 0.05 s and
the integration time step is dt = 0.01 s.
Training. Each network was initially trained to produce planar reaching
trajectories, mirroring the experimental hand trajectories. The training
and testing data set were constructed by pooling the hand trajectories
xtarget for successful trials during the baseline epochs from all experi-
mental sessions, which resulted in 2238 trials of length 4 s (90%/10%
randomly split into training/testing). The held out testing data was
used to validate that the model had been trained successfully during
the initial training period. Model simulations were implemented using
PyTorch75 and training was performed using the Adam optimizer76 with
a learning rate of 0.0001 (β1 = 0.9, β2 = 0.999). The initial training
consisted of 500 training trials. The loss function was defined as
L =
1
BðT (cid:1) 50Þ2
B
∑
b
T
∑
t= 50
∑
d= x,y
(cid:1)
xout,d
t,b
(cid:1) xtarget,d
t,b
(cid:3)
2
+ Eweights + Erates
ð5Þ
where the regularization term on the weights is given by (∣∣ . ∣∣ indicates
L2 norm)
Eweights = αð∣∣Win,UP∣∣ + ∣∣Win,PMd∣∣ + ∣∣Wout∣∣ + ∣∣WPMd∣∣ + ∣∣WM1∣∣
+ ∣∣WPMd-M1∣∣ + ∣∣WUP∣∣ + ∣∣WUP-PMd∣∣Þ
the regularization term on the rates is given by
Erates = β 1
BTN
B
∑
b
T
∑
t
(cid:4)
(cid:1)
N
∑
n
(cid:1)
tanh xPMd,n
t,b
(cid:3)
(cid:3)
2
(cid:1)
(cid:1)
+ tanh xM1,n
t,b
(cid:3)
(cid:3)
2
(cid:1)
(cid:1)
+ tanh xUP,n
t,b
ð6Þ
(cid:5)
(cid:3)
(cid:3)
2
ð7Þ
with batch size B = 80, time steps T = 400 and neurons N = 400. The
regularization parameters were set to α = 0.001, β = 0.8. We clipped
the gradient norm at 0.2 before we applied the optimization step. For
the VR adaptation, we trained the initial network for another 100 trials
with the target trajectory rotated 30° (or 60° or 90° for the case of the
larger VRs). For the VR reassociation task we shuffled the stimulus s
across reaching directions but kept the targets xtarget fixed, as indicated
in Fig. 8A (colours correspond to the given stimulus and sketched
reaching trajectories correspond to the assigned target). The network
had again 100 trials to adapt to this perturbation.
Data analysis
We quantified the changes in actual and simulated neural activity fol-
lowing adaptation using two measures: changes in trial-averaged
activity (or peristimulus time histogram, PSTH), and changes in cov-
ariance. We calculated both metrics within a window that started 600
ms before the go signal and ended 600 ms after it. The change in
activity was calculated by
∣PSTHLateadaptation (cid:1) PSTHBaseline∣
σBaseline
ð8Þ
model, 100 trials with similar go signal timing), PSTHLateadaptation is the
trial-averaged activity in the late adaptation epoch (experimental data:
last 150 trials of the adaptation epoch; simulation data: on a model
trained to counteract the perturbation, 100 trials with similar go signal
timing), and σBaseline is the neuron-specific standard deviation across
time and targets during the baseline epoch. To summarize the change
in trial averaged activity across all neurons, time points, and targets, we
calculated their median; this provided one single value for each
experimental session or simulation run. The change in covariance was
calculated using the same trial-averaged data from the baseline and the
late adaptation epoch. We calculated the covariance in each of these
two epochs and then quantified the similarity by calculating the
Pearson correlation coefficient between the corresponding entries of
the two matrices. The change in covariance is then defined by 1 minus
the correlation coefficient. For the experimental sessions, we
computed a lower bound for each measure using the control sessions
in which monkeys were not exposed to a perturbation. To account for
the fact that there could be activity changes unrelated to motor
adaptation65,66, we compared the activity during 150 consecutive trials
from the first half of the control session with 150 consecutive trials
from the second half of the control session.
To compute the magnitude of the weight changes after networks
learned to counteract the perturbation, we computed the average
absolute weight change as
dW =
∣WLateadaptation (cid:1) WBaseline∣
WBaseline
ð9Þ
.
where ∣
∣ indicates the element wise absolute value, WBaseline is
defined as the model parameter (either Win,PMd, Win,UP, WUP, WUP-PMd,
WPMd, WPMd-M1, or WM1) after the initial training phase but before training
on the VR perturbation, and WLateadaptation is defined as the same model
parameter after training on the VR perturbation. To obtain one sum-
mary value for each simulation run, we calculated the median of all
weight entries for a given parameter. To measure the dimensionality of
weight change we calculated the singular values ki of WLateadaptation −
WBaseline and defined the dimensionality, using the participation ratio77:
(cid:4)
(cid:5)
2
ki
∑
i
k2
i
= ∑
i
ð10Þ
Statistics
To statistically compare the change in activity found in the control
sessions with the change found in the VR sessions, we performed a
linear mixed model analysis using R (lmer package). The brain area
(PMd or M1) and whether the experimental session included a per-
turbation phase or not were included as fixed effects, whereas monkey
and session identity were included as random effects. A significance
threshold of P = 0.05 was used.
Simulation of synaptic fluctuation (Fig. 6)
To simulate synaptic fluctuation we added random values to the
learned connectivity changes during adaptation. Those random values
were drawn from a normal distribution with zero mean and s.d. ten
times larger than the s.d. of the learned weight changes distribution.
With that, we created synaptic noise which was completely unstruc-
tured across connection sites. We did not add or delete any synapses in
the model.
where PSTHBaseline is the trial-averaged activity in the baseline epoch
(experimental data: all baseline trials; simulated data: on a trained
Reporting summary
Further information on research design is available in the Nature
Research Reporting Summary linked to this article.
Nature Communications |
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https://doi.org/10.1038/s41467-022-32646-w
Data availability
The data that support the findings in this study are available from the
corresponding authors upon reasonable request. Source data are
provided with this paper.
Code availability
All code to reproduce the main simulation results can be found on
GitHub (https://github.com/babaf/motor-adaptation-local-vs-input.git).
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Acknowledgements
This work has been funded by BBSRC (BB/N013956/1 and BB/N019008/
1), Wellcome Trust (200790/Z/16/Z), the Simons Foundation (564408)
(all to C.C.), the EPSRC (EP/R035806/1 to C.C. and EP/T020970/1 to
JAG), and the ERC (ERC-2020-STG-949660 to J.A.G.). The funders had
no role in study design, data collection and analysis, decision to publish,
or preparation of the manuscript.
Author contributions
Conceptualization: B.F., J.A.G., and C.C. Methodology: B.F., J.A.G., and
C.C. Experimental data collection: M.G.P. Modelling: B.F. Analysis and
interpretation of data: B.F., J.A.G., and C.C. Supervision: J.A.G. and C.C.
Writing/review of the paper: all.
63. Liu, Y. H., Smith, S., Mihalas, S., Shea-Brown, E. & Sümbül, U. Cell-
type-specific neuromodulation guides synaptic credit assignment
Competing interests
The authors declare no competing interests.
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Additional information
Supplementary information The online version contains supplementary
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Juan A. Gallego or Claudia Clopath.
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Data Availability Statement: All relevant data are
within the paper and its Supporting Information
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|
All relevant data are within the paper and its Supporting Information files.
|
RESEARCH ARTICLE
Vibration of symmetrically layered angle-ply
cylindrical shells filled with fluid
Nurul Izyan Mat Daud1,2, K. K. ViswanathanID
1,3*
1 UTM Centre for Industrial and Applied Mathematics, Ibnu Sina Institute for Scientific & Industrial Research,
Universiti Teknologi Malaysia, Johor Bahru, Johor, Malaysia, 2 Department of Mathematical Sciences,
Faculty of Science, Universiti Teknologi Malaysia, Johor Bahru, Johor, Malaysia, 3 Department of
Mathematics, Kuwait College of Science and Technology, Doha District, Safat, Kuwait
* [email protected], [email protected]
Abstract
Vibrational behaviour of symmetric angle-ply layered circular cylindrical shell filled with qui-
escent fluid is presented. The equations of motion of cylindrical shell in terms of stress and
moment resultants are derived from the first order shear deformation theory. Irrotational of
inviscid fluid are expressed as the wave equation. These two equations are coupled. Strain-
displacement relations and stress-strain relations are adopted into the equations of motion
to obtain the differential equations with displacements and rotational functions. A system of
ordinary differential equation is obtained in one variable by assuming the functions in sepa-
rable form. Spline of order three is applied to approximate the displacement and rotational
functions, together with boundary conditions, to get a generalised eigenvalue problem. The
eigenvalue problem is solved for eigen frequency parameter and associate eigenvectors of
spline coefficients. The study of frequency parameters are analysed using the parameters
the thickness ratio, length ratio, angle-ply, properties of material and number of layers under
different boundary conditions.
Introduction
Composite materials are widely used in petroleum, chemical industry etc., due to the high stiff-
ness and strength. Other characteristics of composite materials are resistance to corrosion and
light in weight. The applications of these kinds of materials can be seen in industries like trans-
portation, aircraft, construction, marine and consumer products. Hence, the investigation on
the vibrational behaviour of the structure is carried out in order to determine its natural fre-
quency. The important of finding frequency is to prevent the structure from resonance thus to
improve the life-span of the structure. There are many literature studied the vibrational behav-
iour of the shell structure especially in cylindrical shell itself by considering different theories
and method of solution. Warburton and Higgs [1] used Rayleigh-Ritz method to solve a canti-
lever cylindrical shell by considering Flugge’s shell theory. Using the same method, Song et al.
[2] investigated the free vibration of symmetrically laminated composite cylindrical shell with
arbitrary boundary conditions.
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OPEN ACCESS
Citation: Mat Daud NI, Viswanathan KK (2019)
Vibration of symmetrically layered angle-ply
cylindrical shells filled with fluid. PLoS ONE 14(7):
e0219089. https://doi.org/10.1371/journal.
pone.0219089
Editor: Fang-Bao Tian, University of New South
Wales, AUSTRALIA
Received: February 2, 2019
Accepted: June 14, 2019
Published: July 3, 2019
Copyright: © 2019 Mat Daud, Viswanathan. This is
an open access article distributed under the terms
of the Creative Commons Attribution License,
which permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: All relevant data are
within the paper and its Supporting Information
files.
Funding: Funded by (K.K.Viswanathan) Grant
number: PR17-16SM-05. Kuwait Foundation for
the Advancement of Sciences. www.kfas.org/. The
funders had no role in study design, data collection
and analysis, decision to publish, or preparation of
the manuscript.
Competing interests: The authors have declared
that no competing interests exist.
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
1 / 18
Vibration of cylindrical shell with fluid
Among the researchers those who used Finite Element Method (FEM) in their analysis
were Sivadas and Ganesan [3], Lam and Wu [4]. The wave propagation method was applied by
Li [5], Zhang [6] and Iqbal et al. [7]. Lopatin and Morozov [8] solved the problem of a cantile-
ver composite cylindrical shell using Galerkin method to find the fundamental frequencies. In
addition, Haar wavelet method was used by Xie et al. [9] to analyse the free vibration of cylin-
drical shell based on Goldenveizer-Novozhilov shell theory. Meanwhile, Jin et al. [10] applied
First Order Shear Deformation Theory (FSDT) to examine the vibration of functionally graded
cylindrical shell. A spline strip method was adopted in studying the vibration of cross-ply lami-
nated cylindrical shells [11]. Bickley-type spline method was applied to analyse the frequencies
of free vibration of cylindrical shell [12–15]. Besides that, a spline-based differential quadrature
method was used by Javidpoor et al. [16] and Ghasemi [17]. Ferreira et al. [18] used multi-
quadric radial basis function method to determine the natural frequencies of doubly curved
cross-ply composite shells.
Moreover, the structure can also interact with fluid either the structure filled with, partially
with, or submerged. The fluid can be flowing or non-flowing fluid. This type of investigation is
known as fluid structure interaction. The characteristics of fluid itself affect the behaviour of
the structure. Hence, the investigation has to consider both shell and fluid in order to get better
results. Recently, the investigation on fluid structure interaction has get attention among the
researchers.
Finite Element Method (FEM) was applied in the problem free vibration of isotropic, verti-
cal cylindrical shell partially and completely filled with stationary liquid [19]. The shell equa-
tions were constructed using Sanders’ thin shell theory. Selmane and Lakis [20] applied FEM
in solving the vibration of an anisotropic cylindrical shell submerged and subjected simulta-
neously to an internal and external flow by considering Sanders’ thin shell theory. Other litera-
tures applied FEM in their analysis are Kochupillai et al. [21], Kochupillai et al. [22], Toorani
and Lakis [23], Toorani and Lakis [24].
Gunawan et al. [25] conducted a study on cylindrical shells filled with fluid based on
elastic foundation by considering Sanders’ thin shell theory. Krishna and Ganesan [26] investi-
gated the results of free vibration of cylindrical shells filled with fluid. The shell was governed
by first order deformation theory. Lakis et al. [27] analysed the isotropic and anisotropic plates
and shells with and without fluid for linear and nonlinear vibration with the shell equations
were based on Sanders’ shell theory and dynamic pressure of fluid was derived from Bernoul-
li’s equation. Galerkin method was used by Goncalves et al. [28] in solving the nonlinear
dynamic behaviour of cylindrical shells filled with fluid with Donnell’s nonlinear shallow shell
theory.
A study on the vibration of vertical circular cylindrical shell partially filled by an incom-
pressible, compressible, quiescent and inviscid fluid using Rayleigh-Ritz method was analysed
by Amabili [29]. The shell was constrained by simply-supported boundary conditions. In addi-
tion to that, Kwak et al. [30] studied the clamped-free cylindrical shell partially submerged in
fluid using Sanders’ shell theory.
Vibrational analysis of fluid filled double-walled carbon nanotubes using the wave propaga-
tion method was carried out by Natsuki et al. [31] and the shell equations were based on sim-
plified Flu¨gge shell theory. Iqbal et al. [32] applied Love’s thin shell theory to study the
vibration of a Functionally Graded Material (FGM) circular cylindrical shell filled with fluid
and the fluid was an incompressible non-viscous fluid. A study on cylindrical shells filled with
fluid resting on elastic foundations was carried out by Shah et al. [33] using wave propagation
method. The shell was constrained with simply supported at the both ends and the Love’s thin
shell theory was applied to the problem. A nonlinear vibration of cantilevered circular
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
2 / 18
Vibration of cylindrical shell with fluid
cylindrical containing quiescent fluid based on Flu¨gge’s shell theory and the fluid motion was
modelled by linearized potential flow theory was investigated by Paak et al. [34].
A dynamic stiffness method was studied by Tran and Manh [35] to investigate the free
vibration of cross-ply laminated composite circular cylindrical shells filled with fluid partially
and also complete filling with fluid under clamped-free boundary conditions. Reissner-Mind-
lin theory was used for the shell equations. The fluid considered as non-viscous and incom-
pressible. In addition, spline method was applied to solve the free vibration of layered
cylindrical shell filled with fluid using Love’s thin shell theory [36]. Nurul Izyan et al. [37]
applied the spline method in their analysis to determine the frequencies of anti-symmetric
angle-ply laminated composite cylindrical shell filled with fluid. The shells’ equations were for-
mulated based on FSDT.
According to a nonlocal theory, there are two types of models which are structural harden-
ing and softening models. Li et al. [38] and Shen and Li [39] proved that both the hardening
and softening models are correct and they are related to different types of surface effects, i.e.
relaxation or tension of surface atomic lattices. Consequently, the two different models are
caused by the long range attractive and repulsive interactions in pair potentials between atoms,
respectively.
Different approach study is done in order to study the fluid structure interaction. The aim
of this study is to determine the vibrational behaviour of symmetric angle-ply laminated com-
posite cylindrical shell. The quiescent fluid-filled shell is considered. The quiescent fluid
means that the vibration of fluid is depends on the vibration of the shell. Once the shell
vibrates, the fluid will vibrate accordingly. Bickley-type spline is used to approximate the dis-
placements and rotational functions since it gives better accuracy and also uses of lower order
approximation in solving boundary value problem [40]. The shells’ equations are based on
FSDT. Three and five layered shell under clamped-clamped and simply-supported boundary
conditions are studied. The material properties of Kevler-49 Epoxy (KGE) and AS4/3501-6
Graphite/Epoxy (AGE) are used. Parametric studies on shell geometry i.e, length and thickness
of the shells, type of materials, ply orientations, number of layer of the materials, and boundary
conditions on frequencies are studied.
Formulation of the problem
Equations of shell
Fig 1 shows the geometry of the circular cylindrical shell with the shell coordinates defined as
(x,θ,z) where x is along the axial direction, θ is in the circumferential and z is along the normal
direction. The length of the shell is ‘, thickness is h and radius is r. The displacement compo-
nents u,v,w are expressed under the first order shear deformation theory [41] as
uðx; y; z; tÞ ¼ u0ðx; y; tÞ þ zcxðx; y; tÞ;
vðx; y; z; tÞ ¼ v0ðx; y; tÞ þ zcyðx; y; tÞ;
wðx; y; z; tÞ ¼ w0ðx; y; tÞ;
ð1Þ
where u,v,w are the displacements in x,θ,z directions. u0,v0,w0 are mid-plane displacements
and ψx,ψθ are the rotational functions of the normal to the mid-plane with respect to the x-
and θ- axes. Equations of motion for cylindrical shell are formulated using FSDT [42, 43]. The
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
3 / 18
Vibration of cylindrical shell with fluid
Fig 1. A geometry and coordinate system of a circular cylindrical shell.
https://doi.org/10.1371/journal.pone.0219089.g001
equations of cylindrical shell which included fluid are written as
¼ I1
@2u
@t2
;
þ
Qy ¼ I1
;
1
r
1
r
þ
þ
þ
þ
@Nx
@x
@Nxy
@x
@Qx
@x
@Mx
@x
@Mxy
@x
@Nyx
1
@y
r
@Ny
1
@y
r
@Qy
1
@y
r
@Mxy
1
@y
r
@My
1
@y
r
(cid:0)
þ
(cid:0) Qx ¼ I3
(cid:0) Qy ¼ I3
@2v
@t2
@2w
@t2
@2cx
@t2
@2cy
@t2
;
:
Ny ¼ I1
(cid:0) p;
ð2Þ
Here, p is the fluid pressure. I1 and I3 are the normal and rotary inertia coefficients, given
by [42,43].
R
ðI1; I3Þ ¼
rðkÞð1;z2Þdz;
where ρ(k) is the material density of the k-th layer of the shell.
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
ð3Þ
4 / 18
Stress and moment resultants are expressed as
Vibration of cylindrical shell with fluid
R
z
ðsx; sy; txy; txz; tyzÞdz;
ðNx; Ny; Nxy; Qx; QyÞ ¼
ðMx; My; MxyÞ ¼
R
z
ðsx; sy; txyÞzdz:
ð4Þ
Using stress-strain relations and strain-displacement relations of the k-th layer by neglect-
ing the transverse normal strain and stress, the stress and moment resultants are obtained as
follows
0
B
B
B
B
B
B
B
B
B
B
B
@
¼
1
C
C
C
C
C
C
C
C
C
C
C
A
0
B
B
B
B
B
B
B
B
B
B
B
@
Nx
Ny
Nxy
Mx
My
Mxy
A11 A12 A16 B11
A12 A22 A26 B12
A16 A26 A66 B16
B12
B22
B26
B16
B26
B66
B11 B12 B16 D11 D12 D16
B12 B22 B26 D12 D22 D26
B16 B26 B66 D16 D26 D66
1
0
C
C
C
C
C
C
C
C
C
C
C
A
B
B
B
B
B
B
B
B
B
B
B
B
B
B
B
B
B
B
B
B
@
@u0
@x
@v0
1
@y
r
@u0
1
@y
r
@cx
@x
@cy
1
@y
r
@cx
1
@y
r
þ
þ
w
r
@v
@x
þ
@cy
@x
1
C
C
C
C
C
C
C
C
C
C
C
C
C
C
C
C
C
C
C
C
A
;
and
!
Qy
Qx
¼ K
A44 A45
A45 A55
0
! cy þ
B
B
@
cx þ
(cid:0)
@w
@y
1
r
@w
@x
v0
r
1
C
C
A:
Here Aij, Bij and Dij are extensional rigidities, bending-stretching coupling rigidities and
bending rigidities, respectively and defined as
ð5Þ
ð6Þ
Aij ¼
XN(cid:0) 1
k¼1
QðkÞ
ij ðzk (cid:0) zk(cid:0) 1Þ; Bij ¼
1
2
XN(cid:0) 1
QðkÞ
ij ðz2
k¼1
k (cid:0) z2
k(cid:0) 1Þ;
Dij ¼
1
3
and
XN(cid:0) 1
QðkÞ
ij ðz3
k¼1
k (cid:0) z3
k(cid:0) 1Þ; ði; j ¼ 1; 2; 6Þ;
Aij ¼ K
XN(cid:0) 1
k¼1
Qij
ðkÞðzk (cid:0) zk(cid:0) 1Þ; ði; j ¼ 4; 5Þ:
Here zk and zk−1 are boundaries of the k-th layer and K is the shear correction factor which
is depends on lamination scheme [44, 45]. Since shell is considered to be a symmetric angle-
ply, therefore, the coefficients A16,A26,A45,D16,D26 and Bij are identically zeroes [13].
The displacements u0, v0, w and shear rotations ψx,ψθ are assumed in the form of
u0ðx; y; tÞ ¼ UðxÞcosnyeiot;
v0ðx; y; tÞ ¼ VðxÞsinnyeiot;
wðx; y; tÞ ¼ WðxÞcosnyeiot;
cxðx; y; tÞ ¼ CxðxÞcosnyeiot;
cyðx; y; tÞ ¼ CyðxÞsinnyeiot;
ð7Þ
5 / 18
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
Vibration of cylindrical shell with fluid
in which ω,t and n are the angular frequency, time and circumferential node number
respectively.
Non-dimensional parameters used are as follows
L ¼
X ¼
R ¼
H ¼
‘
r
x
‘
r
‘
h
r
l ¼ o‘
dk ¼
hk
h
; a length parameter;
; a distance coordinate;
; a radius parameter;
; the thickness parameter;
r
; a frequency parameter;
ffiffiffiffiffiffiffi
I1
A11
; a relative layer thickness of k(cid:0) th layer:
ð8Þ
Substituting Eqs (5) and (6) into Eq (2), then, using Eqs (7) and (8), the differential equa-
tions are obtained in terms of displacement and rotational functions and it can be written in
the matrix form as follows
0
B
B
B
B
B
B
B
B
@
L11 L12 L13 L14 L15
L22 L22 L23 L24 L25
L31 L32 L33 L34 L35
L41 L42 L43 L44 L45
L51 L52 L53 L54 L55
1
0
C
C
C
C
C
C
C
C
A
B
B
B
B
B
B
B
@
1
C
C
C
C
C
C
C
A
U
V
W
CX
Cy
1
C
C
C
C
C
C
C
A
;
0
B
B
B
B
B
B
B
@
0
0
0
0
0
¼
ð9Þ
where Lij are differential operators given as follows
L11 ¼
d2
dX2
(cid:0) S10
n2
R2
þ l2; L12 ¼ ðS2 þ S10Þ
n
R
d
dX
L14 ¼ L15 ¼ 0; L21 ¼ (cid:0) ðS2 þ S10Þ
n
R
d
dX
; L22 ¼ S10
L23 ¼ (cid:0) ðS3 þ KS13Þ
�
¼ L32; L24 ¼ 0; L25 ¼ KS13
�
L33 ¼ KS14
(cid:0)
S3
þ KS13
d2
dX2
n2
R2
�
þ 1 þ
rf
I1
; L13 ¼ S2
1
R
�
;
d
dX
n2
R2
S3
(cid:0)
d2
dX2
1
R
JnðRÞ
nðRÞ
J0
; L31 ¼ (cid:0) S2
�
l2;
�
1
R2
þ l2;
þ KS13
1
R
d
dX
;
n
R2
1
R2
n2
R2
1
R
n2
R2
L34 ¼ KS14
d
dX
L44 ¼ S7
d2
dX2
(cid:0)
; L35 ¼ KS13
�
n
R
; L41 ¼ L42 ¼ 0; L43 ¼ (cid:0) KS14
�
S12
þ KS14
þ l2p1; L45 ¼ ðS12 þ S8Þ
;
d
dX
d
n
dX
R
;
L51 ¼ 0; L52 ¼ KS13
�
; L53 ¼ KS13
�
L55 ¼ S12
d2
dX2
(cid:0)
S9
þ KS13
þ l2p1;
n
R
; L54 ¼ (cid:0) ðS12 þ S8Þ
n
R
d
dX
;
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
6 / 18
with
S2 ¼
A12
A11
; S3 ¼
A22
A11
; S7 ¼
D11
‘2A11
; S8 ¼
S12 ¼
D66
‘2A11
; S13 ¼
A44
A11
; S14 ¼
A55
A11
; S9 ¼
D12
‘2A11
I3
‘2I1
; P1 ¼
:
Vibration of cylindrical shell with fluid
D22
‘2A11
; S10 ¼
A66
A11
;
Equation of fluid
The fluid pressure, p is obtained as an explicit expression and coupled to the equations of the
shell through radial displacement. The wave equation is obtained for irrotational flow of an
inviscid fluid undergoing small oscillations in the cylindrical coordinates system (x, θ, r) [46]
as
@2p
@r2
þ
1
r
@p
@r
þ
1
r2
@2p
@y2 þ
@2p
@x2
¼
@2p
c2@t2
;
where c is the speed sound of the fluid.
The pressure is assumed in the separable form as
pðx; y; r; tÞ ¼ cðxÞcosðnyÞJnðrÞeiot:
ð10Þ
ð11Þ
Here Jn is the Bessel function of order n.
The permeability condition on the fluid- shell interface ensures that the fluid remains in
contact with the shell wall and written as
(cid:0)
1
iorf
@p
@r
�
�
�
�
¼
r¼R
�
�
�
�
@w
@t
;
r¼R
ð12Þ
where ρf is the density of the fluid. Eq (12) is solved by using the displacement component in
the normal direction given in the Eq (7) together with the Eq (11), hence, the following relation
is obtained
cðxÞ ¼
o2rf
nðrÞ
J0
WðxÞ:
Then, by applying Eq (13) into Eq (11), the fluid pressure, p is obtained as follows
pðx; y; r; tÞ ¼ (cid:0) rf
JnðrÞ
nðrÞ
J0
@2w
@t2
:
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
ð13Þ
ð14Þ
7 / 18
Vibration of cylindrical shell with fluid
Solution procedure
Spline collocation method
The displacement functions U,V,W and rotational functions CX and Cθ are approximated
using cubic splines as
U �ðXÞ ¼
V �ðXÞ ¼
X2
i¼0
X2
aiXi þ
ciXi þ
XN(cid:0) 1
j¼0
XN(cid:0) 1
i¼0
j¼0
bjðX (cid:0) XjÞ3HðX (cid:0) XjÞ;
djðX (cid:0) XjÞ3HðX (cid:0) XjÞ;
W�ðXÞ ¼
X2
eiXi þ
XN(cid:0) 1
i¼0
j¼0
fjðX (cid:0) XjÞ3HðX (cid:0) XjÞ:
CX
�ðXÞ ¼
X2
i¼0
giXi þ
XN(cid:0) 1
j¼0
pjðX (cid:0) XjÞ3HðX (cid:0) XjÞ;
Cy
�ðXÞ ¼
X2
liXi þ
XN(cid:0) 1
i¼0
j¼0
qjðX (cid:0) XjÞ3HðX (cid:0) XjÞ:
ð15Þ
Here, H(X−Xj) is the Heaviside step function and N is the number of intervals in the range
of X2[0,1] is divided. These splines are lower order approximation and an effective method
since it has fast convergence and high accuracy. The points of division X ¼ Xs ¼ s
0; 1; 2; . . .NÞ are chosen as the knots of the splines as well as the collocation points. Assuming
that the differential equations given by Eq (9) are satisfied by these splines given in Eq (15) at
the knots, a set of 5N+5 homogeneous equations into 5N+15 unknown spline coefficients ai,bj,
ci,dj,ei,fj,gi,pj,li,qj (i = 0,1,2;j = 0,1,2,. . .,N−1) is obtained.
; ðs ¼
N
Boundary conditions
Two types of boundary conditions are used to analyse the problem
i. Clamped-Clamped (C-C)(both the ends are clamped);
U ¼ 0; V ¼ 0; W ¼ 0; CX ¼ 0; Cy ¼ 0 at X ¼ 0 and X ¼ 1:
i. Simply supported–Simply supported (S–S)(both the ends are simply supported);
V ¼ 0; W ¼ 0; Cy ¼ 0; Nx ¼ 0; Mx ¼ 0 at X ¼ 0 and X ¼ 1:
The system will get ten more equations on spline coefficients by imposing any one of the
boundary conditions. Combining these ten equations with the earlier 5N+5 homogeneous
equations, one can get 5N+15 equations in the same number unknown coefficients. This can
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
8 / 18
Vibration of cylindrical shell with fluid
be written as
½P�fqg ¼ l2½Q�fqg:
ð16Þ
Here, [P] and [Q] are the square matrices of order (5N+15)×(5N+15). {q} is the column
matrix of the spline coefficients of order (5N+15)×1 and λ is the frequency parameter.
Results and discussion
Convergence and comparative studies
The convergence study has been made in order to determine the number of iteration. This is
done by fixing the circumferential node number, thickness ratio, length ratio, number of layers
and orientation of the material under C-C and S-S boundary conditions. The number of
knots, N is taken as 16 since the change in percentage for next following values of N is 0.29%.
In the case of comparison studies, none of literature has been done on symmetric angle-ply
shell with consideration of fluid. There are studies on symmetric angle-ply shells but limited to
empty shells only [4, 13]. Hence, an investigation on the empty shell as well as the fluid-filled
shells with respect to the length parameter is carried out as shown in Fig 2. The effects of the
fluid on angular frequency ωm(m = 1,2,3) of three layered symmetric angle-ply shells using the
materials Kevler-49 epoxy (KGE) and AS4/3501-6 Graphite/epoxy (AGE) are arranged in the
order of KGE-AGE-KGE with the angle orientations at (30˚/0˚/30˚) are presented. The param-
eters n = 2, H = 0.02 are fixed. The shell is clamped at both the ends. According to Fig 2, the
Fig 2. Effect of length parameter on the angular frequency of three layered symmetric angle-ply shells under C-C boundary conditions. Layer materials:
KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g002
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
9 / 18
Vibration of cylindrical shell with fluid
frequency of fluid-filled shell is lower than the frequency of the empty shell. This result is
expected as the fluid in the shell gives an added mass to the shell.
Analysis
Three and five layered symmetric angle-ply circular cylindrical shells with fluid are analysed.
The materials which are KGE and AGE are used [47]. The shear correction factor K = 5/6 is
fixed throughout this analysis [44] and first three frequency parameters are studied for all the
cases.
Fig 3 shows the variation of angular frequencies ωm(m = 1,2,3) on length parameter is stud-
ied for three layered shell with the combination of the materials KGE and AGE with C-C
boundary conditions. The parameters n = 4 and H = 0.015 are fixed and the ply-angles are
arranged as 30˚/0˚/30˚, 45˚/0˚/45˚ and 60˚/0˚/60˚ using the materials AGE and KGE and
ordered as KGE-AGE-KGE. Since the frequency parameter λm is explicitly a function of length
of the cylinder, hence when studying the influence of the length of the cylinder on its vibra-
tional behaviour, the angular frequency ωm(m = 1,2,3) is considered instead of λm. The rela-
tionship between the frequency and the length of the shell can be seen as in [48]. The natural
frequency or equivalent rigidity increases with increasing the non-dimensional scale parame-
ter [49].
From the analysis, it can be seen that the frequency decreases as the length parameter
increases and the frequency is higher for higher modes. The frequency decreases fast at L rang-
ing from 0.5 to 0.75. Later, it decreases slowly. It also can be seen that the frequency for m = 1
of Fig 3(A) is the lowest compared to Fig 3(B) and 3(C). As for m = 2,3, the values of the fre-
quencies are the lowest for Fig 3(C), followed by Fig 3(B) and 3(A). Further, investigation on
S-S boundary conditions is presented in Fig 4 by fixing the parameters as in Fig 3. The trend
shown by the graph of Fig 4 is similar to Fig 3. The results show that the frequencies obtained
by S-S boundary conditions are lower than C-C boundary conditions.
Fig 3. Effect of length parameter on the angular frequency of three layered symmetric angle-ply shells under C-C boundary conditions. Layer materials:
KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g003
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
10 / 18
Vibration of cylindrical shell with fluid
Fig 4. Effect of length parameter on the angular frequency of three layered symmetric angle-ply shells under S-S boundary conditions. Layer materials:
KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g004
Fig 5 corresponds to the effect of length parameter on angular frequency ωm(m = 1,2,3) of
five layered angle-ply arranged materials in the order KGE-AGE-KGE-AGE-KGE with ply-
angles of 45˚/30˚/0˚/30˚/45˚, 30˚/45˚/0˚/45˚/30˚ and 60˚/30˚/0˚/30˚/60˚, respectively for C-C
conditions. The values of n = 4 and H = 0.02 is fixed. The figure shows that the frequency
decreases as the length parameter increases. The investigation is continued by applying S-S
boundary conditions using the same parameters as shown in Fig 6. The trend of graph is
Fig 5. Effect of the length parameter on the angular frequency of five layered symmetric angle-ply shells under C-C boundary conditions. Layer materials:
KGE-AGE-KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g005
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11 / 18
Vibration of cylindrical shell with fluid
Fig 6. Effect of the length parameter on the angular frequency of five layered symmetric angle-ply shells under S-S boundary conditions. Layer materials:
KGE-AGE-KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g006
similar to the Fig 5. The values of ωm(m = 1,2,3) in Fig 6 are lower than the value of
ωm(m = 1,2,3) in Fig 5.
Fig 7 shows the effect of thickness parameter on frequencies λm(m = 1,2,3) by considering
three layered shells arranged in KGE-AGE-KGE materials with n = 4 and L = 1.5 are fixed
under C-C boundary conditions. The shell is arranged in the order of 30˚/0˚/30˚, 45˚/0˚/45˚
Fig 7. Effect of thickness parameter on the frequency for three layered symmetric angle-ply shells under C-C boundary conditions. Layer materials:
KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g007
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
12 / 18
Vibration of cylindrical shell with fluid
Fig 8. Effect of thickness parameter on frequency for three layered symmetric angle-ply shells under S-S boundary conditions. Layer materials: KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g008
and 60˚/0˚/60˚. From the analysis, it can be seen clearly that the frequency rises as the thick-
ness parameter rises. The frequencies are greater for larger modes. The values of λm(m = 1,2,3)
in Fig 7(A) are the lowest compared to Fig 7(B) and 7(C). In addition, Fig 8 presents the varia-
tion of frequencies λm(m = 1,2,3) under S-S boundary conditions. Results show that the values
of λm(m = 1,2,3) in Fig 8 are lower than the values of λm(m = 1,2,3) in Fig 7.
Fig 9 shows the variation of λm(m = 1,2,3) with respect to the thickness parameter for five
layered angle-ply by fixing n = 4 and L = 1 for C-C boundary conditions. The materials are
arranged as KGE-AGE-KGE-AGE-KGE with angle orientation at 45˚/30˚/0˚/30˚/45˚, 30˚/45˚/
Fig 9. Effect of thickness parameter on frequency for five layered symmetric angle-ply shells under C-C boundary conditions. Layer materials:
KGE-AGE-KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g009
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13 / 18
Vibration of cylindrical shell with fluid
Fig 10. Effect of thickness parameter on frequency for five layered symmetric angle-ply shells under S-S boundary conditions. Layer materials:
KGE-AGE-KGE-AGE-KGE.
https://doi.org/10.1371/journal.pone.0219089.g010
Fig 11. Effect of length parameter on frequency for three and five layered symmetric angle-ply shells under C-C boundary conditions.
https://doi.org/10.1371/journal.pone.0219089.g011
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14 / 18
Vibration of cylindrical shell with fluid
Fig 12. Effect of thickness parameter on frequency for three and five layered symmetric angle-ply shells under C-C boundary conditions.
https://doi.org/10.1371/journal.pone.0219089.g012
0˚/45˚/30˚ and 60˚/30˚/0˚/30˚/60˚. Clearly, the frequency is higher for higher values of thick-
ness parameter. Fig 9(A) has the lowest frequency compared to Fig 9(B) and 9(C). Applying
the same parameters as in Fig 9, investigation on S-S boundary conditions is carried out as
depicted in Fig 10. It can be seen that Fig 10(A) has the lowest frequency, followed by Fig 10
(B) and 10(C). It can be observed that the values of λm(m = 1,2,3) under S-S boundary condi-
tions are lower compared to the values of λm(m = 1,2,3) under C-C boundary conditions.
By fixing n = 3, the effects of length parameter for both three and five layered shells on fre-
quencies under C-C boundary conditions are investigated as depicted in Fig 11. The materials
are arranged as KGE-AGE-KGE with angle orientation at 45˚/0˚/45˚ as shown in Fig 11(A).
Meanwhile, Fig 11(B) used KGE-AGE-KGE-AGE-KGE materials with angle orientation at
30˚/45˚/0˚/45/30˚. From Fig 11, it can be seen that the frequencies decrease as the length
parameter increases. It decreases fast in the range 0.5 < ωm < 0.75. Also, the frequencies of
five layered shell are higher than the frequencies of three layered shell.
Next, the frequencies with respect to thickness parameter are analysed as shown in Fig 12.
The frequencies of five layered shell in Fig 12(B) are higher than the frequencies of three lay-
ered shell in Fig 12(A).
Conclusion
The vibrational behaviour of layered cylindrical shell with symmetric angle-ply is investigated
using spline method. The shell contained a quiescent fluid. The equations of motion of the
PLOS ONE | https://doi.org/10.1371/journal.pone.0219089 July 3, 2019
15 / 18
Vibration of cylindrical shell with fluid
shell are based on first order shear deformation theory. Investigations on empty and fluid-
filled shells show that the frequency value reduces as the fluid term is included. This is due to
the fluid in the shell that provides added mass to the shell.
Results show that by increasing the length of the shell, the frequency decreases. In contrast,
the frequency increases as the shell thickness increases. Meanwhile, frequency of C-C bound-
ary conditions is higher than the frequency of S-S boundary conditions. It can be concluded
that the geometric parameters, material properties, angle orientations, number of layers and
boundary conditions significantly affects the frequency of the shell.
Acknowledgments
This work was funded partially by Kuwait Foundation for the Advancement of Sciences
(KFAS) under Project code: PR17-16SM-05 and thanks to the President of KCST for his con-
tinues support to complete this research work.
Author Contributions
Funding acquisition: K. K. Viswanathan.
Methodology: Nurul Izyan Mat Daud, K. K. Viswanathan.
Software: K. K. Viswanathan.
Supervision: K. K. Viswanathan.
Writing – original draft: Nurul Izyan Mat Daud.
Writing – review & editing: K. K. Viswanathan.
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© 2020. Published by The Company of Biologists Ltd | Disease Models & Mechanisms (2020) 13, dmm041962. doi:10.1242/dmm.041962
RESEARCH ARTICLE
Cell-specific and athero-protective roles for RIPK3 in a murine
model of atherosclerosis
Sarah Colijn1,2,*, Vijay Muthukumar1,‡, Jun Xie1, Siqi Gao1,2 and Courtney T. Griffin1,2,§
ABSTRACT
Receptor-interacting protein kinase 3 (RIPK3) was recently
implicated in promoting atherosclerosis progression through a
proposed role in macrophage necroptosis. However, RIPK3 has
been connected to numerous other cellular pathways, which raises
questions about its actual role in atherosclerosis. Furthermore, RIPK3
is expressed in a multitude of cell types, suggesting that it may be
physiologically relevant
to more than just macrophages in
atherosclerosis. In this study, Ripk3 was deleted in macrophages,
endothelial cells, vascular smooth muscle cells or globally on the
Apoe−/− background using Cre-lox
technology. To induce
atherosclerosis progression, male and female mice were fed a
Western diet for three months before tissue collection and analysis.
Surprisingly, necroptosis markers were nearly undetectable in
atherosclerotic aortas. Furthermore, en face lesion area was
increased in macrophage- and endothelial-specific deletions of
Ripk3 in the descending and abdominal regions of
the aorta.
Analysis of bone-marrow-derived macrophages and cultured
endothelial cells revealed that Ripk3 deletion promotes expression
of monocyte chemoattractant protein 1 (MCP-1) and E-selectin in
these cell
respectively. Western blot analysis showed
upregulation of MCP-1 in aortas with Ripk3-deficient macrophages.
Altogether, these data suggest that RIPK3 in macrophages and
endothelial cells protects against atherosclerosis through a
mechanism that
involve necroptosis. This
protection may be due to RIPK3-mediated suppression of pro-
inflammatory MCP-1 expression in macrophages and E-selectin
expression in endothelial cells. These findings suggest a novel
and unexpected cell-type specific and athero-protective function
for RIPK3.
likely does not
types,
This article has an associated First Person interview with the first
author of the paper.
KEY WORDS: Necroptosis, Macrophages, Endothelial cells, MCP-1,
Mouse
1Cardiovascular Biology Research Program, Oklahoma Medical Research
Foundation, Oklahoma City, OK 73104, USA. 2Department of Cell Biology,
University of Oklahoma Health Sciences Center, Oklahoma City, OK 73190, USA.
*Present address: Department of Cell Biology and Physiology, Washington
University in St. Louis, School of Medicine, St. Louis, MO 63110, USA. ‡Present
address: The Jackson Laboratory, Bar Harbor, ME 04609, USA.
§Author for correspondence ([email protected])
C.T.G., 0000-0001-8100-3171
This is an Open Access article distributed under the terms of the Creative Commons Attribution
License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use,
distribution and reproduction in any medium provided that the original work is properly attributed.
Received 14 August 2019; Accepted 18 December 2019
INTRODUCTION
Atherosclerosis is a highly complex pathology that is influenced by
a multitude of environmental and genetic factors. The cellular
mechanisms that have been linked to atherosclerosis development
are vast in number and include metabolic imbalances, inflammation,
fibrosis, mechanotransduction and cell death (Lusis, 2000; Tabas
et al., 2015). Occasionally, these mechanisms are controversial
when there are conflicting reports about the role of a particular gene
in atherosclerosis. However,
in order to safely translate new
knowledge into a clinical setting, the benefits and disadvantages
of targeting specific genes must be explored.
Cell death is one of the leading causes of inflammation and
necrotic core formation in atherosclerosis (Van Vré et al., 2012).
Although apoptosis and secondary necrosis occur in a variety of
cells in atherosclerotic plaques (Van Vré et al., 2012), recent reports
propose that plaque macrophages also undergo necroptosis, a newly
identified form of programmed cell death (Lin et al., 2013; Meng
et al., 2015; Karunakaran et al., 2016; Leeper, 2016). Necroptosis
relies on the essential executioner receptor-interacting protein
kinase 3 (RIPK3) and phosphorylation of its downstream effector
mixed lineage kinase domain-like protein (MLKL), which then acts
to permeabilize the plasma membrane (Dhuriya and Sharma, 2018;
Linkermann and Green, 2014). Similar to secondary necrosis,
necroptosis culminates with a release of intracellular components
that initiate an immune response. This type of programmed death is
often associated with immune cells, and several studies show that
wild-type macrophages are susceptible to necroptosis, whereas
Ripk3−/− macrophages are protected (Karunakaran et al., 2016; Lin
et al., 2013; Meng et al., 2015). As RIPK3 is necessary for
necroptosis – and as necroptosis is considered to be inherently
inflammatory – researchers have suggested that RIPK3 or MLKL
should be targeted to decrease atherosclerosis severity in the clinical
setting (Zhe-Wei et al., 2018; Coornaert et al., 2018).
However, more recent work has revealed that RIPK3 has
pleiotropic roles beyond necroptosis (Silke et al., 2015; Moriwaki
and Chan, 2016; Vince and Silke, 2016; He and Wang, 2018;
Weinlich et al., 2016). These new mechanisms include NF-κB-
induced cytokine production and NLRP3 inflammasome-induced
or caspase 8-induced IL-1β activation, which expand the pro-
inflammatory capacity of RIPK3 activity beyond necroptosis.
Surprisingly, RIPK3 has also been reported to promote aerobic
metabolism through phosphorylation of several metabolic enzymes
(Yang et al., 2018), thus it is also possible for RIPK3 to act in a non-
inflammatory manner. Overall,
these alternative functions for
RIPK3 are often unacknowledged in disease studies.
When Ripk3 is genetically deleted in a murine model of
atherosclerosis, one report shows that atherosclerotic lesion area,
necrotic area and macrophage infiltration are decreased (Lin et al.,
2013). Another report shows that the necroptosis chemical inhibitor
necrostatin-1 improves atherosclerosis severity (Karunakaran et al.,
2016). However, these reports do not fully explore the pleiotropic
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Disease Models & Mechanisms (2020) 13, dmm041962. doi:10.1242/dmm.041962
roles of RIPK3, and instead propose that RIPK3 causes plaque
macrophages to undergo inflammatory necroptosis. Moreover, as
necrostatin-1 has many off-target effects and can inhibit apoptosis
and necroptosis-independent inflammatory pathways (Vandenabeele
et al., 2012), it is a non-ideal inhibitor for examining the specific
effects of necroptosis. Furthermore, these studies do not address the
fact that different cell types tend to use pro-inflammatory components
very differently (Mussbacher et al., 2019), and thus RIPK3 could be
playing alternative roles in each of the various cell types of the plaque.
As RIPK3 is a widely expressed protein – as reported by the
Human Protein Atlas (Uhlén et al., 2015) – there is potential for
RIPK3 to have tissue- or cell-specific functions. To explore the cell-
specific function of RIPK3 in the vasculature, and to confirm which
cell types – if any – undergo necroptosis in atherosclerosis, we
developed a conditional model of Ripk3 deletion that utilizes a
Ripk3 locus integrated with loxP sites (Colijn et al., 2019). We
conducted this study by using the Ripk3-floxed mice crossed with
macrophage-, vascular smooth muscle cell- and endothelial cell-
specific Cre recombinases on the Apoe−/− murine model of
atherosclerosis. This conditional deletion of RIPK3 aids in
understanding how cell-specific RIPK3 inhibition affects
atherosclerosis and gives insight
into the consequences of
targeting components of the necroptosis pathway in a disease
context.
We now report that RIPK3 plays a biologically relevant role in
atherosclerosis in macrophages and endothelial cells through an
athero-protective – and likely non-necroptotic – mechanism. Our
data indicate that RIPK3 plays an anti-inflammatory role in these
cell
types, possibly through the suppression of monocyte
chemoattractant protein-1 (MCP-1; also known as CCL2) in
macrophages and E-selectin (SELE) in endothelial cells. These
results provide novel information about unexpected roles for RIPK3
in an inflammatory vascular disease, and raise questions about our
previous understanding of
the relationship between RIPK3,
necroptosis, inflammation and atherosclerosis.
RESULTS
Ripk3 transcripts are present in atherosclerotic plaques at
very low copy numbers
To explore the role of RIPK3 in the various cell
types of
atherosclerosis, we first attempted to look at RIPK3 expression in
the plaque regions. Unfortunately, as is fairly common for plaque
immunostaining, all commercial antibodies that we used to detect
RIPK3 showed widespread non-specific staining, which was
confirmed by using Ripk3-knockout plaques as controls (data not
shown). As an alternative to immunostaining, we used RNA in situ
hybridization with RNAScope® technology to identify the
expression pattern of Ripk3. After confirmation of the specificity
of the Ripk3 probe (Fig. S1) and after identifying plaque areas with
endothelial cells, macrophages and smooth muscle cells, we showed
that Ripk3 transcripts were nearly undetectable in these regions
(Fig. 1A-H). In fact, Ripk3 levels were even lower than Polr2a
levels, which is a ubiquitously expressed positive control gene that
is known to produce very low transcript copy numbers per cell
(Fig. 1I-N) (Bingham et al., 2017). This very low copy number for
Ripk3 transcripts prevented dual immunostaining to identify cell
types with Ripk3 expression, as the additional steps would wash
away the probe signal; however, we were able to immunostain
sequential sections to confirm that all the pertinent cell types were
present (Fig. 1A-D). Regardless, it is apparent that Ripk3 transcript
copy number
in our
atherosclerotic plaques, and that immunostaining is not ideal for
is very low in all cell
types present
detecting RIPK3 protein in plaque tissues. However, as previous
studies have already linked RIPK3 and atherosclerosis (Lin et al.,
2013; Meng et al., 2015), we suspected that this low Ripk3 transcript
copy number did not accurately predict RIPK3 activity in the aorta.
RIPK3 deletion in macrophages or endothelial cells
exacerbates atherosclerosis
Next, we wanted to determine the biological relevance of cell-specific
RIPK3 in atherosclerosis, so we conditionally deleted Ripk3 in
macrophages (Ripk3ΔMΦ-Cre), smooth muscle cells (Ripk3ΔSMC-Cre),
endothelial cells (Ripk3ΔEC-Cre) and globally (Ripk3ΔGlobal) on the
Apoe−/− background using Cre-lox technology and LysM (Lyz2)-Cre,
SM22 (Tagln)-Cre, VE-Cadherin (Cdh5)-Cre and germline excision,
respectively. For brevity and clarity, simplified nomenclature is used
throughout the article in place of the complete genotypes. The full
genotypes, associated nomenclature, and important notes are
described in Table 1. These mice were then fed a Western diet for
three months, at which point the tissues were collected for analysis. It
should be noted as a caveat to our study that we did not obtain as
many of the Ripk3ΔGlobal mice as we did the cell-specific knockouts
owing to the difficulties associated with breeding and maintaining the
Apoe−/− lineage.
of
by
deletion
As VE-Cadherin-Cre has been reported to delete in a portion of
the adult bone marrow (Alva et al., 2006), and LysM-Cre is
occasionally inefficient (Clausen et al., 1999), we investigated the
efficiency
bone-marrow-derived
macrophages (BMDMs) and analyzing their RIPK3 expression
levels (Fig. 2A-F). LysM-Cre showed robust deletion efficiency by
transcript and protein analysis. As expected, VE-Cadherin-Cre
showed a partial deletion of RIPK3 in BMDMs as well, meaning
that we could not
ignore a potential role for Ripk3-deficient
macrophages in Ripk3ΔEC-Cre mice.
isolating
We also sought to confirm that the Ripk3-floxed allele – which
results in removal of the first nine out of the ten exons of Ripk3 after
Cre-mediated excision (Colijn et al., 2019) – does not produce a
transcribed version of exon 10. This exon encodes a functional
domain that is involved in several kinase-independent processes
(Moriwaki et al., 2017), which, if still translated, could confound
our results. However, transcript analysis using primers designed
specifically for exon 10 show that
there is no possibility for
translation of a truncated form of RIPK3 (Fig. 2G). Furthermore,
Ripk3ΔGlobal aortas
show no detectable RIPK3 protein by
immunoblotting (Fig. S2), altogether indicating that we were able
to generate a true knockout allele.
If
are
correct
reports
previous
that RIPK3
increases
atherosclerosis severity and that necroptotic macrophages are the
main source of that increase in severity, then we would expect to see
less atherosclerotic phenotypic severity in the Ripk3ΔGlobal,
Ripk3ΔHet, and Ripk3ΔMΦ-Cre mice. En face Oil Red O staining
revealed that Ripk3ΔMΦ-Cre and Ripk3ΔEC-Cre aortas showed an
increase in percent atherosclerotic lesion area, whereas Ripk3ΔHet
and Ripk3ΔGlobal aortas were no different from control, which
conflicts with the previously published genetic study addressing the
role of RIPK3 in atherosclerosis progression (Fig. 3A,B) (Lin et al.,
2013). Instead, our data suggest
that RIPK3 plays an athero-
protective role in macrophages and endothelial cells.
We also observed that the bulk of the increased plaque burden in
Ripk3ΔMΦ-Cre and Ripk3ΔEC-Cre mice was detected in the
descending and abdominal
the aorta, which are
typically athero-protected, as opposed to the athero-prone arch
region (Fig. 3C-E). In addition, we saw no significant differences in
lesion size, necrotic core size, macrophage area, smooth muscle cell
regions of
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Disease Models & Mechanisms (2020) 13, dmm041962. doi:10.1242/dmm.041962
Fig. 1. Ripk3 transcripts are present in
atherosclerotic plaques at very low copy
numbers. (A-D) Sequential cross sections of
control aortic roots were immunostained for the
endothelial cell marker CD31 (green) and
macrophage marker CD68 (red) (A,C) or for the
smooth muscle cell marker aSMA (red) (B,D) and
were co-stained to identify nuclei (Hoechst; blue).
Two plaque regions that contain all three cell types
are shown. (E-N) RNAScope® RNA in situ
hybridization was performed on sequential
sections of the two separate regions of control
aortic roots shown in A-D. Ripk3 probe was used to
identify Ripk3 transcripts ( pink) and co-stained
with DAPI (blue) to identify nuclei (E,G). F and H
show magnifications of the boxed regions (without
DAPI) in E and G, respectively. Positive control
probes Ubc ( pink; high transcript copy number)
and Polr2a (red; low transcript copy number) were
used to show the efficacy of the assay (I,L). J,K and
M,N show magnifications of the boxed regions
(without DAPI) in I and L, respectively. Positive
signal is determined by the presence of ‘dots’
which are each meant to represent a single
transcript. Images are representative of in situ
hybridization experiments performed on sections
from three separate control mice (n=3). Scale bars:
25 µm.
area, collagen area or calcification in the athero-prone aortic roots
within the arch region (Fig. 4A-R and Fig. S3). We also detected no
increase in apoptosis in the aortic root, though apoptotic cells were
infrequent enough that quantification could not be performed (data
not shown).
Interestingly, western blot analysis of the different aortic
regions (arch, descending and abdominal; as demarcated in
Fig. 3C) showed a significant increase in CD11b signal in the
arch region of Ripk3ΔEC-Cre aortas (Fig. 4S,T). As CD11b is a
in
assists
that
monocyte/macrophage
leukocyte trafficking (Schittenhelm et al., 2017),
these data
suggest that there is an increase in macrophage number in the arch
receptor component
region of Ripk3ΔEC-Cre aortas that is not reflected in the anti-
CD68 immunostained aortic roots (Fig. 4R) or en face analyses
(Fig. 3E).
Triglyceride, cholesterol, glucose, and blood cell counts are
unchanged between the genotypes
To confirm that the changes in Ripk3ΔMΦ-Cre and Ripk3ΔEC-Cre mice
were not due to a change in overall metabolism or blood content, we
analyzed plasma triglyceride, cholesterol and glucose levels and
found no difference between the genotypes (Fig. S4). We also found
no difference in peripheral mononuclear cells and other blood cells
(Fig. S5).
Table 1. Genotypes, nomenclature, Cre-specificity and other important notes
Genotype
Nomenclature
Cre specificity
Notes
Apoe−/−;Ripk3fl/fl
Apoe−/−;Ripk3fl/Δ
Apoe−/−;Ripk3Δ/Δ
Apoe−/−;Ripk3fl/fl;LysM-Cre+
Apoe−/−;Ripk3fl/fl;SM22-Cre+
Apoe−/−;Ripk3fl/fl;VE-Cadherin-Cre+
*Ripk3ΔHet and Ripk3ΔGlobal mice were generated by utilizing the germline excision phenomenon that occurs when Cre activity aberrantly turns on in the gonads of
the breeders (Harno et al., 2013), thereby altering the Ripk3-floxed allele into a Ripk3-knockout allele.
–
–
–
Macrophages and neutrophils
Vascular smooth muscle cells
Endothelial cells and a subset of hematopoietic cells
Cre-negative littermate controls
*Global heterozygous knockout of Ripk3
*Global homozygous knockout of Ripk3
Clausen et al., 1999
Holtwick et al., 2002
Alva et al., 2006
Control
Ripk3ΔHet
Ripk3ΔGlobal
Ripk3ΔMΦ-Cre
Ripk3ΔSMC-Cre
Ripk3ΔEC-Cre
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Disease Models & Mechanisms (2020) 13, dmm041962. doi:10.1242/dmm.041962
Fig. 2. Bone-marrow-derived macrophages
exhibit significant reduction in RIPK3 levels in
Ripk3ΔGlobal, Ripk3ΔMΦ-Cre and Ripk3ΔEC-Cre
mice. (A,B) BMDMs were isolated, differentiated on
chamber slides for 7 days, immunostained for
macrophage markers CD68 (red; A) and CD11b
( pink; B), and co-stained for nuclei (Hoechst; blue).
All cells from seven separate BMDM isolations
were positive for these markers (n=7). (C) A
phagocytosis assay was performed on BMDMs
with fluorescent polystyrene beads. Phagocytic
cells display TRITC+/Hoechst+ signal, and 85% of
cells from two separate BMDM isolations were
double positive (n=2). (D-F) Protein or RNA was
collected from control, Ripk3ΔGlobal, Ripk3ΔMΦ-Cre
and Ripk3ΔEC-Cre BMDMs. RNA was converted to
cDNA and analyzed by qPCR for Ripk3 levels (D).
Protein lysates were immunoblotted to identify
CD11b, RIPK3 and β-actin (loading control) (E) and
quantified (F). (G) RNA from control and
Ripk3ΔGlobal BMDMs was converted to cDNA and
analyzed by qPCR for Ripk3-Exon 10 levels. For
panels D,F,G, each dot represents a BMDM
isolation from an individual animal. Statistics for
panels D and F were calculated using one-way
ANOVA with Dunnett’s multiple comparisons test.
Overall ANOVA P-values ( prior to the post hoc
tests) are 0.0002 (D) and <0.0001 (F). Statistics for
panel G were calculated using an unpaired t-test
with Welch’s correction. *P<0.05, **P<0.01,
***P<0.001, ****P<0.0001. Data are mean±s.d.
Scale bars: 25 µm.
The main role of RIPK3 in atherosclerosis is likely not to
initiate necroptosis
Owing to the unexpected exacerbation of atherosclerosis in
Ripk3ΔMΦ-Cre and Ripk3ΔEC-Cre mice, we questioned whether
necroptosis – which is considered to be inherently inflammatory and
should increase atherosclerosis severity – was detectable in our
atherosclerotic aortas. Because of widespread non-specific staining
that occurred with the commercial antibodies that we used to
immunostain
phosphorylated MLKL ( p-MLKL), we
alternatively used western blot techniques to detect this marker of
necroptosis. We found that p-MLKL levels were so low as to be mostly
undetectable by western blotting using two different anti-p-MLKL
antibodies (Fig. 5A-C and Fig. S6). Thus, we suspect that the main role
of RIPK3 in atherosclerosis is not to cause macrophage necroptosis,
but rather to prevent macrophages and endothelial cells from becoming
pro-inflammatory.
for
Furthermore, we found that RIPK3 protein levels in different
aortic regions and genotypes were not significantly different from
control levels by western blot (Fig. 5D,E). If macrophages, smooth
muscle cells or endothelial cells predominantly expressed RIPK3
over the other cell types, then we would have expected to see a
decrease in RIPK3 expression in the corresponding mutant
genotype. As we did not, this suggests that the bulk of RIPK3
expression detected by western blotting in the aorta is not restricted
to any one of these three cell types.
Ripk3 deficiency impacts MCP-1 and IL-1β expression in
BMDMs, and MCP-1 and E-selectin expression in cultured
endothelial cells
To try to understand how Ripk3 deletion in macrophages could lead
to an increase in atherosclerosis severity, we isolated and cultured
BMDMs from control and Ripk3ΔMΦ-Cre bone marrow and
performed real-time quantitative PCR (qPCR) for a panel of genes
that are related to necroptosis, inflammation, macrophage activation
and endothelial cell activation (Fig. 6A and Fig. S7A). We found
that Ccl2 (MCP-1) and Il1b (IL-1β) transcripts were significantly
changed in Ripk3ΔMΦ-Cre BMDMs. Ccl2 was upregulated almost
12-fold in Ripk3ΔMΦ-Cre BMDMs over control BMDMs, and
ELISA analysis of the medium confirmed the increase in MCP-1
and decrease in IL-1β (Fig. 6B,C). RIPK3 has already been
implicated in IL-1β processing (Weinlich et al., 2016) and has been
shown to promote Il1b transcription (Moriwaki et al., 2017), but this
is the first report implicating RIPK3 in the suppression of Ccl2
expression.
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Fig. 3. Ripk3ΔMΦ-Cre and Ripk3ΔEC-Cre en face aortas
exhibit increased lesion areas in the descending and
abdominal aortic regions. (A) Representative images of
control and Ripk3-deficient aortas from male and female
mice that were fed the Western diet for 3 months. Aortas
were then dissected, cut open en face and stained with ORO
to visualize lesions. (B) Lesion area was quantified as the
percent lesion area of the whole aortic area. (C) Aortic areas
were analyzed separately and divided into the arch,
descending and abdominal regions. The arch region
extends from where the aorta enters the heart to the end of
the curvature. The descending region extends to the renal
arteries. The abdominal region extends to the iliac arteries.
(D,E) Lesion area was quantified for the descending and
abdominal regions (D) and arch region (E). For panels B,D,
E, each dot represents an aorta from an individual animal.
Statistics were calculated using one-way ANOVA and
Dunnett’s multiple comparisons test for panels B and
D. Overall ANOVA P-values ( prior to the post hoc tests) are
0.005 (B), 0.001 (D) and 0.33 (E). Data are mean±s.d.
To try to understand how Ripk3 deletion in endothelial cells could
lead to an increase in atherosclerosis severity, we utilized a cultured
murine pancreatic endothelial cell line (MS1 cell line), which we
chose for this study because it expresses high levels of endogenous
RIPK3. By knocking down RIPK3 using siRNA oligos and looking
at a similar panel of genes, we found that Ccl2 transcripts and
MCP-1 protein levels were also elevated in endothelial cells,
to the extent seen in BMDMs (Fig. 6D-F and
although not
Fig. S7B). Furthermore, Sele
transcripts were
(E-selectin)
upregulated approximately fourfold in RIPK3-knockdown MS1
cells. This is relevant as E-selectin is a glycoprotein surface receptor
on endothelial cells that assists in the recruitment of circulating
leukocytes (McEver, 2015).
Based on these data, we hypothesized that increased macrophage
MCP-1 levels contributed to the more severe atherosclerosis we
detected in Ripk3ΔMΦ-Cre mice, as macrophage-specific expression
of MCP-1 is known to exacerbate atherosclerosis (Aiello et al.,
1999). We also hypothesized that increased endothelial MCP-1 and
E-selectin levels contributed to the elevated atherosclerosis severity
in Ripk3ΔEC-Cre mice, as these molecules would increase the
recruitment of leukocytes and therefore accelerate atherosclerosis.
MCP-1 levels are elevated in Ripk3ΔMΦ-Cre abdominal aortas,
and E-selectin levels trend higher in Ripk3ΔEC-Cre aortas
To see whether the BMDM and MS1 cell functions of RIPK3
translated to our
in vivo tissues, we analyzed MCP-1 and
E-selectin levels in the arch, descending and abdominal regions
of mouse aortas using western blotting. Ripk3ΔMΦ-Cre aortas
exhibited an increase in MCP-1 in the abdominal region that was
if variable, compared to controls (Fig. 7A,B). This
robust,
supports the hypothesis that
loss of RIPK3 in macrophages
increases macrophage MCP-1 levels in the abdominal region of
Ripk3ΔMΦ-Cre aortas, which correlates with the increase in abdominal
lesion area (Fig. 3D).
In contrast, Ripk3ΔEC-Cre aortas did not show an increase in
MCP-1 but showed an upward trend in E-selectin levels by western
blot (Fig. 7C,D). We immunostained regions of the descending aorta
to see whether the increase in E-selectin would be more apparent using
another technique; however, we did not see an increase in E-selectin
intensity (Fig. S8A,B), though this could be attributed to the fact that
the E-selectin signal was already very high in control aortas and thus
it was difficult to see a change in intensity. We also examined
ICAM1 and VCAM1 levels because of their high expression in
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Fig. 4. Aortic root analyses reveal no differences in lesion area, necrotic area or macrophage area, though Ripk3ΔEC-Cre aortas exhibit higher CD11b
signal. (A-R) After 3 months on a Western diet, hearts were dissected and aortic roots were sectioned and analyzed for lesion area, necrotic area and
macrophage area. Aortic roots were stained with ORO and hematoxylin to visualize lesion area (black arrows) (A-E). Lesion area was reported as a fraction of the
total aortic area (P). Aortic roots were stained with H&E to visualize necrotic areas (F-J). Necrotic areas were defined as acellular and are outlined in black.
Necrotic area was reported as a percent of the lesion area (Q). Aortic roots were immunostained for CD68 (red) and nuclei (Hoechst; blue) to visualize
macrophage-occupied area (K-O). Macrophage area was reported as the CD68+ percent of the lesion area (R). (S,T) Protein was collected from control (n=8),
Ripk3ΔMΦ-Cre (n=5) and Ripk3ΔEC-Cre (n=4) aortas. Protein lysates were immunoblotted to identify CD11b and β-actin (loading control) (S) and quantified (T). For
panels P,Q,R,T, each dot represents an individual animal. Statistics for panels P-R were calculated using one-way ANOVA. Overall ANOVA P-values ( prior to the
post hoc tests) are 0.42 (P), 0.01 (Q) and 0.30 (R). Despite the significant overall ANOVA P-value for panel Q, Dunnett’s multiple comparisons test shows no
significant difference from control aortic roots. Statistics for panel T were calculated using two-way ANOVA with Dunnett’s multiple comparisons test with an overall
ANOVA P-value of 0.01. Data are mean±s.d. Scale bars: 200 µm.
athero-prone regions and their connection to inflammation
(Nakashima et al., 1998). However, neither gene was altered in
Ripk3-deficient BMDMs or MS1 cells (Fig. S7); nor were ICAM1
in Ripk3ΔEC-Cre or
and VCAM1 levels significantly different
Ripk3ΔMΦ-Cre aortas (Fig. S8C-E).
In addition, as RIPK1 is a homologous kinase upstream of
RIPK3 and is often tied to RIPK3 function (Moriwaki and Chan,
2016), we immunoblotted for RIPK1 in the various regions of the
aorta. When Ripk3 is deleted in a cell-specific manner, RIPK1
levels are not noticeably altered in the aorta lysate (Fig. S9A).
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Fig. 5. p-MLKL levels are nearly
undetectable in advanced plaques.
(A-C) After 3 months on a Western diet,
protein was collected from control (n=7),
Ripk3ΔMΦ-Cre (n=5), Ripk3ΔEC-Cre (n=3)
and Ripk3ΔSMC-Cre (n=3) aortas. Protein
lysates were immunoblotted to identify
p-MLKL (Abcam; #ab196436), MLKL and
β-actin (loading control) (A) and quantified
(B,C). A faint positive p-MLKL signal can
be seen in the representative blot in the
control arch region; however, we could only
detect p-MLKL in two out of the 18 aortas
analyzed (B). Note that the same transfer
membrane used for detecting CD11b (in
Fig. 4S) was reprobed for p-MLKL and
MLKL in A; the β-actin control blots are
therefore the same in both figures.
(D,E) Protein lysates were immunoblotted
to identify RIPK3 and GAPDH (loading
control) (D) and quantified (E). For panels
B,C,E, each dot represents an individual
animal. Statistics were calculated using
two-way ANOVA. Overall ANOVA P-values
are 0.76 (B), 0.07 (C) and 0.46 (E). Data
are mean±s.d.
However, aortas with heterozygous and global deletion of Ripk3
show an appreciable decrease in RIPK1 levels (Fig. S9B),
indicating that RIPK1 protein levels are tied to RIPK3 levels.
However, owing to the fact that RIPK1 plays roles in regulating
necroptosis, apoptosis, autophagy, inflammation and cell survival
pathways (Lin, 2014), it is difficult to speculate how the substantial
decrease in RIPK1 affects atherosclerosis in Ripk3-deficient
animals.
Plasma IL-1β levels are increased in Ripk3ΔGlobal mice,
whereas plasma MCP-1 levels are unaffected by Ripk3
deletion
To determine whether the in vitro changes we detected in MCP-1 or
IL-1β levels could be seen in the plasma of our mutant mice, we
performed an ELISA assay on the plasma samples collected from
the different genotypes. However, we detected no differences in
MCP-1 levels (Fig. 8A). Although Ripk3ΔMΦ-Cre plasma did not
show a decrease in IL-1β levels as would have been expected from
the BMDM data, we did see a significant increase of IL-1β in the
Ripk3ΔGlobal plasma (Fig. 8B). This suggests that, although RIPK3
has been reported to positively regulate IL-1β processing (Weinlich
et al., 2016), it may also play a suppressive role in certain conditions
or cell types.
DISCUSSION
Until now, RIPK3 has been associated primarily with necroptosis
and – to a lesser extent – other pro-inflammatory pathways separable
from necroptosis. In this study, which is the first to explore the cell-
specific function of RIPK3 in the atherosclerotic aorta, we
demonstrate that RIPK3 plays an unexpected athero-protective
role in macrophages and endothelial cells. Here, we propose that the
main role of RIPK3 in atherosclerosis is neither to promote
IL-1β processing, which are the previously
necroptosis nor
described functions for RIPK3 (Weinlich et al., 2016). Instead,
our data indicate that RIPK3 may play an anti-inflammatory role by
suppressing MCP-1 expression in macrophages and E-selectin
expression in endothelial cells (data summarized in Fig. S10). These
results provide novel information about RIPK3 in an inflammatory
vascular disease and raise questions about the efficacy and safety of
targeting it in a clinical setting.
We were surprised by the fact that our mice with global and
heterozygous Ripk3 deletions did not resemble previously reported
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Fig. 6. Ripk3-deficiency impacts MCP-1 and IL-1β expression in BMDMs, and MCP-1 and E-selectin expression in cultured endothelial cells.
(A-C) BMDMs were isolated from control (n=6) and Ripk3ΔMΦ-Cre (n=4) bone marrow, and RNA and medium were collected 7 days later. RNA was converted to
cDNA and analyzed by qPCR (A). ELISA assays for MCP-1 (B) and IL-1β (C) were performed on the BMDM medium. Each dot (n value) represents a BMDM
isolation from an individual animal. (D-F) MS1 endothelial cells were transfected with NS- and RIPK3-siRNA oligos for 24 h and were cultured in low-serum
medium for another 24 h before RNA, medium and protein were collected (n=4 independent experiments). RNA was converted to cDNA and analyzed by qPCR
(D). Protein lysates were immunoblotted for RIPK3 and the loading control, GAPDH (n=4 independent experiments) (E). An ELISA assay for MCP-1 was
performed on the BMDM medium (n=3 independent experiments) (F). Statistics were calculated using unpaired t-tests, with Welch’s correction when necessary.
*P<0.05, **P<0.01. Data are mean±s.d.
Ripk3 mutant mice that showed a dose dependent improvement in
atherosclerotic lesion area (Lin et al., 2013). It is possible that this
inconsistency may be due to different background strains in the mice
that were analyzed. The Ripk3−/− mice used in the original study
were derived from C57BL/6N embryonic stem cells (Newton et al.,
2004), whereas our Ripk3fl/fl mice were derived from C57BL/6J
embryonic stem cells (Colijn et al., 2019). Lin et al. reported that
they performed their study on a C57BL/6J background; however, it
is unclear for how many generations the original C57BL/6N strain
was crossed onto the C57BL/6J strain. Although this distinction
may appear to be minor, much work has been done to map the
genetic and metabolic differences between the two backgrounds,
and a difference of phenotype is entirely possible (Fontaine and
Davis, 2016). Thus, in addition to revealing cell-specific roles for
RIPK3, we may also have uncovered a background-specific
regulation or function of RIPK3 that future studies should consider.
Another potential cause of the discordant results from our genetic
study and that of Lin et al. is the different environments in which the
mice were housed and analyzed. The two studies were performed at
different institutions and with different suppliers of the Western diet
(Lin et al., 2013). This raises questions about the contribution of
microbiota to RIPK3-dependent functions within the context of
atherosclerosis. It has already been well established that
the
microbiome can influence atherosclerosis (Jie et al., 2017), thus
microbiota that differentially affect inflammatory pathways could
also differentially affect RIPK3 activation. As humans have such
diverse and dissimilar microbiota, the effect of the microbiome on
RIPK3 function should be explored before RIPK3 is considered as a
therapeutic target.
It is also possible that differences between the Ripk3−/− genetic
model used by Lin et al. and our Ripk3fl/fl genetic model could
contribute to the discrepancies between our studies. Specifically,
whereas our Ripk3fl/fl mouse model results in removal of exons one
through nine of Ripk3 upon Cre-mediated recombination, only the
first three exons of Ripk3 are targeted for deletion in the Ripk3−/−
mouse model (Colijn et al., 2019; Newton et al., 2004). Ripk3 has
been reported to have two alternative splicing variants in addition to
the full length form (Yang et al., 2005), and although part of the
alternative spliced sequences include the first three exons and
therefore may not be transcribed in the Ripk3−/− mouse, this was not
addressed in the design of the Ripk3 knockout locus. Though
unlikely, it is possible that a truncated or frame-shifted form of
RIPK3 was present in the mice used by Lin et al. that could account
for the difference between our results.
Finally, it is worth noting that another study that looked at
atherosclerosis in an Apoe−/−;Ripk3−/− mouse model did not
completely replicate the study by Lin et al., although it did conclude
that RIPK3-mediated necroptosis contributes to atherosclerosis
pathology (Meng et al., 2015). The authors reported no difference in
macrophage infiltration and did not observe a significant difference
in aortic root lesion area in very advanced plaques, which is contrary
to the study by Lin et al. Though Meng et al. did not bring attention
to these differences, it is clear that there is some variation in RIPK3
atherosclerosis studies that should be considered.
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Fig. 7. MCP-1 levels are elevated in Ripk3ΔMΦ-Cre
abdominal aortas, and E-selectin levels trend
higher in Ripk3ΔEC-Cre aortas. (A-E) After 3 months
on a Western diet, protein was collected from control
(n=8), Ripk3ΔMΦ-Cre (n=5) and Ripk3ΔEC-Cre (n=4)
aortas. Protein lysates were immunoblotted to identify
MCP-1, E-selectin, GAPDH and β-actin (loading
controls) (A,C) and quantified (B,D,E). The
immunoblot in panel C shows non-contiguous lanes
of a single gel. For panels B,D,E, each dot represents
an individual animal. Statistics were calculated using
two-way ANOVA, and Sidak’s multiple comparisons
test in panel B. Overall ANOVA P-values ( prior to the
post hoc tests) are 0.09 (B), 0.02 (D) and 0.99 (E).
Data are mean±s.d.
despite
notable
Surprisingly,
atherosclerotic
detecting
phenotypes associated with Ripk3 deficiency, we were unable to
detect much Ripk3 transcript expression in atherosclerotic plaques.
Although the commercial RIPK3 antibodies we used were
unsuitable for assessing patterns of RIPK3 expression in plaque
tissues by immunostaining, we were able to determine by
immunoblotting that neither macrophages, smooth muscle cells,
nor endothelial cells are the main sources of RIPK3 expression in
plaques, and that RIPK3 protein expression is not restricted to a
particular region of the aorta. Nevertheless, the limitations in RIPK3
immunostaining prevented us from assessing Cre specificities and
efficiencies directly in plaque tissues, which would have been ideal.
As plaque tissue is difficult to immunostain owing to high levels of
non-specific background signal, we propose that the best way to
Fig. 8. Plasma IL-1β levels are increased in
Ripk3ΔGlobal mice, whereas plasma MCP-1
levels are unaffected by Ripk3 deletion.
(A,B) After mice were fed a Western diet for
3 months, plasma was collected and analyzed
by ELISA for MCP-1 (A) and IL-1β (B). Each dot
represents an individual animal. Statistics for
both panels were calculated using Kruskal–
Wallis tests, and Dunn’s multiple comparisons
test for panel B. Overall ANOVA P-values ( prior
to the post hoc tests) are 0.97 (A) and 0.01 (B).
Data are mean±s.d.
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determine RIPK3 protein expression patterns accurately in the
context of atherosclerosis would be to use a RIPK3-tagged reporter
mouse, such as the RIPK3-GFP mouse developed by Moriwaki
et al. (2017).
A major finding from our study is that RIPK3 plays unexpected
anti-inflammatory roles in atherosclerosis and contributes to the
athero-protection of the descending and abdominal aortic regions.
However, our study is not the first to indicate that RIPK3 activity
can lead to the suppression of
inflammation. One report
demonstrates that promoting RIPK3 activation in cultured mouse
fibroblasts – through TNF-treatment and caspase inhibition – results
in a marked decrease in secretion of inflammatory cytokines
(Kearney et al., 2015). Our findings that IL-1β is elevated in plasma
from Ripk3ΔGlobal mice (Fig. 8B) and that MCP-1 is upregulated in
the abdominal aortic region of Ripk3ΔMΦ-Cre mice (Fig. 7B) provide
in vivo evidence of anti-inflammatory roles for RIPK3. In addition,
the upward trends in E-selectin (Fig. 7D) and in CD11b (Fig. 4T)
expression in Ripk3ΔEC-Cre aortas provide further indications that
RIPK3 activity suppresses inflammation in a cell-type specific
manner during atherosclerosis. Intriguingly, the marked elevation in
pro-inflammatory IL-1β levels from Ripk3ΔGlobal plasma did not
track with an increase in plaque severity. In fact, aortic plaques were
less severe in our Ripk3ΔGlobal mice than in our Ripk3ΔEC-Cre and
Ripk3ΔMΦ-Cre animals. Ultimately, we do not know the reason for
the phenotypic differences between our mice with global and cell-
specific Ripk3 deletion, but our findings indicate that RIPK3 may
play opposing roles in different interacting cell types and that global
deletion may negate the damaging effects of cell-specific RIPK3
deletion in the context of atherosclerosis.
suppresses
One important question that arises from our findings is whether
RIPK3-mediated necroptosis
inflammation during
atherosclerosis progression, as has been suggested for the cultured
mouse fibroblast study cited above (Kearney et al., 2015). It has been
proposed that Mlkl deletion is a more definitive genetic approach than
Ripk3 deletion for determining how necroptosis influences various
pathologies, as RIPK3 has roles outside of necroptosis and MLKL is
downstream of RIPK3 in the necroptosis pathway (Newton et al.,
2016). As one published abstract hints that Mlkl-deficiency does not
improve atherosclerosis (Rasheed et al., 2018), and as we were unable
to detect p-MLKL in the atherosclerotic plaques we analyzed
(Fig. 5A,B and Fig. S6), we propose that necroptosis contributes
minimally to atherosclerosis progression and to the anti-inflammatory
roles we have defined for RIPK3 in this study.
Altogether, we believe this study challenges the field to
reevaluate the prevalent idea that RIPK3 promotes pathologies
exclusively through necroptotic or other pro-inflammatory
mechanisms. Our data indicate that RIPK3 has cell-specific
functions and that some of those may be beneficial and anti-
inflammatory in the context of the vasculature. Exploring other
protective roles for RIPK3 will help clarify the potential risks and
benefits of targeting RIPK3 therapeutically in various diseases.
MATERIALS AND METHODS
Mice (Mus musculus)
Apoe−/− mice on the C57BL/6J background (Piedrahita et al., 1992), SM22-
Cre transgenic mice (Holtwick et al., 2002), LysM-Cre transgenic mice
(Clausen et al., 1999), VE-Cadherin-Cre transgenic mice (Alva et al., 2006)
and Ripk3-floxed (Ripk3fl/fl) mice on the C57BL/6J background (Colijn
et al., 2019) have been described. Ripk3-knockout (Ripk3Δ/Δ) mice were
generated by utilizing the germ-line excision phenomenon that occurs when
Cre activity aberrantly turns on in the gonads of the breeders (Harno et al.,
2013), thereby altering the Ripk3-floxed allele into a Ripk3-knockout allele.
Mice were maintained and interbred on the C57BL/6J background at the
Oklahoma Medical Research Foundation (OMRF) animal facility. Male and
female breeders were used interchangeably for many generations to ensure
all target genotypes were on a highly uniform background strain for the
analyses. The OMRF Institutional Animal Care and Use Committee
approved all animal use protocols.
Genotyping
Apoe−/−, SM22-Cre, LysM-Cre, VE-Cadherin-Cre and Ripk3-floxed
mice were genotyped as previously described (Colijn et al., 2019;
Holtwick et al., 2002; Goren et al., 2009; Mani et al., 2013; Wiley et al.,
2015). Ripk3-knockout genotyping was performed by PCR using the
forward primer 5′-CCATCCTCCCTTCATCAAAA-3′ and reverse primer
5′-GAATGCAAATGCAGGGTCTT-3′, which are located upstream of the
5′ LoxP site and downstream of the 3′ LoxP site, respectively. The PCR
produced a 312-bp band to signify that Ripk3 excision had occurred.
Atherosclerosis induction
Apoe−/− mice were crossed with the Ripk3fl/fl line and either SM22-Cre,
LysM-Cre or VE-Cadherin-Cre mice to generate the target genotypes:
Apoe−/−;Ripk3fl/fl;SM22-Cre (n=18), Apoe−/−;Ripk3fl/fl;LysM-Cre (n=19),
Apoe−/−;Ripk3fl/fl;VE-Cadherin-Cre
(n=9),
Apoe−/−;Ripk3Δ/Δ (n=9) and Apoe−/−;Ripk3fl/fl Cre-negative littermates as
controls (n=36). Two-month-old male and female mice were fed a Western
diet (21.2% fat, 0.2% cholesterol; TD.88137, Envigo) for three months to
induce atherosclerosis progression. The mice were then euthanized. A
cardiac puncture was performed to collect blood. Mice were then perfused
with PBS followed by 4% paraformaldehyde (PFA). Aortas were cleaned of
fat and removed along with the hearts. Bone marrow was collected from the
femur and tibia as described (Amend et al., 2016).
(n=14), Apoe−/−;Ripk3fl/Δ
En face analysis
The aorta was cut open longitudinally from the iliac arteries to the aortic root
and pinned open on parafilm. After further fixation with 4% PFA, lesions
were visualized with an Oil Red O stain (ORO, Newcomer Supply), and
residual fat was removed. Individual high-resolution images were stitched
together by hand to create the entire en face aorta images. Aortic images
were further analyzed with NIS-Elements software for ORO staining, and
data are reported as the percentage of the aortic surface covered by lesions.
Aortic root analysis
Hearts were fixed in 1% PFA overnight, placed in 20% sucrose, then
incubated in a 1:1 mixture of 20% sucrose and Optimal Cutting Temperature
compound (OCT; Sakura Finetek) overnight and frozen in OCT the next
day. Whole aortic roots were sectioned at 10 µm with a Microm HM 505 E
cryotome (Microm International) and adhered to Denville UltraClear
Microscope Slides (Denville Scientific). Slides were frozen until further use.
All analyses were performed using NIS-Elements software.
Lesion area
Aortic roots were stained with ORO to identify lesion area. Slides were first
immersed in water, then 60% isopropanol for 30 s, ORO for 30 min, then
60% isopropanol for 30 s to rinse. Slides were co-stained with hematoxylin,
mounted with 1,4-diazabicyclo[2.2.2]octane (DABCO) and coverslipped.
Six aortic root sections per mouse were analyzed at 60 μm apart. The
average lesion area from each mouse was normalized to the average total
aortic area and reported as a fraction.
Necrotic area
Aortic roots were stained with hematoxylin and eosin (H&E) for necrotic
core quantification. Three aortic root sections per mouse were analyzed at
120 μm apart. Necrotic cores were identified as acellular areas (negative for
H&E). The average necrotic area was reported as the percent necrotic area of
the total lesion area.
Macrophage and smooth muscle cell area
Macrophages and smooth muscle cells of the aortic root were visualized
using rat anti-CD68 (1:250; #MCA1957; Bio-Rad) and Cy3-conjugated
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anti-aSMA (1:250; #C6198; Sigma-Aldrich) antibodies,
respectively.
Sections were blocked with 5% bovine serum albumin (BSA) for 2 h,
incubated with primary antibody overnight, and incubated with secondary
antibody Cy3 donkey anti-rat IgG (1:500; Jackson ImmunoResearch) for
CD68 and Hoechst for nuclei (20 µg/ml) for 1 h. For macrophages, three
aortic root sections per mouse were analyzed at 120 μm apart. For smooth
muscle cells, one aortic root section per mouse was analyzed from the
middle of the root. The average CD68+ area or aSMA+ area was reported as
the percent area of the total lesion area.
Collagen deposition
Aortic roots were stained with the Picrosirius Red Stain Kit (Polysciences)
for collagen area quantification. Sections were stained with Solution A for
2 min, Solution B for 1 h and Solution C for 2 min. Two aortic root sections
per mouse were analyzed at 180 μm apart. Collagen was identified as the
green, yellow and red colors that can be visualized under polarized light. The
average collagen area was reported as the percent collagen area of the total
lesion area.
Calcification
Aortic roots were stained with Alizarin Red S (Sigma-Aldrich) to detect
calcification. Sections were stained with a 1% Alizarin Red S ( pH 4.2)
solution for 5 min. Two aortic root sections were analyzed at 180 μm apart.
Calcification was recorded as either present or absent.
Plasma triglyceride, cholesterol and glucose analysis
After blood was drawn by cardiac puncture, plasma was isolated using
Microvette CB 300 LH tubes (Sarstedt). The concentrations of total
cholesterol, LDL/VLDL cholesterol, HDL cholesterol and triglycerides
were determined using enzymatic colorimetric assays (#E2HL-100 and
#ETGA-200; BioAssay Systems) as per the manufacturer’s instructions.
Glucose levels were detected using the Contour®Next EZ Blood Glucose
Monitoring System with Contour®Next test strips.
Complete blood count
Blood was collected into Microvette 500 K3E tubes (Sarstedt). Complete
blood counts were measured with a Hemavet 950 veterinary hematology
analyzer (Drew Scientific).
RNA in situ hybridization
Hearts were fixed in 4% PFA for 24 h and passed through a sucrose
gradient as per RNAScope® protocol, then embedded in OCT. After 10 μm
aortic root sections were adhered to slides coated with Poly-L-Lysine
(#P4707; Sigma-Aldrich), slides were then frozen until use. RNA in situ
hybridization was performed using the RNAScope® Fluorescent
Multiplex Reagent Kit (#320850; Advanced Cell Diagnostics). RNA
retrieval was performed first by boiling the slides for 6 min in the Target
Retrieval Buffer (#322000; Advanced Cell Diagnostics) and then 1 h with
Protease III at 40°C. RNAScope® probe hybridization protocol was
followed for the Ripk3 probe (#462541-C3; Advanced Cell Diagnostics).
Positive control probes for Ubc and Polr2a (#320881; Advanced Cell
Diagnostics) were used for each sample. After mounting with Prolong
Gold (Thermo Fisher Scientific), images were obtained with a Nikon
Eclipse Ti-E microscope.
Immunofluorescence in tissue sections
Hearts were fixed in 1% PFA overnight, placed in 20% sucrose, then
incubated in a 1:1 mixture of 20% sucrose and OCT overnight and frozen in
OCT the next day. Sections were cut at 10 µm and frozen until use. Sections
were permeabilized in 0.1% Triton X-100 in PBS for 15 min then blocked in
5% BSA for 2 h at room temperature. Sections were incubated in primary
antibody in 1% BSA overnight at 4°C, washed three times quickly in ice-
cold 1% BSA, then incubated for 1 h at room temperature with secondary
antibody in 1% BSA with Hoechst (20 µg/ml). Sections were quickly
washed three times with cold 1% BSA and coverslipped with DABCO.
Images were obtained using a Nikon Eclipse Ti-E microscope with NIS-
Elements software. Primary antibodies used for immunofluorescence were:
goat anti-PECAM-1 (1:100; #AF3628; R&D Systems), rat anti-CD68
(1:250; #MCA1957; Bio-Rad), Cy3-conjugated anti-aSMA (1:250;
#C6198; Sigma-Aldrich) and chicken anti-E-selectin (1:100; #AF575;
R&D Systems). Secondary antibodies used were: Cy3 donkey anti-rat IgG
(#712-165-153), FITC donkey anti-goat IgG (#705-095-003) and Alexa 594
donkey anti-chicken IgY (#703-585-155). All secondary antibodies were
acquired from Jackson ImmunoResearch and used at a 1:500 dilution.
Isolation and differentiation of BMDMs
BMDMs were isolated from tibias and femurs of Apoe−/−;Ripk3fl/fl, Apoe−/−;
Ripk3fl/fl;LysM-Cre, Apoe−/−;Ripk3fl/fl;VE-Cadherin-Cre or Apoe−/−;Ripk3Δ/Δ
mice and differentiated into macrophages using DMEM (#12-604F; Lonza)
supplemented with 10% fetal bovine serum (FBS; HyClone), 1× antibiotic-
antimycotic (#15240-062; Gibco), 2 mM L-glutamine (#95057-448;
HiMedia), 1 mM sodium pyruvate (#25-000-Cl; Mediatech), 1× MEM
non-essential amino acids (#11140-050; Gibco) and rhM-CSF (20 ng/ml;
#78057; Stemcell Technologies) for 7 days. Differentiation was confirmed
by a phagocytosis assay and by immunocytochemistry for the macrophage
markers CD11b and CD68. For the phagocytosis assay, BMDMs were
treated with FluoSpheres polystyrene microspheres (#F13082; Thermo
Fisher Scientific) for 4 h, co-stained with Hoechst (10 µg/ml), washed,
fixed and then visualized on a Nikon Eclipse Ti-E microscope. Phagocytic
cells were identified as TRITC+ and quantified.
Immunocytochemistry
Bone marrow was plated on chamber slides (Lab-Tek) and differentiated
into BMDMs as described above. On day 7, slides were fixed with 4% PFA
for 10 min, permeabilized with 0.5% saponin for 10 min, blocked [1% BSA,
22.52 mg/ml glycine in PBS with 0.1% Tween 20 (PBST)] for 1 h and
incubated in primary antibody diluted in 1% BSA in PBST overnight at 4°C.
After washing with PBS, slides were incubated in secondary antibody with
Hoechst (20 µg/ml) in 1% BSA in PBST for 1 h. After mounting with
DABCO, images were obtained with a Nikon Eclipse Ti-E microscope.
Primary antibodies used for immunocytochemistry were: rabbit anti-CD11b
(1:250; #EPR1344; Abcam) and rat anti-CD68 (1:250; #MCA1957;
BioRad). Secondary antibodies used were acquired from Jackson
ImmunoResearch and used at a 1:500 dilution: Cy3 donkey anti-rat IgG
(#712-165-153) and Cy5 donkey anti-rabbit IgG (#711-175-152).
Cell culture and treatment
The murine MS1 pancreas-derived endothelial cell
line (#CRL-2279;
ATCC) was maintained in DMEM supplemented with 5% FBS (HyClone)
and 1× antibiotic-antimycotic (#15240-062; Gibco). MS-1 cells were tested
quarterly for mycoplasma contamination by PCR. For RIPK3 knockdown,
cells were treated with RNAiMAX transfection reagent (Thermo Fisher
Scientific) and 50 nM of RIPK3 Silencer Select or non-targeting control
siRNA oligonucleotides (#s80756 and #4390844, respectively; Ambion) in
serum-free OptiMEM (Invitrogen). After 24 h, medium was replaced with
low-serum medium. After another 24 h, cells and medium were harvested
for subsequent
transcript or protein analyses. On day 7 of BMDM
differentiation, BMDMs and medium from either Apoe−/−;Ripk3fl/fl or
Apoe−/−;Ripk3fl/fl;LysM-Cre mice were harvested for subsequent transcript
or protein analyses.
Western blot assays
MS1 cells and BMDMs were lysed in RIPA buffer [50 mM Tris-HCl
( pH 7.4), 150 mM NaCl, 1% NP-40, 0.1% SDS, 1 mM EDTA, 0.5%
sodium deoxycholate] with Protease Inhibitor Cocktail (#78430; Thermo
Fisher Scientific) and Phosphatase Inhibitor Cocktail (#78420; Thermo
Fisher Scientific). Aorta tissues were flash frozen and ground with a mortar
and pestle then resuspended in RIPA buffer with the protease and
phosphatase inhibitors. Protein concentration was determined using the
Pierce BCA Protein Assay Kit (#23227, Thermo Fisher Scientific) and a
NanoDrop 2000 from Thermo Fisher Scientific. Then, 5-10 μg protein was
electrophoresed on a 12% SDS-PAGE gel, then transferred to a PVDF
membrane, and then blocked in 5% nonfat dry milk in Tris-buffered saline
with 0.1% Tween 20 (TBST) for 1 h. Membranes were cut into sections
based on target protein molecular weights to optimize the number of
proteins that could be detected. Primary antibodies (diluted in TBST for
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detection of phosphorylated proteins or 5% milk-TBST for all other
proteins) were incubated at 4°C overnight with gentle agitation, and
membranes were then washed three times (10 min each) in TBST. HRP-
conjugated secondary antibodies (diluted in 5% milk-TBST) were applied at
room temperature for 1 h with gentle agitation, and membranes were then
washed four times (15 min each) in TBST. Secondary antibodies were
detected using ECL Western Blotting Detection Reagent (#34076 or
#34096; Thermo Fisher Scientific). Membranes were then stripped using
Restore™ PLUS Western Blot Stripping Buffer (#46430; Thermo Fisher
Scientific) and re-blotted with primary antibodies raised in a different
residual HRP-signal. Densitometry analysis was
species to prevent
software. Primary antibodies used for
performed using ImageJ
anti-ICAM1 (1:5000; #AF796; R&D
immunoblotting were: goat
Systems), goat anti-VCAM1 (1:1000; #AF643; R&D Systems), rabbit
anti-CD11b (1:3000; #EPR1344; Abcam), chicken anti-E-selectin (1:1000;
rabbit anti-RIPK3 (1:4000; #NBP1-77299;
#AF575; R&D Systems),
NOVUS Biologicals), goat
anti-MCP-1 (1:2000; #AF479; R&D
Systems), rabbit anti-MLKL (1:1000; #orb32399; Biorbyt), rabbit anti-
phosphorylated-MLKL (1:1000; #ab196436; Abcam),
anti-
phosphorylated-MLKL (1:1000; #37333; Cell Signaling Technology),
rabbit anti-β-actin
rabbit anti-RIPK1 (1:1000; #ab202985; Abcam),
(1:10,000; #4970; Cell Signaling Technology) and rabbit-anti-GAPDH
(1:20,000, #G9545; Sigma-Aldrich).
rabbit
qPCR assays
To analyze transcript levels, total RNA isolated from MS1 endothelial cells
or BMDMs was purified and treated with RNase-free DNaseI (Qiagen).
cDNA was prepared using the iSCRIPT™ Reverse Transcriptase Kit (Bio-
Rad), and qPCR was performed using 2X SYBR green qPCR master mix
(Applied Biosystems) and the CFX96 Real-Time System (Bio-Rad) with
gene-specific primers. Primers used for qPCR are listed and described in
Table S1. The relative fold change in transcription was determined using the
comparative CT method and three housekeeping genes (Gapdh, Rn18s and
Actb) as internal controls.
ELISA
Maxisorb Immunolon 4HBX 96-well plates (Thermo Fisher Scientific)
were used with mouse MCP-1 and mouse IL-1β ELISA kits (#432705 and
respectively; BioLegend) according to the manufacturer’s
#432605,
instructions to detect MCP-1 or IL-1β levels in plasma samples or
medium from cell culture experiments. Colorimetric values were detected
using a FLUOstar Omega plate reader.
Statistical analysis
Data shown are mean±s.d. of n independent experiments or n animals (when
necessary, n is reported in the corresponding figure legends). Statistical
analyses were performed using GraphPad Prism 8. Data normality was
determined by using the D’Agostino-Pearson omnibus test. Outliers were
identified using the ROUT method (Q=1%). Statistical analyses, post-hoc
tests and P-values are all described in corresponding figure legends.
Significance was determined by a P-value of 0.05 or less. There were no
statistically significant differences between male and female mice.
Acknowledgements
We thank current and past Griffin lab members for helpful discussions.
Competing interests
The authors declare no competing or financial interests.
Author contributions
Conceptualization: S.C., C.T.G.; Methodology: S.C., V.M., J.X., S.G., C.T.G.;
Validation: S.C., S.G., C.T.G.; Formal analysis: S.C., S.G., C.T.G.; Investigation:
S.C., V.M., J.X., S.G.; Resources: C.T.G.; Data curation: S.C., C.T.G.; Writing -
original draft: S.C.; Writing - review & editing: S.C., C.T.G.; Visualization: S.C.;
Supervision: C.T.G.; Project administration: C.T.G.; Funding acquisition: C.T.G.
Funding
This study was supported in part by National Institutes of Health grants HL134778
and HL144605 awarded to C.T.G., and GM114731 (to C.T.G., as part of a
multi-investigator grant awarded to Rodger McEver, Oklahoma Medical Research
Foundation), by a grant from the Oklahoma Center for the Advancement of Science
and Technology (HR15-078) awarded to C.T.G., by grants from the American Heart
Association awarded to C.T.G. (15GRNT25090015) and S.G. (19PRE34380708),
and by grants from the Presbyterian Health Foundation awarded to C.T.G.
Supplementary information
Supplementary information available online at
http://dmm.biologists.org/lookup/doi/10.1242/dmm.041962.supplemental
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| null |
10.1093_pnasnexus_pgad113.pdf
|
Data availability
The processed experimental files for all single-cell data sets used
in this study are available on Zenodo at https://doi.org/10.5281/
zenodo.7474099; Table 1 lists the Gene Expression Omnibus
(GEO) accession numbers for each data set. The saved model
weights for DELAY are available on Zenodo at https://doi.org/10.
5281/zenodo.7474115. All experimental logs from this study
are available at https://tensorboard.dev/experiment/RBVBetLM
RDiEvO7sBl452A. We have provided an open-source implementa-
tion of DELAY in PyTorch with listed requirements and documen-
tation at https://github.com/calebclayreagor/DE
|
Data availability The processed experimental files for all single-cell data sets used in this study are available on Zenodo at https://doi.org/10.5281/ zenodo.7474099 ; Table 1 lists the Gene Expression Omnibus (GEO) accession numbers for each data set. The saved model weights for DELAY are available on Zenodo at https://doi.org/10. 5281/zenodo.7474115 . All experimental logs from this study are available at https://tensorboard.dev/experiment/RBVBetLM RDiEvO7sBl452A . We have provided an open-source implementation of DELAY in PyTorch with listed requirements and documentation at https://github.com/calebclayreagor/DELAY .
|
PNAS Nexus, 2023, 2, 1–13
https://doi.org/10.1093/pnasnexus/pgad113
Advance access publication 30 March 2023
Research Report
Depicting pseudotime-lagged causality across single-cell
trajectories for accurate gene-regulatory inference
Caleb C. Reagor
a,b,c,*, Nicolas Velez-Angel
a and A. J. Hudspeth
a
aHoward Hughes Medical Institute and Laboratory of Sensory Neuroscience, The Rockefeller University, New York, NY 10065, USA
bTri-Institutional PhD Program in Computational Biology and Medicine, New York, NY 10065, USA
cPresent address: 1230 York Avenue, Campus Box 314, New York, NY 10065, USA
*To whom correspondence should be addressed: Email: [email protected]
Edited By: Shibu Yooseph
Abstract
Identifying the causal interactions in gene-regulatory networks requires an accurate understanding of the time-lagged relationships
between transcription factors and their target genes. Here we describe DELAY (short for Depicting Lagged Causality), a convolutional
neural network for the inference of gene-regulatory relationships across pseudotime-ordered single-cell trajectories. We show that
combining supervised deep learning with joint probability matrices of pseudotime-lagged trajectories allows the network to overcome
important limitations of ordinary Granger causality-based methods, for example, the inability to infer cyclic relationships such as
feedback loops. Our network outperforms several common methods for inferring gene regulation and, when given partial ground-
truth labels, predicts novel regulatory networks from single-cell RNA sequencing (scRNA-seq) and single-cell ATAC sequencing
(scATAC-seq) data sets. To validate this approach, we used DELAY to identify important genes and modules in the regulatory network
of auditory hair cells, as well as likely DNA-binding partners for two hair cell cofactors (Hist1h1c and Ccnd1) and a novel binding
sequence for the hair cell-specific transcription factor Fiz1. We provide an easy-to-use implementation of DELAY under an open-
source license at https://github.com/calebclayreagor/DELAY.
Keywords: gene-regulatory inference, gene-regulatory networks, deep learning, single-cell omics, auditory hair cells
Significance Statement
The sequencing of genes expressed in single cells provides detailed information about the developmental programs that define the
identities and states of various cell types, but few computational methods can use the dynamic information encoded in these repre-
sentations to identify causal mechanisms. By exploiting advances in machine learning, we develop a deep neural network that learns
from temporal features of gene regulation to identify direct regulatory interactions between transcription factors and their target
genes. Our method provides mechanistic insights into the development and function of cells by generating high-confidence predic-
tions for interactions in complex gene-regulatory networks.
Introduction
Single-cell sequencing technologies can provide detailed data for
the investigation of heterogeneous populations of cells collected
at specific times—so-called snapshots—during cellular differenti-
ation or dynamic responses to stimulation (1). However, owing to
inherent delays in molecular processes such as transcription
and translation, static measurements from individual cells
cannot reveal the causal interactions governing cells’ dynamic re-
sponses to developmental and environmental cues (2–4). Because
population-level heterogeneity in tissues often reflects the asyn-
chronous progression of single cells through time-dependent
processes, observed patterns of gene expression can nonetheless
indicate the stages of development to which individual cells be-
long (5). Many algorithms exploit these cell-to-cell differences to
infer dynamic trajectories and reconstruct cells’ approximate
temporal progressions along inferred lineages in pseudotime
(6, 7).
Several methods for gene-regulatory inference rely on pseudo-
time in Granger causality tests, which try to determine whether
new time series can add predictive power to inferred models of
gene regulation (8, 9). However, Granger causality-based methods
can be error-prone when genes display nonlinear or cyclic interac-
tions or when the sampling rate is uneven or too low (9–12).
Because pseudotime
these problems,
Granger causality-based methods often underperform model-free
approaches that exploit pure statistical dependencies in gene
expression data (9, 13, 14).
trajectories exhibit
By contrast, deep learning-based methods make no assump-
tions about the temporal relationships or connectivity between
genes in complex regulatory networks; instead, these data-driven
Competing Interests: The authors declare no competing interest.
Received: September 23, 2022. Revised: March 21, 2023. Accepted: March 23, 2023
© The Author(s) 2023. Published by Oxford University Press on behalf of National Academy of Sciences. This is an Open Access article
distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits
unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
2
| PNAS Nexus, 2023, Vol. 2, No. 4
approaches learn general features of regulatory interactions
(15, 16). Here, we describe a deep learning-based method termed
Depicting Lagged Causality (DELAY) that learns gene-regulatory
interactions from discrete joint probability matrices of paired,
pseudotime-lagged gene expression trajectories. Our data suggest
that DELAY can address many shortcomings of current Granger
causality-based methods and provide a useful, complementary
approach to overcome common limitations in the inference of
gene-regulatory networks from single-cell data.
Results
A convolutional neural network predicts
pseudotime-lagged gene-regulatory relationships
To predict gene-regulatory relationships from single-cell data,
we developed a convolutional neural network based on
Granger causality (17). The input to DELAY consisted of stacks
of two-dimensional joint probability matrices for pairs of tran-
scription factors, putative target genes, and highly correlated
“neighbor” genes (18). We constructed the input matrices by
aligning the gene expression trajectories of a transcription fac-
tor A at several lagged positions in pseudotime relative to a
target gene B to generate joint probability distributions from
two-dimensional histograms of gene coexpression at each lag
(Fig. 1A). The value of a given lag indicated the ordinal differ-
ence between cells’ rank-ordered positions in pseudotime.
Each input matrix consisted of the L2-normalized cell number
counts from a two-dimensional gene coexpression histogram
with 32 fixed-width bins in each dimension, spanning each
gene’s minimum and maximum expression values. Although
the marginal probability distributions for both A and B re-
mained essentially unchanged at each lag except for cells
lost at the leading and lagging edges of the shifted trajectories,
realigning the gene expression in pseudotime altered key fea-
tures of the resulting joint probability matrices. In other
words, causally related genes share important pseudotime-
lagged patterns of gene coexpression with nearby cells in
single-cell trajectories.
Using ground-truth labels from cell type–specific chromatin
immunoprecipitation sequencing (ChIP-seq) data (14), we con-
ducted supervised learning to train our neural network to pre-
dict whether A directly regulates B. This procedure resembled
a regression in a Granger causality test (17), in which values of
a time series Y at timepoints yt are regressed against values
from another time series X at timepoints xt, xt−1, xt−2, . . . , xt−T
up to some maximum lag T to determine whether any time-
lagged values of X add explanatory power to Y’s autoregres-
sive model. DELAY likewise learned higher weights for gene
coexpression matrices at specific pseudotime
lags that
indicated the true regulatory relationship between genes.
After comparing several neural network architectures, we
selected a six-layered convolutional network trained on
pseudotime-aligned
(T = 0) and five pseudotime-lagged
(T ∈ {1, 2, 3, 4, 5}) gene coexpression matrices to predict direct
gene-regulatory relationships (Fig. 1B). We also trained the
network on lagged coexpression matrices of two highly corre-
lated neighbor genes per gene, that is, the two transcription
factors with the highest cross-correlation with A and B along
the single-cell trajectory. Because the neighbor genes can pre-
sent stronger alternatives to the primary hypothesis that A
directly regulates B, including these matrices for A and B ver-
sus their highly correlated transcription factors reduced false-
positive predictions.
DELAY outperforms several common methods of
gene-regulatory inference
We trained DELAY on gene expression data sets from human em-
bryonic stem cells (hESCs) (19), mouse embryonic stem cells
(mESCs) (20), and three lineages of mouse hematopoietic stem
cells (mHSCs) (21). We generated separate training data sets for
each of the hematopoietic lineages, and all data sets contained
at least 400 cells per lineage (Table 1). Each trajectory was oriented
according to known experimental timepoints or precursor cell
types and lineages, and pseudotime values were inferred separ-
ately with Slingshot (6) for each lineage (Fig. S1). We chose these
data sets because the cell types and trajectories are well charac-
terized and offer cell type–specific ChIP-seq data to generate
ground-truth networks (14). Although the three hematopoietic
data sets contained similar numbers of examples of true regula-
tion and no interaction, both of the embryonic data sets were
class-imbalanced and contained fewer examples of true regula-
tion. To maximize the network’s generalizability, we trained
DELAY simultaneously on all five gene expression data sets but
validated it on each data set individually. We first generated ran-
domly segregated 70–30% splits of all possible gene pair examples
for each data set and then merged the 70% splits to create a
combined training data set. In a separate analysis, we also cross-
validated DELAY using inductive splits wherein specific transcrip-
tion factors appeared in only the training or validation splits.
After training DELAY on the combined 70% splits, the network
outperformed eight of the most popular approaches for inferring
gene-regulatory relationships, including six unsupervised meth-
ods (8, 22–26 ) (Fig. 1C) and two deep convolutional neural net-
works (18, 27) (Fig. 1D). We measured the performance of the six
unsupervised methods across the combined training and valid-
ation splits for each data set and then compared the results
with the performance of the supervised methods on the held-out
examples alone. With one exception, the deep learning-based
methods outperformed all others according to the areas under
both the precision–recall (PR) and receiver operating characteris-
tic (ROC) curves (Fig. S2). Moreover, DELAY outperformed all the
other methods according to both metrics, even though one of
the deep learning-based methods, DeepDRIM, was trained on
5-fold as many neighbor gene matrices. Upon separate cross-
validation, DELAY performed slightly worse on inductive splits
but with a single exception outperformed all other methods on
average (Fig. 1E). Across three of the training data sets, DELAY
also outperformed a modified version of DeepDRIM that was
trained on the same pseudotime-lagged input matrices as
DELAY (Fig. S2). Together, these results suggest that DELAY out-
performs other methods because it can better learn important
gene-regulatory features from pseudotime-lagged gene coexpres-
sion matrices.
Transfer learning allows DELAY to predict novel
gene-regulatory networks from new single-cell
data sets
To test whether DELAY generalizes to new data sets, we examined
the human hepatocyte (hHep) gene-regulatory network using an
additional data set with over 400 single cells and known ground-
truth interactions from ChIP-seq data (14, 28). We inferred the
network by the previous methods and found that tree- and mu-
tual information-based methods performed slightly better than
deep learning-based methods, which were not initially trained
on the new data and consequently performed comparably to ran-
dom predictors (Fig. 1F). To determine whether this lack of
Reagor et al.
| 3
Fig. 1. Pseudotime-lagged causality allows accurate inference of gene-regulatory networks. A) Shifting the gene expression trajectory of transcription
factor A forward in pseudotime with respect to that of target gene B generates a series of unique joint probability distributions. The resulting joint
probability matrices contain gene coexpression signatures—in the upper-left, upper-right, and lower-right regions—that indicate A directly regulates B.
B) The inverted architecture of DELAY is wide at the beginning of the network and progressively narrows to a one-dimensional vector followed by a linear
classifier and sigmoid activation function to generate gene regulation probabilities. The network uses leaky ReLU activations and padded 3 × 3
convolutions throughout. C and D) DELAY outperforms eight of the most popular methods for inferring gene-regulatory interactions across several
benchmark scRNA-seq data sets, including six unsupervised methods (C) and two supervised methods (D). E) All three supervised methods perform
slightly worse upon cross-validation, but DELAY still outperforms all other methods on average, with the exception of PPCOR for a single metric. F and G)
DELAY does not immediately generalize to a new testing data set (F) but outperforms all other methods if fine-tuned on a small percentage of the new
data (G). Values for the area under the precision–recall curve (AUPRC) in C), D), F), and G) are normalized by the proportion of positive examples per data
set (horizontal lines, E) and averaged across five model replicates for supervised methods. Boxes in E) show the first quartiles, means, and third quartiles
for the per- transcription factor AUPRC values across the k = 5 validation folds. The statistical significance between DELAY and the next-best neural
network was assessed using a one-sided Wilcoxon signed-rank test (*P ≤ 0.05; **P ≤ 0.01; ***P ≤ 0.001).
ABCEFGD4
| PNAS Nexus, 2023, Vol. 2, No. 4
Table.1. Summary of the data sets used to train, test, and evaluate the neural network.
Data sets
Networks
Cell type
TC/S
GEO
Set
hESC
mESC
mHSC-E
mHSC-GM
mHSC-L
hHep
mOHC (RNA)
mOHC (ATAC)
TC
TC
S
S
S
TC
TC
S
GSE75748
GSE98664
GSE81682
GSE81682
GSE81682
GSE81252
GSE137299
GSE157398
Train/Val
Train/Val
Train/Val
Train/Val
Train/Val
Test
Eval
Eval
Cells
758
421
1,071
889
847
425
1,563
391
TFs
Targets
Examples
Edges
Density
37 (4)
125 (17)
33
23
16
33 (3)
56
48
541
642
533
523
516
536
556
382
20,017
80,250
17,589
12,029
8,256
17,688
1,112*
764*
3,166
20,580
9,592
6,587
4,026
6,171
166*
157*
15.82%
25.64%
54.53%
54.76%
48.76%
34.89%
14.93%*
20.55%*
Columns cell type to cells describe the single-cell data sets used to train, test, and evaluate DELAY, and columns TFs to density describe the corresponding
gene-regulatory networks. For three of the networks, differentially expressed transcription factors without target genes (in parentheses) were included only as target
genes. Network density is equal to the number of edges from the ground-truth ChIP-seq data divided by the total number of examples. E, erythroid lineage; GM,
granulocyte–monocyte lineage; L, lymphoid lineage; mOHC, mouse outer hair cell; S, snapshot; TC, time course; TF, transcription factor. *Partial ground-truth
network.
generalizability arises from batch effects in the single-cell data,
we used transfer learning to fine-tune the three deep learning-
based methods on a small number of randomly segregated exam-
ples from the new data set while validating on the rest of the
examples (Fig. 1G). After training each network on only 1% of
the new examples and validating it on the remaining 99%, the net-
works’ performance matched or exceeded that of the unsuper-
vised methods; training on up to 20% of the new examples
yielded further performance increases. DELAY again outper-
formed every other deep learning-based method. During fine-
tuning, we also observed a monotonic increase in the value of
the mean validation metric across PR and ROC curves, suggesting
that the networks can learn useful features of gene regulation
after longer training periods. Moreover, these results demonstrate
that DELAY can accurately predict gene-regulatory relationships
from new data sets with partially known ground-truth labels.
single cells (Fig. 2C) or additional gene-dropout noise (Fig. 2D),
we also discovered that the network was more sensitive to down-
sampling of single cells than to gene expression losses in low-
expressing cells alone. These results indicate that DELAY relies
more heavily on highly expressing cells and therefore assigns lar-
ger input weights for the first lagged input because on average
that input contains stronger features of gene activation than other
lags (Fig. 2E and F). To investigate this hypothesis, we used aug-
mented input matrices with masked regions to show that
DELAY relies heavily on the combined upper-left, upper-right,
and lower-right regions (AON ∪ BON) across all lagged matrices
(Fig. 2G). By performing a post hoc analysis of the statistical dis-
persion across correctly inferred gene pair examples, we addition-
ally found that DELAY generally performs better on transcription
factors with stable gene expression along single-cell trajectories
(Fig. S3).
DELAY performs well with new input
configurations, augmented matrices, and
modified data sets
Using different numbers of pseudotime-lagged gene coexpression
matrices or neighbor gene matrices, as well as examples from
modified data sets with fewer cells or additional gene dropouts,
we next examined the performance of DELAY across various input
configurations. We employed the original data sets to train new
models on gene coexpression matrices of up to 10 pseudotime
lags (Fig. 2A) or up to 10 neighbor genes, as well as on gene coex-
pression matrices with varying dimensions and resolutions
(Fig. S3). Training DELAY on at least one pseudotime-lagged ma-
trix or with at least one neighbor gene greatly increased the net-
work’s performance across all data sets. Although training
DELAY on up to 10 pseudotime-lagged matrices resulted in com-
parable or slightly better performance across all data sets, train-
ing the network on more than two neighbor gene matrices per
gene decreased performance in some instances. Adding channel
masks for specific lagged matrices suggested that DELAY relies
on redundancies across all available lagged inputs (Fig. S3).
We also characterized DELAY’s performance on pseudotime-
shuffled trajectories and observed a sharp decrease in perform-
ance after reordering nearby cells in each trajectory (Fig. 2B).
This result suggests that the network relies heavily on the specific
ordering of adjacent cells in each trajectory. Upon examining
DELAY’s performance on modified data sets containing fewer
internal
DELAY recognizes causal relationships in
hierarchical and cyclic gene-regulatory
interactions
To further investigate how the selection of neighbor genes can
alter DELAY’s
representations and subsequent
gene-regulatory inferences, we modified gene pair examples in
the original 30% validation splits to exclude all neighbor genes C
with known interactions across several classes of three-gene mo-
tifs. First, we used DELAY to infer gene regulation for potential
hierarchical and cyclic interactions across validation set exam-
ples (Fig. 3A), including mutual interactions (MIs), feedback loops
(FBLs), and three classes of feedforward loops (FFLs). Unlike ordin-
ary Granger causality, DELAY performed well across cyclic inter-
actions including 2-cycles (MIs) and 3-cycles (FBLs), which are
ubiquitous among gene-regulatory networks (29). We next ex-
cluded from the same validation set examples all input matrices
for any neighbor gene of either A or B known from the ChIP-seq
data to be involved in potential FBLs or FFLs, replacing the inputs
for all omitted neighbors C with the matrices of other highly cor-
related neighbor genes. Because we saw a significant decrease in
performance upon excluding these neighbors C in most cases of
shared and sequential gene regulation, but not for downstream
targets, DELAY apparently recognizes the differences between in-
put matrices of causally related genes and those of merely corre-
lated genes. Moreover, these results suggest that although our
network uses principles of Granger causality, it can achieve true
Reagor et al.
| 5
DELAY performs best on zinc-finger proteins,
bHLH factors, and other chromatin remodelers
To explore how DELAY performs on classes of transcription fac-
tors containing different types of DNA-binding domains, we ana-
lyzed the enrichment of gene ontology (GO) terms across correctly
inferred transcription factors (Fig. 3B). We found that DELAY per-
forms best on zinc-finger proteins, bHLH factors, and other chro-
matin remodelers. Although DELAY performs well on C2H2-type
zinc-finger proteins in terms of the total number of correct predic-
tions, we found that it performs better on other chromatin remod-
elers and plant homeodomain (PHD) zinc-finger proteins by the
overall term enrichment (Table S1). Interestingly, these results in-
dicate that training the network on cell type–specific ChIP-seq
data allows the network to identify regulatory relationships in-
volving some non sequence-specific transcription factors and co-
factors that nevertheless associate with specific targets at
preferred chromatin conformations.
Predicting the gene-regulatory network of
auditory hair cells through multi-omic transfer
learning
We next sought to generate predictions for a cell type with com-
plex but incompletely characterized gene-regulatory dynamics.
We devised a pipeline for multi-omic transfer learning to infer
the gene-regulatory network for developing mouse outer hair
cells, the mechanical amplifiers of the inner ear. We used both
gene expression (30) and chromatin accessibility (31) data sets to
fine-tune our network. By first calculating the cell-by-gene acces-
sibility scores across annotated genes, we were able to generate
lagged input matrices for the single-cell ATAC sequencing
(scATAC-seq) data set (Fig. 4A). Because the underlying gene ex-
pression and gene accessibility distributions are both
zero-inflated (8), the resulting coaccessibility matrices are qualita-
tively similar to gene coexpression matrices.
To determine whether pseudotime-lagged gene coaccessibility
matrices contain features that indicate direct gene-regulatory re-
lationships, we fine-tuned DELAY on the scATAC-seq matrices us-
ing ground-truth examples collected from two cell type–specific
data sets of Sox2 and Atoh1 target genes (32, 33). Seventy percent
of the randomly segregated ground-truth examples were used for
fine-tuning, and the remaining 30% were held out for validation
(Fig. 4B). DELAY performed slightly worse by the metric of area
under the PR curve than by area under the ROC curve, indicating
that the network is better at discriminating false positives than
selecting true positives. Although DELAY did not outperform all
other deep learning-based methods, the network’s performance
was comparable with previous training and validation on small
fractions of the hHep single-cell RNA sequencing (scRNA-seq)
data set, which suggests that gene coaccessibility matrices are
also useful for inferring direct gene-regulatory interactions.
We separately fine-tuned the network on all available Sox2 and
Atoh1 ground-truth examples from an additional gene expression
data set for mouse outer hair cells (30). With previously deter-
mined hyperparameters for scRNA-seq data, training DELAY
on two graphics processing units (GPUs) required 230 ± 1 min
(mean ± SD) per model. We then compared the target gene rank
correlations between the inferred transcription factor-only
gene-regulatory networks to determine whether networks in-
ferred from scRNA-seq data and scATAC-seq data were similar
(Fig. 4C). Although we observed stronger correlations between
predictions from data set-specific models than between average
predictions across data sets, the target gene rank correlations
Fig. 2. The neural network relies on cell order in pseudotime and gene
expression strength. A) Training new models of DELAY on increasing
numbers of pseudotime-lagged matrices gives the largest performance
increase when using up to a single lag. B) Reordering single cells in
pseudotime sharply decreases performance, suggesting that DELAY relies
on the specific ordering of adjacent cells in each trajectory. C and D) The
network is sensitive to random down-sampling of cells across data sets (C)
but relatively more robust to induced, additional gene dropouts in weakly
expressing cells (D), suggesting that DELAY relies heavily on highly
expressing cells. E and F) The network learns larger input weights for
lagged matrices of the first pseudotime lag (E), which also contain more
cells in the combined “ON” region (AON ∪ BON; dotted outline, F) on
average across training data sets (dotted line, E). The combined “ON”
region is comprised of the upper-left “ON–OFF” quadrant (AON ∩ BOFF),
upper-right “ON–ON” quadrant (AON ∩ BON), and lower-right “OFF–ON”
quadrant (AOFF ∩ BON). G) Masking different regions of the input matrices
shows that the network relies heavily on the combined “ON” region. The
lines and shaded regions in A–E) show the average and full range of values
across five model replicates, and the markers in G) show the average
values across model replicates. The statistical significance in G) was
assessed with a Kruskal–Wallis test (***P ≤ 0.001).
causal inference for genes involved in several classes of hierarch-
ical and cyclic regulatory interactions by avoiding several limiting
assumptions of ordinary Granger causality.
ABCDEFG6
| PNAS Nexus, 2023, Vol. 2, No. 4
Fig. 3. DELAY uncovers causal, cyclic, and context-specific gene-regulatory relationships. A) The network’s performance when inferring putative
transcription factor-target gene pairs across two- and three-gene motifs in the validation set suggests that DELAY can distinguish between different types
of hierarchical and cyclic gene regulation. Upon exclusion of one or more neighbor genes C from the input features of the validation examples, the
network’s performance declines significantly if C is a shared or sequential regulator of A and B, but not if C is a shared target. B) GO-term enrichment
indicates that DELAY performs best on zinc-finger proteins (PHD-type, GATA-type, C2H2-type, NHR-type, and C5HC2-type), bHLH factors (Myc-type), and
other chromatin remodelers (SNF2-related, chromodomain, bromodomain, HDA domain, and helicase). Markers and error bars in A) show the average
values and full range of performance across five model replicates. The statistical significance in A) was assessed with a one-sided Wilcoxon signed-rank
test (*P ≤ 0.05) and in B) with a Fisher’s exact test (Padjusted ≤ 0.05).
between the two data sets were highly variable, and the predic-
tions of some transcription factors agreed better than others.
Reasoning that the inferences with better agreement across data
sets constituted the best predictions and highest confidence
interactions, we derived the consensus hair cell gene-regulatory
network from the average predictions across both data sets.
The resulting network consisted of 347 predicted transcription
factor–target interactions with gene regulation probabilities >0.5.
DELAY identifies important genes, interactions,
and modules in the hair cell gene-regulatory
network
We used hierarchical clustering to group transcription factors and
target genes in the transcription factor-only gene-regulatory
network for hair cells by similarities in their predicted targets
and regulators, respectively (Fig. 4D). This procedure revealed
two distinct developmental modules corresponding to prosen-
sory genes such as Sox2, Id2, Hes1, and Prox1 and hair cell-
specific genes such as Atoh1, Pou4f3, Gfi1, Lhx3, and Barhl1. We
sought to validate the predicted interactions by comparing the
locations of known transcription factor-binding sites (34, 35) to
the locations of open-chromatin peaks (31) within 50 kb of target
genes’ transcription start sites. Twenty-two of 28 predicted in-
teractions were confirmed by the accessibility of transcription
factor-binding sites. Of the six remaining interactions, three
were instances of predicted target-gene regulation by transcrip-
tional cofactors lacking true DNA-binding domains. We add-
itionally identified 13 reported interactions that were not
detected by DELAY (31, 36–54).
The most notable feature of the inferred gene-regulatory
network for hair cells is that Sox2 and Id2—in addition to their
proteins’ well-known roles in regulating target genes and main-
taining a prosensory cell fate—are themselves the targets of a
wide variety of transcription factors including Sox proteins,
homeobox factors, zinc-finger proteins, and Notch effectors.
Eleven of the 22 interactions confirmed by our binding-site acces-
sibility analysis represented direct regulation of Sox2 and Id2, in-
cluding mutually activating interactions between Sox2 and Sox9,
Sox11, Prox1, and Hes1, and mutual inhibition with Hist1h1c. One
other study has suggested that Hes1 directly regulates Sox2 (55).
Another notable feature of the inferred hair cell network is that
the LIM-homeobox transcription factor Lhx3 regulates its own ex-
pression as well as that of two other LIM-only transcription factors
(Lmo4 and Lmo1). This result implies a role for Lhx3 in maintain-
ing the later expression of these important early Sox2 inhibitors
(31, 47, 49). Other key features of the network include Sox11 regu-
lation by Hes1, Nfkbia regulation by Gfi1, and regulation of the spli-
cing factor gene Srsf2 by the products of three different prosensory
genes. Srsf2 was recently predicted to play a role in the splicing of
an important deafness gene in humans (56).
Discriminative motif analysis of target-gene
enhancer sequences enables de novo discovery of
DNA-binding motifs
DELAY permits a complementary approach
typical
gene-regulatory inference workflows such as SCENIC (57) that
use cis-regulatory sequences to identify and discard false-positive
interactions resulting from indirect gene regulation (11, 30, 31).
to
ABReagor et al.
| 7
Fig. 4. DELAY accurately predicts gene-regulatory interactions in the auditory hair cell network through multi-omic transfer learning. A) An example of
an empirical joint probability matrix from scATAC-seq trajectories. B) After fine-tuning the network on lagged scATAC-seq input matrices, DELAY
performs comparably with other neural networks and to previous testing on hHep scRNA-Sseq data. C) Training DELAY separately on scRNA-seq and
scATAC-seq data sets of hair cell development reveals a stronger correlation between predictions from model replicates than between data sets across
the transcription factor-only network. D) Average gene regulation probabilities P across the hair cell gene-regulatory network accurately predict
interactions between transcription factors (rows) and targets (columns), when comparing known binding sites to open-chromatin peaks in the target
genes’ enhancer sequences. Hierarchical clustering with WPGMA reveals distinct gene modules for prosensory genes (Sox2, Id2, Hes1, and Prox1) and hair
cell genes (Atoh1, Pou4f3, Gfi1, Lhx3, and Barhl1). Up- or down-regulation was deduced from the correlation in the gene expression data. Markers and error
bars in B) show the average values and full range of performance across five model replicates for each neural network. Markers in C) show the median
target gene rank correlations across comparisons. The statistical significance in C) was assessed with a Kruskal–Wallis test (***P ≤ 0.001).
Because these methods rely on databases of known DNA-binding
motifs, they necessarily overlook predictions for cofactors and pu-
tative transcription factors with unknown binding sequences.
Instead of using cis-regulatory sequences to refine our initial pre-
dictions, we introduced enhancer sequence information post hoc
to perform discriminative motif analysis within the enhancers of
predicted targets in the hair cell network (Figs. 5A and S4). We
identified enriched motifs that closely resembled known
DNA-binding motifs for nine of 11 transcription factors with at
least one predicted target gene in the transcription factor-only
hair cell network (Table S2).
We additionally sought to predict the mechanisms by which
several identified hair cell cofactors accomplish sequence-specific
gene regulation in the absence of true DNA-binding domains.
Specifically, we compared sequences enriched in the enhancers
of cofactors’ predicted targets to several databases of known
DNA-binding motifs to identify the cofactors’ DNA-binding part-
ners (so-called guilt by association). Through this analysis, we
were able to determine that the most significantly enriched se-
quence in the enhancers of the histone Hist1h1c’s predicted target
genes closely matched known binding motifs for several SoxB2/A
transcription factors (Fig. 5B). In addition, a sequence enriched in
the enhancers of cyclin Ccnd1’s targets accorded with known
motifs for the Pbx family of homeobox transcription factors
(Fig. S5). These cofactors might form complexes with the identi-
fied transcription factors to regulate their target genes in hair
cells.
As a final demonstration of DELAY’s high-confidence predic-
tions, we used the fine-tuned model for the scRNA-seq data to
generate regulatory predictions for transcription factors ex-
pressed in at least 20% of developing hair cells (Table S3). After
considering these additional transcription factors, we identified
the putative C2H2 zinc-finger protein Fiz1 as a likely regulator of
Sox2 and Hes6. Discriminative motif analysis of these genes’ en-
hancer sequences (Fig. 5C) uncovered a likely Fiz1 consensus
DNA-binding sequence (5′-CGCTGC-3′) similar to that of other
Sox2 regulators from the Zic family of C2H2 zinc-finger proteins
(58).
Discussion
Building upon several deep learning-based methods (18, 27), we
have demonstrated that combining fully supervised deep learning
with joint probability matrices of pseudotime-lagged single-cell
trajectories can overcome certain limitations of current Granger
causality-based methods of gene-regulatory inference (9, 12),
ADBC8
| PNAS Nexus, 2023, Vol. 2, No. 4
Fig. 5. Accurate target-gene predictions enable de novo discovery of DNA-binding motifs. A) Three examples of motifs enriched in the enhancer
sequences of predicted target genes (bottom row) closely resemble known DNA-binding motifs (top row) for transcription factors with at least one
predicted target gene in the transcription factor-only hair cell gene-regulatory network. B and C) Sequences for putative transcription factors or cofactors
may represent novel DNA-binding motifs or indicate sequence-specific interactions through multi-protein complexes. Motifs for two hair cell genes
closely match known DNA-binding sequences, suggesting that the linker histone Hist1h1c (B, top row) forms complexes with SoxB2/A factors (B, bottom
row) and that the putative C2H2 zinc-finger protein Fiz1 (C, top row) recognizes motifs similar to Zic family C2H2 zinc-finger proteins (C, bottom row). The
statistical significance of each motif alignment was estimated using the cumulative density function of all possible comparisons of known motifs across
enriched sequences for A) or inferred motifs across all database motifs for B) and C) (**P ≤ 0.01; *** P ≤ 0.001).
such as their inability to infer cyclic regulatory motifs. Although
our convolutional neural network DELAY remains sensitive to
the ordering of single cells in pseudotime, the network can never-
theless accurately infer direct gene-regulatory interactions from
both time course and snapshot data sets, unlike many supervised
methods that rely strongly on the number of available time course
samples (15, 16). We suspect that DELAY is sensitive to the specific
ordering of adjacent cells in trajectories because pseudotime in-
ference methods such as Slingshot (6) infer lineages from min-
imum spanning trees that directly depend on cell-to-cell
similarities in gene expression values (7).
We have presented a multi-omic paradigm for fine-tuning
DELAY on both gene expression and chromatin accessibility
data sets for the development of auditory hair cells. The network’s
ABCaccurate predictions allow de novo inferences of known and
unknown DNA-binding motifs, establishing DELAY as a comple-
mentary approach to common methods of gene-regulatory infer-
ence. Our method’s high-confidence predictions across the
hair cell gene-regulatory network also support it as an attractive
option for experimentalists with limited resources to predict
true gene-regulatory relationships from complex, large-scale
gene-regulatory networks while avoiding spurious, indirect inter-
actions often introduced through unsupervised methods (14).
We have additionally identified with high confidence interac-
tions between cofactors and target genes in the regulatory net-
work of hair cells that methods such as SCENIC (57) would have
overlooked. Using “guilt by association,” we predict that the cyclin
Ccnd1—a known transcriptional cofactor found at the enhancers
of several Id genes during retinal development (59)—forms com-
plexes with the Pbx family of homeobox transcription factors, of
which at least one is a known target of Prox1 in the inner ear
(60). Moreover, we predict that the retina-specific linker histone
Hist1h1c (61) forms complexes with the SoxB2 family of transcrip-
tion factors, which have known antagonistic effects on Sox2 ex-
pression in hair cells (62). Finally, we predict that the putative
hair cell-specific C2H2 zinc-finger protein Fiz1—which is also ex-
pressed during retinal development (63)—is a regulator of Sox2
in hair cells and identified its likely DNA-binding sequence in
the enhancers of predicted target genes.
Believing that DELAY will be a valuable resource to the commu-
nity, we have provided an easy-to-use and open-source imple-
mentation of the algorithm as well as pre-trained model weights
for subsequent fine-tuning on new single-cell data sets and partial
ground-truth labels. Unlike other deep learning-based methods,
our implementation of DELAY maximizes usability and prioritizes
model flexibility. Although we chose to fine-tune DELAY on cell
type–specific ChIP-seq data, future studies may choose to fine-
tune DELAY on curated interactions from databases or from
gain- or loss-of-function experiments, especially in the absence
of ChIP-seq data (14). These additional interactions can also sup-
plement smaller ground-truth data sets, such as those of Sox2 and
Atoh1 target genes, to mitigate false-negative predictions. We be-
lieve that the modest computational cost of training new models
of DELAY will prove a worthwhile investment for future investiga-
tions into complex gene-regulatory networks.
Materials and methods
Preparing single-cell RNA-seq data sets to train
and test the convolutional neural network
To train our convolutional neural network, we used scRNA-seq
data sets from two time course studies of endodermal specifica-
tion of hESCs (19) and mESCs (20) and an in vivo snapshot study
of erythroid (E), granulocyte–monocyte (GM), and lymphoid (L)
specification in mHSCs (21). We additionally employed a data
set from a time course study of the differentiation of hHeps
from induced pluripotent stem cells to test our network (28). For
each of these studies, we collected the normalized gene expres-
sion values, pseudotime values, and ground-truth networks
from BEELINE’s supplementary data files (14). In BEELINE,
Pratapa et al. collected the normalized gene expression values
from the original studies or obtained the values themselves by log-
transforming the transcripts per kilobase million. Moreover, those
authors used Slingshot (6) to infer the pseudotime values separ-
ately for each data set, orienting the inferred trajectories by
known experimental timepoints or precursor cell types and
Reagor et al.
| 9
lineages. Finally, Pratapa et al. selected genes with differential ex-
pression across pseudotime by applying generalized additive
models (GAMs) to compute gene variances and their associated
P values. To train DELAY, we utilized their gene variances and cor-
rected P values to select differentially expressed transcription fac-
tors (Padjusted<0.01) and 500 additional genes with the highest
variance for each data set. We also collected the ground-truth la-
bels from BEELINE’s supplementary data files, which contained
tables of transcription factor–target gene interactions curated
from cell type–specific ChIP-seq experiments in the ENCODE
(64), ChIP-Atlas (65), and ESCAPE (66) databases. Table 1 provides
details for each data set including descriptions of the ground-
truth networks.
We also characterized our network on modified data sets with
shuffled pseudotime, fewer cells, and additional gene-dropout
noise. We shuffled pseudotime values across single-cell trajector-
ies using np.random.normal in NumPy (v1.20.2) to select the indi-
ces of single cells either leading or lagging successive cells in each
trajectory at some length scale σ before swapping the cells’ posi-
tions in pseudotime. We also used np.random.choice to select
the indices of single cells to retain when down-sampling the num-
ber of cells in a data set. Lastly, we induced additional gene-
dropout noise in data sets by setting the gene expression values
to 0 with a probability of p for the bottom p percent of cells ex-
pressing each gene in a given data set.
Generating examples of transcription factor–
target gene pairs from single-cell data sets
For each data set, we generated mini-batches of 512 transcription
factor–target gene pair examples by first enumerating all possible
combinations of differentially expressed transcription factors and
potential target genes—including both transcription factors and
highly varying genes. We then generated aligned and pseudotime-
lagged gene coexpression matrices for up to five lags with the fol-
lowing configurations as separate input channels: transcription
factor–target, transcription factor–transcription factor, target–
target, transcription factor–neighbor (for two neighbors), and tar-
get–neighbor (for two neighbors). We concatenated the input
channels for each example to form three-dimensional stacks of
input matrices with dimensions 42 × 32 × 32 (channels × height ×
width). For each gene, we used np.correlate in NumPy to select the
transcription factors with the highest absolute cross-correlation
at a maximum offset of five pseudotime lags to use as neighbor
genes. We trained five model replicates on unique, randomly seg-
regated 70–30% splits of all possible gene pair examples generated
with the random split function in PyTorch (v1.8.1). Each random
split achieved a strict segregation of unique gene pair examples
into either the training or validation sets, though gene pairs for
the same transcription factor but different target genes appeared
in both sets. For separate model cross-validation, we generated
five inductive splits across each data set wherein specific tran-
scription factors appeared in only the training (80%) or validation
(20%) splits. For both analyses, training splits from individual data
sets were subsequently merged to create combined training data
sets.
We later used the original randomly segregated validation
splits to characterize our network on augmented coexpression
matrices and matrices generated from modified single-cell data
sets. To augment gene coexpression matrices, we masked with ze-
ros either specific region across all input channels or entire input
channels corresponding to specific pseudotime lags.
10
| PNAS Nexus, 2023, Vol. 2, No. 4
Constructing a convolutional neural network to
classify lagged gene coexpression matrices
We designed a convolutional neural network based on an inverted
VGGnet (67) that uses five convolutional layers to first expand the
input to 1,024 channels and then successively halve the number
of channels to 64 before classifying examples as either true regu-
lation or no interaction with a fully connected linear layer. Each
convolutional layer sums over the two-dimensional cross-
correlations (⋆) of 3 × 3 kernels and input channels i to find the
features for a given output channel j, as shown in Equation 1:
output (Nk, Coutj ) = bias (Coutj ) +
Cin
i=1
weights 3×3 (Cini
, Coutj ) ⋆ input (Nk, Cini
),
(1)
in which the weights and bias are trainable parameters, N is the
mini-batch size, C is the number of channels, Cout = Cin/2 for
layers 2 through 5, and all convolutions are zero-padded at the
edges of matrices. To preserve the gradient flow during training,
we used leaky rectified linear units (ReLUs) with a negative slope
of 0.2 (Equation 2) as our nonlinear activation function after
each convolutional layer:
Leaky ReLU (x) = max (0, x) + 0.2∗min (0, x).
(2)
As shown in Equation 3, we additionally used 2 × 2, unpadded
max-pooling layers between convolutional layers to identify im-
portant features and down-sample activation maps:
hin
2
,
win
2
= stride
2×2
max
m,n ∈ {0,1}
input (Nk, Cinj , xm,n)
,
output Nk, Coutj ,
(3)
in which x represents the 2 × 2 input windows and h, w are the
height and width of the input channel j. After the final convolu-
tional layer, we used global-average pooling (Equation 4) to reduce
the remaining 64 feature maps j to a single, 64-dimensional
vector x:
output (Nk, Coutj ) = avg
hin×win
input (Nk, Cinj ).
(4)
We lastly used a fully connected linear layer (Equation 5) with a
sigmoid activation function (Equation 6) to generate gene regula-
tion probabilities:
output (Nk) = bias FC +
64
i=1
weights FC (xi)∗input (Nk, xi),
(5)
Sigmoid (x) =
1
1 + exp(−x)
,
(6)
where a probability of P > 0.5 indicates a true gene-regulatory
interaction for the given gene pair example.
Training and fine-tuning the network on
pseudotime-lagged gene coexpression matrices
We used PyTorch’s implementation of stochastic gradient descent
(SGD) to optimize our network with respect to the class-weighted
binary cross-entropy loss, summed across each mini-batch and
scaled by the overall batch size 512, as shown in Equation 7:
L(y, ˆy) = −
wN
512
N
n=1
yn∗log ˆyn + (1 − yn)∗log (1 − ˆyn),
(7)
in which y and ˆy are the target and predicted values (respectively),
wN is the fraction of true examples in the mini-batch, and N is the
size of the current mini-batch (which might be <512). Prior to
optimization, we used He initialization (68) with uniform priors
to set the weights for all convolutional and linear layers. We
used a learning rate (LR) of 0.5 to train each model for up to 100
epochs, validating performance after each epoch and stopping
training after 10 or more epochs without an improvement in the
mean validation metric across PR and ROC curves. For fine-tuning,
we trained each model for up to a maximum of 5,000 additional
epochs due to the observed monotonic increase in the value of
the mean validation metric. We occasionally reduced the LR to
0.25 or 0.1 if the training became unstable, and we tried several
mini-batch sizes ≥24 for fine-tuning and separate model cross-
validation. All training and testing was performed on two Nvidia
RTX 8000 GPUs.
Comparing DELAY to other top-performing
gene-regulatory inference methods
We compared the performance of our neural network to two other
convolutional neural networks, as well as the top six best-
performing methods identified in a previous benchmarking study.
Using BEELINE, we inferred the gene-regulatory networks for all
training and testing data sets with the tree-based methods
GENIE3 (22) and GRNBoost2 (23), the mutual information-based
method PIDC (24), and the partial correlation and regression-
based methods PPCOR (25), SCODE (26), and SINCERITIES (8). We
utilized the best parameter values identified in BEELINE for the
partial correlation and regression-based methods. For the two
deep learning-based methods [CNNC (27) and DeepDRIM (18)],
we used the original studies to reconstruct the neural networks
in PyTorch before training models on the same randomly segre-
gated training examples as DELAY. In addition to training both
neural networks on pseudotime-aligned gene coexpression matri-
ces for primary transcription factor–target gene pairs, we also
trained DeepDRIM on 10 neighbor gene matrices per gene as in
the original study. Moreover, we separately trained DeepDRIM
on five pseudotime-lagged matrices per gene pair with 10 neigh-
bors across the same inductive splits as DELAY to compare the
cross-validated performance between the networks.
Analyzing enrichment of GO terms across
correctly inferred gene pair examples
We used Enrichr (69) (https://maayanlab.cloud/Enrichr/) to ana-
lyze GO-term enrichment across correctly inferred transcription
factors for terms related to InterPro DNA-binding domains (70).
We used a Fisher’s exact test with Benjamini–Hochberg correction
for multiple-hypothesis testing (Padjusted<0.05) to assess the statis-
tical significance for each GO term.
Preparing single-cell multi-omics data sets to
infer the hair cell gene-regulatory network
We used two single-cell data sets from developing mouse outer
hair cells (30, 31) to predict the consensus hair cell gene-
regulatory network. First, we collected the normalized gene
expression values from the original scRNA-seq study (30) and
then used reciprocal PCA to integrate single cells across four time-
points of sensory epithelium development into a single data set in
Seurat (71) (v3.1.4). Then, we used Slingshot (6) (v1.0.0) to infer
pseudotime values across the outer hair cell trajectory and ap-
plied LOESS regressions and GAMs to select the genes that were
differentially expressed across both the sensory epithelium and
pseudotime, respectively. We again selected all differentially ex-
pressed transcription factors (P<0.01 after Bonferroni correction
for multiple-hypothesis testing) and 500 additional genes with
the highest variance and used the integrated gene expression as-
say in Seurat to generate the corresponding gene coexpression
matrices. In a separate analysis, we broadened our selection cri-
teria to encompass all genes that were differentially expressed
in at least 20% of the outer hair cells, regardless of their expression
across the full sensory epithelium.
For the scATAC-seq data set, we first collected the cell-by-peak
chromatin accessibility data from the original study (31). Then,
we used the function createGmatFromMat in SnapATAC (72)
(v1.0.0) to calculate the cell-by-gene accessibility scores as the
counts of each 5 kb bin per gene in the UCSC mouse genome
mm10 (73) (TxDb.Mmusculus.UCSC.mm10.knownGene; v3.4.4)
that contained at least one open-chromatin peak for a given cell.
These values were then log-normalized. We again used Slingshot
to infer pseudotime values across the outer hair cell trajectory
and applied GAMs to the raw accessibility counts to select the dif-
ferentially accessible genes across pseudotime. For the inferred
scATAC-seq network, we selected all differentially accessible tran-
scription factors and variable genes (Padjusted<0.01) that were also
differentially expressed along the scRNA-seq trajectory. Because
the scATAC-seq data set had fewer cells than the scRNA-seq data
set, we used 24 fixed-width bins in each dimension to generate
the corresponding gene coaccessibility matrices prior
to
fine-tuning.
Discriminative motif analysis to discover de novo
transcription factor-binding motifs
We used the UCSC mouse genome mm10 and twoBitToFa to
download the 100 kb enhancer sequences spanning 50 kb up-
stream and downstream of all target genes’ transcription start
sites in the transcription factor-only hair cell gene-regulatory net-
work and then divided them into 100 bp fragments and sorted the
resulting sequences into primary (predicted targets) and control
(predicted no interaction) groups for each transcription factor
with at least one target gene in the network. We then used
STREME (74) (v5.4.1) to perform discriminative motif analysis
with a P value threshold of 0.05 to identify enriched motifs in pre-
dicted target genes’ enhancers, which we then compared with ei-
ther the transcription factors’ known binding motifs from CIS-BP
(34), or to all motifs from the JASPAR (75), UniPROBE (76) (mouse),
and Jolma et al. (77) databases using TOMTOM (78) (v5.4.1) with an
E value threshold of 10 for significant alignments.
Acknowledgments
The authors would like to acknowledge Junyue Cao, Viviana Risca, and
Christina Leslie, as well as Adrian Jacobo, Agnik Dasgupta, Emily Atlas,
and other members of the Laboratory of Sensory Neuroscience for
helpful discussions and comments on the manuscript.
Supplementary material
Supplementary material is available at PNAS Nexus online.
Funding
Reagor et al.
| 11
Author contributions
C.C.R. and N.V. conceived the study, and all authors designed the
analysis. C.C.R. carried out all experiments and analysis and
wrote the paper. A.J.H. supervised the project, and all the authors
edited the paper.
Data availability
The processed experimental files for all single-cell data sets used
in this study are available on Zenodo at https://doi.org/10.5281/
zenodo.7474099; Table 1 lists the Gene Expression Omnibus
(GEO) accession numbers for each data set. The saved model
weights for DELAY are available on Zenodo at https://doi.org/10.
5281/zenodo.7474115. All experimental logs from this study
are available at https://tensorboard.dev/experiment/RBVBetLM
RDiEvO7sBl452A. We have provided an open-source implementa-
tion of DELAY in PyTorch with listed requirements and documen-
tation at https://github.com/calebclayreagor/DELAY.
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10.1371_journal.pone.0294847.pdf
|
Data Availability Statement: All relevant data are
within the paper and its Supporting information
files.
|
Data Availability Statement: All relevant data are within the paper and its Supporting information files. Funding: The ATL1102 in DMD clinical trial was funded in its entirety by the sponsor Antisense Therapeutics Ltd. Authors Ms Desem and Dr Tachas are employees of the sponsor and so received payment for services from the sponsor as employees. Ms. Desem and Dr Tachas hold an equity interest in the sponsor. Dr Tachas and Ms Desem along with other sponsor employees and sub-contracted specialists were involved in the study design and data analysis. Authors Dr Woodcock and Dr Ryan were at the time of the trial employees of the Royal Children's Hospital and Murdoch Children's Research Institute and are not affiliated with the sponsor in any way and have not received any direct personal payment or honoraria from the sponsors, nor do they or their family members hold a financial interest or stock in the sponsor company. Dr Woodcock is still an employee of the above institutions, but Dr Ryan has since left the employment to take up public office. Dr Woodcock and Dr Ryan were involved in the trial design as unpaid consultants. As this was a clinical trial, publication was always planned from trial inception. No employees of the sponsor were involved in the data collection, although Ms Desem did liaise closely with the MCRI/RCH site staff and Clinical Trial Organisation throughout the trial. Author Dr Button was paid for services as the study statistician. None of the other authors received any payment from the sponsor to conduct this study. All other authors had input into writing or revising this manuscript. ATL1102 is a second-generation immunomodulatory 2'MOE gapmer antisense oligonucleotide which specifically targets human CD49d RNA. After binding to the RNA of CD49d, intracellular RNase H attaches resulting in downregulation of CD49d RNA. ATL1102 has previously been trialled to treat Relapsing Remitting Multiple Sclerosis (RRMS), noting that CD49d high expressing T cells are the effector and central memory T cells in RRMS. In this phase 2 RRMS clinical trial, ATL1102 dosed 200mg three times weekly in the first week and twice weekly to 8 weeks substantially reduced inflammatory brain lesions by 88.5% and circulating lymphocytes and T lymphocytes by 25% [10] . Reported here, collaborators from the same institution ran two separate but complementary studies. The initial trial, a phase 2 clinical trial examining for the first time the safety and efficacy of a low dose ATL1102 treatment for 24 weeks in non-ambulant patients with DMD on concomitant corticosteroid treatment. The second, a pre-clinical study in the mdx mouse model for DMD, conducted using a mouse specific second generation CD49d ASO (ISIS 348574) to show that monotherapy treatment can reduce CD49d mRNA expression in muscle and decrease contraction induced muscle damage.
|
RESEARCH ARTICLE
A phase 2 open-label study of the safety and
efficacy of weekly dosing of ATL1102 in
patients with non-ambulatory Duchenne
muscular dystrophy and pharmacology in
mdx mice
1,2,3*, George Tachas4, Nuket Desem4, Peter J. Houweling2,3,
Ian R. WoodcockID
Michael Kean5, Jaiman Emmanuel5, Rachel KennedyID
1,2,6, Kate Carroll1,2, Katy de
Valle1,2,6, Justine Adams2, Shireen R. Lamande´ 2,3, Chantal Coles2, Chrystal Tiong2,
Matthew Burton2, Daniella Villano1, Peter Button7, Jean-Yves Hogrel8, Sarah Catling-
Seyffer1,2, Monique M. Ryan1,2,3, Martin B. Delatycki9,10, Eppie M. Yiu1,2,3
1 Department of Neurology, The Royal Children’s Hospital, Melbourne, Australia, 2 The Murdoch Children’s
Research Institute, Melbourne, Australia, 3 Department of Paediatrics, University of Melbourne, Melbourne,
Australia, 4 Antisense Therapeutics Ltd, Melbourne, Australia, 5 Department of Medical Imaging, The Royal
Children’s Hospital, Melbourne, Australia, 6 Department of Physiotherapy, University of Melbourne,
Melbourne, Australia, 7 McCloud Consulting Group, Sydney, Australia, 8 Institut de Myologie, GH Pitie´ -
Salpêtrière, Paris, France, 9 Victorian Clinical Genetics Service, Melbourne, Australia, 10 Murdoch
Children’s Research Institute, Bruce Lefroy Centre for Genetic Health Research, Melbourne, Australia
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
OPEN ACCESS
* [email protected]
Citation: Woodcock IR, Tachas G, Desem N,
Houweling PJ, Kean M, Emmanuel J, et al. (2024)
A phase 2 open-label study of the safety and
efficacy of weekly dosing of ATL1102 in patients
with non-ambulatory Duchenne muscular
dystrophy and pharmacology in mdx mice. PLoS
ONE 19(1): e0294847. https://doi.org/10.1371/
journal.pone.0294847
Editor: Julie Dumonceaux, UCL: University College
London, UNITED KINGDOM
Received: June 29, 2023
Accepted: October 19, 2023
Published: January 25, 2024
Peer Review History: PLOS recognizes the
benefits of transparency in the peer review
process; therefore, we enable the publication of
all of the content of peer review and author
responses alongside final, published articles. The
editorial history of this article is available here:
https://doi.org/10.1371/journal.pone.0294847
Copyright: © 2024 Woodcock et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Abstract
Background
ATL1102 is a 2’MOE gapmer antisense oligonucleotide to the CD49d alpha subunit of VLA-
4, inhibiting expression of CD49d on lymphocytes, reducing survival, activation and migra-
tion to sites of inflammation. Children with DMD have dystrophin deficient muscles suscepti-
ble to contraction induced injury, which triggers the immune system, exacerbating muscle
damage. CD49d is a biomarker of disease severity in DMD, with increased numbers of high
CD49d expressing T cells correlating with more severe and progressive weakess, despite
corticosteroid treatment.
Methods
This Phase 2 open label study assessed the safety, efficacy and pharmacokinetic profile of
ATL1102 administered as 25 mg weekly by subcutaneous injection for 24 weeks in 9 non-
ambulatory boys with DMD aged 10–18 years. The main objective was to assess safety and
tolerability of ATL1102. Secondary objectives included the effect of ATL1102 on lymphocyte
numbers in the blood, functional changes in upper limb function as assessed by Perfor-
mance of Upper Limb test (PUL 2.0) and upper limb strength using MyoGrip and MyoPinch
compared to baseline.
PLOS ONE | https://doi.org/10.1371/journal.pone.0294847 January 25, 2024
1 / 16
PLOS ONEData Availability Statement: All relevant data are
within the paper and its Supporting information
files.
Funding: The ATL1102 in DMD clinical trial was
funded in its entirety by the sponsor Antisense
Therapeutics Ltd. Authors Ms Desem and Dr
Tachas are employees of the sponsor and so
received payment for services from the sponsor as
employees. Ms. Desem and Dr Tachas hold an
equity interest in the sponsor. Dr Tachas and Ms
Desem along with other sponsor employees and
sub-contracted specialists were involved in the
study design and data analysis. Authors Dr
Woodcock and Dr Ryan were at the time of the trial
employees of the Royal Children’s Hospital and
Murdoch Children’s Research Institute and are not
affiliated with the sponsor in any way and have not
received any direct personal payment or honoraria
from the sponsors, nor do they or their family
members hold a financial interest or stock in the
sponsor company. Dr Woodcock is still an
employee of the above institutions, but Dr Ryan
has since left the employment to take up public
office. Dr Woodcock and Dr Ryan were involved in
the trial design as unpaid consultants. As this was
a clinical trial, publication was always planned from
trial inception. No employees of the sponsor were
involved in the data collection, although Ms Desem
did liaise closely with the MCRI/RCH site staff and
Clinical Trial Organisation throughout the trial.
Author Dr Button was paid for services as the
study statistician. None of the other authors
received any payment from the sponsor to conduct
this study. All other authors had input into writing
or revising this manuscript.
Competing interests: The ATL1102 in DMD clinical
trial was funded in its entirety by the commercial
sponsor Antisense Therapeutics Ltd. Antisense
Therapeutics Ltd is a publicly traded company,
listed on the Australian ASX. At the time of the trial,
authors Ms Desem and Dr Tachas were employees
of the sponsor and so received payment for
services from the sponsor as employees. Ms.
Desem and Dr Tachas hold an equity interest in the
sponsor. Dr Tachas and Ms Desem along with
other sponsor employees and sub-contracted
specialists were involved in the study design and
data analysis. Ms Desem has since left the
company and no longer is employed by the
sponsor. Authors Dr Woodcock and Dr Ryan were
at the time of the trial employees of the Royal
Children’s Hospital and Murdoch Children’s
Research Institute and are not affiliated with the
sponsor in any way and have not received any
direct personal payment or honoraria from the
sponsors, nor do they or their family members
Phase 2 clinical trial of ATL1102 in non-ambulatory DMD
Results
Eight out of nine participants were on a stable dose of corticosteroids. ATL1102 was gener-
ally safe and well tolerated. No serious adverse events were reported. There were no partici-
pant withdrawals from the study. The most commonly reported adverse events were
injection site erythema and skin discoloration. There was no statistically significant change
in lymphocyte count from baseline to week 8, 12 or 24 of dosing however, the CD3+CD49d+
T lymphocytes were statistically significantly higher at week 28 compared to week 24, four
weeks past the last dose (mean change 0.40x109/L 95%CI 0.05, 0.74; p = 0.030). Func-
tional muscle strength, as measured by the PUL2.0, EK2 and Myoset grip and pinch mea-
sures, and MRI fat fraction of the forearm muscles were stable throughout the trial period.
Conclusion
ATL1102, a novel antisense drug being developed for the treatment of inflammation that
exacerbates muscle fibre damage in DMD, appears to be safe and well tolerated in non-
ambulant boys with DMD. The apparent stabilisation observed on multiple muscle disease
progression parameters assessed over the study duration support the continued develop-
ment of ATL1102 for the treatment of DMD.
Trial registration
Clinical Trial Registration. Australian New Zealand Clinical Trials Registry Number:
ACTRN12618000970246.
Introduction
Duchenne muscular dystrophy (DMD), a severe, progressive, X-linked genetic muscle disease
is the most common muscle disorder in boys, affecting 1 in 5000 live male births worldwide
[1]. Boys with DMD have onset of progressive muscle weakness in the first decade of life, with
death due to cardiorespiratory failure expected in the late third or early fourth decades [2].
Currently the only disease modifying medical treatment is corticosteroid therapy, which delays
loss of ambulation by a median 3 years, to 13 years of age [3–5] but carries a significant treat-
ment burden of adverse effects [5].
DMD is associated with absence of dystrophin from muscle. This causes increased suscepti-
bility to contraction-induced muscle damage, with activation of the innate immune macro-
phages in turn activating the adaptive immune system T lymphocytes, leading to upregulation
of pro-inflammatory cytokines, including the extracellular structural protein osteopontin,
resulting in chronic inflammation, fibrosis and reduced muscle strength [6]. CD49d, the alpha
chain subunit of integrin very late antigen 4 (VLA-4) is expressed widely on immune cells in
this cascade and can bind osteopontin [7].In patients with DMD, the number of CD49d high
expressing T lymphocytes is inversely proportional to ambulation speed, with highest concen-
tration seen in non-ambulant patients [8]. Patients with higher concentrations have more
severe weakness and are more likely to lose ambulation before 10 yrs of age despite corticoste-
roid use, suggesting CD49d may be a biomarker of disease severity or activity [9]. In ex vivo
studies a monoclonal antibody to VLA-4 prevented patient T-cell binding to muscle cells and
transendothelial migration, highlighting a potential therapeutic avenue [9].
PLOS ONE | https://doi.org/10.1371/journal.pone.0294847 January 25, 2024
2 / 16
PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
hold a financial interest or stock in the sponsor
company. Dr Woodcock is still an employee of the
above institutions, but Dr Ryan has since left the
employment to take up public office as a Member
of the Australian Parliament. Dr Woodcock and Dr
Ryan were involved in the trial design as unpaid
consultants. Dr Woodcock has received honoraria
for work performed including educational activities
and attendance at advisory board meetings from
pharmaceutical companies Biogen, Novartis,
Roche and Avidity and an educational travel
bursary to attend an international conference in
2016 from Biogen. Dr Woodcock has received
grants for research work from FSHD Global
Research Foundation, FSHD Society and Fulcrum
Therapeutics. Dr Woodcock has been principal
investigator on a number of industry-sponsored
clinical trials. None of these disclosures affected
the work Dr Woodcock performed on this clinical
trial. Dr Ryan has received honoraria for work
performed including educational activities and
attendance at advisory board meetings from
pharmaceutical companies Biogen, Novartis,
Roche. Dr Ryan has been principal investigator on
a number of industry-sponsored clinical trials.
None of these disclosures affected the work Dr
Ryan performed on this clinical trial. Dr Yiu has
received advisory board honoraria from Biogen and
Roche, and has received research support from
Biogen, Roche, Pfizer and PTC therapeutics
unrelated to the content of this manuscript. Dr Yiu
has been principal investigator on a number of
industry-sponsored clinical trials. None of these
disclosures affected the work Dr Yiu performed on
this clinical trial. Prof. Delatycki has received grant
awards from NHMRC and is principal investigator
in industry sponsored clinical trials including trials
sponsored by Rearta and PTC. As this was a
clinical trial, publication was always planned from
trial inception. No employees of the sponsor were
involved in the data collection, although Ms Desem
did liaise closely with the MCRI/RCH site staff and
Clinical Trial Organisation throughout the trial. As
the study statistician, author Dr Button was paid a
consultancy fee for his services from the trial
sponsor commercial company Antisense
Therapeutics Ltd. Authors Dr Houweling, Dr Coles
and Dr Tiong were recipients of a grant to perform
the MDX studies. This grant was paid by the
sponsor Antisense Therapeutics Ltd. None of the
other authors received any payment from the
sponsor to conduct this study. All other authors
had input into writing or revising this manuscript.
The authors confirm that the involvement of
employees of the sponsor Antisense Therapeutics
Ltd in the trial design, data analysis and decision to
ATL1102 is a second-generation immunomodulatory 2’MOE gapmer antisense oligonucle-
otide which specifically targets human CD49d RNA. After binding to the RNA of CD49d,
intracellular RNase H attaches resulting in downregulation of CD49d RNA. ATL1102 has pre-
viously been trialled to treat Relapsing Remitting Multiple Sclerosis (RRMS), noting that
CD49d high expressing T cells are the effector and central memory T cells in RRMS. In this
phase 2 RRMS clinical trial, ATL1102 dosed 200mg three times weekly in the first week and
twice weekly to 8 weeks substantially reduced inflammatory brain lesions by 88.5% and circu-
lating lymphocytes and T lymphocytes by 25% [10].
Reported here, collaborators from the same institution ran two separate but complementary
studies. The initial trial, a phase 2 clinical trial examining for the first time the safety and effi-
cacy of a low dose ATL1102 treatment for 24 weeks in non-ambulant patients with DMD on
concomitant corticosteroid treatment. The second, a pre-clinical study in the mdx mouse
model for DMD, conducted using a mouse specific second generation CD49d ASO (ISIS
348574) to show that monotherapy treatment can reduce CD49d mRNA expression in muscle
and decrease contraction induced muscle damage.
Methods
Ethics statement
The clinical trial received approval from the Royal Children’s Hospital Human Research Ethics
Committee with assigned number HREC/17/RCHM/121. The trial was subsequently regis-
tered at the Australian New Zealand Clinical Trials Registry (ACTRN12618000970246). An
independent Data Safety Monitoring Board (DSMB) was established to provide safety over-
sight for the trial. Participant consent to participate in the trial was sort from parents. Pre-clin-
ical mdx mouse analyses were approved by the Murdoch Children’s Research Institute
(MCRI) animal care and ethics committee (ACEC; approval number A899).
Pre-clinical studies in mice
The mdx mouse model is commonly used to study DMD. We tested efficacy of the second gen-
eration 2’MOE gapmer mouse specific CD49d ASO ISIS 348574 as ATL1102 is specific to
human CD49d RNA and not homologous to mouse. Mdx mice do not have circulating lym-
phocytes with high CD49d but have high CD49d expressing lymphocytes in the lymph nodes
at 9 weeks [11]. Symptomatic 9 week old mdx mice were treated for 6 weeks to determine the
effect of ISIS 348574 on CD49d mRNA expression and muscle function measures.
Male mdx and age matched C57Bl10/J wild-type controls were purchased from the Jackson
laboratories at 5 weeks of age and acclimatised to the MCRI facility for a total of 4 weeks. Ani-
mals were housed in a specific-pathogen-free environment at a constant ambient temperature
of 22˚C and 50% humidity on a 12 h light-dark cycle, with ad libitum access to food and water.
The mdx mice (n = 12 /group) were randomly assigned to 4 treatment groups (saline, low
(5mg/kg) and high (20mg/kg) dose ISIS 348574, and a control gapmer oligonucleotide with
the same 20 nucleotides scrambled such that it is not complementary to CD49d or other RNA
(20mg/kg)). Mdx Mice received weekly subcutaneous injections of either saline, ISIS348574
and control oligonucleotide for a total of 6 weeks. Wild-type controls (n = 12) received saline
only. The high dose (20mg/kg/week) equates to 1.6mg/kg/w dose in human equivalent body
surface area (BSA) and the low dose (5mg/kg/week) equates to 0.4mg/kg/week dose on BSA.
After treatment mice were anaesthetised using inhaled isoflurane (0.6 ml per min) and muscle
function was examined using the Arora Scientific 1300A whole mouse test system and 701C
stimulator as previously published [12]. Mice were then euthanised by cervical dislocation and
the spleen and skeletal muscle (quadriceps) were collected for further analysis.
PLOS ONE | https://doi.org/10.1371/journal.pone.0294847 January 25, 2024
3 / 16
PLOS ONEpublish this data does not alter our adherence to
PLOS ONE policies on sharing data and materials.
Phase 2 clinical trial of ATL1102 in non-ambulatory DMD
Flow cytometry
The mdx spleen was perforated to isolate the splenic sub-cellular content and incubated in red
blood cell lysis buffer (Thermofisher) for ten minutes at 4˚C. Splenocytes were centrifuged
1500 g for five minutes at 4˚C. Cell pellets were washed in wash buffer (PBS:1% BSA (bovine
albumin serum)). CD4+ and CD8+ T cell populations were identified using anti-CD4-V450
(Biolegend, San Diego, CA, USA) and anti-CD8a-allophycocyanin–cyanine 7 (anti-CD8a-
APC-Cy7) (Biolegend, San Diego, CA, USA). Stained cells were analysed using BD LSRFor-
tessa™ X-20 Cell Analyzer to identify populations of CD4+ and CD8+ T cells.
Clinical trial design
This was a phase 2 open-label clinical trial assessing the safety of ATL1102 in non-ambulant
boys with DMD concomitantly with their usual corticosteroid therapy, in all but one partici-
pant who discontinued corticosteroids years prior to the study. CONSORT flow diagram of
study design is shown in Fig 1. Eligibility criteria for the clinical trial are included as S1 Fig.
Participants were recruited from a single site in Melbourne, Australia with the study running
from August 2018 until January 2020.
After providing written informed consent, participants received weekly subcutaneous injec-
tions of 25mg of ATL1102 for twenty-four weeks. Injections were administered into subcuta-
neous fat of the abdomen by a registered nurse or trained parent. Injection sites were rotated
in quadrants around the umbilicus. Parents monitored injection sites for cutaneous reactions
and participant discomfort for fourty-eight hours post-administration. Adverse events were
recorded in a diary which was returned to the study coordinators at each fortnightly visit.
Participants underwent fortnightly venepuncture for exploratory and safety blood tests.
This included monitoring of haematology, biochemistry and inflammatory markers and at
point of care urinalysis dipstick to monitor kidney function. Participants were seen monthly
by the study team for physical examination and respiratory function assessments.
Participant safety was monitored routinely and at regularly scheduled meetings by the inde-
pendent DSMB.
Fig 1. CONSORT flow diagram of study design.
https://doi.org/10.1371/journal.pone.0294847.g001
PLOS ONE | https://doi.org/10.1371/journal.pone.0294847 January 25, 2024
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Outcome measurements
The primary endpoint of the trial was safety of ATL1102 as assessed by the frequency and
intensity of adverse events, including injection site reactions and any laboratory value
derangement.
Secondary outcome measures included both laboratory and functional efficacy endpoints.
Laboratory efficacy outcome measures included lymphocyte-modulation activity determined
by cell surface flow cytometry measuring variation in the number and percentage of total lym-
phocytes as well as those CD4 and CD8 T lymphocytes expressing high levels of CD49d
(CD49dhi) to week twenty-four of treatment and to week twenty-eight, four weeks past the
last treatment.
Changes in upper limb muscle strength and function were measured at baseline and again
at weeks five, eight, twelve and twenty-four. Muscle function was assessed by a questionnaire-
based outcome measure of disease burden (Egen Klassifikation Scale version 2—EK2) and per-
formance-based measures (the Performance of the Upper Limb scale version 2 (PUL 2.0), and
the Moviplate 30 second finger tapping score of the MyoSet tool). The Myoset tool also mea-
sured distal upper limb strength as determined by the MyoPinch (key pinch strength) and
MyoGrip (hand grip strength) scores [13–15]. Other outcome measures assessed were respira-
tory function (forced vital capacity (FVC) and forced expiratory volume in one second
(FEV1)), and quality of life assessed using the neuromuscular module of the Pediatric Quality
of Life Instrument (PedsQL NMD™).
Muscle Magnetic Resonance Imaging (MRI)
Participants underwent MRI of the dominant forearm at baseline, week twelve and week
twenty-four. Unilateral upper-limb MRI was performed at 1.5T (Siemens Aera; Siemens,
Erlangen, Germany) using a flexible surface matrix coil (4-Channel Flex Coil) wrapped around
the forearm. Participants lay in the scanner in the head-first supine position, with the arm to
be imaged lying in a comfortable position on the scanner bed alongside the torso. Two point-
Dixon images were acquired (3D gradient-echo TE1/TE2/TR = 2.39/4.44/6.99ms, flip angle
10˚, nine 6mm axial slices, slice gap 0mm, FOV 18x18cm, matrix 320×320, pixel size
0.56×0.56mm, NEX = 4). Fat fraction maps were obtained using on scanner tools.
Change over time in muscle composition (atrophy, oedema and fatty infiltration) was mea-
sured on the muscles of the central, proximal, and distal forearm using Short Tau Inversion
Recovery (STIR) and 3-point Dixon sequences on MRI. Changes in muscle composition were
scored using the semi-quantitative visual scoring Mercuri method and by quantitative fat frac-
tion analysis [16–18]. Due to fatty infiltration, identification of individual muscles was chal-
lenging, such that a compartment composite score of volar, dorsal and ECRLB Br (extensor
carpi radialis longus/brevis and brachioradialis) compartments was used as per a previous
published study [19]. The lean muscle mass was calculated using previously published meth-
ods: Cross-sectional muscle compartment area x ((100 –total muscle compartment fat percent)
/ 100) [19].
Statistical analysis
Based upon data from a previous study of ATL1102 in RRMS patients analyzing blood 3 days
after the last dose in week 8, the laboratory efficacy end point of lymphocyte modulation
potential was established as a reduction in total lymphocyte count of 0.47x109/L (25% reduc-
tion) [10]. For the sample size calculation, the level of significance was set to 0.05 with a
2-sided paired t-test, mean difference of 0.47 (x109/L) from baseline to end of treatment, and
standard deviation of 0.428 (x109/L). Using nQuery (Version 8.5.2.0, Table MOT1-1 Paired t-
PLOS ONE | https://doi.org/10.1371/journal.pone.0294847 January 25, 2024
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
test for differences in means, Statistical Solutions Ltd.), a sample size of 9 participants was cal-
culated as required to achieve a power of 80%. Nine participants were considered sufficient to
investigate the safety, tolerability and PK and PD profile of ATL1102 in this rare target patient
population. Data were analysed using SAS1 Version 9.4. primary and secondary efficacy mea-
sures were analysed using the paired t-test and the non-parametric Wilcoxon sign-rank test.
The study was not powered to see a change on the secondary efficacy endpoints from baseline
to end of treatment. The study protocol and statistical analysis plan are available as supplemen-
tary data in “Protocol” and eSAP1 and eSAP2 respectively. Repeated measures analysis of lym-
phocytes and T lymphocyte and NK lymphocyte subsets in a post hoc analysis was conducted
comparing baseline to a linear combination of values measured three days post-dose at weeks
8, 12 and 24. Associations between variables was tested using a Pearson correlation test.
Preclinical mdx mouse analyses were performed in Graphpad Prism (V9, Graphpad Soft-
ware Inc.). For in situ muscle function, one-way ANOVA with Tukey correction for multiple
testing was performed (n = 9 animals / treatment). Unpaired T-Tests were used for CD4 and
CD8 T-cell analyses (n = 5–6 samples / treatment). All data shown as mean with 95% confi-
dence intervals, unless otherwise stated in the figure legends.
Results
Proof of concept preclinical study using mdx mice
Ex vivo analyses of monocytes collected from mdx mice (n = 3), showed that the ASO to
mouse CD49d, ISIS 348574 can reduce the expression of CD49d mRNA (Fig 2A). We then
examined the in vivo response to ISIS 348574 in mdx mice treated for 6 weeks which showed
that CD49d mRNA expression was reduced in skeletal muscle by approximately 40% when
treated with either a low (5mg/kg/week) or high (20mg/kg/week) dose of ISIS 348574, com-
pared to saline controls (Fig 2B, One-way ANOVA, summary p<0.01, with Tukey correction
displayed on the graphs, p = * <0.05, ** <0.01).
This study also found that mdx mice treated with the 20mg/kg/week dose of ISIS 348574
showed a reduction in the percentage of splenic CD4+ (30%, p<0.05) and CD8+ (21%,
p = 0.058) T lymphocytes, compared to saline treated mice (Fig 2C and 2D). Furthermore in
situ muscle funcation analyses show that the high dose (20mg/kg/week) treated mdx mice
were protected from the effects of eccentric muscle damage, producing 72% of the original
muscle force (P<0.01). This was in contrast to mdx mice treated with either saline, scrambled
control or low dose (5mg/kg) ISIS 348574, which generated approximately 50% of the original
force following eccentric muscle contractions. (Fig 2E and 2F, One-way ANOVA summary
p = <0.001, with Tukey correction displayed on the graphs, p = * <0.05, ** <0.01,
*** <0.001).
Clinical trial results
Eleven adolescent males with DMD were screened for participation. All had been non-ambu-
lant for at least six months prior to screening. Two screened participants were excluded (one
participant had started cardioprotective medication within three months of the initial visit and
the other participant exceeded the pre-determined weight limit for inclusion).
Nine participants were enrolled into the open-label study. All had a confirmed pathogenic
variant in DMD, with a clinical phenotype consistent with DMD as assessed by their treating/
referring clinician and the study investigator. Participant demographics are summarized in
Table 1.
Safety. There were no serious adverse events (SAEs) or suspected or unexpected serious
adverse reactions (SUSARs). A total of 136 adverse events were recorded (Table 2), with all
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Fig 2. Pre-clinical data using the mdx mouse model of DMD to test the effects of ISIS 348574 (mouse specific
Cd49d oligonucleotide to ATL 1102) in vivo. A) Monocytes were isolated from the spleens of mdx mice (n = 3) and
exposed to a single dose of ISIS 348574 for 48hrs in vitro to show that we could achieve a reduction in CD49d mRNA
using ISIS 348574 to mouse CD49d RNA. B) Following 6 weeks of treatment CD49d mRNA expression was reduced in
mice treated with either the low (5mg/kg/week) or high (20mg/kg/week) dose of ISIS 348574, compared to saline
controls (One-way ANOVA with Tukey correction, p = * <0.05, ** <0.01). C and D) Proportion of CD4+ and CD8+ T
cells from the spleens of mdx mice with and without ISIS 348574 drug treatment. Cells are expressed as a proportion of
total live cells isolated from the spleen. One way ANOVA with Fishers LSD test, * p < 0.05. E and F) In situ muscle
physiology analyses shows that mdx mice treated with either saline (red, ~45% force recovery), scrambled (grey, ~45%
force recovery) or low dose (orange, ~ 50% force recovery) ISIS 348574 were susceptible to eccentric muscle
contraction damage compared to wild-type (black) controls, whereas the mice treated with a high dose of ISIS 348574
were resistant to the effects of eccentric muscle damage and produced 72% of the original force following the eccentric
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
muscle damaging protocol. This was still significantly less than the 95% force recovery seen in WT mice, however this
improvement in force following a muscle damage protocol suggests that the use of a 20mg/kg/week dose of ISIS 348574
was able to protect the muscles of mdx mice. One-way ANOVA with Fishers LSD test, p = * <0.05, ** <0.01, ***
<0.001), ****<0.0001).
https://doi.org/10.1371/journal.pone.0294847.g002
participants reporting at least one adverse event. Sixty-three percent of the reported adverse
events were injection site related, with all but one participant experiencing transient erythema
within twenty-four hours of the administration of ATL1102. Six (67%) participants had mild
post-inflammatory hyperpigmentation of the skin of their abdomen which was persistent; four
had resolved and two were ongoing but improving at the post completion follow-up study
visit. The hyperpigmentation was noticed in the first participant after receiving eleven weekly
doses of ATL1102. The DSMB was made aware and the participant informed consent form
updated. In the five subsequent participants who had a similar reaction it was seen after four to
eleven doses. The hyperpigmentation was not regarded as a clinical safety concern by the
DSMB. Pain, discomfort or atrophy of the subcutaneous tissues were not reported, and there
were no signs of systemic involvement. No participants withdrew from the study. There were
no other significant adverse events felt to be related to ATL1102 or its administration.
Efficacy. Lymphocyte Count: There was no statistically significant decrease in lymphocyte
count from baseline to week eight, week twelve or week twenty-four of dosing (Table 3). There
was no statistically significant decrease in CD49d+CD3+CD8+ or CD49d+CD3+CD4+ T lym-
phocytes seen between baseline, weeks 8, 12 or 24 (Table 3). This 9 participant trial did not
achieve the pre-specified laboratory activity outcome measure of a significant -0.47x109/L
(25% reduction) in total lymphocyte count.
There was, though, a consistent trend toward declines in the mean number of lymphocytes,
and CD49d+ T lymphocytes measured 3 days post-dose at week 8, 12 and 24. The mean num-
ber of CD3+CD49d+ T lymphocytes (i.e. CD3+CD4+ and CD3+CD8+ expressing CD49d)
measured at week 28 was statistically significantly higher compared to end of dosing at week
24 (mean change 0.40x109/L 95%CI 0.05, 0.74; paired T-Test, p = 0.030) (Table 3). Repeated
measures analysis of CD3-CD49d+ NK lymphocytes in a post hoc analysis comparing baseline
to a linear combination of values measured three days post-dose at weeks 8, 12 and 24 was sig-
nificantly lower compared to baseline (p = 0.018), with comparable NK lymphocyte numbers
at week 28 (Fig 3).
Functional outcome measures. There were no statistically significant changes in any
upper limb functional outcome measures at week 24 compared to baseline (Table 4). The
PUL2.0 score remained stable with no significant change between baseline and week twenty-
Table 1. Summary of participant demographics.
Characteristic
Sex
Age (years)
Weight (kg)
Height (cm)
BMI
Time since non-ambulant (years)
Corticosteroid Medication
https://doi.org/10.1371/journal.pone.0294847.t001
Category
Male
Yes
Prednisolone
Deflazacort
Statistic
n (%)
Mean (SD)
Median (range)
Mean (SD)
Mean (SD)
Mean (SD)
Median (range)
n (%)
ATL1102
N = 9
9 (100)
14.9 (2.1)
14.0 (12–18)
52.7 (9.8)
141.1 (10.0)
27.1 (7.4)
2.2 (0.6–9.2)
8 (88.9)
3 (33.3)
5 (55.6)
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Table 2. Treatment emergent adverse events reported in at least two participants.
SYSTEM ORGAN CLASS
Preferred Term
Participants reporting any AEs
All
N = 9
Participants (%) [No. of Events]
9 (100.0%) [136]
GENERAL DISORDERS AND ADMINISTRATION SITE CONDITIONS
Injection site erythema
Injection site pain
Injection site swelling
Injection site bruising
Pyrexia
SKIN AND SUBCUTANEOUS TISSUE DISORDERS
Skin discolouration
GASTROINTESTINAL DISORDERS
Vomiting
Constipation
RESPIRATORY, THORACIC AND MEDIASTINAL DISORDERS
Cough
Nasal congestion
Oropharyngeal pain
INFECTIONS AND INFESTATIONS
Lower respiratory tract infection
Nasopharyngitis
NERVOUS SYSTEM DISORDERS
Migraine
https://doi.org/10.1371/journal.pone.0294847.t002
8 (88.9%) [59]
5 (55.6%) [7]
3 (33.3%) [6]
4 (44.4%) [4]
2 (22.2%) [4]
6 (66.7%) [7]
2 (22.2%) [4]
2 (22.2%) [2]
2 (22.2%) [2]
2 (22.2%) [2]
2 (22.2%) [2]
2 (22.2%) [2]
2 (22.2%) [2]
2 (22.2%) [2]
four with a mean increase in PUL2.0 score of 0.9 (95%CI -1.33, 3.11, where a higher score indi-
cates better function) EK2 scores were stable throughout the trial period. ATL1102 treatment
showed no significant effect on lung function throughout the 24 week trial period (Table 4).
The components of the Myoset all reflected stable grip and pinch strength over the course of
the trial.
Table 3. Summary of lymphocytes mean change from baseline to weeks 24 and 28.
White blood cell type (X109
cells per litre)
Mean Baseline count (x109
cells per litre)
Mean Change from baseline
Median percentage change from
baseline (%)
Paired T-Test
(p value) of mean
change
Lymphocytes
CD3+ T cells
CD3+ CD49d+ T cells
CD4+ T cells
CD4+ CD49d+ T cells
CD8+ T cells
CD8+ CD49d+T cells
Week 8 Week
12
Week
24
Week
28
Week 8 Week
12
Week
24
Week
28
between week 28
and 24
-0.56
-0.53
-0.50
-0.30
-0.28
-0.20
-0.22
-0.53
-0.33
-0.39
-0.20
-0.22
-0.09
-0.12
-0.28
-0.18
-0.28
-0.15
-0.19
-0.02
-0.05
+0.19
+0.25
+0.11
+0.11
+0.01
+0.14
+0.11
-4.63
-10.9
-12.3
-12.3
-12.5
-9.35
-10.9
-7.14
-5.46
-10.0
-5.23
-7.09
-5.21
-7.32
-4.22
+11.81
0.86
+17.11
-9.78
-1.12
-16.7
-2.62
-5.79
+9.93
+16.50
+1.73
+17.99
+13.37
0.051
0.056
0.03*
0.063
0.073
0.068
0.064
3.68
2.93
2.44
1.57
1.20
1.22
1.17
The Lymphocyte mean number of cells at week 24 (at the end of dosing) is trending significantly lower vs week 28 (p = 0.051 paired T test).
*The mean number of CD3+CD49d+T lymphocytes (CD4+CD49d+ and CD8+CD49d+ T lymphocytes) at week 24 is statistically significantly lower vs week 28
(p = 0.030 paired T test).
https://doi.org/10.1371/journal.pone.0294847.t003
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Fig 3. Showing lymphocyte baseline, week 8, 12 and 24 week data 3 days post each dose and the week 28 data, four
week past end of dosing data is shown as a bee swarm plot with mean expression values of lymphocytes.
https://doi.org/10.1371/journal.pone.0294847.g003
MRI.
In this trial, there was some variation in the quality of proximal and distal slices due
to variable positioning of the participant’s forearm in consecutive scans. The quality of the cen-
tral slices through the muscle body in the forearms muscles was not compromised and so this
measurement was chosen for detailed comparison between baseline and week 24 scans for
each participant. No significant change was apparent between baseline and week twenty-four
for the mean Mercuri semi-quantitative score of fatty infiltration (0.1 point change), atrophy
(0 point change) and muscle oedema (0.3 point change) measuring the central slice around the
elbow (Table 5). There was a trend towards minor improvement in the percentage fat fraction
in all muscle groups measuring the central slice, although statistical significance was not
achieved. There was no significant pattern of change in cross-sectional muscle area of any
muscle group (Table 6).
Table 4. Change in functional outcome measures from baseline to week 24.
Change from Baseline to Week 24
MyoGrip (dom)
(% Pred)
MyoPinch (dom)
(Kg)
MyoPinch (dom)
(% Pred)
MoviPlate
Score
(dom)
% Predicted FVC % Predicted PEF EK2*
Patient No.
PUL 2.0
01–001
01–002
01–003
01–004
01–006
01–008
01–009
01–010
01–011
+2
+2
0
+2
-3
+7
0
0
-2
MyoGrip
(dom)
(Kg)
-0.63
0.22
0.68
1.09
-0.27
1.00
-0.33
0.05
0.11
-4.49
0.49
1.02
1.01
-0.60
1.11
-3.75
0.11
-1.31
0.03
-0.02
-0.40
0.37
0.07
0.30
-0.22
0.06
-0.18
-0.62
-0.29
-6.59
2.99
0.94
2.77
-4.97
0.72
-3.63
Mean
Change
(95% CI):
+0.9
(-1.33,
3.11)
+0.2
(-0.25,
0.67)
-0.7
(-2.33, 0.90)
0.0
(-0.18, 0.19)
-1.0
(-3.56, 1.63)
*Higher score = greater disability.
#Reduction in Fat Fraction (%) = improvement.
https://doi.org/10.1371/journal.pone.0294847.t004
-14.0
13.0
-3.0
7.0
8.0
3.0
7.0
-15.0
11.0
1.9
(-6.08,
9.85)
-3.20
-14.8
-9.10
0.80
-6.50
-7.70
-9.10
-0.40
-1.10
6.30
-17.3
8.70
7.20
6.90
-18.2
-4.30
9.20
2.00
+1
+1
+2
+2
-6
-1
+2
-1
+2
-5.68
(-9.60, -1.76)
0.06
(-8.33, 8.44)
0.2
(-1.80,
2.25)
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Table 5. Mercuri visual semi-quantative score in whole forearm compartment from baseline to week 24.
Fatty Infiltration
Atrophy
Oedema
Whole Forearm
Baseline
5.2
1.6
2.6
Wk 24
Change
5.3
1.6
2.9
0.1
0.0
0.3
https://doi.org/10.1371/journal.pone.0294847.t005
Table 6. Change in the MRI Central reading fat fraction, cross sectional area and lean muscle mass from baseline
to week 24.
Mean Change (95% CI) from Screening/Baseline to Week 24
MRI Parameter
Fat Fraction (%)
Volar Muscle
Dorsal Muscles
ECRLB-Br
Average Fat Fraction
Cross Sectional Muscle Area (mm2)
Volar Muscle
Dorsal Muscles
ECRLB-Br
Total Area
Lean Muscle Mass (mm2)
N
MRI Central Reading Mean (95%CI)
9
9
9
9
9
9
9
9
9
-0.57 (-7.81, 6.68)
-0.88 (-3.41, 1.65)
-0.12 (-6.42, 6.17)
-0.52 (-5.62, 4.58)
22.78 (-31.2,76.73)
0.89 (-18.9,20.65)
-1.33 (-8.94, 6.28)
22.33 (-36.8,81.42)
13.9 (72.6, 100.4)
ECRLB-Br = extensor carpi radialis longus/brevis and brachioradialis. Volar Muscles; flexor digitorum profundus
and flexor pollicis longus (FDP), flexor digitorum superficialis and palmaris longus (FDS), flexor carpi ulnaris (FCU),
flexor carpi radialis (FCR). Dorsal Muscles: Extensor carpi ulnaris (ECU), extensor digiti minimi (EDM), extensor
digitorum (ED), extensor pollicis longus (EPL), abductor pollicis longus (APL), extensor carpi radialis longus/brevis
and brachioradialis (ECRLB-Br), but the ECRL-BR are not included in the Dorsal muscle measurement in the
Central Reading. Change in the MRI Proximal reading average Fat Fraction (%) from baseline to week 24 was -2.14
[95%CI -7.60; 3.3] for the 9 patients.
https://doi.org/10.1371/journal.pone.0294847.t006
Correlation of parameters assessed in the Phase 2 study. Correlation analyses were per-
formed across assessment measures PUL2.0, Myoset and MRI.
Positive correlations were observed in the Phase 2 study between the different measures of
muscle function of Moviplate scores and the PUL 2.0 scores of the distal domain (r = 0.664)
which support the consistency of the observed changes across the measures assessed in the
study over the 24 week ATL1102 treatment period (S2 Fig).
Positive correlations were also observed in the Phase 2 study between the MRI results of the
lean muscle area (non-fat) and MyoGrip results (r = 0.604), suggesting a consistency of results
across the different parameters of muscle structure and muscle strength (S3 Fig).
Discussion
Safety
This open-label phase 2 clinical trial met its primary safety end point. All but one participant
experienced post-injection site erythema, swelling or discomfort suggesting that the investi-
gation product is a mild irritant, as has been observed with other MOE antisense drugs, and
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
is commonly reported with subcutaneiously injected drugs. Future clinical trials of ATL1102
could consider including using ice as a pre-injection site treatment to minimise these reac-
tions. Six participants experienced an unexpected post-inflammatory skin hyperpigmenta-
tion which resolved or faded at the completion of the study. Interestingly this reaction has
not been previously reported in other clinical trials of ATL1102 and was not viewed as a
safety concern [10].
The dose chosen for this 24 week trial (25mg/week) was considered as a presumed safe dose
in this patient population. In a previous phase 2 trial in individuals with RRMS a loading dose
of 200mg every other day for one week was administered then 400mg/week (twice weekly
200mg) for seven weeks [10]. This DMD trial was the first clinical trial to investigate the safety
of ATL1102 over a six-month period.
Lymphocyte modulation
Given the previously observed action of ATL1102 of reducing lymphocytes in the RRMS
study, the trial sample size was calculated to see a 25% reduction in total lymphocyte count
when the drug is at equilibrium from week 8. This activity endpoint was not met in this trial.
There was however a consistent trend toward declines in the mean number of lymphocytes at
week 8, 12 and 24 each measured 3 days past dosing, and statistically significant reductions in
the mean number of CD49d+ NK lymphocytes at week 8, 12 and 24 weeks of treatment, using
repeated measures analysis. The mean number of CD49d+ T lymphocytes (i.e CD3+CD4
+ and CD3+CD8+ that are CD49d+) was statistically significantly higher at week 28 compared
to week 24, indicating a rebound elevation of CD49d+ T lymphocytes four weeks post the last
treatment dose. These results collectively suggest that ATL1102 suppresses CD49d expressing
lymphocytes at a dose of 25mg per week. It is anticipated that higher doses will increase the
level of lymphocyte reduction whilst maintaining a favourable safety profile in part due to
sparing of the majority of T lymphocytes and NK lymphocytes. Future studies will look at dose
escalation as supported by this study, and modelling with ATL1102.
PUL2.0 and EK2 upper limb function
PUL2.0 measures shoulder, elbow, and wrist finger dimensions of disease burden and is a reli-
able measure of disease severity and progression in DMD where a lower score indicates loss of
function. The mean increase from baseline to week twenty-four in the PUL2.0 was 0.9 (95% CI
-1.33 to 3.11). Although the Minimal Clinical Important Difference (MCID) for the PUL2.0
has not been established, an external historical cohort with same inclusion criteria as in the
ATL1102 phase 2 trial, showed a decrease in PUL2.0 score of 2.0 (standard deviation 3.02)
from baseline over a six month period [20]. In the ATL1102 phase 2 study four of the nine
patients achieved an increase in their PUL2.0 score of +2, and another three patients were sta-
bilized in the PUL2.0 score (Table 4). This is an encouraging trend that warrants further inves-
tigation. A previously published data from a historical cohort also reported that over a twelve
month period a mean decrease in PUL2.0 score of 2.17 can occur, albeit in a cohort not
directly comparable to the participants in the phase 2 study due to older age and larger propor-
tion not on corticosteroids [21].
There was no change in the EK2 over the course of the trial period. This composite outcome
measure encompasses multiple aspects of disease burden and as such is a useful clinical moni-
toring tool (higher score equals greater disease burden) but is not likely to be as responsive as
the PUL2.0 measure to small changes in upper limb function. As such, a stabilisation over the
six month trial periods is encouraging and needs to be confirmed in future studies.
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Myoset tests: MoviPlate, MyoGrip, and MyoPinch
The MyoSet functional outcome measures consist of the MoviPlate muscle function assess-
ment of repetitive flexion extension of the wrist and fingers, and MyoGrip and MyoPinch
assessment of muscle grip and pinch strength [13,14]. These measures have been validated for
use in clinical trials of DMD; MyoGrip and MyoPinch in particular have been shown to be
sensitive to change in non-ambulant boys and to correlate well with lean muscle mass on MRI
[15]. There was no change in any of these measures over the trial period. Previous natural his-
tory studies have shown significant deterioration over six months (Grip -0.5kg [95%CI -1.01;
0.002] and Pinch -0.38kg [95%CI -0.53; -0.22]) [15,18]. Matching the MyoGrip and MyoPinch
protocol with that of a previously published natural history cohort allowed for comparison of
change in grip and pinch strength over a six month period, yielding a statistically significant
improvement on grip (p = 0.03) and pinch (p = 0.003) strength [19]. The lack of decline in
these measures with ATL1102 during the trial period is once again encouraging and warrants
further investigation.
MRI of upper limb
Magnetic Resonance Imaging of muscle is increasingly used as a biomarker for disease stage
and progression. The most widely used scoring method is the Mercuri Score, which requires a
skilful investigator to visually score the chosen muscles based upon a standardised set of crite-
ria encompassing degree of atrophy, oedematous changes and fatty infiltration of the muscle,
to create an aggregate score. The more recent development of automated fat fraction analysis
reduces the inter-user variability and provides a more quantitative measure of assessment.
Matching the MRI protocol with that of a previously published natural history cohort allowed
for direct comparison of change in fat fraction over a six month period [19]. From this pub-
lished natural history data, disease is expected to progress with a mean increase of central fore-
arm muscle fat fraction percentage of 3.9% (95%CI 1.9,5.7) over six months. The apparent
trend towards a decrease in mean forearm muscle fat fraction of 0.52% (95% CI -5.62, 4.58;
Median 1.4%) seen after six months of treatment with ATL1102 may suggest that ATL1102
could be modifying the rate of fatty infiltration into these muscles. These changes were repli-
cated in the proximal and distal muscle groups. For future MRI studies it would be important
to set a clear protocol with imaging tags placed over surface landmarks to ensure uniformity of
subsequent scans.
Conclusion
The proof of concept pre-clinical data supports a potential protective effect of an antisense oli-
gonucleotide to CD49d RNA in the mdx mouse model of DMD. This phase 2 open-label clini-
cal trial has shown that ATL1102 has a good safety profile and is well tolerated with minor
injection site reactions the only treatment-related adverse events reported. The positive obser-
vations in functional efficacy outcomes suggesting stabilization, and results compared with
historical natural history data, particularly the PUL2.0, MyoGrip, MyoPinch and MRI fat frac-
tion analysis, justifies the ongoing drug development program of ATL1102 in non-ambulant
boys with DMD and provides a rationale to proceed with larger placebo-controlled studies of
this novel therapeutic agent.
Supporting information
S1 Checklist. TREND statement checklist.
(PDF)
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
S1 Fig. Inclusion and Exclusion criteria for the clinical trial.
(DOCX)
S2 Fig. Scatter Plot showing the association between the Moviplate scores and the PUL 2.0
distal dimension scores over the 24 Week ATL1102 treatment period with a linear regres-
sion line plotted.
(TIF)
S3 Fig. Scatter plot showing the association of the Grip Strength scores and the MRI data
of the forearm lean muscle area (non-fat) over the 24 week ATL1102 treatment period:
The MRI is the determined lean muscle mass compartment across the mid (central) domi-
nant forearm. The linear regression line is also plotted.
(TIF)
S4 Fig. Gating strategy for identification of murine CD4+ and CD8+ T cell populations
isolated from spleen of mdx mice treated with ISIS 348574. A) Singlets (FSC-H vs FSC-A),
B) Live cells (Propidium Iodide vs FSC-A) and C) Lymphocytes (SSC-A vs FSC-A) were gated
to remove doublets, dead cells, debris and large/granular cells. D) Anti-CD4-V450 and anti-
CD8a APC-Cy7 to were used to gate populations of CD4+ and CD8+ T cells.
(TIF)
S5 Fig. Correlation of the Moviplate scores and the PUL 2.0 distal dimension scores over
the 24 Week ATL1102 treatment period.
(TIF)
S6 Fig. Correlation of the Grip Strength scores and the MRI data of the lean muscle area
(non-fat) across the mid (central) dominant forearm over the 24-week ATL1102 treatment
period.
(TIF)
S7 Fig. Table of Participant specific genetic variant within Dystrophin Gene.
(DOCX)
S1 File.
(PDF)
S2 File.
(PDF)
S3 File.
(PDF)
S4 File.
(PDF)
Acknowledgments
The authors wish to acknowledge the contribution of Isabelle Ledoux and Simone Birnbaum
of the Insitute of Myology, Paris, France who provided support with the quality control and
analysis of the MyoSet functional outcome measures; Valeria Ricotti of the Dubowitz Neuro-
muscular Centre, London UK, who provided support on the comparative analysis of the MRI
observations; and Annabell Leske and Vicky Beal and the team at Avance Clinical, Adelaide,
Australia.
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PLOS ONEPhase 2 clinical trial of ATL1102 in non-ambulatory DMD
Author Contributions
Conceptualization: George Tachas, Peter J. Houweling, Monique M. Ryan.
Data curation: Ian R. Woodcock, Peter J. Houweling, Michael Kean, Jaiman Emmanuel.
Formal analysis: Ian R. Woodcock, Nuket Desem, Jaiman Emmanuel, Chantal Coles, Chrystal
Tiong, Peter Button, Jean-Yves Hogrel.
Funding acquisition: George Tachas.
Methodology: Ian R. Woodcock, George Tachas, Peter J. Houweling, Chrystal Tiong, Moni-
que M. Ryan.
Project administration: Ian R. Woodcock, Nuket Desem, Peter J. Houweling, Rachel Ken-
nedy, Kate Carroll, Katy de Valle, Sarah Catling-Seyffer.
Resources: George Tachas, Shireen R. Lamande´.
Software: Michael Kean, Peter Button.
Supervision: Peter J. Houweling, Kate Carroll, Shireen R. Lamande´, Daniella Villano, Moni-
que M. Ryan, Martin B. Delatycki, Eppie M. Yiu.
Writing – original draft: Ian R. Woodcock, George Tachas, Peter J. Houweling, Eppie M. Yiu.
Writing – review & editing: Ian R. Woodcock, George Tachas, Nuket Desem, Peter J. Hou-
weling, Michael Kean, Jaiman Emmanuel, Rachel Kennedy, Kate Carroll, Katy de Valle, Jus-
tine Adams, Shireen R. Lamande´, Chantal Coles, Chrystal Tiong, Matthew Burton, Daniella
Villano, Peter Button, Jean-Yves Hogrel, Sarah Catling-Seyffer, Monique M. Ryan, Martin
B. Delatycki, Eppie M. Yiu.
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10.1107_s2052252522010612.pdf
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research papers
IUCrJ
ISSN 2052-2525
CRYOjEM
Received 17 June 2022
Accepted 3 November 2022
Edited by L. A. Passmore, MRC Laboratory of
Molecular Biology, United Kingdom
Keywords: cryoEM; automated cryoEM data
collection; computer vision; microscope
automation software; machine learning; deep
learning; automation; single-particle cryoEM.
Supporting information: this article has
supporting information at www.iucrj.org
Published under a CC BY 4.0 licence
Learning to automate cryo-electron microscopy
data collection with Ptolemy
Paul T. Kim,a Alex J. Noble,a Anchi Chengb and Tristan Beplera*
aSimons Machine Learning Center, Simons Electron Microscopy Center, New York Structural Biology Center, New York,
NY USA, and bSimons Electron Microscopy Center, New York Structural Biology Center, New York, NY USA.
*Correspondence e-mail: [email protected]
Over the past decade, cryo-electron microscopy (cryoEM) has emerged as an
important method for determining near-native, near-atomic resolution 3D
structures of biological macromolecules. To meet the increasing demand for
cryoEM, automated methods that
improve throughput and efficiency of
microscope operation are needed. Currently, the targeting algorithms provided
by most data-collection software require time-consuming manual tuning of
parameters for each grid, and, in some cases, operators must select targets
completely manually. However, the development of fully automated targeting
algorithms is non-trivial, because images often have low signal-to-noise ratios
and optimal targeting strategies depend on a range of experimental parameters
and macromolecule behaviors that vary between projects and collection
sessions. To address this, Ptolemy provides a pipeline to automate low- and
medium-magnification targeting using a suite of purpose-built computer vision
and machine-learning algorithms,
including mixture models, convolutional
neural networks and U-Nets. Learned models in this pipeline are trained on a
large set of images from real-world cryoEM data-collection sessions, labeled
with locations selected by human operators. These models accurately detect and
classify regions of interest in low- and medium-magnification images, and
generalize to unseen sessions, as well as to images collected on different
microscopes at another facility. This open-source, modular pipeline can be
integrated with existing microscope control software to enable automation of
cryoEM data collection and can serve as a foundation for future cryoEM
automation software.
1. Introduction
Cryo-electron microscopy (cryoEM) is a rapidly growing
method for determining the structure of proteins in near-
native conformations at high resolution (Bai et al., 2015).
CryoEM structure determination typically starts with the
application of a solution containing purified protein to an EM
grid, a holey substrate supported by a thin metal mesh (Cheng
et al., 2015). The sample droplet is then reduced to a thin liquid
film and the grid is plunged into a cryogen, converting the thin
film to a layer of vitrified ice (Egelman, 2016). The grid is then
transferred to a transmission electron microscope (TEM) to
collect high-magnification (high-mag) micrographs of
the
particles suspended in vitreous ice within the holes. Vitreous
ice containing particles is found in windows in the grid termed
‘squares’ [Fig. 1(a)]. Within these squares are circular ‘holes’
[Fig. 1(b)] and particle images are obtained by taking high-
resolution micrographs of the ice within these holes [Fig. 1(c)].
Each micrograph will typically provide numerous individual
2D projections of the protein particles, and these images can
be processed to produce a three-dimensional map of the
protein of interest (Wu & Lander, 2020). Solving a protein
structure to high resolution usually requires tens to many
90 https://doi.org/10.1107/S2052252522010612
IUCrJ (2023). 10, 90–102
research papers
Figure 1
Example square, hole and highest-magnification exposure. Windows in the cryoEM grid containing ice are known as ‘squares’. Within squares are
circular ‘holes’. Highest-magnification exposures are taken within holes. Ideal highest-magnification exposures contain particles (as shown) and have
thin ice.
thousands of
hundreds of
individual randomly oriented
particle projection images which often requires collecting
many thousands of high-quality high-resolution micrographs.
Because EM grid preparation is not a well controlled process,
the locations where highest-magnification data are to be
collected must be identified from a series of successively
increasing magnification images (Chua et al., 2022).
The process of collecting high-magnification data begins by
taking low-magnification images of the grid [Fig. 2(a)], typi-
cally acquired at a pixel size of (cid:2)200–500 nm pixel(cid:3)1. Squares
are selected from these images, and medium-magnification
images [Fig. 2(b)] with a pixel size of (cid:2)10–100 nm pixel(cid:3)1 are
taken within these squares. Holes and subsequent high-
Figure 2
Example low- and medium-magnification images: carbon grid (left) and
gold grid (right). First,
low-magnification images of the grid, where
squares are visible, are acquired at a pixel size of (cid:2)200–500 nm pixel(cid:3)1.
Subsequently, medium-magnification images are acquired at a pixel size
of (cid:2)10–100 nm pixel(cid:3)1 by imaging the regions inside the squares.
magnification collection locations are identified from the
medium-magnification images. Not all squares or holes will be
suitable for collection; the goal is to identify squares and holes
in the grid with vitreous ice of suitable quality, ice that is the
right thickness (typically slightly thicker than the largest
diameter of the particle) and that contains a reasonable
number of particles, ideally oriented in a range of angles
(Noble et al., 2018). Ultimately, the success of a data collection
is determined by the quality of the resulting 3D reconstruc-
tion, which is a function of the number of particles found, the
range of orientation angles present among the 2D projections,
and the maximum resolution and signal-to-noise ratio (SNR)
of the micrographs.
Automated data-collection software such as Leginon
(Carragher et al., 2000; Suloway et al., 2005), SerialEM
(Mastronarde, 2005) or EPU (made by ThermoFisher Scien-
tific) provide several built-in tools for identifying potentially
promising squares and holes. These tools include template-,
correlation- or feature clustering-based image analysis algo-
rithms and automated selection capabilities. However, none of
these tools generalize out-of-the-box across the wide variety
of grids that are encountered in practice. They can struggle to
both detect holes and squares under contaminated or low-
SNR conditions and to reliably prioritize good collection
locations across different macromolecule specimens. This
means that microscope operators must often manually identify
squares in low-magnification images and tune parameters used
for automated targeting of holes in medium-magnification
images (https://em-learning.com). Additionally, existing hole
targeting algorithms fail on a non-trivial percentage of cases,
especially on noisy, contaminated or carbon grids with
minimal contrast variation between the holes and substrate.
Operators are then required to manually target holes in
medium-magnification images which is a labor-intensive task.
The human operator time required for targeting limits the
efficiency of collection on expensive and over-subscribed cryo-
transmission electron microscopes (cryo-TEMs). Additionally,
with increasing detector speeds, automated targeting would
IUCrJ (2023). 10, 90–102
Paul T. Kim et al.
(cid:4) Learning to automate cryoEM data collection with Ptolemy 91
research papers
allow for better utilization of microscope time that is other-
wise wasted waiting for human input. Thus, fully automated
targeting methods are needed to not only reduce the burden
on human operators, but also to increase access and
throughput for the entire scientific research community.
However, human-free automation of cryoEM data collec-
tion is challenging. Many types of EM grids exist, each with
holes and squares of different shapes, sizes and spacings. The
grids themselves are made from different materials (e.g.
carbon or gold), which causes the resulting low- and medium-
magnification images to have very different properties (Fig. S1
of the supporting information). Carbon grids, for example,
have significantly less contrast between collection regions of
interest (ROIs) in holes and background substrate at medium
magnification compared with gold grids (Fig. S1). This is
further complicated by variable sample preparation conditions
leading to variable ice thickness and empty regions of the grid,
along with deformations, contamination and lesions, all of
which introduce visual artifacts (Fig. S1). In addition, cryoEM
images have low SNR, especially at high magnification, and
microscope parameters such as electron beam dose (often
between 40 and 80 e(cid:3) A˚ (cid:3)2) can significantly alter image
properties (Cheng et al., 2015). Furthermore, images at each
magnification level may contain many collection ROIs or none
at all (Lyumkis, 2019). Finally, even if good candidate collec-
tion ROIs are found, it is challenging to find ice containing
many particles with enough diversity of projection orienta-
tions to produce high-quality 3D reconstructions.
In recent years, machine-learning techniques have trans-
formed single-particle cryoEM data analysis. Tools such as
MicAssess (Li et al., 2020) and MicrographCleaner (Sanchez-
Garcia et al., 2020) allow for efficient post-processing of high-
resolution micrographs collected, whereas others such as
Topaz (Bepler et al., 2019), CASSPER (George et al., 2021),
Warp (Tegunov & Cramer, 2019) and crYOLO (Wagner et al.,
2019) use deep learning to automate particle picking and
image denoising. Machine-learning-based 3D reconstruction
algorithms have also emerged, including cryoSPARC (Punjani
et al., 2017) and CryoDRGN (Zhong et al., 2021). These
methods have significantly improved our ability to analyze
high-resolution cryoEM data quickly and thoroughly after
collection. However, comparatively little attention has been
given to accelerating or automating data collection itself.
Yokoyama et al. (2020) recently introduced a machine-
learning method for detection and classification of ROIs in
medium-magnification images, but it requires retraining a
model with an annotated medium-magnification image dataset
for each data-collection session.
To address these challenges in cryoEM data collection, we
present Ptolemy, a pipeline that uses computer vision algo-
rithms and pre-trained convolutional neural networks (CNNs)
to navigate cryoEM grids at low and medium magnification
and determine high-quality targeting locations without human
input. We train the Ptolemy models on large datasets of low-
and medium-magnification images with corresponding
collection locations selected by operators from 55 different
data-collection sessions. These sessions include carbon and
Figure 3
Pipeline overview. High-magnification images are taken from holes in
medium-magnification images, which come from squares
in low-
magnification images. (a) Ptolemy detects, crops and then classifies
squares in low-magnification images, which have a pixel size of
approximately 200–500 nm pixel(cid:3)1. (b) Next, Ptolemy detects, crops
and then classifies holes in subsequent medium-magnification images,
which have a pixel size of approximately 10–100 nm pixel(cid:3)1.
gold holey grids and feature a variety of proteins, grid
conditions, magnifications and electron beam dosages. Rather
than attempting to learn separate models for different grid
types or for different particles, we develop a single unified
pipeline to localize and classify ROIs to approximate user
selection locations in low- and medium-magnification cryoEM
images (Fig. 3).
We demonstrate that Ptolemy can effectively detect and
classify squares and holes in low- and medium-magnification
images. We evaluate these predictions with comparison
against operator-selected locations, while noting that opera-
tors target incompletely. We validate the models by holding-
out entire data-collection sessions to confirm that the models
generalize well to unseen sessions. Additionally, we compare
our medium-magnification localization algorithm to an
existing method (Yokoyama et al., 2020) that performs
this is
medium-magnification localization (in that study,
referred to as low-magnification localization) and show that
our method yields
superior generalization performance.
Finally, a separate companion paper has been published:
‘Fully automated multi-grid CryoEM screening using Smart
Leginon’, where the utility of Ptolemy in real-world collection
cases is demonstrated and analyzed (Cheng et al., 2022).
The Ptolemy source code is freely available for academic
use at (https://github.com/SMLC-NYSBC/ptolemy) under CC
BY-NC 4.0 license. Ptolemy is designed to be modular and to
integrate directly with existing microscope control software.
More information on Ptolemy can be found in Appendix A.
2. Methods
To automate microscope targeting for single-particle cryoEM
data collection, we divide the problem into four sub-problems:
(1) low-magnification square localization, (2) low-magnifica-
92 Paul T. Kim et al.
(cid:4) Learning to automate cryoEM data collection with Ptolemy
IUCrJ (2023). 10, 90–102
tion square classification, (3) medium-magnification hole
localization and (4) medium-magnification hole classification.
For low- and medium-magnification localization, the goal is
to identify all possible collection ROIs: squares in low
magnification and holes
in medium magnification. The
cropped ROIs are then fed into separate classification models
at each level that determine whether these ROIs should be
collected. Low-magnification localization is solved by pixel-
wise image segmentation using a mixture model, whereas
medium-magnification localization is solved using a U-Net
with a novel lattice-fitting algorithm (Gupta & Sortrakul, 1998;
Ronneberger et al., 2015). Classification at low magnification is
achieved using a feedforward CNN whereas medium-magni-
fication classification uses the U-Net localization probabilities
because they outperformed a separate downstream classifier
in our experiments. Training and hyperparameter information
for all trained models can be found in Appendix B.
2.1. Datasets and splits
The data used to train and validate all models and algo-
rithms come from 55 cryoEM data-collection sessions
the Simons Electron Microscopy Center
performed at
(SEMC), a center within the New York Structural Biology
Center (NYSBC), from 2018 to 2021. The sessions include gold
and carbon grids, featuring regularly spaced and lacey holes,
with tilted and untilted collection. Lacey-hole grids and tilted
collection images were only used for low-magnification
(square) localization and classification. Positive labels repre-
sent targeted selection locations used in these sessions. All
labeled squares are manual operator selections on the low-
magnification images. On the other hand, labeled holes on the
medium-magnification images are generally automated selec-
tions optimized by operators using template-correlation-based
hole localization and ice-thickness-based hole classification. A
minority of labeled holes were also manually selected by
operators. Data-collection sessions generally involve different
samples, preparation methods and microscope settings
(Weissenberger et al., 2021). This results in considerable
variation between sessions in the appearance of collection
locations especially at medium magnification, as well as in the
characteristics that make for good collection locations (Fig.
S1). Therefore, to ensure that our models can generalize to
research papers
unseen data-collection sessions with different experimental
parameters, we primarily use session splits, where a set of
sessions (termed ‘held-out sessions’) are withheld from the
dataset used to train the models (training set). All perfor-
mance metrics are reported from results on these held-out
sessions.
2.2. Square localization
The goal of square localization is to locate all squares
(windows in the grid that may contain imageable ice) in low-
magnification grid images. The input is a low-magnification
image, and the output is a set of rectangular boxes tightly
bounding the squares (Fig. 4). We find these boxes using a
mixture model-based image segmentation algorithm followed
by a geometric algorithm for identifying the aligned minimum
bounding rectangles surrounding each square. Pixels in the
image are first separated into two classes based on pixel
intensity using a Poisson mixture model [Fig. 4(b)] (Forbes,
2018). Mixture model separation works because the distribu-
tion of pixels in the image can be accurately decomposed into
low-intensity pixels coming from the thick grid bars in the
surrounding background and higher-intensity pixels coming
from the much thinner squares (Fig. S2). This approach avoids
the need for a user to set a specific intensity threshold for
identifying squares, which changes from session to session.
Next, we apply a flood filling algorithm to identify discrete
regions from the segmented square pixels and then find a
minimum bounding convex polygon to bound the pixels in
each square [Fig. 4(c)]. Finally, we take advantage of the fact
that the squares are axis-aligned to find the angle (cid:2), for each
low-magnification image where the minimum bounding
rectangles aligned with (cid:2) bounding each minimum bounding
convex polygon have the smallest total area. Formally, we seek
i Ai; (cid:2) for N polygons, where Ai, (cid:2) is the area of the
argmin(cid:2)
minimum bounding rectangle around the ith polygon, aligned
at angle (cid:2). We find this angle (cid:2) using bounded optimization
(Brent, 1973), and the resulting minimum bounding rectangles
are used to obtain aligned crops of the squares in the low-
magnification image [Fig. 4(d)]. This algorithm is applied to
1304 low-magnification images, resulting in 41 000 crops of
squares.
PN
Figure 4
Example of the square localization procedure. (a) Original input image. (b) Mask recovered after segmenting pixels. (c) Finding convex polygons around
the separate regions in the mask. (d) Aligned minimum bounding rectangles around the polygons, used for crops of the images.
IUCrJ (2023). 10, 90–102
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(cid:4) Learning to automate cryoEM data collection with Ptolemy 93
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2.3. Hole localization
The goal of hole localization is to detect all hole locations in
medium-magnification images. However, unlike in square
localization, a mixture model-based segmentation approach
intensities
does not work, because the difference in pixel
between the holes and the surrounding background is negli-
gible, particularly for carbon grids. Some medium-magnifica-
tion images even have ‘inverted’ holes where the pixel
intensity within the hole is lower than the surrounding region
(Fig. 5).
Here, our choice of model is informed by the available data.
Although we do not have a dataset of bounding boxes around
holes, we do have a large dataset of 28k carbon and gold holey
grid medium-magnification images with locations at or near
the center of holes where operators collected high-magnifi-
cation micrographs. Therefore, we seek to learn the hole
centers in each pixel-normalized medium-magnification input
image by training a U-Net model to output a map with the
same dimensions as the input containing 1 at the locations
where the operator collected and 0 everywhere else (Figs. 5
and 6). We choose a U-Net architecture, because the neurons
in the bottleneck layer have large receptive fields, allowing
them to capture needed context, while the output layers use
the information propagated from the bottleneck, as well as
high-resolution features, to find the hole centers. The pixels in
the medium-magnification image are normalized to control for
variance in electron dose.
Additionally, holes are known to lie on a regular square
lattice, so we post-process the output of the U-Net to find the
best fitting lattice. Given the lattice points in the image, we
then crop around those points to extract hole images (Fig. 7).
This helps to extend the predicted map from the U-Net to
capture all holes in the image, not just the holes that the
operators picked, while simultaneously cleaning erroneously
detected regions. We find the lattice from the U-Net output
map by searching pairs of candidate anchor points and
selecting the pair for which the lattice produced by these
anchor points has the smallest pixelwise error against the
output map. We find
argmina; b
XN
i
(cid:3)1 oi (cid:3) li
ð
ð
Þ 1 (cid:3) li
ð
Þ þ (cid:3)2 li (cid:3) oi
Þ lið Þ; oi 2 O; li 2 La; b;
where O is the output of the U-Net, N is the number of pixels
in the image, La, b is the lattice generated by anchor points a
and b, and (cid:3)1 and (cid:3)2 allow us to independently weight the cost
for false positives and false negatives. Candidate anchor point
pairs are found by taking centroids of high-probability regions
in the U-Net output map, and for each centroid, pairing with
Figure 5
Example medium-magnification images. Human operator-selected locations are marked in yellow. The input to the U-Net is the image without any
marking for the selection locations, and the output is a map with a 1 at each pixel where a selection was made and 0 elsewhere. In rare cases (right), holes
can be darker than the surrounding region.
Figure 6
Example hole-center detection without lattice fitting. For some cases, taking the centroids of the high-probability regions predicted by the U-Net is
sufficient. (a) Input image. (b) U-Net output. (c) Centroids from high-probability regions in U-Net output (red).
94 Paul T. Kim et al.
(cid:4) Learning to automate cryoEM data collection with Ptolemy
IUCrJ (2023). 10, 90–102
research papers
Figure 7
Example hole-center detection on a difficult image. On this low-contrast image, lattice fitting extends to missed holes while removing erroneous
detections. (a) Input image. (b) U-Net output. (c) Centroids from high-probability regions in U-Net output (red). Many locations outside holes are
detected incorrectly, and one hole (orange) is missed. (d) Running the optimal-lattice-finding algorithm results in finding lattice anchor points (cyan). (e)
The lattice generated by these anchor points (cyan) results in coverage of all holes and cleans the incorrect detections.
the K closest to other centroids. K trades performance for run
time. Here we use K = 6.
Imposition of a regular square lattice over the U-Net output
causes Ptolemy to be unable to handle tilted data collection
because the tilt causes the hole centers to lie on a parallelo-
gram-shaped (oblique) lattice rather than a regular square
lattice. Support for tilted data collection will be added to a
near-future update of Ptolemy.
To improve training, we apply Gaussian blur to the model
output before computing the loss (Shorten & Khoshgoftaar,
2019). This helps, because the exact location the operator
selects in a hole is noisy: the selection location that is near the
center of the hole but there is often deviation from the exact
center pixel, and the direction and magnitude of displacement
from the center varies between medium-magnification images.
Therefore, this smoothing allows the model to learn the
centers of these holes, rather than having to learn the displa-
cement from the center for every hole image. We also perform
gradient descent on the sigma parameter of the Gaussian blur
simultaneously with training the U-Net weights to allow the
model to learn the optimal level of smoothing over training
time (Fig. S3).
To improve generalization, we apply both random 90(cid:5)
rotation augmentation to the images during training as well as
random inversion of the normalized pixels. Inversion of pixels
is helpful, because for some sessions, particularly with carbon
grids, the pixels in the holes are darker than the background
pixels. Although pixel
inversion augmentation allows for
better carbon grid hole targeting, it does not affect gold grid
images which do not suffer from contrast inversions.
2.4. Square and hole classification models
In square and hole classification, we aim to obtain rankings
of squares and holes in images to prioritize the ordering with
which they are targeted. Although there are many possible
parameters that may be important for determining whether a
square or hole contains high-quality particles, experienced
operators are able to consistently find good locations,
suggesting that at least some features of good target locations
are identifiable in low- and medium-magnification images.
Therefore, for each magnification we train a separate CNN to
classify squares or holes as collected or not collected by
operators. The input to our model is a cropped image of a
square or hole, extracted using the square-localization method
or hole-localization method above, and the output is a scalar
probability.
2.4.1. Square classification. We train our square classifica-
tion model on a dataset containing 41k square crops, of which
11k were squares collected. Square images are normalized
based on the intensity of all pixels within the bounding boxes
for the squares in each low-magnification image to control for
electron dose. We also include random forest (RF) and logistic
regression (LR) models trained on summary statistics of the
pixels extracted from the square image crops. This is because
the operators typically use characteristics like the size/area
and brightness of
the squares to make their selections.
Therefore, we include baselines which reflect this knowledge.
The summary statistics used as features are mean intensity,
maximum intensity, minimum intensity, variance in intensity,
kurtosis, skew and crop area.
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2.4.2. Hole classification. We compare the summed pixel-
wise probabilities output by our localization U-net within each
hole against two CNNs trained on a dataset containing 571k
hole crops, of which 410k were targeted by operators. The
dimensions of the holes and, therefore, the dimensions of the
resulting crops vary widely between data-collection sessions.
However, we do not want the model to use the size of the
input image to decide if a hole is good or bad. We hypothesize
that the location of image features within each hole (e.g.
crystalline ice) is not important for classification. Rather, the
presence, absence or proportion of these features is the main
concern. Therefore, we compare between a standard CNN
model that pads all input images to the same dimension and
one which averages over non-channel dimensions of the final
map before the fully connected layer, thereby treating the
image as a bag of regions. Both CNNs normalize images based
on pixels in the crop to control for difference in electron dose.
Aside from the difference in padding versus average pooling,
all other hyperparameters of the two models are identical.
3. Results and discussion
Ptolemy can accurately locate and rank collection locations
within low- and medium-magnification images, with each stage
producing good performance metrics, and results that appear
inspection. Furthermore, Ptolemy
reasonable on visual
generalizes well to new sessions without user intervention or
retraining on a session-by-session basis.
3.1. Ptolemy localization of squares in low-magnification
images
The square localization algorithm successfully detects
almost all operator-selected locations, as well as squares that
were not collected, with few errors. Our algorithm successfully
detects 98.8% of operator-selected locations (Table 1). An
additional 30k unselected squares are detected, and visual
inspection confirms that these are real squares that were not
selected by the operator (Fig. 8).
Table 1
Statistics from running the square localization procedure on low-
magnification images.
No. of operator-selected locations
No. of operator-selected locations detected
Total no. of locations detected
10993
10857
41301
Table 2
Performance metrics of different ML models on the square classification
task measured on held-out sessions and held-out square images.
We compare the performance of LR, an RF and a CNN based on two metrics.
ROC AUC: area under receiver-operating characteristic curve.
Session split
Random split
Model
ROC AUC Average precision ROC AUC Average precision
0.539
LR
RF–5 feature 0.603
0.608
CNN
0.258
0.344
0.331
0.499
0.867
0.733
0.259
0.734
0.489
3.2. Square classifier learns to rank squares effectively
For square classification, we explored three different
models: an LR and RF on summary statistics (details in
Appendix C) extracted from square images, and a CNN on the
images themselves. Both the RF and the CNN perform simi-
larly on this task.
3.2.1. Classifying squares for new sessions without prior
knowledge. Square ranking without any information about the
sample is a challenging task, but our models perform well and
are significantly better than random guessing (Table 2). The
task of ranking squares given the session split is particularly
difficult, because the characteristics that make up good
squares can vary from session to session. For optimum
performance in this setting, a model would need to extract
enough information from the square images to identify the
optimal sample conditions and then predict the quality of the
square accordingly. Although this is probably not possible for
a classifier such as ours, which makes predictions for each
square independently, we hypothesize that there are, at least,
characteristics of squares that are always bad and maybe
squares that are always good that can still provide useful
Figure 8
Example square localizations on low-magnification images. Ptolemy successfully segments bounding boxes around squares in the grid without human
intervention.
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Figure 9
Example square classifications in low-magnification images. The model successfully prioritizes larger, brighter squares without cracks or contamination.
Model-predicted probabilities for squares are in red. Colors from high to low score: dark blue, light blue, white, yellow, orange, red.
one-to-one with an operator-collected hole, a false negative as
an operator-collected hole that contains zero or more than one
(2+) model selection locations, and a false positive as a model
selection location that is not contained in any operator-
collected holes, or is only contained in operator-collected
holes that also contain other model selection locations. For
more information on how we defined ‘model selection loca-
tions’ for each model in Table 3, see Appendix D.
We find our U-Net, without
lattice fitting, can learn
operator-selected locations exceptionally well, and can iden-
tify 98.4% of all operator-selected holes with 70.3% precision
(Table 3, row 2). We compare this method with the Yolov5-
based model trained by Yokoyama et al. (2020) on the same
dataset and find that the U-Net is superior in both recall and
precision (Redmon & Farhadi, 2018).
guidance. The difficulty of this task is evident in comparison
with the performance of the models on random splits of the
data, where without the difficulty of generalizing to unseen
sessions, the RF and CNN models perform significantly better
(Table 2). Nonetheless, Ptolemy ranks squares significantly
better than random guessing even in the session split setting.
On visual inspection of predictions on held-out sessions, we
the CNN makes reasonable predictions, with
find that
unbroken and larger squares prioritized over smaller, broken
squares (Fig. 9). Additional example images with both model
scores and user selection locations can be found in Fig. S4.
3.2.2. Simple extracted features exhibit good performance
on square classification. The RF performing comparably to
the CNN on an image classification task is a surprising result
for which there are several possible explanations. First,
examining the feature importance of the extracted features for
the RF models, using feature permutation, shows that area and
mean pixel
intensity are the most important features for
predicting whether a square was selected (Fig. 10). This result
aligns with our expectations, as operators usually use area and
brightness of squares as primary criteria for selection. We
hypothesize that the importance of area as a feature may
partly explain the good performance of the RF relative to the
CNN, as area may be a feature that is difficult for a CNN to
learn. Additionally, since our dataset is not exhaustively
labeled, a more complex CNN model may be learning
redundant, irrelevant features that do not generalize well from
training set to test set. Nevertheless, the CNN does not require
a burdensome computational cost (it runs very quickly on
commodity CPU hardware), and likely has a higher potential
performance if a larger and cleaner dataset is curated. We
therefore use it as the default model for Ptolemy.
3.3. Ptolemy retrieves more holes with fewer false positives
Next, we examine the performance of our methods for hole
localization on medium-magnification images (Table 3). Since
we do not have bounding box annotations for our dataset, we
define a true positive as a model selection location that maps
Figure 10
Feature importance for square classification. Results obtained for feature
importance of square image summary statistics to predict whether a
square is selected using an RF model. Area and mean pixel intensity are
the most important features.
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Table 3
Performance metrics of different methods on held-out sessions for hole
localization from medium-magnification images.
Reported metrics are aggregated by session and averaged. Definitions of true
positive, false positive and false negative used for computing precision, recall,
and F1 can be found in Section 3.3 and Appendix D.
Model
Precision Recall F1
Yolov5 (from Yokoyama et al., 2020)
U-Net
U-Net + Lattice Fitting
U-Net + Lattice Fitting + Probability Threshold
0.395
0.703
0.549
0.802
0.669
0.984
0.993
0.891
0.459
0.815
0.702
0.837
3.3.1. Lattice fitting reduces false negative rate. With the
addition of lattice fitting (Table 3, row 3), we reduce the false
negative rate by a factor of 2, from 1.6% to 0.7%. Although
the precision is also reduced with lattice fitting, we are
primarily concerned with improving the false negative rate (1-
recall) as our aim is to recover all the holes at this stage. In the
manual inspection, we find that the U-Net with lattice fitting
correctly locates holes across diverse images (Fig. 11). Because
many holes are not selected by the operators, we expect that,
for the goal of detecting all holes (selected and not selected),
lattice fitting is helpful. Additionally, only keeping lattice tiles
based on a probability taken from the U-Net output (Table 3,
row 4) significantly improves precision at the cost of recall.
3.3.2. U-Net + Lattice Fitting generalizes hole localization
to an external dataset. To further test generalization, we
predict holes in the dataset by Yokoyama et al. (2020) using
our U-Net + Lattice Fitting model. Yokoyama et al. (2020)
reported 95–97% recall of their own Yolov5 based model on
these data. We find that the U-Net + Lattice Fitting model
generalizes well, achieving 0.685 precision, 0.950 recall and
0.796 F1 score. The images in this dataset were collected from
an external facility, using a different microscope (Ptolemy data
were collected primarily on a TFS Krios and a Glacios; this
dataset was collected on a JEM-Z300CF) and with different
magnification compared with the images in our training
dataset (Yokoyama et al., 2020), demonstrating that Ptolemy
generalizes effectively.
3.4. Ptolemy successfully classifies holes in medium-
magnification images after localization
Next, we examine the performance of our hole classification
models (Table 4). Both the padded model and the average-
pool model perform well on the hole classification task. In
example images, we see that the model can effectively sepa-
rate good, unblemished holes from those with blemishes and
artifacts on both gold and carbon grids (Fig. 12).
3.4.1. Average-pooling improves hole classification. The
average-pool model slightly outperforms the padded model,
which supports our hypothesis that the location in the image
where features occur is not as important in determining hole
quality, and that given the wide variance of hole sizes, a model
that uses average pooling is preferable to padding all crops to
the same size.
Table 4
Performance of hole classification CNNs on hold-out sessions.
ROC AUC: area under receiver operating characteristic curve.
Model
Accuracy ROC AUC Average precision
0.748
CNN (padding)
CNN (average pool)
0.758
U-Net + Probability Threshold 0.846
0.742
0.796
0.868
0.808
0.878
0.867
3.4.2. Classifying holes using the localization U-Net
output. We compare the dedicated CNN classifiers against
the sum of the hole localization U-Net probabilities within a
crop to determine the probability of picking a hole (Table 4,
row 3). Surprisingly, the U-Net score outperforms the dedi-
cated CNN classifiers in accuracy and ROC AUC. This is
probably because the U-Net uses the context around the hole
to help predict where the hole was collected from. The U-Net
is deep to allow large holes to fit entirely within the receptive
field of the bottleneck-layer neurons. This means that, for
Figure 11
Examples of hole localization using the U-Net + Lattice Fitting. Ptolemy
successfully detects all holes across a wide range of hole sizes, brightness
and contrast conditions, from easily visible gold grids (bottom left) to
very low contrast carbon grids that are difficult to see even for humans
(top right).
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Figure 12
Example hole classifications in medium-magnification images using the average-pooling model. Ptolemy can successfully prioritize complete holes free of
contaminants. Model-predicted probabilities for holes are in red. Colors from high to low score: dark blue, light blue, white, yellow, orange, red.
grids with smaller holes, the U-Net will have information
about the location of the hole on the grid and the character-
istics of nearby holes that our classifiers, which use only hole
crops, lack.
3.5. Training and evaluating human operator selections
One of the major challenges in developing Ptolemy is the
lack of fully annotated data for training and assessment of
model performance. We rely on training data composed of
incomplete expert operator selections. These selections only
represent an expert guess at the best collection locations and
our models are trained to recapitulate these operator selection
decisions as a surrogate for selecting high-quality data. Ideally,
we would train and evaluate our models based on the true end
goal of cryoEM data collection, particle quantity and quality,
as determined by the resulting 3D structures, but these data
are currently unavailable.
Furthermore, the operators do not exhaustively select all
possible viable collection locations. Since our model evalua-
tion considers locations that the operator did not select as
ground-truth negatives, the reported precision values are
likely to underestimate the true precision of Ptolemy models.
This lack of exhaustive selection also creates biases in the
training data, especially on the hole and square classification
tasks, which may be learned by our models. For example, due
to the microscope setup at the SEMC/NYSBC, holes near the
edge of medium-magnification images are often not collected
even though they may be viable collection locations.
3.6. Future work
A large fraction (the bulk majority at NYSBC) of cryoEM
data-collection experiments involve gold or carbon holey grids
generated via blotting and collected without tilting. Devel-
opment, training and validation of Ptolemy were carried out
with the goal of providing a system for automated collection
on these grids. However, this leaves a long tail of less used but
significant grid types and preparation methods for which
future work is required. These include lacy grids, grids
generated via spray or spotting methods, and tilted collection.
Furthermore, Ptolemy currently lacks the ability to update its
predictions dynamically to adjust to a given collection session.
Ptolemy is designed to allow for modular improvement over
time, so future updates of Ptolemy can build on the current set
of algorithms to cover these cases as well. Tilted images can be
corrected with basic image processing, as the angle of the tilt
will be known in advance, and then the un-tilted images can be
processed as normal. Grids generated by spray or spotting
methods may need new purpose-built algorithms, but they
may also be effectively handled by an on-the-fly learning
algorithm. Lacy grids will likely require the most customiza-
tion,
including separate segmentation and prioritization
algorithms at the medium-magnification level.
4. Conclusions
Increasing throughput and reducing cost through automation
is necessary to meet increasing demand for cryoEM. In this
work, we present Ptolemy, an open-source, modular package
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using
images
for automatic targeting and classification of cryoEM low- and
purpose-designed
medium-magnification
computer vision and deep-learning algorithms. Ptolemy
accurately localizes and ranks squares and holes in low- and
medium-magnification images across a wide range of image
and sample conditions. By training on large datasets of sparse
microscope operator selection locations, the Ptolemy locali-
zation algorithms generalize to diverse gold and carbon holey
grids and rank potential collection locations effectively
without session-specific parameters, as we have demonstrated
on held-out collection sessions within the SEMC/NYSBC
dataset and on an independent dataset from another facility.
Additionally, Ptolemy has been integrated with the micro-
scope control software Leginon to enable automated data
collection in real-life use cases (Cheng et al., 2022).
Ptolemy is similar to the recent works SmartScope (Bouv-
ette et al., 2022) and CryoRL (Li et al., 2022), which both offer
automated collection capabilities. SmartScope focuses on
automated screening and providing a helpful user interface to
view and control screening in real time, whereas CryoRL
focuses on optimizing the cryoEM data collection as a path-
planning problem and does not clearly address the square- and
hole-detection problem. Both primarily repurpose existing
deep-learning object detection and classification algorithms.
Ptolemy, on the other hand, uses novel algorithms that are
purpose-built for detection and classification of holes and
squares in cryoEM images.
Although Ptolemy identifies and generally ranks ROIs
remarkably well, it is unable to incorporate session-specific
information to reprioritize targets on-the-fly. In future work,
we plan to use the current Ptolemy classification models as
prior models, and dynamically update these prior models
during each collection session based on the quality of highest-
magnification exposures that are collected from explored
squares and holes in an active-learning framework.
Ptolemy is a significant advance in the automation of
cryoEM data collection, allowing for fully unattended data
collection, and increasing microscope and operator efficiency.
To accelerate cryoEM collection for the whole community,
Ptolemy is open source and freely available for academic use
at https://github.com/SMLC-NYSBC/ptolemy. We anticipate
that Ptolemy will become an integral part of the data-collec-
tion pipeline and will serve as the basis for future work in
cryoEM automation.
The supporting information file pw5021sup1.xlsx contains
the metadata for the various data-collection sessions used to
train and test the models in Ptolemy.
APPENDIX A
Ptolemy implementation details and default models
Ptolemy is an operating system and microscope control soft-
ware agnostic and requires only Python (3+) and a few
installed packages to run. Package dependencies can be found
in the github repository at https://github.com/SMLC-NYSBC/
ptolemy. By default, Ptolemy is configured to use the mixture
model for low-magnification square detection, the CNN for
low-magnification square classification, the U-Net with grid
fitting for medium-magnification hole detection and the
average-pooled CNN for medium-magnification hole classifi-
cation. It runs fully on CPU and requires a maximum of only
2.7 GB RAM to detect and classify squares in a low-magnifi-
cation image and 3.6 GB RAM to detect and classify holes in a
medium-magnification image.
After installation, running Ptolemy during data collection
involves the following steps.
(1) Microscope control software captures tiled low-magni-
fication mrc(s) of the grid and saves the file.
(2) Call python lowmag_cli.py (path to low-magnifi-
cation mrc). This returns a JSON containing a list of diction-
aries with the fields (i) vertices corresponding to vertex
coordinates of squares, (ii) center corresponding to the centers
of squares, (iii) area corresponding to areas of squares, (iv)
brightness corresponding to mean brightness of pixels in
squares, (v) score corresponding to CNN predicted score
(between 0 and 1) of squares.
(3) Use the output coordinates and scores to select the
collection location(s) to collect medium-magnification images.
(4) Microscope control software captures medium-magni-
fication mrc(s) within squares and saves to file.
(5) Call python medmag_cli.py (path to medium-
magnification mrc). This returns a JSON containing a list of
dictionaries with the fields (i) vertices corresponding to vertex
coordinates of hole crops, (ii) center corresponding to the
centers of holes, (iii) area corresponding to areas of hole crops,
(iv) score corresponding to CNN predicted score (between 0
and 1) of holes.
(6) Use the output coordinates and scores to select the
the highest-magnification
collection location(s) to collect
exposures.
(7) Return to step (3) to explore new medium-magnification
collection locations from existing low-magnification images, or
step (1) to select new low-magnification collection locations.
For an example of integrating Ptolemy into cryoEM data-
collection software in practice, please refer to the companion
‘Fully automated multi-grid CryoEM
paper to Ptolemy,
screening using Smart Leginon’ (Cheng et al., 2022).
APPENDIX B
Training and hyperparameters
All deep-learning and machine-learning models were trained
using default hyperparameters in PyTorch (Paszke et al., 2019)
and scikit-learn (Pedregosa et al., 2011) except where stated
otherwise. All deep-learning model parameters were fitted
with the default Adam, except for the sigma parameter of the
Gaussian smoothing, which was initialized to e and trained
with an Adam optimizer with a learning rate of 0.1 (Kingma &
Ba, 2017). Binary-cross-entropy loss was used for all deep-
learning models, and for the U-Net a positive weight of 100
was applied.
The square classification CNN was trained for two epochs
and used two 5 (cid:6) 5 convolutional layers followed by three 3 (cid:6)
3 convolutional layers, with 64 channels per layer and with a
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batch size of 128, whereas the hole classification CNN was
trained for five epochs and used one 5 (cid:6) 5 convolutional layer,
followed by three 3 (cid:6) 3 convolutional layers with 128 channels
per layer, with a batch size of 32. Both models used batch
normalization, max-pooling and ReLU activations (LeCun et
al., 2015; Ioffe & Szegedy, 2015).
The U-Net for hole localization was trained for 6000 steps
and used nine down-blocks and nine up-blocks, with each
down-block and up-block using a 64 channel 3 (cid:6) 3 kernel
convolutional layer. The model also used ReLU activations
for down- and up-blocks, max-pooling for downsampling in
down-blocks, and nearest interpolation for upsampling in up-
blocks. Batch norm was not used. Also, the bias of the final
convolutional layer which produces the final output of the
model was initialized at (cid:3)10 to allow the model to initially
predict all or mostly zeros in the output, since the target image
contains zeros everywhere except for the few pixel locations
where the operator made a selection.
Random 90(cid:5) rotation augmentation is applied while training
square and hole classification CNNs. Random 90(cid:5) rotation
augmentation is combined with random pixel inversion when
training the U-Net for hole localization.
APPENDIX C
Random forest and logistic regression model details
The RF and LR models were trained on the following features
for the squares: mean pixel intensity, maximum pixel intensity,
minimum pixel intensity, variance of pixel intensities, skew of
pixel intensities, kurtosis of pixel intensities and area. Default
hyperparameters from scikit-learn were used for both models.
APPENDIX D
Definition of ‘predicted collected regions’ for each
model
For U-Net + Lattice Fitting, crops are generated by creating
squares centered at each lattice point with a side length equal
to dl (cid:3) 60, where dl is the distance between lattice points. All
crops are considered predicted collected regions.
For U-Net alone, circles with a radius of 50 pixels around
each centroid of high-probability regions in the U-Net output
map are considered predicted collected regions.
For U-Net + Lattice Fitting + Probability Threshold, we
generated crops like in U-Net + Lattice Fitting, but then only
kept the crops where the sum of pixel probabilities outputted
by the U-Net within the crop was greater than 0.5.
For the Yolov5 model in Yoneo-Locr, which outputs many
bounding boxes at different confidence levels, we had to
decide how to set confidence thresholds which determine the
bounding boxes that are kept. We aimed to be generous to the
model by picking the confidence threshold that gave the
maximum F1 score for each image independently and keeping
all bounding boxes in that image that were predicted with
confidence greater than this threshold.
research papers
Acknowledgements
We thank the SEMC Electron Microscopy Staff for their help
in testing algorithms and models, in particular Mahira Aragon,
Eugene Chua, Huihui Kuang, Kashyap Maruthi, Joshua
Mendez, Anjelique Sawh and Hui Wei. Additionally, we thank
Tohru Terada for providing us with hole localization data from
Yokoyama et al. (2020). Finally, we thank members of the
SEMC at NYSBC, in particular Bridget Carragher and Clint
Potter, for useful discussions.
Funding information
This work was performed at the Simons Electron Microscopy
Center located at the New York Structural Biology Center,
supported by grants from the Simons Foundation (grant No.
SF349247) and NIH National Institute of General Medical
Sciences (grant No. GM103310).
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| null |
10.1371_journal.pone.0243922.pdf
|
Data Availability Statement: All relevant data are
within the paper and its Supporting Information
files.
|
All relevant data are within the paper and its Supporting Information files.
|
RESEARCH ARTICLE
The prevalence of esophageal cancer after
caustic and pesticide ingestion: A nationwide
cohort study
Han-Wei MuID
Dong-Zong HungID
1*
1,2, Chun-Hung Chen1,2, Kai-Wei Yang1,2, Chi-Syuan Pan1,2, Cheng-Li Lin3,
1 Division of Toxicology, China Medical University Hospital, Taichung, Taiwan, 2 Department of Emergency
Medicine, China Medical University Hospital, Taichung, Taiwan, 3 Management Office of Health Data, China
Medical University Hospital, Taichung, Taiwan
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
* [email protected]
Abstract
OPEN ACCESS
Citation: Mu H-W, Chen C-H, Yang K-W, Pan C-S,
Lin C-L, Hung D-Z (2020) The prevalence of
esophageal cancer after caustic and pesticide
ingestion: A nationwide cohort study. PLoS ONE
15(12): e0243922. https://doi.org/10.1371/journal.
pone.0243922
Editor: Gianluigi Forloni, Istituto Di Ricerche
Farmacologiche Mario Negri, ITALY
Received: July 5, 2020
Accepted: November 30, 2020
Published: December 29, 2020
Peer Review History: PLOS recognizes the
benefits of transparency in the peer review
process; therefore, we enable the publication of
all of the content of peer review and author
responses alongside final, published articles. The
editorial history of this article is available here:
https://doi.org/10.1371/journal.pone.0243922
Copyright: © 2020 Mu et al. This is an open access
article distributed under the terms of the Creative
Commons Attribution License, which permits
unrestricted use, distribution, and reproduction in
any medium, provided the original author and
source are credited.
Data Availability Statement: All relevant data are
within the paper and its Supporting Information
files.
Habits such as smoking and alcohol drinking and existing esophageal malfunction are con-
sidered the main risk factors for esophageal carcinogenesis. Caustic ingestion of acidic or
alkaline agents or strong irritants can induce severe esophageal corrosive injury and
increase esophageal cancer risk. We studied the relationship between esophageal carci-
noma and acute detergent or pesticide poisoning by using nationwide health insurance
data. Methodology/Principle findings: We compared a pesticide/detergent intoxication
cohort (N = 21,840) and an age- and gender-matched control cohort (N = 21,840) identified
from the National Health Insurance Research Database between 2000 and 2011. We used
the multivariable Cox proportional model to determine esophageal carcinoma risk. The over-
all incidence density of esophageal cancer was 1.66 per 10,000 person-years in the compar-
ison cohort and 4.36 per 10,000 person-years in the pesticide/detergent intoxication cohort.
The corresponding adjusted hazard ratio (HR) for esophageal cancer was 2.33 (95% confi-
dence interval [CI] = 1.41–3.86) in the pesticide/detergent intoxication cohort compared with
the control cohort. Patients with corrosive and detergent intoxication did not have a higher
risk of esophageal cancer (adjusted HR = 0.98, 95% CI = 0.29–3.33) than those without pes-
ticide/detergent intoxication. However, patients with pesticide intoxication had a significantly
higher risk of esophageal cancer (adjusted HR = 2.52, 95% CI = 1.52–4.18) than those with-
out pesticide/detergent intoxication. Conclusion: In the present study, after adjusting for
conventional risk factors, we observed that pesticide intoxication could exert substantial
effects through increased esophageal cancer risk. However, patients with detergent intoxi-
cation may not have an increased risk of esophageal cancer.
Introduction
Essentially, self-ingestion of caustic agents, detergents, and pesticides is a serious public health
problem in Taiwan. According to the Taiwan health statistics, 600 people ingested liquid tox-
ins, including caustic agents and pesticides, for suicidal attempt in 1 year, and this is the third
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
1 / 11
PLOS ONEFunding: This work was supported by grants from
the Ministry of Health and Welfare, Taiwan
(MOHW108-TDU-B-212-133004), China Medical
University Hospital (DMR-107-192, CMU107-
ASIA-19), Academia Sinica Stroke Biosignature
Project (BM10701010021), MOST Clinical Trial
Consortium for Stroke (MOST 107-2321-B-039
-004-), Tseng-Lien Lin Foundation, Taichung,
Taiwan, and Katsuzo and Kiyo Aoshima Memorial
Funds, Japan. The funders had no role in the study
design, data collection and analysis, decision to
publish, or preparation of the manuscript. No
additional external funding was received for this
study.
Competing interests: The authors have declared
that no competing interests exist.
Esophageal cancer after pesticide ingestion
common method for committing suicide. Caustic substance ingestion is most frequently
encountered in children as a result of accidental swallowing or in adults as a result of self-
harm. It often extensively injures the upper gastrointestinal tract and may lead to extensive
necrosis, perforation, and death. Among the agents for pesticide poisoning in Taiwan, organo-
phosphorus, herbicides, and other pesticides account for 45%, 23%, and 23%, respectively,
according to the admission 2009 data from Taiwan National Health Insurance Database.
Esophageal cancer accounts for >500,000 cancer deaths annually, and the incidence is rap-
idly increasing worldwide [1]. In Taiwan, 2,630 new cases of esophageal cancer and 1,792
deaths caused by esophageal cancer occurred in 2013. The mean age at occurrence was 57 in
men and 62 in women. Most esophageal cancer cases in Taiwan are of squamous cell carci-
noma (93%), and the incidence is still increasing. The risk factors for esophageal cancer are
smoking, alcohol consumption, dietary factors such as betel quid chewing and high tempera-
ture beverage consumption, gastroesophageal reflux disease, and underlying esophageal dis-
eases such as achalasia, and they are substantially different in various parts of the world [1–5].
Some studies have shown that caustic ingestion that induced severe esophageal corrosive
injury might increase esophageal cancer risk [6–12]. Some studies with limited data even esti-
mated a 1,000-fold higher risk [6]. However, these studies were based on a small number of
case control studies; hence, the evidence is not strong.
Pesticides protect plants from weeds, fungi, or insects. Pest control agents are usually
applied through chemical dispersal in a hydrocarbon solvent-surfactant system to provide a
homogeneous preparation. In addition to pesticides, these solvent-surfactants, such as the sur-
factant of glyphosate, produce significant mucosal irritation effects. Some epidemiological
studies have demonstrated high risks of certain cancers from exposure to some solvents [13].
Some pesticides are classified as carcinogenic or potentially carcinogenic to humans, such as
captafol, diazinon, malathion, and glyphosate. Here, our study investigated the relationship
between esophageal cancer and esophageal injuries after caustics ingestion and pesticide
poisoning.
Methods
Data source
This study used data from the National Health Insurance Research Database (NHIRD). The
NHIRD was launched in Taiwan in 1995 and covers nearly 99% of the total population of Tai-
wan with comprehensive healthcare benefits. For this study, we used the deidentified data of
the residents to link two data files (subsets of the NHIRD), namely inpatient claims data and
Registry of Beneficiaries. International Classification of Diseases-9-Clinical Modification
(ICD-9-CM) codes were used to define diseases in the NHIRD. This study was approved by
the Ethics Review Board of China Medical University (CMUH-104-REC2-115).
Study population
Patients with pesticide/detergent intoxication were identified from the NHIRD from January
1, 2000, to December 31, 2005, according to ICD-9-CM codes 983, 989.3–989.4, and 989.6.
Patients diagnosed with cancer (ICD-9-CM codes 140–208) before pesticide/detergent intoxi-
cation or those who lacked continuous health insurance coverage preceding cohort entry were
excluded. Furthermore, all patients aged <20 years were excluded. Moreover, the comparison
cohort of individuals without any history of pesticide/detergent intoxication was identified
from the NHIRD. The comparison cohort also excluded those with cancer history, without
health insurance before entering the study, or aged <20 years. In the final cohort, the pesti-
cide/detergent intoxication cohort was matched to the comparison cohort at a 1:1 ratio by
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
2 / 11
PLOS ONEEsophageal cancer after pesticide ingestion
gender, age, and the year of study entry. We designated 50 and 65 years as the age threshold. A
consensus is lacking regarding the age at which an individual can be considered elderly, but
the World Health Organization defines individuals >65 years as elderly in most developed
countries. In less developed countries, for example in parts of Africa, >50 years old is consid-
ered elderly. Thus, we classified participants into the age groups of <49, 50–64, and >65 to
determine the difference between each group.
The index date was defined as the date of first diagnosis of pesticide/detergent intoxication
in the database. All participants were observed until they were diagnosed with esophageal can-
cer (ICD-9-CM code 150), death, or the end of the study period (December 31, 2011).
Outcome, comorbidity, and medication
The primary clinical outcome was esophageal cancer (ICD-9-CM code 150). Furthermore,
participants in the pesticide/detergent intoxication and control cohorts were compared for
common comorbidities, including hypertension (ICD-9-CM codes 401–405), diabetes mellitus
(ICD-9-CM code 250), chronic obstructive pulmonary disease (ICD-9-CM codes 491, 492,
and 496), obesity (ICD-9-CM code 278), alcohol-related illness (ICD-9-CM codes 291, 303,
305, 571.0, 571.1, 571.2, 571.3, 790.3, A215, and V11.3), ischemic heart disease (ICD-9-CM
codes 410–414), cerebrovascular disease (ICD-9-CM codes 430–438), and gastric disease
(ICD-9-CM codes 530–534). Common comorbidities were identified according to the diagno-
sis records in the inpatient file before the index date.
Statistical analysis
We used descriptive statistics to summarize the characteristics of the pesticide/detergent intox-
ication cohort and matched comparison cohort. A continuous variable, such as age, was used
in an independent t test to examine the mean ages between the two cohorts. Categorical vari-
ables are presented as the number and percentage and included sex and common comorbidity
assessed using the chi-square test. Univariable and multivariable Cox proportional hazard
regression analyses were used to determine esophageal cancer risk, and the results are pre-
sented as hazard ratios (HRs) with 95% confidence intervals (CIs). The differences in the
cumulative incidence of esophageal cancer between the pesticide/detergent intoxication and
control cohorts were estimated using the Kaplan–Meier method with the log-rank test. A two-
tailed p value of <0.05 was considered statistically significant. We used SAS software (version
9.4 for windows; SAS Institute, Cary, NC, USA) for all statistical analyses and Kaplan–Meier
survival curve plots.
Results
This study included 21,840 patients with pesticide/detergent intoxication and 21,840 control
patients. The basic characteristics of the two cohorts are shown in Table 1. The mean ages of
the pesticide/detergent intoxication cohort and comparison cohort were 52.1 ± 17.4 and
51.6 ± 17.6, respectively. No significant difference was noted in sex and age. The majority of
pesticide/detergent intoxication patients were men (62.1%) and <49 years old (48.1%). In gen-
eral, a high proportion of pesticide/detergent intoxication patients had hypertension, diabetes
mellitus, gastric disease, ischemic heart disease, cerebrovascular disease, chronic obstructive
pulmonary disease, alcohol-related illness, and obesity (all p < 0.001). The average follow-up
duration was 5.25 ± 3.86 years for the pesticide/detergent cohort and 6.63 ± 3.29 years for the
comparison cohort. The Kaplan–Meier curve showed that the cumulative incidence of esoph-
ageal cancer was higher in the pesticide/detergent cohort than in the comparison cohort
throughout the 12-year follow-up period (Fig 1). The cumulative incidence of esophagus
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
3 / 11
PLOS ONETable 1. Characteristics of patients with and without pesticide/detergent intoxication.
Pesticide/Detergent intoxication
Yes
(N = 21840)
No
(N = 21840)
Esophageal cancer after pesticide ingestion
Age, year
�49
50–64
� 65
Mean (SD) #
Gender
Female
Male
Comorbidity
Hypertension
Diabetes mellitus
Gastric disease
Ischemic heart disease
Cerebrovascular disease
Chronic obstructive pulmonary disease
Alcohol-related illness
Obesity
Chi-square test.
#t test.
https://doi.org/10.1371/journal.pone.0243922.t001
n
10496
5386
5958
52.1
8269
13571
3454
2136
3027
1783
1875
1044
1071
16
%
48.1
24.7
27.3
17.4
37.9
62.1
15.8
9.78
13.9
8.16
8.59
4.78
4.90
0.07
n
10496
5386
5958
51.6
8269
13571
1870
957
1057
862
934
424
112
6
%
p-value
48.1
24.7
27.3
17.6
37.9
62.1
8.56
4.38
4.84
3.95
3.82
1.94
0.51
0.03
0.99
0.004
0.99
<0.001
<0.001
<0.001
<0.001
<0.001
<0.001
<0.001
<0.001
cancer was significantly different between the pesticide/detergent and comparison cohorts
(log-rank test; p < 0.001).
The overall incidence densities of esophageal cancer were 1.66 and 4.36 per 10,000 person-
years in the comparison and pesticide/detergent cohorts, respectively (Table 2). The corre-
sponding adjusted HR for esophageal cancer was 2.33 (95% CI = 1.41–3.86) compared with
controls after adjusting for age, sex, gastric disease, and alcohol-related illness. Compared with
patients aged <49 years, those aged 50–64 and >65 years had 2.67-fold (95% CI = 1.54–4.64)
and 3.18-fold (95% CI = 1.74–5.80) significantly higher risks of esophageal cancer, respectively.
Compared with women, men had an adjusted HR of 19.8 (95% CI = 4.85–80.8) for esophagus
cancer. Among various comorbidity types, significantly increased risk was observed in those
with alcohol-related illness (adjusted HR = 7.14, 95% CI = 3.63–14.1).
Table 3 presents the incidence and HR of esophageal cancer between patients with and
without pesticide/detergent intoxication. Compared with patients without pesticide/detergent
intoxication, men, patients aged <49 years, and those aged >65 years with pesticide/detergent
intoxication had 2.22-fold (95% CI = 1.34–3.69), 2.84-fold (95% CI = 1.08–7.47), and 2.94-fold
(95% CI = 1.19–7.26) increased esophagus cancer risks, respectively. For patients without
comorbidity, those with pesticide/detergent intoxication had a significantly higher esophageal
cancer risk than those without pesticide/detergent intoxication (adjusted HR = 2.32, 95%
CI = 1.32–4.10). Among patients with non–alcohol-related illness, those with pesticide/deter-
gent intoxication had a higher risk of esophageal cancer than controls (adjusted HR = 2.47,
95% CI = 1.46–4.16).
Table 4 presents the incidence and adjusted HR of esophageal cancer between different
groups of patients with pesticide/detergent intoxication. Patients with corrosive and detergent
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
4 / 11
PLOS ONEEsophageal cancer after pesticide ingestion
Fig 1. Cummulative incidence comparison of esophagus cancer in patients with (dashed line) and without (solid line)
pesticide/detergent intoxication.
https://doi.org/10.1371/journal.pone.0243922.g001
intoxication (ICD-9-CM codes 983 and 989.6) did not have a higher risk of esophageal cancer
(adjusted HR = 0.98, 95% CI = 0.29–3.33) than those without pesticide/detergent intoxication.
Furthermore, patients with only pesticide intoxication (ICD-9-CM codes 989.3 and 989.4) had
a significantly higher risk of esophageal cancer (adjusted HR = 2.52, 95% CI = 1.52–4.18) than
those without pesticide/detergent intoxication.
Discussion
Several factors, including living habits and hobbies, contribute to esophageal cancer develop-
ment. Esophageal cancer has two major subtypes, namely squamous cell carcinoma and ade-
nocarcinoma, which have some same and different risk factors. Several genetic and epigenetic
alterations are implicated in both the development and progression of esophageal cancer.
Mucosal break, inflammation, and toxic injuries caused by excessive alcohol drinking and
heavy smoking, two of the most important and common risk factors, are causes of esophageal
carcinoma. Although the relationship between caustic ingestion and esophageal cancer and
the mechanism of esophageal cancer development are unclear, lye-based cleaner burn has
been found to complicate esophageal strictures and thus increase the risk of esophageal squa-
mous cell carcinoma [6,7,11]. Fewer case series studies have shown that the esophageal cancer
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
5 / 11
PLOS ONEEsophageal cancer after pesticide ingestion
Table 2. Incidence per 10,000 person-years of and risk factors for esophagus cancer.
Variable
Pesticide/Detergent intoxication
Event
PY
Rate#
Crude HR (95% CI)
Adjusted HR& (95% CI)
No
Yes
Age, year
�49
50–64
� 65
Gender
Female
Male
Comorbidity
Hypertension
No
Yes
Diabetes mellitus
No
Yes
Gastric disease
No
Yes
Ischemic heart disease
No
Yes
Cerebrovascular disease
No
Yes
Chronic obstructive pulmonary disease
No
Yes
Alcohol-related illness
No
Yes
Obesity
No
Yes
24
50
22
30
22
2
72
66
8
68
6
64
10
71
3
71
3
71
3
61
13
74
0
144761
114723
137357
66141
55986
100714
158769
238183
21300
247603
11880
242170
17314
248574
10910
248837
10646
254217
5266
254356
5128
259400
83
1.66
4.36
1.60
4.54
3.93
0.20
4.53
2.77
3.76
2.75
5.05
2.64
5.78
2.86
2.75
2.85
2.82
2.79
5.70
2.40
25.4
2.85
0.00
1.00
2.64(1.63, 4.30)���
1.00
2.33(1.41, 3.86)��
1.00
2.85(1.65, 4.95)���
2.55(1.41, 4.61)��
1.00
2.67(1.54, 4.64)���
3.18(1.74, 5.80)���
1.00
22.9(5.63, 93.5)���
1.00
19.8(4.85, 80.8)���
1.00
1.41(0.68, 2.95)
1.00
1.92(0.83, 4.42)
1.00
2.25(1.15, 4.38)�
1.00
0.99(0.31, 3.15)
1.00
1.02(0.32, 3.25)
1.00
2.13(0.67, 6.77)
1.00
1.00
1.00
0.83(0.40, 1.72)
1.00
1.00
1.00
1.00
10.9(5.96, 19.8)���
1.00
7.14(3.63, 14.1)���
1.00
-
1.00
Rate#: incidence rate per 10,000 person-years.
Crude HR, relative hazard ratio.
Adjusted HR&: Multivariable analysis including age, sex, gastric disease, and alcohol-related illness.
�p < 0.05
��p < 0.01
���p < 0.001.
https://doi.org/10.1371/journal.pone.0243922.t002
incidence caused by caustic ingestion is 1.4%–2.6% [6,7,14]. Although the incidence might be
overestimated, most experts agree that corrosive injury might be a risk factor for esophageal
carcinoma and have even alleged that the risk is 1,000 times that in the general population
[15]. However, the results of this study are very different from those in the literature. This
research is a nationwide, population-based cohort study designed to identify whether a
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
6 / 11
PLOS ONEEsophageal cancer after pesticide ingestion
Table 3. Incidence and hazard ratio of esophageal cancer between patients with and without pesticide/detergent intoxication.
Variables
Event
Gender
Female
Male
Age, year
�49
50–64
� 65
Comorbidity
No
Yes
Alcohol-related illness
No
Yes
0
24
6
11
7
20
4
22
2
No
PY
55515
89246
74309
36962
33489
130000
14760
144121
639
Pesticide/Detergent intoxication
Rate#
Event
0.00
2.69
0.81
2.98
2.09
1.54
2.71
1.53
31.3
2
48
16
19
15
30
20
39
11
Yes
PY
45199
69523
63048
29178
22496
90783
23939
110234
4489
Rate#
Crude HR (95% CI)
Adjusted HR&
(95% CI)
0.44
6.90
2.54
6.51
6.67
3.30
8.35
3.54
24.5
-
2.59(1.59, 4.23)���
-
2.22(1.34, 3.69)��
3.16(1.24, 8.08)�
2.23(1.06, 4.68)�
3.19(1.30, 7.83)�
2.84(1.08, 7.47)�
1.63(0.74, 3.57)
2.94(1.19, 7.26)�
2.16(1.22, 3.80)��
3.07(1.05, 8.98)�
2.32(1.32, 4.10)��
2.77(0.92, 8.31)
2.33(1.38, 3.94)���
2.47(1.46, 4.16)���
0.78(0.17, 3.53)
1.26(0.27, 5.94)
PY, person-years.
Rate#: incidence rate per 10,000 person-years.
Crude HR, relative hazard ratio.
Adjusted HR†: Multivariable analysis including age, sex, gastric disease, and alcohol-related illness.
�p < 0.05
��p < 0.01
���p < 0.001.
https://doi.org/10.1371/journal.pone.0243922.t003
significant association exists between caustic ingestion and the risk of subsequent esophageal
cancer. We defined conventional risk factors for esophageal cancer, such as age, sex, smoking,
alcohol abuse, and gastric disease (such as achalasia and GERD), which were already well-
established previously. In this 1-million-people cohort, 4,429 people were included in the
detergent and corrosive intoxication group. The relative risk of esophageal cancer did not
increase in patients with caustic agent and detergent poisoning compared with those without
the poisoning after adjustment for these conventional risk factors. One of the reasons might be
that our study included patients with exposure to detergents with less caustic characteristics.
Detergents with acidic or alkaline characteristics are some of the most used toxic and corrosive
Table 4. Incidence and adjusted hazard ratio of esophageal cancer between different entities of pesticide/detergent intoxication.
Variable
Without Pesticide/Detergent intoxication
With Organophosphate/Carbamate + Pesticide (ICD-9-CM code 989.3, 989.4)
With Detergent (ICD-9-CM code 983, 989.6)
N
21840
17411
4429
No. of Events
24
47
3
Rate#
1.66
5.31
1.14
Adjusted HR†
1.00
2.52
0.98
95% CI
(Reference)
(1.52, 4.18)
(0.29, 3.33)
PY, person-years.
Rate#, incidence rate per 10,000 person-years.
Crude HR, relative hazard ratio.
Adjusted HR†: Multivariable analysis including age, sex, gastric disease, and alcohol-related illness.
�p < 0.05, ��p < 0.01, ���p < 0.001.
https://doi.org/10.1371/journal.pone.0243922.t004
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PLOS ONEEsophageal cancer after pesticide ingestion
chemicals at home. In general, detergents are classified into three categories according to their
surfactant electrical charge: nonionic, anionic, and cationic. Nonionic and anionic detergents
have low toxicity, although they may be mild to moderate irritants. Most serious toxins are cat-
ionic detergents. Most of the detergents used at home are nonionic and anionic. Therefore,
patients with ICD-9-CM codes 983.1 and 983.2 (acidic and alkali corrosive injury), 983.9
(caustic intoxication), or 989.6 (detergent intoxication) were identified, which expanded the
dataset and weakened the results. The grade of esophagus corrosive injury of these cases is not
available in the database. Thus, the true risk of esophageal cancer might be underestimated
because, theoretically, esophageal cancer commonly occurs in patients with high-grade esoph-
ageal corrosive injury. However, based on these data, the results still have considerable
credibility.
Another reason might be that the exposure interval after intoxication is shorter in this
study than in previous studies (only 12 years with an average follow-up duration of only 5
years more). The results might be different if we increased the data and extended the study
period. In previous studies, lye ingestion resulted in squamous cell carcinoma in the esophagus
rather than adenocarcinoma [16]. Despite its uncertain etiology and pathogenesis, the mecha-
nism of esophageal cancer after caustic agent and pesticide ingestion is probably similar to that
of achalasia or esophageal diverticulum. The severe injury of esophagus after caustic ingestion
causes lumen stricture or decreased esophageal motility. Subsequently, esophageal stasis
occurs, which leads to local chronic inflammatory responses in the esophageal mucosa, which
can lead to carcinogenesis. In cases of chronic irritation caused by foods and gastric fluid in
achalasia, reflux esophagitis, or Barrett’s esophagus, the interval between disease diagnosis and
esophageal carcinoma development was approximately 10–15 years [17]. However, the interval
was considered to be shortened to 4 years for patients with aforementioned diseases who were
exposed to airborne toxins that resulted from the terrorist attack of the World Trade Center
[18]. Chemical hazard exposure can accelerate solid tumor development, such as esophageal
carcinoma. In total, 287 chemicals or chemical groups with potential carcinogenic effects were
identified in the field of the World Trade Center, including several organic solvents used in
pesticide synthesis.
In this study, the relative risk of esophageal cancer increased significantly by 2.52× in the
pesticide group, and it was 2.47× even after excluding the comorbidity of alcohol-related ill-
ness. Some pesticides are considered to become carcinogenic over a long time, including their
main ingredients or organic solvents. However, such carcinogenicity was identified for most
of them after chronic exposure in in vitro, in vivo, or epidemiological studies. No study has
examined the relationship of acute large dose exposure with the occurrence of esophageal can-
cer. However, some studies have reported that esophageal cancer is positively associated with
intensive pesticide exposure. Jansson et al. found increased esophageal adenocarcinoma risk
among people with high exposure to pesticides [19]. Meyer et al. showed that esophageal can-
cer is correlated with pesticide exposure because of the high mortality caused by esophageal
cancer in states in Brazil using a high proportion of pesticides [20]. Several pesticides have
been identified as carcinogens, including their main ingredients or solvents. Animal studies
have demonstrated strong genotoxicity for some pesticides, such as diazinon organophos-
phates, malathion, and glyphosate herbicide, due to DNA and chromosomal damage. Further-
more, numerous animal studies have shown strong cellular oxidative stress reactions for them.
Glyphosate herbicide damages the retro-pharynx and esophagus more severely than other pes-
ticides and causes a high rate of morbidity among patients because of its surfactant (poly-
ethoxylated tallowamine) [21,22]. In this cohort study, a high proportion of patients in the
pesticide/detergent intoxication cohort had hypertension, diabetes mellitus, gastric disease,
ischemic heart disease, cerebrovascular disease, chronic obstructive pulmonary disease,
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
8 / 11
PLOS ONEEsophageal cancer after pesticide ingestion
alcohol-relative illness, and obesity (all p < 0.001). Single severe direct esophageal mucosa
damage as well as subsequent inflammation might be one of the causes of carcinogenicity in
these patients with chronic systemic diseases and on long-term medication, with possible mal-
function of the esophagus and stomach. However, in-depth animal experiments and studies
are required to explore the possible mechanisms of the correlation.
Our study has several limitations. The data were collected based on the ICD-9-CM codes in
the database; therefore, some detailed information could not be obtained. First, the grade of
esophageal corrosive injury after caustic ingestion is not provided in the database. This might
underestimate the true risk of esophageal cancer because, theoretically, esophageal cancer
occurs commonly in patients with high-severity esophageal corrosive injury. Second, although
ICD-9-CM codes are used for acidic and alkali corrosive injury (983.1 and 983.2), most doc-
tors in Taiwan refer such patients for the diagnosis of caustic intoxication (ICD-9-CM code
983.9) or detergent intoxication (ICD-9-CM code 989.6). It makes a huge difference in the
case numbers between these diagnoses. Therefore, we cannot evaluate esophageal cancer risk
in patients with acidic and alkaline caustic injury accurately. Third, although caustic, deter-
gent, and pesticide intoxication in Taiwan are mostly through the oral route, using a diagnostic
code to represent all oral-route intoxication could still slightly affect the results. Fourth, due to
the limitation of the ICD-9-CM diagnostic codes, we could categorize the pesticides used for
further detailed analysis. Furthermore, we were unable to extract the exact pathology reports
from the database; thus, we could not further categorize the pathologies into premalignancy
lesions, such as polyp or hyperplasia, or malignancies, such as adenocarcinoma or squamous
cell carcinoma. Fifth, because a health insurance claims database was used, detailed informa-
tion on certain general characteristics, such as obesity, body mass index, smoking, exercise,
and dietary habits, was lacking. To compensate, we tried to use clinical examination-related
morbidities to correct the individual examination index. Lastly, the present research involved
only the Taiwanese general population, which includes 99.5% Han Chinese; thus, differences
may be apparent in a stratified population.
Conclusively, to determine the association between corrosive and detergent intoxication
and esophageal cancer risk, the present study analyzed a population-based cohort from a
nationwide claims database and adjusted for comorbidities to comprehensively assess corro-
sive intoxication-related esophageal cancer risk. We observed that patients with preexisting
corrosive poisoning did not exhibit a higher esophageal cancer risk than the general popula-
tion. However, preexisting pesticide intoxication was associated with a 2.5-fold higher risk of
esophageal cancer compared with the general population. Further investigations are required
to delineate the association between esophageal carcinoma and esophageal corrosive injury or
pesticide poisoning.
Author Contributions
Conceptualization: Han-Wei Mu, Chi-Syuan Pan.
Data curation: Cheng-Li Lin.
Formal analysis: Cheng-Li Lin.
Methodology: Cheng-Li Lin.
Supervision: Chun-Hung Chen, Dong-Zong Hung.
Writing – original draft: Han-Wei Mu.
Writing – review & editing: Kai-Wei Yang, Dong-Zong Hung.
PLOS ONE | https://doi.org/10.1371/journal.pone.0243922 December 29, 2020
9 / 11
PLOS ONEEsophageal cancer after pesticide ingestion
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10.1103_physrevresearch.5.013168.pdf
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PHYSICAL REVIEW RESEARCH 5, 013168 (2023)
Surrogate light curve models for kilonovae with comprehensive wind ejecta outflows
and parameter estimation for AT2017gfo
Atul Kedia ,1 Marko Ristic ,1 Richard O’Shaughnessy ,1 Anjali B. Yelikar
,1 Ryan T. Wollaeger
,2,3 Oleg Korobkin ,2,4
Eve A. Chase ,2,5 Christopher L. Fryer
,2,3,6,7,8 and Christopher J. Fontes
2,9
1Center for Computational Relativity and Gravitation, Rochester Institute of Technology, Rochester, New York 14623, USA
2Center for Theoretical Astrophysics, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
3Computer, Computational, and Statistical Sciences Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
4Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
5Intelligence and Space Research Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
6University of Arizona, Tucson, Arizona 85721, USA
7Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131, USA
8George Washington University, Washington, DC 20052, USA
9Computational Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
(Received 8 November 2022; accepted 20 January 2023; published 13 March 2023)
The electromagnetic emission resulting from neutron star mergers have been shown to encode properties
of the ejected material in their light curves. The ejecta properties inferred from the kilonova emission has
been in tension with those calculated based on the gravitational wave signal and numerical relativity models.
Motivated by this tension, we construct a broad set of surrogate light curve models derived for kilonova ejecta.
The four-parameter family of two-dimensional anisotropic simulations and its associated surrogate explore
different assumptions about the wind outflow morphology and outflow composition, keeping the dynamical
ejecta component consistent. We present the capabilities of these surrogate models in interpolating kilonova
light curves across various ejecta parameters and perform parameter estimation for AT2017gfo both without any
assumptions on the outflow and under the assumption that the outflow must be representative of solar r-process
abundance patterns. Our parameter estimation for AT2017gfo shows these surrogate models help alleviate the
ejecta property discrepancy while also illustrating the impact of systematic modeling uncertainties on these
properties, urging further investigation.
DOI: 10.1103/PhysRevResearch.5.013168
I. INTRODUCTION
Merging neutron stars have been demonstrated to emit
both gravitational waves (GW) and a variety of accessible
electromagnetic counterparts, as shown by the observation
of GW170817 and the following transient AT2017gfo [1–7].
Also emitted during merger is the most unambiguous in-
dication of matter in these systems: nuclear matter ejected
due to the merger itself, which over time expands and heats
through ongoing radioactive decay, producing a distinctive
“kilonova” emission [8–11]. Particularly in conjunction with
gravitational wave observations [1,2,12–17], kilonova discov-
eries can provide insight into the physics and significance of
this radioactive ejecta. On the one hand, these counterparts
probe uncertain nuclear physics [18–22]. On the other, these
processes may be in part responsible for the production of
r-process elements throughout the universe. [8,18,23].
Published by the American Physical Society under the terms of the
Creative Commons Attribution 4.0 International license. Further
distribution of this work must maintain attribution to the author(s)
and the published article’s title, journal citation, and DOI.
Kilonova observations in principle encode the amount and
properties of the ejected material in multiwavelength light
curves (LCs) and spectra [10,24,25]. Previous investigations
have characterized this ejected material via two components,
denoted as dynamical and disk wind ejecta, reflecting differ-
ences in their formation and ejection mechanisms. Several
studies of GW170817 attempted to infer the amount of mate-
rial ejected [3–5,24–33]. However, the amount and properties
of the ejected material from this event remain uncertain and
in considerable tension with theoretical expectations for the
amount of each type of ejecta [32,34–36], likely in part
because of underestimated uncertainties in these theoretical
ejecta estimates [37].
The tension between observation and expectations could
in principle reflect modeling systematic errors. These obser-
vations have historically been interpreted with semianalytic
models [9,10,38] as they can be evaluated quickly and con-
tinuously over the parameters, which characterize potential
merger ejecta. However, it is well known that these semi-
analytic models contain oversimplified physics of already
simplified radiative transfer calculations [39–41] that ne-
glect detailed full
three-dimensional anisotropic radiative
transfer, opacity, sophisticated nuclear reaction networks,
and composition differences. That said, recent calculations
using improved anisotropic radiative transfer and opacity
2643-1564/2023/5(1)/013168(15)
013168-1
Published by the American Physical Society
ATUL KEDIA et al.
PHYSICAL REVIEW RESEARCH 5, 013168 (2023)
calculations still arrive at qualitatively similar conclusions
for AT2017gfo [27,31–33,42,43]: a relatively high mass blue
component outflowing along the poles, and a significant mass
in a red component outflowing preferentially towards the
equator. Reference [32] also identifies a larger velocity for the
blue component, although the result reverses upon excluding
bands that exhibit large uncertainties. However, recent nu-
merical relativity simulations give surprisingly low dynamical
outflow velocities when mass averaged, e.g., see Ref. [34] for
example, and are not in as much disagreement with regards
to the red component. (Some recent calculations with more
complex outflow morphologies, however, recover wind speeds
more consistent with prior expectations [26].) Essentially, the
best-fitting properties of the ejected material in our polar
(blue) and equatorial (red) ejecta are in tension with theoreti-
cal expectations for their physical origin.
Motivated by this tension, in this paper we revisit our
detailed anisotropic radiative transfer calculations and infer-
ence [32,41], now allowing for a wide selection of outflow
morphologies [36] to see impact on ejecta properties of
AT2017gfo. The properties of the outflow that we vary in
this paper are the outflow mass-density profile for each com-
ponent (referred to as the “morphology” for the rest of the
paper) and the nuclear composition using the electron fraction
Ye ≡ (np)/(np + nn) as a proxy, where np is the number of
protons and nn is the number of neutrons in the ejecta. Effects
of different dynamical ejecta morphologies have been studied
in the past to show significant light curve (LC) shifts [36],
with a larger dependence on morphologies as compared to
the anecdotal ejecta masses and velocities. Certain outflow
models create a strong angular differential in the LC by
suppressing the bluer bands along the equatorial plane (also
known as lanthanide curtaining) [44–46].
In this paper we present a new set of surrogate models
describing kilonova LCs resulting from a broad set of neu-
tron star merger ejecta. This paper is organized as follows.
In Sec. II we review our approach of adaptively generating
kilonovae simulations, constructing the surrogate LC model
using Gaussian process regression, and performing param-
eter estimation (PE) for ejecta properties. We also discuss
the specific alternate outflow morphologies and compositions
employed in this paper. For context and to better highlight
current tension with contemporary theoretical models, we also
introduce estimates for the ejected material in each component
applied to interpreting GW170817 given the well-constrained
source distance and inclination. In Sec. III we discuss the new
surrogate LC models and describe our PE results obtained
using them. We further conclude this section with a discussion
on the implications of this tension for joint multimessenger
inference with contemporary ejecta models. We then conclude
in Sec. IV. We provide all the simulation models, the surrogate
models developed and employed in this paper, and sample
codes to generate LCs at a public Zenodo repository [47].
The surrogates and sample codes are also available at a public
GitHub repository [48].
initial simulations for emitted spectra using the radiative trans-
fer code SuperNu. Then our active learning scheme iteratively
chooses the “best” ejecta parameters to simulate until the
simulation space is sufficiently large in size to produce a
robust surrogate model. We then construct high-fidelity mul-
tidimensional surrogate LC models for each morphology and
composition combination using Gaussian process regression
(GP) as was performed in [32]. These surrogate models are
now capable of making predictions of LCs along several
model parameters. The surrogate models are then used to
infer parameters for AT2017gfo and we compare these elec-
tromagnetically inferred ejecta parameters with inferred ejecta
parameters from the corresponding gravitational wave sig-
nal GW170817 using a library of numerical relativity-based
ejecta models. These steps are further discussed and detailed
in the following subsections.
A. Simulation methods and placement
We perform simulations of kilonova LCs using the time-
dependent radiative transfer code SuperNu [49,50], following
the methodology presented in [32,36,39,41] and references
therein. To determine nuclear heating rates, we use the
detailed, time-dependent radioactive isotope composition re-
sults from the nucleosynthesis simulations with the WinNet
code [51,52] and include contributions of individual radiation
species (such as α-, β-, γ -radiation, and fission products)
for each isotope. The contributions are then weighted by
thermalization efficiencies from [53] (a detailed description
of the adopted nuclear heating can be seen in Ref. [39]).
These heating rates and composition effects together along
with the tabulated binned opacities resulting from the the Los
Alamos suite of atomic physics codes [54,55], give the resul-
tant kilonova LCs. The tabulated binned opacities used in this
paper, however, are not calculated for all elements. Instead we
produce opacities from representative proxy elements by com-
bining pure-element opacities of nuclei with similar atomic
properties [55]. The output we obtain from SuperNu are light
spectra for 54 viewing angle bins uniformly distributed be-
tween 0 and 180 deg in cosine space. For each viewing angle
bin, the light rays are collected from across the face of the
ejecta as seen from the direction of that viewing angle.
To simplify comparison with previous paper, we adopted
the same set of representative elements as in past work
[32,41], however, a recent study [56] includes a more com-
prehensive list of elements, including actinides. A comparison
in Fig. 8 in Ref. [56] shows that when the actinide opacities
are improved upon the luminosity varies by ∼15% at its
maximum displacement. As will be discussed later in Sec. III,
this displacement is currently significantly smaller than our
GP interpolation error making the changes with the new ele-
mental approach less significant for the purposes of this paper.
However, any followup work should utilize the complete set
of elemental opacities.
II. METHOD
The workflow pipeline is discussed in detail in this sec-
tion and can be summarized as follows: We start by generating
B. Initial conditions: Wind morphologies and compositions
As initial conditions for the SuperNu code, we employ a
two-component ejecta model, comprising an unbound dynam-
ical ejecta from the merger, followed by the disk wind ejecta.
013168-2
SURROGATE LIGHT CURVE MODELS FOR KILONOVAE …
PHYSICAL REVIEW RESEARCH 5, 013168 (2023)
TABLE I. Ejecta morphologies and compositions studied in this
paper. The composition of the dynamical component is fixed at
Ye = 0.04. In terms of this notation, the previous investigation studied
a TPwind2 outflow [32].
Name
TPwind1
TSwind1
TSwind2
Wind
Morphology
Peanut
Spherical
Spherical
Ye
0.37
0.37
0.27
Dynamical
Torus
Torus
Torus
We set the outflow velocity based on prior understanding
of expected ejecta [57,60,61]. The ejecta velocity profile can
alter the location of the photosphere for any given wavelength
and thus affect the resultant LC. Specifically, the near-UV
radiation peak time can be moved from an hour to a day
postmerger by simply changing the velocity distribution. In
this paper, however, we assume a homologous velocity profile
for the ejecta, which, i.e., it scales as r/t, where r is the
distance from the center and t is the time postmerger. We do
not include a third component that could attribute to the early
blue peak.
All ejecta components are assumed to be expanding homol-
ogously with a prescribed velocity profile, mass distribution
versus angle (see Ref. [36] for their complete description),
and prescribed uniform composition set by its initial electron
fraction Ye. As discussed earlier, we use Ye as a proxy for ejecta
composition in these simulations.
We simulate a range of wind ejecta morphologies and
compositions in order to study their influence on kilonova
LCs, and build robust surrogate models that can be used for
parameter inference of kilonovae observations. The outflow
morphologies we model are selected from previously studied
models [36,41] with a varying set of wind ejecta structure
and electron fraction. Table I shows the morphology and
composition combinations simulated. Here, for instance, the
model labeled TPwind1 comprises a Torus shaped dynamical
ejecta, and a Peanut shaped wind ejecta (S would indicate a
Spherical wind ejecta) with their mathematical form given in
Ref. [36]. The labels “wind1” and “wind2” denote the two
choices of wind ejecta composition. wind1 corresponds to
the less neutron rich configuration with Ye = 0.37 whereas
wind2 corresponds to a more neutron rich Ye = 0.27; wind2
with a Peanut morphology, i.e., TPwind2, was adopted in the
previous paper [32] and hence a new surrogate model for the
case is not generated in this study. As was in previous paper,
we fix the composition of the dynamical ejecta as Ye = 0.04.
For each source morphology and composition, we place an
initial coarse grid with ejecta masses (Me j/M(cid:4)) having val-
ues 0.001, 0.003, 0.01, 0.03, 0.1 and ejecta velocities (ve j/c)
having values 0.05, 0.15, 0.3 for each of the two compo-
nents making our initial grid of (5 × 3)2 = 225 simulations
(see Refs. [17,28,57–59] for a discussion on expected ejecta
masses). The base grid [(5 × 3)2 = 225] for our simulations
is the same as previously studied in Ref. [41] to which we
add additional simulations doubling the grid space via the
active learning technique discussed in Ref. [32]. The iterative
process targets subsequent simulation parameters for investi-
gation, based on the estimated uncertainty of a (simplified)
Gaussian Process estimate for the emitted radiation from the
existing simulation set. By the end of the iterative process
we accumulate 450, 449, and 449 simulations for the three
morphology and composition combinations, respectively. The
TSwind1 and TSwind2 model families each have one fewer
simulation in their training libraries due to isolated instances
of single simulation processing error. We limit the iterative
learning process to 450 simulations because in our experience
from previous study (Ref. [32]) sufficiently accurate surrogate
models can be obtained with a sample size this large.
C. Motivation for alternate morphologies
Inferences made about ejecta properties of the event
AT2017gfo, derived from the kilonova LCs [32], are not con-
sistent with contemporaneous forward-model predictions for
ejecta masses from GW inferences of the masses deduced
for GW170817. Our kilonova analysis suggests that much
larger wind velocities (and masses) will be required, inconsis-
tent with the modeling assumptions usually adopted for polar
winds.
Recently, Nedora et al. [34,62] have proposed an alter-
native mechanism to generate disk outflows: a spiral-wave-
driven wind, which generally distributes over a large solid
angle. For the purposes of our phenomenological kilonova
inference, which focuses on the nature of outflows rather
than their origin, such an outflow will have a different mor-
phology than the polar “peanut” wind and “torus” dynamical
morphology assumed for outflows. Further, Breschi et al.
[26] have performed inference using simplified LCs extracted
from systematically explored one-, two- and three-component
models with several isotropic and anisotropic morphologies.
They find a strong preference for anisotropic models with the
inclusion of multiple components leading to largest evidence.
However, their isotropic model (ISO-DV) makes even the
dynamical components isotropic, whereas in this paper we
choose an anisotropic dynamical ejecta shape (torus). Addi-
tionally, Kawaguchi et al. [31] obtain a strong similarity in
the LCs for AT2017gfo and for a two-component model with
a postmerger wind ejecta that is spherically symmetric.
The effect of morphologies of the ejecta was also studied
extensively in the past [36], where morphologies were shown
to have a greater impact on the LCs than the ejecta masses and
velocities. The effect manifests heavily in the form of altering
the peak luminosity and peak times. We therefore assemble an
expanded archive of actively-learned kilonova models, with
more options for the wind-driven outflow morphology, to as-
sess whether we can better reconcile our kilonova inference
with forward models for the ejecta. To maximize the impact of
altering wind morphology in our study, we adopt spherical and
peanut shaped wind model. Other detailed simulations and the
studies above all naturally produce a morphology much more
similar to our preferred (torus) morphology.
D. Simulation interpolation
Using the set of actively-learned simulations, we follow
our previous approach [32] to interpolate the resulting AB
magnitudes versus simulation parameters (md , vd , mw, vw ),
time postmerger, viewing angle, and wavelength bands.
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FIG. 2. Wavelength interpolation using our surrogate model for
an off-sample wavelength bands CFHT (1451 nm, i.e., between the
J- and H -bands) and F182M (1839 nm, between H - and K-bands),
generated for the TPwind1 model with parameters (md /M(cid:4), vd /c,
mw/M(cid:4), vw/c) = (0.014, 0.183, 0.085, 0.053) viewed along the sym-
metry axis θ = 0. The dashed curves (red for CFHT and green for
F182M) along with their respective bands indicate the predicted LC
from our surrogate model and solid curves indicate the LC generated
from the code SuperNu via the mechanism explained in Sec. II A.
TPwind2 configuration, as was performed in [32], whereas
the bottom panel shows the same for TSwind2 model. Hence,
apparent differences in the two predictions arise solely due to
differences in the wind morphology.
As noted earlier, our GP training scheme interpolates be-
tween filter bands, over a nominal wavelength parameter. As
a result, our GP approach can estimate LCs for filters both in-
cluded and not included in our original training set. We verify
the fidelity of our wavelength interpolation LC prediction by
comparison to SuperNu spectral output convolved with two
new filters. Figure 2 illustrates our wavelength interpolation
LC prediction in dashed curves compared to the SuperNu
spectral output in solid curves convolved with two distinct real
filters not included in our original training set. One of these
filters is the the WIRCam 8105 broadband filter [63] from the
Canada-France-Hawaii Telescope (CFHT), part of the Mauna
Kea Observatory, with an effective wavelength of 1.45 µm.
This filter has minimal overlap with the H-band filter, thus
serving as an independent test of wavelength interpolation
ability. We also show results for the JWST/NIRCam.F182M
filter [64], which lies between the H- and K-bands with small
overlap with the K band and has an effective wavelength of
1.84 µm [65].
Our GP models occasionally produce glitches as can be
seen at t ∼ 10 days in Fig. 2. These glitches occur only
for the wind1 composition models for both TS and TP mor-
phologies (also visible in Fig. 5) and affect the quality of
the predicted LC significantly at times beyond 4 days. This
error-prone training may be resolvable by developing a so-
phisticated hyperparameter selection method that restricts the
hyperparameters to the region of the preceding parameters
hence avoiding large jumps.
E. Ejecta parameter inference
Following Ref. [32] we use conventional Bayesian tech-
niques to reconstruct the ejecta parameters (md , vd , mw, vw )
and emission direction θ most consistent with GW170817,
FIG. 1. Illustrating off-sample interpolations for two morpholo-
gies. Top panel: The bottom panel from Fig. 4 of Ref. [32] showing
interpolation of various LCs versus time for the TPwind2 morphol-
ogy adopted in that paper. Different colors denote different filter
bands, described in the legend. The dashed lines show full simulation
output for each band. The colored points show our interpolated
magnitude predictions at the evaluation times. The simulated param-
eters and viewing angle for this configuration are (md /M(cid:4), vd /c,
mw/M(cid:4), vw/c) = (0.097, 0.198, 0.084, 0.298) at 0◦ [32]. Bottom
panel: As above, but for the TSwind2 model morphology. The shaded
region surrounding each solid curve shows our estimated GP fitting
uncertainty at each time. The differences between these two panels
illustrate the impact of outflow morphology on our results.
Interpolation over simulation parameters and for each band
is performed by Gaussian process regression at fiducial ref-
erence times and fiducial angles (0,30,45,60,75,90 degrees).
A continuous LC over time and angle follows by stitching
together these fiducial results with simple low-dimensional
interpolation. Unless otherwise noted, we quantify the perfor-
mance of our interpolation with the RMS difference between
our prediction and the true value. Because of the substantial
dynamic range of our many outputs, we interpolate in AB
magnitudes using the LSST grizy and 2MASS JHK bands as
our reference bands. Our raw LCs are calculated in absolute
magnitudes, i.e., at a fiducial distance of 10 pc to the source.
In Fig. 1 we show our surrogate model predicting LCs
for off-sample outflow. The prediction is for outflow param-
eters (md /M(cid:4), vd /c, mw/M(cid:4), vw/c) = (0.097, 0.198, 0.084,
0.298). These parameters are chosen such that they are neither
on the primary training grid nor the actively chosen simulation
parameters. Top panel shows the parameter LC predicted for
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FIG. 3. Left panel: Illustration of systematics in modeling ejecta from binary mergers, compared to a fiducial inference of those ejecta
parameters. Black curves are deduced from inferences on GW170817 mass estimates combined with different models for the ejecta; for
example the black solid line is derived from Eqs. (1)–(3). To isolate the effect of ejecta modeling systematics, all predictions are shown under
the optimistic assumption of a perfectly known nuclear equation of state, here APR4 [70], without adding additional uncertainties to account
for estimated fitting errors in the relations between ejecta and binary parameters. While the ejecta predictions for GW170817 are relatively
consistent with one another, they are in tension with our interpretation of the GW170817-associated kilonova’s ejecta assuming a TPwind2
outflow form. Curves correspond to 90% credible regions. Right panel: Parameter inference for LC based on EM paper prior (uniform in
velocities, log-uniform in masses) [32] (blue-solid) and r-process prior [69] (green-dashed), but allowing for relative systematic uncertainty
exp(±0.3) in both ejecta masses. The inner and outer curves on the two-dimensional plots correspond to 68% and 95% credible regions. The
ejecta estimate illustrated from GW includes no systematics, either from uncertainty in the EOS or from intrinsic uncertainty in the estimate
itself; compare to Fig. 6.
using the known source emission distance and taking into
account prior information about the source orientation di-
rection. As previously, we adopt uniform priors in velocity
and log-uniform for masses over the limiting ranges. As
a concrete example,
the blue contours in Fig. 3 show
previously-presented results from [32] for two-component
ejecta properties assuming the TPwind2 morphology.
While our default inference makes no additional assump-
tions about the ejecta, we separately also require that the
merger from AT2017gfo produces a full r-process element
spectrum, consistent with the solar spectrum. Doing so con-
strains the ratio of mw/md to be close to 13.90 (1.76) for the
wind1 (wind2) model assuming FRDM2012 as the nuclear
mass model [67] and fission model by Panov et al. (2010)
[68] as described in [69]. The blue curves in the right panel
of Fig. 3 show an analysis assuming this prior for the relative
amounts of the two ejecta components.
The inferred ejecta properties with these Torus/Peanut
models are, however, somewhat surprising in the context of
conventional theoretical expectations about the two compo-
nents. Most notably, our analysis requires a substantial wind
velocity (cid:6) 0.2c, consistent with previously-reported phe-
nomenological estimates (see, e.g., Table 2 or Fig. 5 in [34]),
but in contrast to most theoretical expectations [35]. This high
wind velocity allows the peanut-morphology wind (which, in
our calculations, explains the rapidly decaying blue compo-
nent after its early peak) to have the short timescales required
for the blue component, while simultaneously matching the
target blue luminosity early on. By contrast, the “dynamical”
red torus component can be consistent with GW170817’s
associated emission with a wide range of velocities [26,35].
In earlier studies [36], it was noted that the dynamical ejecta
mass was poorly constrained, due to the lanthanide curtain-
ing effect [45]. Since lanthanide curtaining occurs in models
with greater velocity difference in the dynamical and wind
components, this makes viewing angle dependence (caused by
the curtaining) more velocity dependent than mass dependent
[36].
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TABLE II. Numerical relativity-based forward models employed
in this work for GW170817 ejecta PE. The velocity fits are common
for all. Dynamical ejecta velocity fit is given in Eq. (7) based on
[28,59]. Wind velocity is set fixed at vw = 0.08c [61].
Name
CoDi19
DiCoSci20
KruFo20
Nedora21
md
(cid:2)
CoDi19
(cid:2)
(cid:2)
mw
(cid:2)
(cid:2)
(cid:2)
CoDi19
Reference
[28]
[17]
[58]
[60]
F. Contemporary forward models for neutron
star merger ejecta
After using parameter inference to deduce the possible
immediate outflow responsible for the kilonova associated
with GW170817, we arrive at inferred ejecta masses and
velocities for that outflow. For context and to help guide our
investigations, we compare these inferred ejecta properties
with the predictions provided by selected contemporary for-
ward models, which attempt to estimate the ejecta properties
from inferred binary properties [17,28,58,59,71]. We use four
discrete models for this purpose, summarized in Table II, and
present details about them here.
We employ the following estimates for the dynamical and
wind ejecta mass [28]. First, the disk mass is estimated as their
Eq. (1),
log10(mdisk[Mtot/Mthr])
(cid:2)
(cid:2)
= max
−3, a
1 + b tanh
(cid:4)(cid:5)(cid:5)
(cid:3)
c − Mtot/Mthr
d
(1)
with a = −31.335, b = −0.9760, c = 1.0474, d = 0.05957.
Mtot is the sum of neutron star masses, and Mthr is the thresh-
old mass for the binary to undergo a prompt collapse to a BH
after merger, which can be estimated by (e.g., Bauswein et al.
2013 [72])
Mth =
2.38 − 3.606
MTOV,
(2)
(cid:2)
(cid:5)
MTOV
R1.6
where MTOV is the maximum gravitational mass of a stable
nonrotating neutron star given the EOS and R1.6 is the radius
of the neutron star for the EOS with a mass 1.6 M(cid:4). The
estimated uncertainty on this relation is of roughly a factor
of 2, or 0.02 M(cid:4). The wind ejecta mass mwind = ξ mdisk where
ξ = 0.3, with an estimated uncertainty of O(1). The dynami-
cal ejecta mass is estimated by their Eq. (2),
(cid:2)
(cid:4)
(cid:3)
log10 mdyn =
a
(1 − 2C1)m1
C1
+ b m2
(cid:5)
n
m1
m2
+ d
2
+ [1 ↔ 2],
(3)
where in this expression m1 and m2 are the neutrons star
masses, a = −0.0719, b = 0.2116, d = −2.42, n = −2.905,
and Ci are the compactnesses of the two neutron stars. [1 ↔ 2]
is a shorthand for the preceding terms in the expression with
permuted subscripts. The estimated uncertainty is for this
relation is 7 × 10−3M(cid:4) when calculated linearly or up to
36% when calculating for log10 mdyn. This model is labeled
“CoDi19” in the relevant plots.
For a more recent estimate, we also utilize the updated
model from Ref. [17] that has been calibrated for a wider
range of binary mass ratios. A new disk mass fitting is calcu-
lated in this study and is given in Eqs. (S4)– (S6) in Ref. [17]
and is the same as Eq. (1) with updated constants. The fitting
parameters here are a = a0 + δa · ξ , b = b0 + δb · ξ , and
2 tanh (β( ˆq − ˆqtrans)), a0 =
the resulting constants are ξ = 1
−1.5815, δa = −2.439, b0 = −0.538, δb = −0.406, c =
0.953, d = 0.0417, β = 3.910, ˆqtrans = 0.900. This model
is labeled “DiCoSci20” in the relevant plots.
As a complementary estimate to highlight their systematic
error, we also provide postprocessing estimates provided with
an alternative set of fits from Kruger and Foucart [58]. In this
approach, the disk mass is estimated as
mdisk,KF = m1max[5 × 10−4, (aC1 + c)d ],
where C1 is the compactness of the lighter of the two neutron
stars, a = −8.1324, c = 1.4820, d = 1.7784 with an error of
order 40%. The dynamical mass is estimated as
(4)
mdyn,KF
10−3M(cid:4)
=
(cid:2)
a
C1
(cid:2)
(cid:5)
n
m2
m1
+ b
(cid:5)
+ c C1
m1 + [1 ↔ 2],
(5)
where a = −9.3335, b = 114.17, c = −337.56, and n =
1.5465, where negative values imply zero ejecta. This model
is labeled “KruFo20” in the relevant plots.
For broader context we also report estimates for the dynam-
ical ejecta mass from GW170817 using the more inclusive
and most recent fitting method by Ref. [60]. Among the
available choices of fitting, we use the quadratic fitting of the
form
log10(mdyn/M(cid:4)) = b0 + b1q + b2 ˜(cid:8) + b3q2 + b4q ˜(cid:8) + b5 ˜(cid:8)2,
(6)
where q is the mass ratio (m2/m1 mass), and ˜(cid:8) is the reduced
tidal deformability. Among the new models introduced in
that paper, this model provides the greatest flexibility with
both mass ratio and tidal deformability dependence, although
we note the conspicuous absence of dependence on binary
total mass. From this paper, we adopt the fitting coefficients
obtained for the reference set + M0/M1 set (labelled as
M0RefSet and M0/M1Set), which include the best available
physics, specifically excluding analyses that omit neutrino re-
absorption and have pertinent systematic differences with the
reference calibration adopted here. The parameters thus used
are (from Table 4 of Ref. [60]): b0 = −1.32, b1 = −3.82 ×
10−1, b2 = −4.47 × 10−3, b3 = −3.39 × 10−1, b4 = 3.21 ×
10−3, b5 = 4.31 × 10−7. We exclude a disk mass model from
Ref. [60] due to large systematics and inconsistent defini-
tion between the original datasets. Instead we employ the fit
by [28]. This model is labeled “Nedora21” in the relevant
plots.
For ejecta velocities in each model we choose the results
from Ref. [28,59]. Hence, for the dynamical ejecta we adopt
the formula
vd /c = a
(1 + c C1) + a
(1 + c C2) + b
(7)
(cid:2)
(cid:5)
m1
m2
(cid:2)
(cid:5)
m2
m1
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FIG. 4. Angular dependence for the three surrogate models for each morphology and composition combination, i.e., TPwind1, TSwind1,
and TSwind2. This figure compares the g-, y-, and K-band luminosity (top to bottom) at select times as a function of viewing angle. Different
colors indicate different extraction times. Points show simulation AB magnitude results vs angle θ, while the solid curves and shaded regions
show our prediction and its expected (statistical interpolation) uncertainty. All simulations and surrogate LCs use the parameters (md /M(cid:4),
vd /c, mw/M(cid:4), vw/c) = (0.097, 0.198, 0.084, 0.298); because this configuration has vw > vd (i.e., wind outside the dynamical ejecta), the wind
ejecta’s emission and angular dependence could dominate trends versus angle. Left column: Angular dependence for TPwind1 light bands.
This model shows the largest viewing angle dependence. Center column: Angular dependence for TSwind1. A change in angular dependence
is highly apparent at late times particularly in the g band. Right column: Angular dependence for TSwind2. Differences from the first two
models are apparent. This configuration shows the weakest angular dependence in its emission and the brightest emission.
with a = −0.309, b = 0.657, and c = −1.879 with an esti-
mated relative uncertainty of 20% [28]. For the velocity of
wind ejecta, we adopt 0.08c as was adopted by [61],
vw = 0.08c.
(8)
The solid-black contours in Fig. 3 show our estimated
ejecta masses using these forward models for ejecta. As inputs
to these expressions, we use the results of detailed parameter
inference applied to GW170817, as described in Lange et al.
(in preparation); see also [73]. Even allowing for reasonable
uncertainties in these ejecta formulas, the tension with our
inferred ejecta parameters is apparent: these models predict
roughly 2× smaller ejecta masses for both components, much
slower wind velocities, and an extremely narrow range of
expected dynamical ejecta velocities.
III. RESULTS
A. Impact of morphology on interpolated light curves
Using
simplified
and more
realistic
[26,74,75]
[31,36,39,76,77] models for kilonovae and the associated
radiative transfer, several previous studies have demonstrated
that the angular distribution of the outflow can imprint its
signature on the outgoing radiation. The first and second
columns of Fig. 4 illustrate the impact of outflow morphology
on the interpolated LCs. The plots show g-, y-, and K-band
luminosity as time proceeds along viewing angles for a sample
model parameter (md /M(cid:4), vd /c, mw/M(cid:4), vw/c) = (0.097,
0.198, 0.084, 0.298). As anticipated from the aforementioned
prior paper, we notice a strong impact from the choice of mor-
phology. In particular, relative to our polar outflow illustrated
in the first column (TPwind1), the spherical wind outflow
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in the second column (TSwind1) produces relatively less
angular variability of the LC, particularly in the bluer bands.
A noticeable feature of TPwind1 LCs is that their angular
dependence flips over in the late times, as can be seen by the
apparent opposite curvature at t = 4 days and t = 8 days. This
behavior is resulting from the dispersion of the dynamical
torus component at late times. Compared to this result, the
TS late time LCs are angle independent both for low and high
electron fraction.
The TPwind1 model is able to also exhibits a peak in the
blue band in the early times (t = 0.5 days) as is noticeable in
the top-left panel. A change in the morphology to TSwind1
changes this blue band LC to be monotonically diminishing,
noticeable in the top-middle panel. This will again be seen
in a Fig. 5 below where parameters fitting AT2017gfo with
TPwind1 and r process prior will produce the short-time blue
kilonova peak. This can, however, be altered and other mor-
phologies be made to produce the blue peak at desired times
by fine-tuning component parameters, thus highlighting the
challenges in replicating this observation.
The late time K band is rather similar for all morphologies
and compositions, and most of the differences are present in
the earlier times. This is because, at late times, the photo-
sphere has moved inwards substantially so morphology effects
are minimized and the temperature at the photosphere is near
the K band.
B. Impact of composition on interpolated light curves
The second and third columns of Fig. 4 illuminate how
ejecta composition (Ye) impacts emitted radiation. As ex-
pected, we find brighter LCs at early and late times for lower
Ye (i.e., wind2 is brighter than wind1) in the g-, y-, and other
lower wavelength bands, and somewhat in the K bands. As a
result, the choice of wind composition (Ye) is partially degen-
erate with wind ejecta mass mw, which is not surprising since
products like Yemw enter naturally into the initial conditions.
Further, their is almost no angular dependence in the
TSwind2 and a small angular dependence in TSwind1 because
the wind outflow surpasses the dynamical and dominates
the kilonova producing a viewing angle-independent signal.
At late times the wind ejecta has substantially outflown the
dynamical ejecta due to having vd > vw and directs the emis-
sion. The TSwind2 model, due to its lower Ye, has a higher
wind-heating rates in comparison to the TSwind1 and results
in a lower optical depth. The shallower optical depths of
TSwind2 in comparison with TSwind1 causes its emission
to be largely driven by the wind ejecta component, which is
uniform along different viewing angles. On the other hand for
TSwind1 the dynamical ejecta contribute relatively more to
the emission and hence shows a stronger angular dependence.
As was noticed in Sec. III A the early blue peak was miss-
ing from the TSwind1 model. This peak is retained again here
in the TSwind2 case.
C. Estimated light curves
Given the substantial flexibility that we allow in our kilo-
nova model families, each of which has five free parameters
(two masses, two velocities and the viewing angle), unsurpris-
ingly, our models can find a good fit for EM observations of
TABLE III. Peak likelihood identified in parameter inference for
GW170817. The mass ratios for the cases where the r-process prior
was used during parameter inference were peaked at mw/md = 13.90
and 1.76 for the wind1 and wind2 models, respectively. The fit
likelihoods correspond to the LCs shown in Fig. 5.
Model
TPwind1
TPwind1
TPwind2
TPwind2
TSwind1
TSwind1
TSwind2
TSwind2
Prior
ln Lmax
ln L
ln(L × p)
Fit likelihood (MaP)
uniform
r process
uniform
r process
uniform
r process
uniform
r process
2.41
1.62
0.61
0.49
−9
−8.78
2.84
2.81
−0.15
−0.97
−0.62
−1.18
−11.22
−14.32
2.38
1.93
6.63
−2.20
6.77
4.23
−4.05
−11.26
9.09
6.77
GW170817’s kilonova LC (taken from [25], which compiles
data from [3–7,23,78–82]). Figure 5 shows the inferred LCs
deduced with each of our models. As previously [32] and
unless otherwise noted henceforth, we adopt a strong angular
prior based on afterglow observations [3,16,29,78,83–85].
In all cases, our unconstrained models fit the observations
reasonably well, albeit less well for the bluest bands. Con-
sistent with prior paper [32], our posterior predictions for the
bluest bands are consistently fainter and more rapidly decay-
ing apart from the TPwind1 case, which fits the ∼1 day peak
of g band very well. Lacking large residuals, however, these
figures provide relatively little insight into the overall good-
ness of fit. In Table III, we report the peak likelihood identified
overall in each analysis (ln Lmax, a measure of the goodness
of fit of our unconstrained five-parameter kilonova model;
and the likelihood associated with the maximum a posteriori
(MaP) parameters [ln(L × p)], a goodness of fit measure,
which requires consistency with the prior (either uniform or r
process). For each morphology and wind composition, the two
estimates reported for ln Lmax derived from our unconstrained
and r process constrained analyses are relatively consistent
as expected: both measure quality of fit of the unconstrained
model. Keeping in mind differences in ln L of order unity
correspond to odds ratio changes of order e1, this table shows
that the TSwind1 models fit the data very poorly, but that the
remaining unconstrained models all fit the data reasonably
well. When the r-process prior is imposed, we disfavor the
TPwind1 and TPwind2 models slightly in favor of TSwind2.
D. Discussion of inferred parameters
Despite similarity in inferred LCs, performing ejecta
parameter inference with LC surrogate models from alter-
nate morphologies and compositions unsurprisingly produces
different inferences for ejecta parameters. In Fig. 6 we illus-
trate parameter inference for AT2017gfo based on surrogate
models for different ejecta models with and without includ-
ing r-process priors. The inferred ejecta properties depend
notably on the choice of the outflow’s morphology and com-
position. For example, for our spherical models, the wind
ejecta mass is much smaller than the dynamical ejecta mass,
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FIG. 5. Posterior predicted LCs for AT2017gfo, compared with AT2017gfo observations. Points and error bars denote the observations,
with each color denoting a different filter band. Following [32], the solid curves and shaded intervals show the median and 90% credible
expected LC, deduced by fitting our models to these observations. The left panel of figures denotes our unconstrained models; the right panels
require each outflow to be consistent with Solar r-process abundance (i.e., we also adopt a prior on mw/md such that the ejected material; see
Sec. II E). First row: TPwind1; second row: TPwind2 [32]; third row: TSwind1; fourth row: TSwind2.
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FIG. 6. Morphology and composition dependent parameter inference. This figure shows parameter inference for ejecta properties (md /M(cid:4),
vd /c, mw/M(cid:4), vw/c) derived from GW170817 and AT2017gfo. Colored solid and dotted curves show purely electromagnetic inferences
derived using different families of two-component LC surrogate models and a prior on source inclination. Different solid colors indicate
different choices of outflow and composition with a uniform logarithmic prior on ejecta masses, while colored dotted curves show inferences
with the corresponding morphology/composition pairs while also requiring consistency with the Solar r-process abundance pattern. The black
solid and dotted curves by contrast show three estimates inferred solely from GW measurements, combined with forward models for the
outflow. The legend indicates the morphology pair (e.g., TP = Torus and Peanut), while the integer indicates the wind composition (1 refers
to the wind1 sequence and so on). The inferred wind (and thus total) mass depends substantially on the assumed wind composition and
morphology. The two-dimensional contours correspond to 90% credible intervals.
and the (dominant) dynamical ejecta mass is strongly con-
strained.
However, despite broadening our model space, our ejecta
inferences remain inconsistent with conventional prior ex-
pectations about ejecta from binary mergers, suggesting that
persistent modeling systematics remain.
E. Discussion
We find that both the alternative morphologies and compo-
sitions have a significant impact on emission at t = 1 day and
later in the g-, y-, and K-bands, and for emission in the equa-
torial direction. Reassessing GW170817, we find modestly
different conclusions about ejecta parameters, conditioned
on outflow morphology and composition. The alternate mor-
phologies help alleviate the tension between observational and
theoretical ejecta properties. However, the systematics remain
insufficient to completely reconcile our interpretation of the
ejecta with our prior expectation about the material ejected
from merger based on GW-only inference and theoretical ex-
pectations for merger ejecta.
After exploring a range of outflow morphologies, compo-
sitions, ejecta masses, and ejecta velocities, we find that the
inferences developed from our two-component ejecta models
continue to exhibit tension both with prior expectations of
ejecta from the merger, using its GW-deduced parameters,
and also with the observed LCs themselves missing a blue
component.
Our investigations here have omitted two directions, which
deserve subsequent attention. First, we have adopted very
sharp initial compositions Ye. Full numerical simulations have
consistently suggested peaked Ye distributions with extended
tails [86]. A small contribution of suitable material could help
explain the bright extended blue component missing in some
of our LCs. Second, and in a similar vein, we have restricted
to a two-component model; an additional third small blue
component enhancer, previously attributed to magnetically-
driven winds could help improve our fit as invoked in previous
paper [75]. The recently observed kilonova and long gamma-
ray burst, GRB211211A, has indicated the presence of an
additional thermal component powered by either a GRB jet
or a central magnetar [87–90]. Such a central power source
has been proposed such as a long-lived magnetar, a black
hole powered by accretion disk or a jet cocoon for previous
observations as well [91–98]. Our current study excludes such
a source to power the emission; however, based on the findings
of those studies we anticipate that adding a central engine
could help alleviate the early blue-component mismatch and
should be investigated further in future work.
Further, we notice that our Gaussian process modeling
produces occasional glitches in the surrogate models. These
glitches occur only for the wind1 composition models and
affect the quality of the predicted LC largely at times beyond
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SURROGATE LIGHT CURVE MODELS FOR KILONOVAE …
PHYSICAL REVIEW RESEARCH 5, 013168 (2023)
4 days. This error-prone training may get resolved by de-
veloping a hyperparameter selection method, which carefully
restricts the hyperparameters to preceding parameter neigh-
borhood.
Our inferences of ejecta properties are in modest tension
with the expected ejecta properties, assuming GW-derived
binary properties and NR-calibrated models for the outflows
expected from different binary mergers. However, while we
performed an analysis only of GW170817 where these NR-
calibrated models are indeed most reliable, at larger mass
ratios these models disagree more substantially [37]. These
tensions could be challenging to resolve as a part of joint
multimessenger GW-EM PE for generic neutron star mergers.
IV. CONCLUSIONS
In summary, we have developed families of surrogate mod-
els for kilonova LCs resulting from binary neutron star merger
events. As previously done, using our Gaussian process in-
terpolation applied to an actively-extended simulation archive
we develop surrogates for different ejecta configurations:
three additional wind morphology and composition combi-
nations in a two-component (dynamical and wind) ejecta
approach. Our suite of four kilonova surrogate models now
covers multiple outflow configurations comprising toroidal
dynamical ejecta, and peanut and spherical shaped wind ejecta
with two compositions. These broad set of surrogate models
can be employed for parameter inference of ejecta compo-
nents when kilonovae observations are made in the future and
will assist in determining the physics of these events. These
kilonovae simulations and their surrogates are available at a
Zenodo repository [47] and the surrogates alone in a GitHub
repository [48].
As expected, we find that wind morphology and, to a lesser
extent, composition (within our constrained set of composi-
tions) have substantial impacts on the outgoing emission’s
time, frequency, and angular dependence. To assess the impact
of these differences, we calculate the likely ejecta properties
associated with GW170817’s kilonova, conditioned on the
assumption that the ejecta and radiation exactly reproduce
one of our assumed ejecta models. We find that the choice
of model most strongly impacts the inferred ejecta masses.
None of our inferences strongly constrains the ejected wind
velocity.
To better understand the context of these calculations,
we compare and contrast them with the inputs and out-
puts expected from GW170817’s merger. On the one hand,
we compare our inferred ejecta masses with the expected
ejecta masses deduced from GW170817’s GW-constrained
masses, using several contemporary estimates for the ejecta.
While the EM- and GW-deduced ejecta can be reconciled
for some ejecta models, allowing for substantial fit and EOS
uncertainty, we generally see considerable tension in the in-
ferred ejecta mass, with the EM-inferred masses generally
larger than the GW-deduced ejecta masses when assuming
a single plausible equation of state. Such tension between
GW-deduced (and hence numerical-relativity informed) ejecta
masses has been repeatedly highlighted in the literature
[17,28,37,58,59,71] (a recent paper indicates the possibility of
relieving this tension with the use of new heating rate fitting
formulas [99,100]). Our corroboration of this finding, even us-
ing state-of-the-art ejecta calculations, suggests the resolution
of this discrepancy must invoke other sources of systematic
error, for example in the ejecta initial conditions. On the other
hand, we repeat our ejecta mass inferences while requiring
the ejected r-process mass abundances to be consistent with
Solar r-process patterns. While this constraint sharply reduces
the range of ejecta masses allowed, it does not significantly
change any of the aforementioned conclusions:
the EM-
deduced ejecta masses remain large, while EM-constrained
ejecta velocities remain weakly constrained. Our r-process
constraints on mw/md remain qualitatively consistent with the
corresponding ratios expected from forward-modeling ejecta
starting from GW inferences about binary masses.
Our kilonova generation work has limitations in the fol-
lowing ways, which should be addressed in future work.
The two-ejecta component model is known to account for
the lanthanide rich and lanthanide free outflow materials to
a considerable degree. However, the LC being substantially
different for differing morphologies implies that we would
need a more exhaustive calculation of ejecta LCs with other
morphologies or account for that with a third component.
Hence, adding a third component or a continuous ejecta model
could cause a shift in LCs. Similarly, our present and previ-
ous work suggests that adjusting our assumptions about the
composition, both in median and distribution, can also notably
impact the LCs. We have also highly simplified the underly-
ing nuclear physics, both in our assumptions about heating
[18,19,53] and in using Ye as a proxy for the detailed isotopic
composition. Finally, our results depend on our present un-
derstanding of pertinent opacities, which, while dramatically
improved over prior work, does not yet include the latest
actinide opacities, let alone non-LTE physics at late times.
For technical convenience, our discussion of the tension
between our direct inferences about ejecta from EM and
secondhand conclusions about ejecta derived from GW infer-
ence of GW170817 adopted a fixed nuclear equation of state
(APR4) to predict ejecta properties from binary properties.
By eliding uncertainty in the nuclear equation of state in our
figure, we somewhat underestimate the systematic uncertainty
in ejecta estimates derived from GW measurements, artifi-
cially strengthening the apparent tension between GW- and
EM-deduced ejecta properties.
ACKNOWLEDGMENTS
The authors thank Erika M. Holmbeck and Matthew R.
Mumpower for stimulating discussions throughout the devel-
opment of this research. A.K. and M.R. acknowledge support
from National Science Foundation (NSF) Grant No. AST-
1909534. R.O.S. acknowledges support from NSF Grant No.
AST-1909534, NSF Grant No. PHY-2012057, and the Simons
Foundation. A.B.Y. acknowledges support from NSF Grant
No. PHY-2012057. R.T.W., O.K., E.A.C., C.L.F., and C.J.F.
were supported by the U.S. Department of Energy through
the Los Alamos National Laboratory (LANL). This research
also used resources provided by LANL through the institu-
tional computing program. Los Alamos National Laboratory
is operated by Triad National Security, LLC, for the Na-
tional Nuclear Security Administration of U.S. Department
013168-11
ATUL KEDIA et al.
PHYSICAL REVIEW RESEARCH 5, 013168 (2023)
of Energy (Contract No. 89233218CNA000001). Research
presented in this paper was supported by the Laboratory Di-
rected Research and Development program of Los Alamos
National Laboratory under Project No. 20190021DR.
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10.1017_jfm.2023.90.pdf
|
Data availability statement. The codes used in this study are openly available in GitHub at https://github.
com/Maplenormandy/qg-edgeofchaos.
|
Data availability statement. The codes used in this study are openly available in GitHub at https://github. com/Maplenormandy/qg-edgeofchaos .
|
J. Fluid Mech. (2023), vol. 958, A28, doi:10.1017/jfm.2023.90
Rossby waves past the breaking point in zonally
dominated turbulence
Norman M. Cao†
Courant Institute of Mathematical Sciences, New York University, New York, NY 10012, USA
(Received 10 August 2022; revised 21 January 2023; accepted 25 January 2023)
The spontaneous emergence of structure is a ubiquitous process observed in fluid and
plasma turbulence. These structures typically manifest as flows which remain coherent
over a range of spatial and temporal scales, resisting statistically homogeneous description.
This work conducts a computational and theoretical study of coherence in turbulent
flows in the stochastically forced barotropic β-plane quasi-geostrophic equations. These
equations serve as a prototypical two-dimensional model for turbulent flows in Jovian
atmospheres, and can also be extended to study flows in magnetically confined fusion
plasmas. First, analysis of direct numerical simulations demonstrates that a significant
fraction of the flow energy is organized into coherent large-scale Rossby wave eigenmodes,
comparable with the total energy in the zonal flows. A characterization is given for
Rossby wave eigenmodes as nearly integrable perturbations to zonal flow Lagrangian
trajectories, linking finite-dimensional deterministic Hamiltonian chaos in the plane to
a laminar-to-turbulent flow transition. Poincaré section analysis reveals that Lagrangian
flows induced by the zonal flows plus large-scale waves exhibit localized chaotic regions
bounded by invariant tori, manifesting as Rossby wave breaking in the absence of critical
layers. It is argued that the surviving invariant tori organize the large-scale flows into a
single temporally and zonally varying laminar flow, suggesting a form of self-organization
and wave stability that can account for the resilience of the observed large-amplitude
Rossby waves.
Key words: geostrophic turbulence, jets, wave–turbulence interactions
1. Introduction
In seeming contradiction to the conception of turbulence as a mixing phenomenon,
turbulence often exhibits the spontaneous emergence of structured flows. A prototypical
† Email address for correspondence: [email protected]
© The Author(s), 2023. Published by Cambridge University Press. This is an Open Access article,
distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/
licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original
article is properly cited.
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N.M. Cao
example is the formation of large-scale coherent vortices from small-scale stirring in
two-dimensional Navier–Stokes turbulence, a process due to the inverse cascade posited
by Kraichnan (1967). This structure can take many forms in other systems, but of
particular interest to this work are the banded, zonally directed shear flows known as
zonal flows, found ubiquitously in planetary atmospheres and magnetically confined fusion
plasmas (Diamond et al. 2005; Galperin & Read 2019). Prominent examples of zonal
flows occur in both natural and engineered systems, such as the majestic alternating
bands of Jupiter (Vasavada & Showman 2005) and the sheared E × B flows that form
in high-confinement-mode (H-mode) fusion plasmas (Wagner 2007).
More than just an aesthetic quirk, zonal flows are known to play a crucial
in fluid and plasma flows which are rendered
role in the regulation of transport
quasi-two-dimensional by strong rotation or magnetization. Zonally directed flows can
accumulate significant amounts of energy from the turbulent flows, acting to regulate
the turbulent mixing by limiting the extent of eddies and other structures transverse
to the sheared zonal flows; see for example the reviews in Galperin & Read (2019)
and Diamond et al. (2005). Despite the importance of these flows in climate and
fusion modelling, many open questions remain about the dynamics of zonally dominated
turbulence.
Characterizing the dynamics of zonally dominated flows requires an understanding of
how the turbulence organizes over long time scales outside of statistical equilibrium. For
example, Jupiter’s bands were observed to be nearly steady for centuries before suddenly
losing one of the jets in the period 1939–1940 (Rogers 2009). Similarly, global gyrokinetic
simulations and experimental evidence suggest that zonal flows in tokamak plasmas
also organize into long-lived discrete bands, which are only occasionally interrupted by
mesoscale ‘avalanches’ (Dif-Pradalier et al. 2015, 2017). Recent work in Bouchet, Rolland
& Simonnet (2019) and Simonnet, Rolland & Bouchet (2021) has suggested that zonal flow
states are in fact metastable, finding predictable noise-induced transition paths between
different numbers of zonal bands in stochastically forced turbulent flows.
This work focuses on the organization of turbulence in the stochastically forced
barotropic β-plane quasi-geostrophic model, referred to here as the QG model. This is
a two-dimensional model for a single-layer rapidly rotating flow in the presence of a
background gradient of potential vorticity (PV) called the β effect (see Salmon 1998).
The restoring force provided by the β effect supports the propagation of Rossby waves,
which will prove to be crucial to the large-scale flow organization. This model has
long been used as a prototype for jet formation in the atmospheres of Jovian planets
(Vasavada & Showman 2005). Furthermore, this model shares essential features with the
Charney–Hasegawa–Mima equations, another prototypical model used to understand the
dynamics of drift-Rossby wave turbulence relevant to various plasma and fluid systems
(Connaughton, Nazarenko & Quinn 2015).
Zonal flows are typically not driven directly by background gradients of density or
pressure, instead requiring a net transfer of energy from non-zonal components of the flow
to sustain themselves against dissipation. This transfer process is frequently identified with
the ‘inverse cascade of energy’ in two-dimensional turbulence introduced by Kraichnan
(1967), and later Rhines (1975) in the context of atmospheric flows. A great deal of
work has gone into extending the ideas of the cascade to QG and related models; see
for example the review in Connaughton et al. (2015) and references therein. However,
two-dimensional cascades relevant to the QG model are generally found to be ‘non-local’,
meaning that large-scale flows can directly interact with small-scale fluctuations without
proceeding through intermediate scales in a self-similar cascade. Thus, this work considers
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Rossby waves past the breaking point in turbulence
the following question: once the large-scale flows have formed, in lieu of a self-similar
cascade picture, how are their dynamics and influence on smaller scales best described?
Describing the dynamics of the large scales from a purely statistical perspective
is challenging, as the coherence and memory of structured flows impart non-trivial
spatiotemporal correlations into the turbulence statistics. Finite-size effects also must
be taken into account, which makes the application of scale separation arguments
difficult. As a concrete illustration of these challenges, consider the principle of spatially
inhomogeneous mixing leading to ‘potential vorticity staircases’, used to understand the
resilience of zonal jets to turbulence (Baldwin et al. 2007; Dritschel & McIntyre 2008).
Spatial inhomogeneity implies that the two-point correlation function of the velocity will
depend not only on the separation of the points, but also on the centre of mass of the points.
Thus, even a complete description of the anisotropic Fourier energy spectrum E(kx, ky)
of the flows cannot describe this effect. This can be viewed as a form of spontaneous
symmetry breaking, where the metastable banded zonal states lack the translational
symmetry of the original system.
The aim of this work is to study such departures from statistical homogeneity in a
finite-size turbulent system primarily exhibiting large-scale wave behaviour atop a zonal
flow background. In the parameter regimes studied, it is shown that the strong zonal
flows act as a ‘waveguide’ supporting discrete Rossby wave eigenmodes, which have
properties that distinguish them from Fourier modes. Surprisingly, even though the waves
can contain energy comparable with the zonal flows and induce perturbations to the flow
velocity comparable with their phase velocities, they retain a coherent linear character. To
investigate this, the statistics of turbulence will be shown to correlate with deterministic
properties of the Lagrangian flow induced by the zonal flows plus coherent waves.
To study these wave-induced Lagrangian flows, the discrete and coherent character of
the waves will allow the usage of Poincaré section techniques. These techniques have been
previously applied in a number of geophysical and plasma contexts (see e.g. Chirikov
1979; Behringer, Meyers & Swinney 1991; Pierrehumbert 1991; Del-Castillo-Negrete
& Morrison 1993; Haynes, Poet & Shuckburgh 2007). Crucially,
these techniques
demonstrate that
the wave-induced flows can be understood as a single zonally
and temporally varying laminar shear flow that is organized by ‘invariant-torus-like
Lagrangian coherent structures’ (LCSs) (Beron-Vera et al. 2010). It is also shown how this
laminar flow does not distort itself due to self-advection under the Poincaré map, which
is interpreted as form of nonlinear wave stability that can account for the resilience of the
observed large-amplitude coherent Rossby waves.
The core arguments are organized in the paper as follows. First in § 2, the model
equations are introduced and studied with direct numerical simulation (DNS). In a
regime of weak forcing and damping relevant to turbulent flows, it is shown that a
significant fraction of flow energy, comparable with the zonal flows, is organized into
coherent large-scale Rossby wave eigenmodes. Next in § 3, a theorem is given for
the Liouville integrability of Lagrangian flows of time-periodic solutions to the QG
equations, and a connection is given to laminar flows. Flow configurations consisting of a
superposition of Rossby wave eigenmodes atop zonal flows are singled out as ‘optimally
near-integrable’ perturbations to the integrable zonal flow Lagrangian dynamics. Finally in
§ 4, the wave-induced Lagrangian flows observed in the DNS are analysed using Poincaré
sections. Lagrangian chaos induced by the wave flows is shown to closely correlate to
inhomogeneous mixing in the DNS, and the survival of invariant tori is linked to a certain
nonlinear wave stability result. This leads to a proposal that the large-scale flow dynamics
in the observed regimes of Rossby wave turbulence self-organizes into ‘nearly-integrable
Rossby waves past the breaking point in zonally dominated turbulence’.
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2. Identifying Rossby waves in simulations
N.M. Cao
2.1. Model equations and simulation set-up
This work focuses on the stochastically forced barotropic β-plane QG model (see Salmon
1998; Connaughton et al. 2015). The model equations describe the two-dimensional
advection of a scalar q = q(x, y, t), the relative vorticity, by a non-divergent flow which
is in approximate geostrophic balance:
∂tq + {ψ, q + βy} = −αq − νh(−∇2)hq +
(2.1)
√
αη,
(2.2)
Here ψ is the streamfunction, β is a constant approximating the gradient of the Coriolis
parameter and the Poisson bracket is defined as follows:
q = ∇2ψ.
{f , g} := ∂xf ∂yg − ∂yf ∂xg.
(2.3)
In this model the PV q + βy, the sum of the relative plus planetary components of the
vorticity, is a scalar material invariant, meaning its value is conserved along fluid parcel
trajectories in the absence of dissipation.
Note that this system can be thought of as the Charney–Hasegawa–Mima equations
in the limit of infinite Rossby deformation radius or gyroradius. However, the infinite
gyroradius limit is not a physically relevant limit for magnetized plasmas, so the QG
system is best considered in the context of atmospheric flows.
The boundary conditions are taken to be doubly-periodic in a square box D of side
lengths L × L. In the absence of forcing and dissipation, these equations will conserve the
quadratic invariants of energy E and enstrophy Q, given by
(cid:2)
E = − 1
2L2
Q = 1
2L2
(cid:4)ψq(cid:5) dx dy,
D
(cid:2)
(cid:4)q2(cid:5) dx dy.
D
(2.4)
(2.5)
(2.6)
The forcing is chosen to be white-in-time with a given correlation function:
(cid:4)η(x, y, t)η(x
(cid:6), y
(cid:6), t
(cid:6))(cid:5) = C(x − x
(cid:6), y − y
(cid:6))δ(t − t
(cid:6)).
Choosing mass units such that the fluid density is 1, the average energy input rate per unit
mass ε is given by
(2.7)
In the absence of (hyper)viscosity, the average kinetic energy of the flow will be (cid:4)E(cid:5) =
ε/α.
ε = 1
2
αL2(∇−2C)(0).
The DNS here focus on weakly damped and forced parameter regimes where inertial and
Coriolis forces are expected to dominate, relevant for a Rossby wave turbulence regime.
Parameters were chosen to be comparable with those used in previous studies of the Jovian
atmosphere by Bouchet et al. (2019).
To non-dimensionalize the equations, length units are chosen such that L = 2π and time
units are chosen to fix β = 8. In this case, the form of the equations as written does not
change. The forcing was chosen to be uniform in an annular ring kf ∈ [14, 15], which is of
small scale compared with the box size.
The equations were solved pseudospectrally using the Dedalus framework (Burns
et al. 2020) using the built-in second-order modified Crank–Nicolson Adams–Bashforth
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Rossby waves past the breaking point in turbulence
Name
Resolution
Box size
Beta
Friction
Hyperviscosity
Normalized forcing rate
Symbol
Nx × Ny
L × L
β
α
ν2
ε/α
Value
2048 × 2048
2π × 2π
8
1.2 × 10−3
1.5 × 10−8
1
2π2 (case 2)
1 (case 1);
Table 1. Parameters used in the DNS.
(a)
Case 1
3
2
1
0y
–1
–2
–3
20
10
0
–10
–20
–30
–2
0
x
2
q + βy
Case 2
3
2
1
0
–1
–2
–3
(b)
3
2
1
0
–1
–2
–3
–2
2
0
U(y)
–2
0
x
3
2
1
0
–1
–2
–3
20
10
0
–10
–20
2
q + βy
0.5
0
U(y)
Figure 1. Representative snapshots from the DNS of the PV q + βy and the zonally averaged zonal flow profile
U( y) for (a) case 1 and (b) case 2. To emphasize the banded structure, the PV is displayed with a cyclic colour
scheme that is shifted separately for each case to align with the observed zonal flows.
√
adaptive time-stepping scheme, which treats the linear terms implicitly and the nonlinear
terms explicitly. The forcing was applied as a time-dependent function normalized by
δt, where δt is the time step. De-aliasing was applied using the 2/3 rule to deal with
1/
the quadratic nonlinearity.
Two cases were studied: case 1 is in a parameter regime studied by Bouchet et al. (2019)
but with higher resolution and lower-order hyperviscosity, while case 2 is a similar case
with greatly reduced forcing. These changes cleanly separate the large-scale discrete waves
from the dissipation scales, ensuring that any observed effects of wave discreteness are not
due to a premature truncation of the dynamic range of the turbulence. The exact values of
parameters used are shown in table 1.
After about three frictional relaxation times t = 2400 ≈ 3/α, the simulations reach a
quasi-stationary state. Some representative snapshots from this state are shown in figure 1.
This work primarily focuses on two sequences of 256 snapshots, one from each case
taken after reaching this quasi-stationary state, spaced evenly apart with (cid:10)t = 0.25. The
number and spacing of snapshots were chosen to resolve the linear oscillation frequency
of the Rossby waves over several cycles. The length of the interval of observation
[2400, 2463.75] is much shorter than a frictional relaxation time, and the zonal flows did
not evolve significantly over this time interval.
One-dimensional energy spectra E(k), energy fluxes ΠE(k) and enstrophy fluxes ΠQ(k)
are shown in figure 2. Following Frisch (1995), these can be defined in terms of
the low-pass filter operator Pk which filters out components with wavenumber greater
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(a)
Case 1
100
E(k)
10–4
10–8
)
3
–
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×
(
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(
E
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N.M. Cao
(b)
E(k)
)
4
–
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1
×
(
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k
(
E
Π
Case 2
k –5/3
k –4
100
10–3
10–6
10–9
1.0
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–0.5
–1.0
k –5/3
k –4
4
2
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–4
)
1
–
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×
(
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(
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Π
)2
2
–
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×
(
)
k
(
Q
Π
1
0
–1
–2
100
101
102
103
100
101
102
103
k
k
Figure 2. Top row: time-averaged one-dimensional energy spectra E(k) from (a) case 1 and (b) case 2. Bottom
row: corresponding nonlinear energy flux ΠE(k) (blue, solid) and enstrophy flux ΠQ(k) (green, dashed). The
forcing scale is marked with a red vertical line.
than k:
(cid:3)
E(k) := d
dk
(cid:4)
(cid:4)qPk[ψ](cid:5) dx dy
,
(cid:2)
D
− 1
2L2
(cid:2)
ΠE(k) := − 1
L2
(cid:2)
ΠQ(k) := 1
L2
(cid:4){ψ, q}Pk[ψ](cid:5) dx dy,
D
(cid:4){ψ, q}Pk[q](cid:5) dx dy.
D
(2.8)
(2.9)
(2.10)
In practice, (cid:4)·(cid:5) is computed by time-averaging over all snapshots.
For scales with k > kf , there is a flux of enstrophy from the forcing scales to higher
wavenumbers with relatively little flux of energy, reminiscent of a direct cascade of
enstrophy. The energy spectra appear to follow an approximately k−4 scaling, consistent
with observations in for example Danilov & Gryanik (2004) and Scott & Dritschel (2012)
of energy spectra in the strong zonal jet regime. Note that this k−4 is not necessarily
indicative of a self-similar cascade, and has been proposed to be a result of spatially
localized ‘sawtooth’ behaviour in the PV profile (Danilov & Gurarie 2004). For scales
with k < kf , there is a flux of energy from the forcing scales to lower wavenumbers with
relatively little transfer of enstrophy, reminiscent of an inverse cascade of energy. However,
due to wavenumber discreteness, it is unclear if there is a single self-similar scaling law
that describes the energy spectrum in this range.
2.2. Data-driven identification of Rossby waves
It has been observed that β-plane QG turbulence with an infinite deformation radius
typically exhibits a strong wave-like character above the Rhines scale k (cid:2) kRh :=
(β/2urms)1/2; see for example the studies and discussion in Rhines (1975), Shepherd
(1987), Sukoriansky, Dikovskaya & Galperin (2008) and Suhas & Sukhatme (2015). The
basic argument is that in the absence of any background flows, the Rossby wave dispersion
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Rossby waves past the breaking point in turbulence
relation for Fourier modes at wavenumber k is given by
ω0,k = −
βkx
k2
.
(2.11)
Meanwhile, the time scale for turbulent motions at a characteristic scale k should scale as
1/τturb,k ∼ kurms. The Rhines scale gives a rough estimate for what scales k linear effects
should start to dominate over nonlinear effects, ω0,kτturb,k ∼ (k/kRh)−2. For the DNS
snapshots, the Rhines scale can be computed directly using the time- and space-averaged
root mean square velocities, resulting in kRh ≈ 1.46 for case 1 and kRh ≈ 6.5 for case 2.
Noting the power-law decay of the energy spectrum, this suggests that a significant fraction
of turbulent flow energy is concentrated into modes where the Rossby wave dispersion
relation can play a significant role.
A natural question that arises is how to quantify how ‘good’ linear Rossby waves
are at describing the observed flows in the DNS. One way to do this in a data-driven
manner is through proper orthogonal decomposition (POD) (Berkooz 1993), also
known as the method of empirical orthogonal functions. Briefly summarizing, given
an observable field w(x, t), POD finds a ranked set of r orthonormal spatial basis
functions {w1(x), . . . wr(x)} and corresponding orthonormal temporal basis functions
{a1(t), . . . , ar(t)}. The approximation ˆwn of w by the first n ≤ r basis functions,
ˆwn(x, t) :=
n(cid:5)
k=1
σkak(t)wk(x),
(2.12)
will be ‘optimal’ in the sense that it minimizes the squared residual integrated over the
spatial domain D and some fixed time interval T:
(cid:2)
(cid:2)
(cid:11)w − ˆwn(cid:11)2 :=
|w − ˆwn|2 d2x dt.
(2.13)
T
D
This minimization is taken over all possible sets of r orthonormal spatial and temporal
basis functions. In practice, the observable is sampled over a regular spatial and temporal
grid so the integrals are replaced by sums, and r is finite so the basis functions span only
a subspace of the set of all possible functions.
To apply POD to the DNS snapshots, the observable w = (−∇−2)1/2q is used so the
(cid:6)
standard inner product gives the energy norm for each snapshot E ∝
D w2 d2x. The
resultant POD modes will be ranked in terms of their contribution to the time-integrated
energy of the snapshots. These modes are ‘optimal’ in the sense that the projection of
the snapshot data to the first n modes will minimize the energy in the residual. The
streamfunctions ψ = (−∇−2)−1/2w for a few selected POD modes are shown in figure 3,
and the total energy captured by the first n POD modes is shown in figure 4.
Analysing the POD modes in case 1 first, the zonal flows are primarily captured by POD
mode 0 and account for about 72 % of the total time-averaged energy. The next few POD
modes form sine/cosine pairs in their temporal evolution and x (zonal) variation, showing
a high degree of spatial and temporal coherence. The POD modes 1–4 form two pairs
which account for about 24 % of the time-averaged energy, or about 86 % of the non-zonal
energy. Higher POD modes are increasingly incoherent in both space and time, but make
up only around 4 % of the time-averaged energy. Case 2 has a similar breakdown of energy,
where zonal flows account for 56 % of the time-averaged energy, and the next three pairs of
POD modes account for 74 % of the non-zonal energy. Thus, despite the turbulent nature
of the flow, the vast majority of energy in both cases is organized into POD modes which
exhibit regular structure in both space and time.
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x
0
Mode 0
2
Case 1
Mode 1
Mode 37
(a)
–2
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2
0
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N.M. Cao
(b)
2
0
–2
Case 2
ψ(x, y)
Mode 0
Mode 1
Mode 37
a(t)
0
20 40
t
60 0
20 40 60 0
20 40 60
0
20 40 60 0
20 40 60 0
20 40 60
Figure 3. A selection of POD modes from (a) case 1 and (b) case 2 displaying the streamfunction ψ(x, y) and
time traces a(t) associated with each mode. Note that the POD modes and time traces are normalized, so the
units are arbitrary.
t
o
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E
n
E
/
1.0
0.8
0.6
Case 1
Case 2
100
101
ntrunc
Figure 4. Cumulative energy fraction En/Etot captured by the first n POD modes for case 1 (blue, solid) and
case 2 (orange, dashed).
102
2.3. Eigenmode character of Rossby waves
The strong wave-like character of the spatiotemporal structures identified by POD suggests
comparison with the Rossby wave dispersion relation frequencies ω0,k. However, the
presence of nearly steady large-amplitude zonal flows also suggests comparison of the
POD modes with the eigenfrequencies and eigenmodes of the QG equations linearized
around a zonal flow background.
For a reference zonal flow state U( y), the equations of motion (2.1) and (2.2) in
the absence of forcing and dissipation can be linearized and Fourier transformed in the
symmetry direction x to derive an eigenvalue equation:
(cid:6)(cid:6)( y))∇−2]˜q = iωeig ˜q.
ikx[U( y) + (β − U
(2.14)
In the absence of background flows U( y) = 0, the eigenfrequencies reduce to the
dispersion relation frequencies ω0,k and the eigenmodes reduce to Fourier modes in both y
and x. For the following analysis, the zonally averaged zonal flow profile time-averaged
over the snapshots with no additional smoothing is used as a reference flow profile.
The reference profile satisfies the Rayleigh–Kuo criterion β − U(cid:6)(cid:6)( y) > 0 everywhere,
ensuring that all eigenmodes will be neutrally stable (Kuo 1949).
Figure 5 shows a comparison between selected pairs of POD modes with
their corresponding dispersion relation frequencies, and corresponding Rossby wave
eigenmodes and eigenfrequencies. The eigenmodes well capture the temporal frequency
and spatial structure of the POD modes, which deviate from the dispersion relation. In
particular, these eigenmodes have a strong spatial localization of ˜q( y) to regions of large
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Rossby waves past the breaking point in turbulence
(a)
Eigenmode
POD modes
ψ(x, y)
Case 1, modes 1 + 2
kx = 1, ky = 1
ω
eig ª –4.33
POD ª –4.32
ω
ω
0, k = –4.0
(b)
Case 2, modes 1 + 2
kx = 1, ky = 3
ω
eig ª –0.87
POD ª –0.86
ω
0, k = –0.8
ω
(c)
Case 2, modes 5 + 6
kx = 3, ky = 1
eig ª –2.53
ω
POD ª –2.51
ω
0, k = –2.4
ω
2
0 y
–2
2
0 y
–2
2
0 y
–2
0
5
0
2
0
–0.25
q˜
Figure 5. Streamfunction ψ(x, y) for eigenmodes and corresponding pairs of POD modes. The text on the
left-hand side gives a comparison of the POD frequency with the eigenfrequency and dispersion relation
frequency. The rightmost plots show a comparison of the eigenfunction envelope ˜q( y) for the eigenmode
(orange, dashed) and the POD modes (blue, solid) at the average amplitudes observed in the DNS.
PV gradient associated with the reference flow ¯q(cid:6)( y) + β := −U(cid:6)(cid:6)( y) + β, giving them
a somewhat ‘interfacial’ rather than ‘bulk’ character. This localization corresponds to a
strong broadening in ky at fixed kx, characteristic of ‘zonons’ identified in simulations of
QG turbulence by Sukoriansky et al. (2008).
The observation that the first few POD modes correspond very closely to Rossby wave
eigenmodes suggests that the QG dynamics linearized around the reference zonal flow
state plays a significant role in organizing the large-scale coherent flows. However, it is
not immediately obvious from non-dimensional measures of wave amplitude why the
linear character of the Rossby wave dynamics should persist in the DNS. For example,
one estimate of the ratio of nonlinear to linear time scales for the waves is given by
τnl/τlin ∼ uwave/uph. Here, uwave is the maximum zonally directed velocity induced by
the wave and uph is the zonal component of the wave phase velocity. For the eigenmode
with the largest amplitude, uwave/uph ≈ 0.24 in case 1 and uwave/uph ≈ 0.36 in case
2. The phase and amplitude of these modes remain coherent for much longer times
than this simple estimate would suggest. This raises a key question of how ‘large
amplitude’ can be reconciled with ‘linear coherence’ for the observed Rossby wave
eigenmodes.
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2.4. Isolating linearly coherent Rossby waves
While POD modes are orthogonal under the energy inner product, the Rossby wave
eigenmodes are not. Thus, isolating the coherent Rossby wave flow component requires
expanding the snapshot data in the numerically computed eigenmode basis,
then
determining which of the eigenmodes has a strong linear character. Fourier transforming
of the snapshot data in x and expanding each kx component in the eigenmode basis results
in a complex eigenmode amplitude aj(tk) for each eigenmode j and snapshot time tk. To
provide a quantitative cutoff between ‘linearly coherent’ and ‘not linearly coherent’ Rossby
waves, the following coherence statistic is used:
r2
min
( j) := min
s∈S
max
β∈C
⎢
⎢
⎢
⎢
⎢
⎣
⎡
⎤
N−s(cid:5)
(cid:10)
(cid:10)
(cid:10)2
(cid:10)aj(tk+s) − βaj(tk)
k=1
1 −
(cid:10)
(cid:10)
(cid:10)2
(cid:10)aj(tk+s)
N−s(cid:5)
k=1
⎥
⎥
⎥
⎥
⎥
⎦
.
(2.15)
Here N is the number of snapshots and S = {1, 2, . . . , smax} is a set of time delays.
The inner max of (2.15) is the r2 statistic of a least-squares fit of the linear model
ˆaj(tk+s) = βaj(tk), and can also be interpreted as an estimator for the squared lag-s
autocorrelation coefficient of a time-stationary signal. A signal with purely linear
oscillatory dynamics described by aj(tk+s) = exp(−iωeig,js(cid:10)t)aj(tk) would have r2 = 1.
The outer min of (2.15) selects the minimum r2 over the set of time delays. Choosing
smax = 64, r2
min measures whether or not the signal remains linearly coherent over time
windows of up to smax(cid:10)t = 16. Signals with r2
min close to 1 will only experience small
fluctuations in their amplitude and phase relative to a purely linear oscillatory signal, while
signals with r2
min close to 0 experience relatively large fluctuations.
A plot of the r2
min statistic for all numerically computed eigenmodes with 1 ≤ kx ≤ 8 is
> 0.4 is used to identify the coherent modes. These
shown in figure 6. A cutoff of r2
coherent eigenmodes have zonally directed phase velocities which satisfy uph < U( y)
everywhere, and hence correspond to non-singular eigenfunctions. Observing that uph ≈
−β/k2, modes with large negative phase velocities are seen to correspond to large-scale
Rossby waves. These are referred to as ‘large-scale coherent modes’ in the following.
min
3. Near-integrability of wave-induced Lagrangian flows
3.1. Integrability and laminar flow
Following the text of Arnold (1989) on classical mechanics, a 2n-dimensional smooth
continuous-time Hamiltonian system is said to be Liouville integrable if it has n
independent, Poisson commuting first integrals of motion, and furthermore the level sets
of the integrals of motion are compact. The Liouville–Arnold theorem states that if a
Hamiltonian system is Liouville integrable, then there exists a canonical transformation
to action-angle coordinates in which the integrals of motion, including the Hamiltonian,
depend only on the action coordinates. The action-angle coordinates are not necessarily
global, and different regions of phase space may have different action-angle coordinates.
One corollary of the existence of action-angle coordinates is that the level sets of the
action variables (locally) foliate the phase space into tori which are invariant under the
Hamiltonian flow. In physical terms, a Hamiltonian system that is Liouville integrable has
a phase space flow which is ‘laminar’, with the ‘laminae’ consisting of the invariant tori.
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Rossby waves past the breaking point in turbulence
Case 1
Case 2
–8
–6
–4
–2
0
2
1.00
0.75
0.50
0.25
0
1.00
0.75
0.50
0.25
0
1.00
0.75
0.50
0.25
0
0.3
0.2
0.1
0
–8
–6
–4
–2
0
2
–8
–6
–4
–2
0
2
–8
–6
–4
–2
0
2
uph
Figure 6. (a) Eigenmode coherence r2
min versus zonally directed phase velocity uph for all eigenmodes with
1 ≤ kx ≤ 8. Green triangles denote the large-scale coherent modes used in the study. The red shaded region
shows the range of the zonal flows U( y). (b) Time-averaged eigenmode amplitude, measured by the maximum
of the zonally directed velocity induced by the mode uwave, versus uph. Labelling is the same as in (a).
uph
In the absence of forcing and dissipation and with a constant Galilean shift c, the ideal
QG PV advection equation can be written as
∂tq + {ψ + cy, q + βy} = 0.
This can be thought of as a Hamiltonian evolution equation for q + βy, with
time-dependent Hamiltonian ψ(x, y, t) + cy. Given a streamfunction ψ(x, y, t), (3.1) can
be transformed into an autonomous Hamiltonian system by introducing a new momentum
coordinate ξ conjugate to t and redefining the Poisson bracket:
(3.1)
{f , g} := ∂xf ∂yg − ∂yf ∂xg + ∂tf ∂ξ g − ∂ξ f ∂tg.
(3.2)
With this new Poisson bracket, the advection equation then becomes a single Poisson
commutation condition:
{ψ(x, y, t) + cy − ξ, q(x, y, t) + βy} = { ˆψ(x, y, t, ξ ), ˆq(x, y, t)} = 0.
(3.3)
From (3.3), ˆψ and ˆq are seen to be independent integrals of motion for the dynamics
generated by the Hamiltonian − ˆψ, which corresponds to flow along Lagrangian flow
trajectories
dx
ds
= {x, − ˆψ} = vx,
dy
ds
= {t, − ˆψ} = 1.
⎫
⎪⎪⎬
= {y, − ˆψ} = vy,
⎪⎪⎭
dt
ds
(3.4)
In physical terms, the PV is a materially conserved scalar invariant, so the flow will
be confined to contours of constant PV. This leads to the following theorem, originally
reported in Brown & Samelson (1994), restated and proved here for clarity:
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THEOREM 3.1 (Liouville integrability of time-periodic solutions). Given a smooth
time-periodic solution q(x, y, t) = q(x, y, t + T) to the ideal QG equations (3.1) and (2.2),
the Lagrangian flow specified by (3.4) for z = (x, y, t, ξ ) ∈ T4 is integrable in the Liouville
sense.
Proof . We can identify ξ with ξ + Lξ such that the level sets of cy − ξ are compact. Then,
since ψ and q are time-periodic, we can identify t with t + T so the 4-dimensional phase
space (x, y, t, ξ ) can be identified with the 4-torus T4. Then, since ˆψ and ˆq are smooth,
their level sets are compact, hence satisfying the requirements of the Liouville–Arnold
(cid:3)
theorem.
In physical terms, the theorem implies that the Lagrangian flow of smooth time-periodic
solutions to the ideal QG equations is necessarily laminar due to the existence of a
conserved scalar material invariant. This property follows from the principle of PV
conservation, which can be seen as a general consequence of the particle relabelling
symmetry of the Lagrangian formulation of the QG equations (Salmon 1988; Müller
1995). Such symmetries are also linked to Casimirs of functional Poisson brackets relevant
to a variety of fluid and plasma systems (Holm et al. 1985; Morrison 1998; Webb & Anco
2019).
3.2. Eigenmodes and near-integrability
To establish the link between Rossby wave eigenmodes and near-integrability, note that
time-independent zonal flow states q = q0( y) satisfy the requirements of Theorem 3.1.
The integrals of motion are ˆψ0 := ψ0 − ξ and ˆq0 := q0 + βy, which satisfy
{ψ0( y) − ξ, q0( y) + βy} = 0.
(3.5)
Furthermore, if the Rayleigh–Kuo condition is satisfied everywhere, then the integrals of
motion are independent over the entire domain, and hence the flow is laminar globally.
Now, consider periodic approximate solutions of the QG equations of the form Q =
ˆq0( y) + (cid:16)q1(x, y, t), where (cid:16) is a formal perturbation parameter. These approximate
solutions induce a Lagrangian flow with Hamiltonian given by
Ψ := ˆψ0( y, ξ ) + (cid:16)∇−2q1(x, y, t).
(3.6)
Since Q is no longer an exact solution to the equations of motion, the exact commutation
condition (3.3) will no longer hold in general. Using the bilinearity of the Poisson bracket,
Q can be shown to instead satisfy an approximate commutation condition:
{Ψ, Q} = (cid:16)[{ψ0 − ξ, q1} + {∇−2q1, q0 + βy}] + (cid:16)2{∇−2q1, q1} =: (cid:16)R1 + (cid:16)2R2.
To identify flows Ψ which have the perturbed PV Q as an approximate integral of
motion, the leading-order remainder term R1 is set to zero, which results in an equation
that determines q1:
(3.7)
{ψ0 − ξ, q1} + {∇−2q1, q0 + βy} = [∂t + U∂x + (β − U
(cid:6)(cid:6))∂x∇−2]q1 = 0.
(3.8)
Comparing (3.8) with (2.14) shows that
the approximate integrability condition
coincides with the linearized evolution equation describing Rossby wave eigenmodes.
Thus, regular eigenfunctions are singled out as the perturbations to the zonal flow
dynamics which give both (i) approximate solutions to the equations of motion and
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Rossby waves past the breaking point in turbulence
(ii) nearly integrable perturbations to the zonal flow Lagrangian dynamics. They are
‘optimal’ perturbations with respect to this formal perturbation expansion, since no O((cid:16))
terms remain in the approximate commutation condition (3.7). Note that the condition
R1 = 0 can also be relaxed into a condition that R1 is small, corresponding to q1 which
approximately satisfy the linear evolution equation.
By appealing to Kolmogorov–Arnold–Moser (KAM) theory extended to non-twist
systems (Delshams & Llave 2000), the near-integrability of eigenmodes suggests that the
majority of invariant tori will survive finite-amplitude perturbation by the eigenmodes. In
physical terms, the invariant tori in the unperturbed system correspond to contours of the
PV ˆq0. These tori are material curves in the fluid, meaning that fluid parcels do not pass
through them transversally. The KAM theory implies that under suitably small amplitude
of perturbation, ‘many’ of these tori will experience only reversible deformations under
the perturbed flow. Tori with zonal velocities that are incommensurate with the wave phase
velocities are the most robust, and can survive as transport barriers in the perturbed flow.
In many cases the surviving tori, known as ‘KAM tori’, are known to form sets of positive
measure (finite area/volume). See Arnold (1989) for an introduction or de la Llave (2001)
for a review of KAM theory.
These transport barriers fall under the umbrella of LCSs, with most of the invariant
tori corresponding to elliptic LCSs defined in Haller (2015). The non-twist tori from the
minima and maxima of the zonal flow correspond to parabolic LCSs. These barriers are
also called ‘invariant-torus-like Lagrangian coherent structures’, described in Beron-Vera
et al. (2010). A key property of the elliptic LCSs is that rather than being isolated
curves which separate regions of different flow character, they instead form families that
fill space in regions of the same flow topology, i.e. regions where a single continuous
set of action-angle coordinates can be given. Note that the survival of separatrices to
perturbation, typically corresponding to hyperbolic LCSs, can be studied through the lens
of Melnikov theory (see e.g. Balasuriya, Jones & Sandstede 1998; Malhotra & Wiggins
1998).
4. Wave-induced Lagrangian flows in turbulence
4.1. Construction of the Poincaré map
Given a set of eigenmode amplitudes and relative phases (in the symmetry direction x), a
wave-induced flow field can be constructed with streamfunction Ψ = ˆψ0 + ∇−2q1. Here
ˆψ0( y, ξ ) = ψ0( y) − ξ is the reference zonal flow streamfunction and q1(x, y, t) is the
superposition of the Rossby wave eigenmodes.
By taking the condition that R1 is small instead of zero, the quasi-periodic time
variation of q1 can be approximated by a periodic one by replacing the eigenfrequencies
with a rational frequency approximation Ω0ni + ckx,i ≈ ωeig,i. Here kx,i and ωeig,i are
fixed for each eigenmode i, while the other parameters Ω0 (the basic frequency), ni (an
integer multiplier) and c (a Doppler shift) are fitted to minimize an amplitude-weighted
approximation error of the eigenfrequencies.
Note that the earlier condition smax(cid:10)t ≈ 2π/Ω0 is a self-consistency requirement to
ensure the eigenmodes remain linearly coherent over one basic period. In particular,
eigenmodes with r2
min close to 1 will have amplitudes and relative phases which evolve very
slowly compared to the the linear time scale 1/Ω0. For both cases 1 and 2, Ω0 ≈ 0.41, with
the eigenfunctions typically completing between 1 and 10 oscillations within this period.
Since this wave-induced flow field is time-periodic, Poincaré sections can be used
to visualize and analyse the fluid parcel trajectories. These sections are constructed by
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initializing tracers at different spatial positions, evolving their positions under the flow
field and then marking their position after each period T = 2π/Ω0 of the flow field.
The map taking each tracer from its initial position to its position after one period is
known as the Poincaré map. Poincaré section techniques have particular application to
near-integrable Hamiltonian systems where they can indicate regions of phase space where
invariant tori have survived perturbation.
In the following, superpositions of the ‘large-scale coherent modes’ marked in figure 6
are used to construct periodic wave-induced flow fields. For each individual DNS snapshot,
eigenmode amplitudes and phases were extracted and used to construct a series of
corresponding Poincaré sections. To identify the presence of chaotic orbits, an iterative
Grassberger–Procaccia method is used to estimate the correlation dimension dC of the
orbit of each tracer under the Poincaré map (see Rosenberg 2020). Orbits which trace out
invariant tori and islands will have dC ≈ 1, while orbits which chaotically fill space will
have dC ≈ 2.
4.2. Localized PV mixing from wave-induced chaos
Focusing first on case 1, a representative Poincaré section is shown in figure 7(a). Visual
inspection suggests that a large majority of invariant tori survive the perturbation by the
waves, and that the chaotic orbits are mostly confined to a particular region of space. To
link the localization of chaos in the wave-induced passive tracer advection to spatially
inhomogeneous mixing in the fully developed turbulence in the DNS, two different
measures of mixing are considered here.
The first measure of mixing considered is the temporally and zonally averaged PV
gradient ¯q(cid:6)( y) + β. Friction and viscosity tend to push ¯q(cid:6)( y) towards zero, pushing the
the PV gradient towards the background value of β. Meanwhile, turbulent mixing tends to
push the PV gradient towards zero. Figure 7(c) shows the PV gradient compared against
the fraction of orbits which are chaotic at some y for cases 1 and 2. This fraction is
computed by computing the average y of the particles, binning them into equally sized
bins based on this average y, then computing the fraction of particles whose orbits have
dC ≥ 1.5.
In every region where there is a significant fraction of chaotic orbits, the PV gradient
is pushed below the background β, indicating a region of sustained turbulent mixing.
Furthermore, in case 2 these chaotic regions and corresponding mixing regions are not in
the centre of their respective broad westward flow regions. The particular combination of
Rossby waves produces an asymmetry in the chaotic regions that matches the asymmetry
in the observed turbulent mixing regions.
A second measure of mixing comes from the consideration that in two dimensions,
enstrophy is typically understood to be anomalously dissipated by viscosity via the
formation of small-scale structure (Boffetta & Ecke 2012). In real space, this small-scale
structure can be formed by the chaotic advection of level set contours of the PV q + βy.
The contours are stretched in directions with non-zero Lyapunov exponent, creating
small-scale meanders and increasing the overall length of the contour. Eventually, the
meanders reach a small enough scale that viscosity acts to reconnect and smooth the
contours, limiting the growth of their length. To quantify this process in the DNS, the
contours of q + βy which encircle the domain are identified, then their length is computed
and time-averaged over all DNS snapshots (cid:19)q. For a pure zonal flow ¯q( y) + βy, the
undisturbed PV contours would be lines of constant y with the minimum possible length
of (cid:19)q = L = 2π.
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Rossby waves past the breaking point in turbulence
(a)
Case 1
dC
3
2
1
0y
–1
–2
–3
3
2
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0
–1
–2
–3
y
–2
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2
Case 2
–2
2
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x
(b)
3
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–1
–2
–3
3
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–1
–2
–3
2.0
1.8
1.6
1.4
1.2
1.0
2.0
1.8
1.6
1.4
1.2
1.0
–2
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2
–2
2
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x
(cid:6)
q
35
30
25
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10
18
16
14
12
10
8
q¯(cid:2)(y) + β
20
40
(c)
3
0
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0
–1
–2
–3
0
0
3
2
1
0
–1
–2
–3
0
0.5
1.0
10
20
30
1.0
0.5
fchaotic
Figure 7. (a) Poincaré sections for the two cases, with tracers coloured by the computed correlation dimension
dC of their orbit. Invariant tori bounding the major chaotic regions are highlighted with an orange dashed line.
(b) Direct numerical simulation snapshots of the PV q + βy. The colour (cid:19)q is the time-averaged length of the
level set contour of q + βy which encircles the domain. The invariant tori are again shown with an orange
dashed line. (c) Comparison of the time- and zonally averaged PV gradient ¯q(cid:6)( y) + β (blue) with the fraction
of orbits which are chaotic fchaotic (orange, filled). The dashed black line shows the background PV gradient β.
Shown in figure 7(b) is the PV q + βy, coloured by (cid:19)q, for the DNS snapshot
whose eigenmode amplitudes and phases were used to construct the Poincaré sections
in figure 7(a). In both cases, all of the chaotic regions identified in the Poincaré sections
correspond to a region of mixing identified in the DNS. These mixing regions only exist
in the broad westward flow regions, and are bounded on either side by regions consisting
of shorter, less disturbed PV contours. The bulged shapes of the mixing regions also line
up well with the invariant tori bounding the corresponding chaotic regions.
Physically, this mixing process corresponds to the formation of elongated filaments of
PV in chaotic ‘surf zones’. These chaotic regions occur in the absence of critical layers
where uph = U( y), and are a result of Rossby waves which are standing in y. Observing
the fate of these filaments in figure 1, some of these filamentary structures undergo
reconnection to form isolated vortex patches. Cusps form in the PV contour at the point of
reconnection. This is reminiscent of the vortex filamentation and ‘microbreaking’ process
observed in Dritschel (1988) and Polvani & Plumb (1992), although here the breaking
occurs in the ‘bulk’ rather than at sharp PV interfaces. Drawing a loose analogy with the
overturning of stably stratified density layers by breaking gravity waves, this Rossby wave
breaking process ultimately leads to an irreversible ‘overturning’ of a stably stratified PV
gradient. Note that there also appears to be a breaking process occurring at the sharp PV
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N.M. Cao
interfaces corresponding to the eastward jets as well, although this is not captured by the
Poincaré section analysis.
Together, these two measures of mixing provide strong evidence that localization of
wave-induced chaos leads to a form of inhomogeneous PV mixing. This is broadly
consistent with the results in for example Del-Castillo-Negrete & Morrison (1993) and
Haynes et al. (2007), which show that the Lagrangian flow induced by zonal flows plus
a few waves will generally create regions of mixing separated by invariant-torus-like
transport barriers. Note from figure 7(c) that the PV gradient is actually close to or above
the background value of β in many of the regions where the invariant tori survive, not just
in the immediate vicinity of the transport barriers at the centre of the eastward jets. Thus,
these tori can act as semi-permeable transport barriers over regions of finite area in the
fully developed turbulence.
4.3. Self-organization into coherent Rossby waves
The paradigm of inhomogeneous PV mixing leading to ‘potential vorticity staircases’ has
been established as a way to understand how turbulence reinforces, rather than destroys,
large-scale zonal structure (Baldwin et al. 2007; Dritschel & McIntyre 2008). Here, the
parameter LRh/Lε = (U/β)1/2/(ε/β)1/5 identified in Scott & Dritschel (2012) is ≈ 6.5
for case 1 and ≈ 2.6 for case 2, suggesting the staircase regime is relevant. Chaos in the
Poincaré sections was found to be localized near zonal flow minima of broad jets with the
strongest westward flow, i.e. in the direction of propagation for the Rossby waves. Since the
net y (meridional) PV flux leads to a net zonal acceleration in the ideal QG model by the
Taylor identity, this mixing would then reinforce the amplitude of the strongest westward
jets. Note that this method of transfer of energy to the zonal flows does not resemble either
a local or a self-similar cascade. The PV perturbations at all scales, including the forcing
scales, are exponentially stretched by the chaotic flows induced by the box-scale waves.
Again, this is broadly consistent with the picture in for example Haynes et al. (2007)
linking the survival of invariant tori to jet formation in QG.
Now moving beyond a zonally averaged sense, one key consequence of the survival
of most invariant tori is that the majority of flow energy can be understood as being
organized into a temporally and zonally varying laminar flow. Here, the remnants of the
invariant-torus-like LCSs which fill space in the DNS are the ‘laminae’ which organize
the flow. Appealing to the near-integrability established earlier, an argument can be
constructed for why these laminar flows predominantly organize into long-lived Rossby
waves. This will show how the paradigm of inhomogeneous mixing can be extended to
describe coherent flow formation in non-zonal and temporally non-stationary components
of the flow.
Since the perturbed PV ˆq0 + q1 for regular Rossby wave eigenmodes is an approximate
integral of motion, the perturbed PV contours will nearly align with the surviving invariant
tori. While these contours will not be mapped exactly back onto themselves by the
Poincaré map, they will still be confined by neighbouring invariant tori. This suggests that
superpositions of Rossby waves with PV perturbations primarily localized to non-chaotic
regions will enjoy a form of long-time nonlinear stability under the Poincaré map, as their
PV perturbations are approximately mapped back onto themselves after any number of
iterations of the map.
This spatially localized stability is demonstrated in figure 8 for cases 1 and 2. In
quiescent regions, contours initially aligned with the perturbed PV contours remain nearly
unchanged after many iterations of the Poincaré map. The example contours shown
in the figure for cases 1 and 2 have undergone 16 iterations of the Poincaré map.
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Rossby waves past the breaking point in turbulence
(a)
Case 1
(cid:6)
q
(b)
Case 2
(cid:6)
q
y
3
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coherent
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(cid:3)q˜ 2
coherent
Figure 8. For (a) case 1 and (b) case 2, the left-hand part of each panel shows the image of a contour of the
perturbed PV ˆq0 + q1 under several iterations of the Poincaré map. Light orange shows the initial contour and
dark orange shows the final contour. A different number of iterations are applied on each contour, as described
(cid:5) carried by the coherent waves
in the text. The right-hand part of each panel shows the ‘enstrophy’ (cid:4)˜q2
at each y. The area enclosed by the curve is coloured by the contour length (cid:19)q corresponding to the amount of
mixing at each corresponding y.
coherent
Meanwhile in the chaotic regions, perturbed PV contours are rapidly distorted. Two
iterations of the Poincaré map in case 1 and four iterations in case 2 are sufficient to
stretch the contours shown in the figure to approximately (cid:19)q. Lyapunov exponents in the
chaotic regions can be estimated from the contour stretching, with λ ≈ 0.048 in case 1
and λ ≈ 0.018 in case 2, which are both a little slower than the Poincaré map frequency
Ω0/(2π) ≈ 0.065.
These nearly-integrable superpositions of Rossby waves can be thought of as
generalizations of exact solutions to the QG equations consisting of pure plane waves in
the absence of a background flow. In the latter, contours of PV align exactly with invariant
tori. Physically, fluid parcels supporting the waves on invariant tori experience completely
reversible perturbations from the large-scale waves. After one period of the Poincaré map,
the material curves corresponding to invariant tori return to their original shapes. This
allows the waves to survive for much longer times than suggested by the simple estimate
τnl/τlin ∼ uwave/uph.
In contrast, large-scale PV perturbations which induce non-wave-like flows would
produce significant misalignment between the perturbed PV contours and the surviving
tori. Examples are non-resonant beat modes between Rossby waves, or
invariant
hydrodynamic vortices. Under the action of the Poincaré map, either chaos from
destroyed tori or frequency shear between neighbouring invariant tori would shear
these perturbations to smaller scales. Since ψ ∼ k−2q, this damps the induced flow
perturbations, with laminar shear due to invariant tori resembling the Orr mechanism (Orr
1907). Thus, non-wave-like flows are prevented from accumulating significant amounts of
energy, leaving only the coherent wave component of the flow.
Combining the factors of (i) inhomogeneous mixing leading to PV staircases, (ii)
near-integrability of the Rossby waves and (iii) damping of non-wave-like perturbations
together suggest that large-scale flows will invariably organize into coherent Rossby
waves on top of zonal flows. Note that although the mechanism for transferring energy
to the waves is not specified here, work in Bakas & Ioannou (2014) and Constantinou,
Farrell & Ioannou (2016) has established that, using the turbulence closure provided by
stochastic structural stability theory, non-zonal perturbations can extract energy from
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small-scale fluctuations. This can be viewed as the small-scale stirring self-organizing
into macroscopically coherent waves.
N.M. Cao
One piece of evidence supporting this picture of wave self-organization in the DNS is
the observation that the most coherent waves tend to have PV perturbations localized to the
regions of weakest turbulent mixing. As shown in figure 8, the zonally averaged squared
magnitude of the PV perturbation (cid:4)˜q2
(cid:5) :=
1 dx, where q1 is the superposition
of the coherent Rossby wave eigenmodes, is localized to regions where the q contours are
stretched the least. This mostly corresponds to the sharp eastward jets, although there also
tend to be larger PV perturbations outside of the large-scale Rossby wave ‘surf zones’ than
inside.
Lx
0 q2
coherent
(cid:6)
Referring back to figure 5, this PV localization of coherent waves is also consistent
with the observed ‘interfacial’ character of the most energetic eigenmodes. This suggests
a possible ‘selection rule’ for determining which of the eigenmodes will maintain large
amplitude and coherence in the fully developed turbulence. For case 1, the wavenumber
(kx, ky) = (1, 1) of the most energetic eigenmode is the largest scale wave which can
approximately align its maximum and minimum with the two sharp eastward jets.
Similarly for case 2, the wavenumber (kx, ky) = (1, 3) of the most energetic eigenmode is
the largest scale wave which can align its three maxima with the three sharp eastward jets.
Meanwhile, waves with more of a ‘bulk’ character are unable to align their minima and
maxima with the surviving invariant tori. Thus ‘bulk’ waves would experience stronger
mixing, presumably reducing their amplitude and coherence.
5. Discussion and outlook
5.1. Open issues in the QG system
Several questions remain regarding the turbulent mixing observed in the DNS. Referring
back to figure 6, although a majority of the non-zonal flow energy is captured in the
large-scale Rossby waves, there are still a number of modes with significant amplitude
which were not included in the Poincaré map. These modes typically did not show a strong
enough coherent character over several cycles to justify approximation by purely periodic
flows. While LCSs can be defined for finite-time and aperiodic flows (see e.g. Haller 2015),
it is not clear if there is a generalization of the KAM theorem to such a situation.
This issue also arises when attempting to generalize the arguments in § 4 to the finite
deformation radius kD > 0 case, where the PV becomes ˆq = ∇2ψ − k2
ψ + βy. While the
D
manipulations in § 3 are also formally valid for the kD > 0 case, it is generally observed
that as kD is increased, the flows tend not to organize into large-scale coherent waves
(Suhas & Sukhatme 2015). One possible avenue for future work is to better characterize the
perturbative behaviour of elliptic LCSs in finite-time and aperiodic settings. This would
clarify if the concept of near-integrability can be applied to identify ‘laminar’ character in
flows which are locally rather than globally organized.
Additionally, the kinematics of transport driven by the wave-induced Lagrangian flows
are not well understood analytically. The zonal flow is non-monotonic, so the Poincaré map
does not satisfy the usual twist criterion (Meiss 1992). The chaos observed in the Poincaré
sections also occurs in the complete absence of first-order resonances, since uph < U( y)
everywhere for the coherent waves. This distinguishes the picture of wave-driven transport
in the QG system from the typical picture of wave-driven transport via overlapping
wave–particle resonances in Vlasov turbulence (Chirikov 1979). It would be interesting
to study how much of the observed route to chaos phenomenology in systems such as the
Chirikov standard map or standard non-twist map (Del-Castillo-Negrete & Morrison 1993)
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Rossby waves past the breaking point in turbulence
carry over to this system. This would provide insight into how the chaotic regions form and
change in response to changes in the wave amplitudes and phases.
While this work does not develop a quantitative model for the long-time large-scale
flow evolution in the QG system, the relevance of coherent Rossby wave eigenmodes
suggests some promising areas for development. The majority of the flow energy can be
described by ‘zonal flows plus a few waves’, i.e. a mean zonal flow profile U( y), and a set
of eigenmode amplitudes and reference phases {Ai, Θi}. Compared with the approach of
discrete wave turbulence using Fourier modes (see e.g. L’vov & Nazarenko 2010), the role
of low-order wave–wave resonances is de-emphasized. Wave–mean flow interactions have
an unmistakable influence on both the Rossby wave eigenfunctions and the small-scale
turbulence statistics. The latter is best understood in a real-space Lagrangian picture.
The clear impact of the wave-induced flows on the turbulence statistics also suggests
that purely ‘quasi-linear’ approaches, which discard all nonlinear interactions between
non-zonal modes, do not account for all of the inhomogeneous mixing in the QG system.
This effect has already been recognized in the development of more general filtered
quasi-linear approaches, such as in Constantinou et al. (2016) and Marston, Chini &
Tobias (2016). However, the influence of small-scale fluctuations on the zonal flows and
coherent waves appears to be small, changing U( y) and {Ai, Θi} slowly compared with
the linear Rossby wave time scales. An intriguing possibility is if the time-scale separation
arguments in Bouchet, Nardini & Tangarife (2013) and Woillez & Bouchet (2019) can
be extended to allow the zonal flows and coherent waves to play the role of ‘slow’
variables. This would represent a significant simplification compared to the general filtered
quasi-linear approach, as the dominant effect of the interaction between zonal modes and
near-zonal modes is to organize the near-zonal modes into eigenmodes.
5.2. Integrability beyond QG
Looking beyond the simple prototypical equations used in this work, waves with a strong
linear character have been observed in turbulent settings in more complex and realistic
flows. One example is shallow water turbulence in the equatorial region, where the
signature of linear waves has been seen both in simulations (Garfinkel et al. 2021; Schröttle
et al. 2022) and in observational data (Wheeler & Kiladis 1999). Another example is the
coexistence of internal gravity waves with turbulent balanced motions in the ocean, which
has also been seen in idealized numerical simulations (Thomas & Yamada 2019; Thomas
& Daniel 2020), global-scale ocean models (Richman et al. 2012; Torres et al. 2018) and
in observational data (Rocha et al. 2016; Lien & Sanford 2019). Thus, it is interesting to
ask if analogues of the results in §§ 3 and 4 hold in more complex, realistic flows.
The Rossby wave self-organization principle proposed in this work relied on three
key ingredients: (i) the existence of enough materially conserved scalar invariants to
guarantee Liouville integrability, i.e. a ‘laminar’ phase-space flow; (ii) KAM theory, which
characterized the persistence of the invariant tori ‘laminae’ under perturbations; and (iii)
the PV inversion equation (2.2), which allowed the near-integrability conditions to be
written into a form coinciding with the linearized evolution equations. Note that points
(i) and (ii) are more ‘kinematic’, in the sense that they would describe the motion of any
passive scalar advected by the flow. Meanwhile, point (iii) is more ‘dynamical’, in the
sense that it links the passive scalar advection back to the fully self-consistent flow.
First considering point (i), the concept of PV conservation persists in a broad range
of fluid and plasma systems (see e.g. Müller 1995; Gurcan & Diamond 2015). Many
fluid and plasma models of interest also conserve other scalar material invariants,
temperature and density.
such as specific entropy or related notions of potential
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Furthermore, recent work has extended notions of Liouville integrability to generic
dynamical systems (Bogoyavlenskij 1998; Zung 2016). This suggests the possibility of
extending the Lagrangian integrability results in § 3 to more complex and realistic flow
models, such as the shallow water or Boussinesq equations. In the absence of forcing
and dissipation, these systems typically conserve some form of PV, with the latter also
typically conserving some form of buoyancy or potential density.
Now considering point (ii), intuitively when a fluid or plasma flow conserves a scalar
material invariant f , the level sets of f will generally form co-dimension one material
surfaces (i.e. curves in two dimensions, surfaces in three dimensions) through which
fluid parcels do not pass transversally. If the dominant motions of these material surfaces
are ‘reversible’, then the surfaces could correspond to invariant-torus-like LCSs. Recent
extensions of KAM theory to measure-preserving dynamical systems (Xia 1992) may shed
light on the conditions necessary for these transport barriers to survive in fully developed
turbulent flows. However for point (iii), in most fluid and plasma systems the velocity field
is typically not determined by scalar material invariants like the PV or specific entropy
alone.
Together, these points suggest the ‘kinematic’ arguments of §§ 3 and 4 regarding the
presence of invariant-torus-like LCSs in fully developed turbulent flows may directly
generalize to more complex flow systems. However, the ‘dynamical’ arguments regarding
the self-organization of flows into waves do not appear to have a direct route for
generalization. The development of these arguments in detail is left for future work.
Finally, one other key aspect which is missing from this work is the presence of linear
instabilities driven by gradients of quantities such as temperature or density, such as
baroclinic instabilities or drift wave instabilities. In systems with marginally unstable
gradients, found for example in fusion plasmas (Diamond & Hahm 1995), the interaction
between zonal flows and turbulent mixing of driving gradients can lead to non-trivial
mesoscale behaviour such as avalanching (Dif-Pradalier et al. 2017). Future work can
also explore how transitions to chaos in Lagrangian flows interplay with linear instability
dynamics.
6. Summary
In summary, this work proposes that the dynamics of large-scale coherent flows in QG
turbulence can be understood as ‘nearly-integrable Rossby waves past the breaking point
in zonally dominated turbulence’. The nearly steady zonal flow background acts as a
waveguide supporting Rossby wave eigenmodes which are standing in y and propagating
in x. The largest-scale modes accumulate a significant fraction of the flow energy yet retain
a strong linear coherent character.
An integrability result on Lagrangian flow in QG was given, and regular Rossby wave
eigenmodes were characterized as minimally perturbing to this integrability. Chaos in
the wave-induced Lagrangian flow was identified using a Poincaré map, demonstrating
that localization of chaos and subsequent ‘wave breaking’ was linked to the observed
inhomogeneous PV mixing in the DNS. This inhomogeneous mixing was linked to a
self-organization principle for the large-scale flows, suggesting that surviving invariant tori
organize the observed zonal jets plus Rossby waves into a single zonally and temporally
varying laminar flow.
More broadly, this Lagrangian picture of turbulent flow organization emphasizes the
importance of considering the combined nonlinear effect of both zonal and non-zonal
modes in the QG system. In the staircase regime when both zonal flows and Rossby waves
are strong, the effects of wave–mean flow interactions were emphasized, whereas the roles
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Rossby waves past the breaking point in turbulence
of low-order wave–wave resonances were de-emphasized. Finally, it was discussed how
there may be opportunities to extend the arguments in this work to more complex and
realistic flow systems.
Acknowledgements. T. Grafke, J. Shatah and E. Vanden-Eijnden are thanked for fruitful discussions with
the author, and several anonymous reviewers are thanked for their constructive commentary and insight.
Funding. This research was supported by the Simons Collaboration Grant on Wave Turbulence, grant no.
617006.
Declaration of interests. The author reports no conflict of interest.
Data availability statement. The codes used in this study are openly available in GitHub at https://github.
com/Maplenormandy/qg-edgeofchaos.
Author ORCIDs.
Norman M. Cao https://orcid.org/0000-0001-9745-0275.
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| null |
10.1371_journal.ppat.1011346.pdf
|
Data Availability Statement: All relevant data are
within the manuscript and its Supporting
Information files.
|
All relevant data are within the manuscript and its Supporting Information files.
|
RESEARCH ARTICLE
A modified Agrobacterium-mediated
transformation for two oomycete pathogens
Luyao Wang1,2, Fei Zhao2, Haohao Liu2, Han Chen2, Fan Zhang2, Suhua Li1, Tongjun Sun1,
Vladimir NekrasovID
3, Sanwen Huang1*, Suomeng DongID
2*
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
OPEN ACCESS
Citation: Wang L, Zhao F, Liu H, Chen H, Zhang F,
Li S, et al. (2023) A modified Agrobacterium-
mediated transformation for two oomycete
pathogens. PLoS Pathog 19(4): e1011346. https://
doi.org/10.1371/journal.ppat.1011346
Editor: Paul Birch, University of Dundee, UNITED
KINGDOM
Received: June 23, 2022
Accepted: April 6, 2023
Published: April 21, 2023
Peer Review History: PLOS recognizes the
benefits of transparency in the peer review
process; therefore, we enable the publication of
all of the content of peer review and author
responses alongside final, published articles. The
editorial history of this article is available here:
https://doi.org/10.1371/journal.ppat.1011346
Copyright: © 2023 Wang et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: All relevant data are
within the manuscript and its Supporting
Information files.
Funding: In this research, S.W. and S.D. received
funding support from Guangdong Major Project of
1 Shenzhen Branch, Guangdong Laboratory of Lingnan Modern Agriculture, Genome Analysis Laboratory of
the Ministry of Agriculture and Rural Affairs, Agricultural Genomics Institute at Shenzhen, Chinese Academy
of Agricultural Sciences, Shenzhen, China, 2 Department of Plant Pathology and Key Laboratory of
Integrated Management of Crop Disease and Pests (Ministry of Education), Nanjing Agricultural University,
Nanjing, China, 3 Plant Sciences and the Bioeconomy, Rothamsted Research, Harpenden, United Kingdom
* [email protected] (SH); [email protected] (SD)
Abstract
Oomycetes are a group of filamentous microorganisms that include some of the biggest
threats to food security and natural ecosystems. However, much of the molecular basis of
the pathogenesis and the development in these organisms remains to be learned, largely
due to shortage of efficient genetic manipulation methods. In this study, we developed modi-
fied transformation methods for two important oomycete species, Phytophthora infestans
and Plasmopara viticola, that bring destructive damage in agricultural production. As part of
the study, we established an improved Agrobacterium-mediated transformation (AMT)
method by prokaryotic expression in Agrobacterium tumefaciens of AtVIP1 (VirE2-interact-
ing protein 1), an Arabidopsis bZIP gene required for AMT but absent in oomycetes
genomes. Using the new method, we achieved an increment in transformation efficiency in
two P. infestans strains. We further obtained a positive GFP transformant of P. viticola using
the modified AMT method. By combining this method with the CRISPR/Cas12a genome
editing system, we successfully performed targeted mutagenesis and generated loss-of-
function mutations in two P. infestans genes. We edited a MADS-box transcription factor-
encoding gene and found that a homozygous mutation in MADS-box results in poor sporula-
tion and significantly reduced virulence. Meanwhile, a single-copy avirulence effector-
encoding gene Avr8 in P. infestans was targeted and the edited transformants were virulent
on potato carrying the cognate resistance gene R8, suggesting that loss of Avr8 led to suc-
cessful evasion of the host immune response by the pathogen. In summary, this study
reports on a modified genetic transformation and genome editing system, providing a poten-
tial tool for accelerating molecular genetic studies not only in oomycetes, but also other
microorganisms.
Author summary
Oomycetes are a unique group of animal and plant pathogens that include some of the
biggest threats to food security and natural ecosystems. However, much of the
PLOS Pathogens | https://doi.org/10.1371/journal.ppat.1011346 April 21, 2023
1 / 27
PLOS PATHOGENSModification of AMT for two oomycete species
Basic and Applied Basic Research
(2021B0301030004); S.D. received funding
support from National Natural Science Foundation
of China (NSFC, 31721004) and China Agriculture
Research System (CARS-09-P20); L.W was
supported by NSFC (31900303) and the
Agricultural Science and Technology Innovation
Program (CAASZDRW202101); V.N. was
supported by the Biotechnology and Biological
Sciences Research Council (BBSRC) through the
Designing Future Wheat (DFW) Institute Strategic
Programme (grant number BB/P016855/1). The
funders had no role in study design, data collection
and analysis, decision to publish, or preparation of
the manuscript.
Competing interests: The authors have declared
that no competing interests exist.
pathogenesis and development in these organisms remains to be learned, largely due to
shortage of efficient genetic manipulation methods for a long time. In this manuscript, we
developed modified Agrobacterium-mediated genetic transformation strategies for Phy-
tophthora infestans, a notorious oomycete species that caused Irish Famine in the 19th cen-
tury, and Plasmopara viticola, the causal agent of grapevine downy mildew that is known
as a highly destructive disease of grapevines in all grape-growing areas of the world. Using
prokaryotic expression of a plant protein in A. tumefaciens, we achieved considerable
increase in transformation rate in different P. infestans strains, and also acquired one posi-
tive transformant of P. viticola, a oomycete species that is extremely hard-to-transform
and cannot be grown as an axenic culture. Using our improved transformation protocol,
combined with the CRISPR/Cas12a system, we performed genome editing and created
loss-of-function alleles in P. infestans. In summary, our study reports on modified genetic
transformation methods, for two important oomycete species, that have the potential to
accelerate the molecular genetic study of many other microorganisms.
Introduction
Oomycetes are regarded as an important lineage of eukaryotic organisms that includes a con-
siderable number of plant pathogens, which pose a threat to natural and arable ecosystems.
Grapevine downy mildew, caused by Plasmopara viticola, is considered to be the most devas-
tating disease of grapevines in climates with relatively warm and humid summers. P. viticola is
an obligate biotrophic oomycete species that cannot be grown as an axenic culture and is very
recalcitrant to genetic transformation as demonstrated in previous studies [1]. The genetic
transformation obstacle in the case of P. viticola has severely hampered functional genomics
research and studies on screening molecular drug targets. Thus, it is important to set up a
workable transformation method for P. viticola and other hard-to-transform biotrophic
microorganisms.
Potato late blight is another one of the most well-known but not well-understood plant dis-
eases in terms of molecular genetics of Phytophthora infestans, its causal pathogenic microor-
ganism. P. infestans, the oomycete pathogen responsible for the devastating potato late blight,
poses a worldwide threat [2], and plays an essential role in studying plant–microbe interac-
tions, epidemiology, and field disease control [3]. Currently, reverse genetics studies in P. infes-
tans are also hampered by inefficient genetic transformation methods. Up until now,
functional genomic research in P. infestans has relied mostly on transient/stable gene overex-
pression or target-gene silencing by RNAi [4, 5]. Although polyethylene glycol (PEG)-medi-
ated transformation, Agrobacterium-mediated transformation (AMT), microprojectile
bombardment and zoospore electroporation have been already set up in P. infestans for years,
we need to be open to new methods as other transformation options are always encouraged
[6–9]. Moreover, phenotypes of Phytophthora transformants often vary significantly between
different pathogen lines, experiment operators, and individual experiments, possibly because
of random gene integration sites and different silencing or overexpression qualities [10].
Despite of multiple attempts to apply CRISPR/Cas9 for the purpose of targeted mutagenesis in
P. infestans, no genome editing events, generated using this system, have been reported so far
[11]. In a recent study, the CRISPR/Cas12a (Cpf1) system was utilized to produce genome
editing events in a P. infestans strain using the PEG-mediated protoplast transformation
method [12]. To propel future research, it is of great interest to expand the range of available
genetic transformation methods for genome editing in P. infestans.
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PLOS PATHOGENSModification of AMT for two oomycete species
Agrobacterium tumefaciens, as a typical plant pathogenic bacterium, causes crown gall dis-
ease in a wide range of plants [13], and was developed into an efficient genetic transformation
tool since Binns and Thomashaw first demonstrated that A. tumefaciens can integrate exoge-
nous gene segments into the plant nucleus [14]. Known as the first example of prokaryote to
eukaryote horizontal gene transfer, the capacity of A. tumefaciens to transfer alien genes to
host cells has become the basis of one of the most essential technologies in manifold research
fields, and plant science in particular [15]. By now, transgenesis, achieved through A. tumefa-
ciens-mediated transformation (AMT), has been established in many model plant species,
including Arabidopsis, tobacco and rice [16–18]. In addition to plants, Agrobacterium is also
able to infect a broad range of other non-plant hosts during the co-cultivation process, includ-
ing microorganisms identified as plant pathogens, and AMT protocols have been developed as
a transformation system for many fungi, including Aspergilus species, Beauveria species, Botry-
tis cinerea, Candida species, Coccidiodes species, Colletotrichum species, Fusarium species, Tri-
choderma species and Verticillium species [19–30]. Attempts to improve the efficiency of AMT
have been undertaken since the method was first reported. However, in most cases, the efforts
were focused on optimization of conditions, such as explant treatment, tissue culture medium
composition, temperature or selectable marker, but not the core tool—A. tumefaciens [31].
One successful attempt to improve the plant transformation ability of A. tumefaciens involved
introducing a compatible plasmid carrying a virG mutant (virGn45D), which constitutively
induced vir gene expression during AMT [32].
The first AMT protocol for P. infestans was established in 2003 by Vijin and Govers; in this
study, the A. tumefaciens LBA1100 strain was selected, and as many as 30 transformants per
107 zoospores could be obtained [7]. A recent study has also described an efficient AMT proto-
col for another oomycete species, Phytophthora palmivora, which produces large amount of
zoospores (2–5 × 106/mL) during in vitro preparation [33]. However, the amount of zoospores
produced may vary dramatically in different Phytophthora strains, and some oomycete species
produce hardly any zoospores under artificial conditions. Thus, the ability to produce suffi-
cient amounts of zoospores under in vitro conditions is likely a serious limiting factor for
applying zoospore-dependent transformation methods in oomycetes [34–36].
Previous studies illustrated that ectopic expression of several plant proteins significantly
improved AMT rate in a range of plant species [37]. A set of proteins from the host are
involved with Agrobacterium-mediated transformation of plant [37]. Overexpressing several
of these host proteins, mostly from Arabidopsis, such as AtVIP1, AtRTNLB1, Ku80, histone
H2A and SGA1, significantly increases AMT efficiency [37–42]. Arabidopsis VirE2-interact-
ing-protein1 (AtVIP1) is known as an important plant protein that contributes to the AMT
process [38, 43]. AtVIP1 has been proven to interact with Agrobacterium effector VirE2, and
its ability to form homomultimeric protein complexes and interact with histone H2A in host
cells is required for Agrobacterium-mediated pathogenicity or stable genetic transformation
[44]. AtVIP1-overexpressing plant lines have shown significantly increased susceptibility to A.
tumefaciens infection, and AtVIP1 seems to facilitate nuclear transport of VirE2 and the
T-DNA complex [42]. It would be more practical if we could directly utilize AtVIP1 protein
during the AMT process instead of constructing AtVIP1 transgenic material prior to transfor-
mation of a gene of interest.
Here we report on a modified AMT method utilizing AtVIP1 as an enhancer in the trans-
formation of two important oomycete pathogens. In this study, an increment in the transfor-
mation efficiency of Phytophthora infestans was achieved by prokaryotic expression of AtVIP1
in the A. tumefaciens EHA105 strain as compared to AMT without AtVIP1. We then extended
application of this modified AMT procedure to Plasmopara viticola. By combining our modi-
fied AMT method and the recently established Cas12a-based genome editing system, we
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PLOS PATHOGENSModification of AMT for two oomycete species
successfully generated genome-edited P. infestans transformants and observed the expected
virulence phenotypes after inoculating potato leaves with these mutants. Our work is provid-
ing a new direction for AMT improvement and a way to potentially accelerate molecular
genetic studies of the two devastating plant pathogens and other microorganisms.
Results
Oomycetes lack homologues of specific plant proteins important for
Agrobacterium-mediated transformation
To better understand the low AMT efficiency in P. infestans and test whether introducing
plant proteins into transformation system would significantly improve Phytophthora transfor-
mation efficiency, we first performed a bioinformatic study of proteins with similarities to pre-
viously identified plant proteins, required for AMT, in different oomycete species. We used
target protein sequences from Arabidopsis to perform local BLAST using publicly available
genomic data from each selected plant or oomycete species. Sequence similarity shown in
Fig 1A is based on the ratio between the highest alignment score (bit-score) of local BLAST
results from a target species and the one from Arabidopsis. In the selected monocotyledonous
and dicotyledonous plants, the sequence similarities of the obtained proteins were all above
0.25, except that the sequence similarity of Rad50 in Solanum tuberosum and Vitis vinifera
were merely 0.04 and 0.17, respectively (Fig 1A and S3 Table). In oomycete species, similar
proteins with sequence similarity greater than 0.45 were detected for IMPA-4, Rab8, SGA1
and histone H2A. For AGP17, PP2C, Ku70, Rad50 and Ku80, sequence similarities of similar
proteins were mostly above 0.15 (average values were 0.19, 0.19, 0.20, 0.18 and 0.15, respec-
tively) in selected oomycete species. Interestingly, sequence similarity of AtVIP1 or its related
Arabidopsis paralogues, including bZIP29, bZIP30, bZIP69, posF21, bZIP18 and bZIP52, were
less than 0.08 in all selected oomycete species, indicating that absence of an AtVIP1 homo-
logue might have a negative impact on the AMT rate in oomycetes.
AtVIP1 enhances Agrobacterium-mediated genetic transformation
To further test our hypothesis that introduction of plant proteins, required for AMT, into a
transformation system increases AMT efficiency in oomycetes, we constructed a vector to
deliver AtVIP1 from Agrobacterium to host cells to potentiate the transformation process. To
make AtVIP1 translocatable by Agrobacterium T4SS, we fused the coding sequence of AtVIP1
to virFΔ42N (truncated virF, lacking the sequence encoding the 42 N-terminal amino acids,
that functions as a C-terminal transport signal for VirB/D4-translocated proteins in Agrobac-
terium [45]), and added green fluorescent protein-encoding sequence (GFP) to the N-terminus
(S1A Fig). As shown in S1B Fig, GFP signal was observed in both cytoplasm and nucleus of
infected Nicotiana benthaminana cells 3 days post leaf infiltration with A. tumefaciens
EHA105 strain carrying p302b-gfp-AtVIP1-virFΔN42. These data suggested that the GFP-At-
VIP1-virFΔ42N fusion protein was translocated into infected cells through T4SS during Agro-
bacterium infection.
To test whether our modified protocol enhances AMT efficiency, we first tested it in wheat,
a cereal crop with low AMT efficiency [46]. We introduced the prokaryotic expression plasmid
p302b-AtVIP1-virFΔN42 (pV1F) and the binary plasmid pWMB110-GUS carrying the β-glu-
curonidase coding gene gus (contains maize adh1 intron) into Agrobacterium strain EHA105
(S2A Fig). By inoculating leaf segments of wheat cv. ‘Fielder’ with A. tumefaciens EHA105
strain containing pV1F and pWMB110-GUS, a significantly higher transient transformation
efficiency in leaf tissue was observed as compared to the control treatment inoculated with
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PLOS PATHOGENSModification of AMT for two oomycete species
Fig 1. (a) The protein similarity analysis of plant proteins, important for AMT of Arabidopsis, and their homologues in other plant and
oomycete species. Representative plants with an established Agrobacterium-mediated transformation protocol and eight oomycete species were
selected for phylogenetic analysis. The left phylogenetic tree was generated by the OrthoFinder software based on variations of single-copy
orthologous genes in released genomic data of different species using IQ-tree with JTT + G4 model of evolution. The left bar indicates amino acid
substitutions per site. The right heatmap indicates sequence similarity of known plant proteins envolved in Arabidopsis AMT process and their
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PLOS PATHOGENSModification of AMT for two oomycete species
homologues in selected plants and oomycete species. The right bar indicates sequence similarity. (b) Schematic representation of the main idea of
our improved transformation strategy. The use of the helper plasmid pV1F results in expression of virFΔN42 tagged AtVIP1. The recombinant
AtVIP1 is delivered into oomycete zoospores via VirB/VirD4 T4SS, and thereby facilitates the process of T-DNA complex (T-complex) targeting
the nucleus of an infected zoospore or an encysted zoospore with a germ tube.
https://doi.org/10.1371/journal.ppat.1011346.g001
EHA105 strain containing the vector lacking the AtVIP1 gene (pEV) (S2B Fig). In addition,
gus expression in root segments increased from 1.8% to 11.6% when transformed with the vec-
tor containing the AtVIP1 gene (S2C and S2D Fig). These results indicate that AtVIP1 is an
effective enhancer of Agrobacterium-mediated genetic transformation in plant tissues.
Expressing AtVIP1 in A. tumefaciens induces T-DNA integration in P.
infestans
To extend our AMT system to a wider range of eukaryotic species, characterized by low trans-
formation efficiency, we tested it in one of the most important phytopathogenic oomycetes, P.
infestans, in which AMT protocols have already been set up since years ago [7, 47]. A sche-
matic illustration of our modified AMT method for P. infestans is presented in Fig 1B. To test
if AtVIP1 also facilitates AMT in P. infestans, we first constructed the binary vector pLY40-gfp
(Fig 2A), which carries a T-DNA region containing the gfp gene driven by Bremia lactucae
Ham34 promoter, and the geneticin (G418) resistance gene nptII driven by Phytophthora sojae
Rpl41 promoter. The pLY40-gfp was introduced into A. tumefaciens strain EHA105 together
with either pV1F or pEV.
A. tumefaciens strains carrying above-mentioned DNA construct combinations (Fig 2A)
were co-cultivated with zoospores of P. infestans strains JH19 and HB1501, and subsequently
geneticin-resistant transformants were obtained according to the methods presented in the
flow diagram in S3 Fig. While G418 resistant colonies were obtained with both tested construct
combinations, co-cultivation with A. tumefaciens containing the pV1F plasmid resulted in sig-
nificantly more G418 resistant colonies (or colonies with observed GFP-signal) in both
HB1501 and JH19 (Fig 2B–2C and Table 1). One of the representative transformants (JH19
background), named as T1, which was obtained with this modified AMT method, expressed a
GFP-size protein and showed a strong GFP signal compared to the transformant T3 (JH19
background) that was obtained using the empty pLY40 as negative control (Fig 2D and 2E).
The Southern blot analysis of representative transformants of the HB1501 strain background
suggested that T-DNA fragments with the nptII gene were integrated into the genomic DNA
of all seven of them (Fig 2F). These results indicate that prokaryotic-expressed AtVIP1 in A.
tumefaciens considerably promotes T-DNA integration during AMT in P. infestans.
Transformation of Plasmopara viticola using the modified AMT procedure
In this study, we also extended application of our modified AMT protocol to P. viticola, a diffi-
cult-to-transform oomycete that causes grapevine downy mildew. Based on the previously
established AMT protocol for the biotrophic fungus Podosphaera xanthii [48], A. tumefaciens
EHA105, carrying LY40-gfp and pV1F, was used for co-cultivation with released zoospores of
P. viticola isolate BS5. After resistance selection, applied by rinsing P. viticola inoculated grape
leaves with G418, we isolated one transformant called T1 (Figs 3 and S5B). We observed a
strong GFP signal in both sporangia and mycelia of T1 during infection using confocal micros-
copy, and the GFP signal was stable on grape leaves in three sub-inoculation generations (Fig
3A and 3C). Western blot analysis indicated that a GFP-size band could also be detected in
protein extracts from the transformant T1 (Fig 3B), and Southern blot analysis, carried out
using PCR-amplified nptII gene as a probe, showed that one T-DNA segment was successfully
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PLOS PATHOGENSModification of AMT for two oomycete species
Fig 2. Generating P. infestans transformants expressing gfp using the modified AMT method. (a) Schematic representation of the constructs used in this
experiment. A. tumefaciens strain EHA105 with pV1F and pLY40-gfp was used for P. infestans transformation. (b) Quantification of colonies that acquired
G418 resistance as a result of transforming gfp into P. infestans strains JH19 and HB1501 using our modified AMT procedure. EHA105 with the helper plasmid
pEV was used as control in this experiment. All data represent average values from three independent experiments with the indicated standard deviations.
Statistical differences among the samples were analyzed with Sˇı´da´k’s multiple comparisons test (P< 0.0021: **, P< 0.0001: ****). (c) Two representative plates
from the transformation experiment shown in (b). (d) Immunoblot of P. infestans JH19 transformant T1, expressing free gfp, probed with an anti-GFP
antibody. Protein extracted from N. benthamiana leaves transiently expressing gfp driven by the CaMV35s promoter was used as positive control in lane 1. (e)
The P. infestans JH19 transformant T1 expressing a detectable GFP signal was obtained by AMT using A. tumefaciens carrying constructs described in (a).
Scale bars = 40 μm. T3, a randomly selected empty vector transformant was used as negative control. GFP expression in the transformant was analysed by
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PLOS PATHOGENSconfocal microscopy. The protein blot was stained with Coomassie Blue to confirm equal loading. (f) Southern blot analysis of representative gfp transformants
of P. infestans strain HB1501. Genomic DNA (4 μg) was digested with HindIII and all blots were probed with a fragment containing the nptII gene to detect the
presence of T-DNA. Numbers on the left indicate the positions of molecular weight markers (kb).
https://doi.org/10.1371/journal.ppat.1011346.g002
Modification of AMT for two oomycete species
integrated into the genome of T1 (Fig 3D). Consequently, the extensibility of our strategy to P.
viticola suggests that AtVIP1 could also be considered for optimizing AMT methods in the
case of other oomycete species with poor efficiency of transformation.
AtVIP1 facilitates Agrobacterium-mediated delivery of LbCas12a into P.
infestans
To test if our modified AMT method could also facilitate genome editing in oomycetes, we
selected P. infestans for the first attempt as the Cas12a-based method had recently been set up
in this species [12]. We first fused the coding sequences of the Phytophthora sojae NLS, human
codon-optimized Lachnospiraceae bacterium Cas12a (LbCas12a) and GFP, and inserted the
recombinant sequence into the T-DNA region of pLY40 to obtain pLY40-Cas12a-gfp (Fig 4A).
A. tumefaciens strain EHA105 carrying pV1F and pLY40-Cas12a-gfp was used to transform
zoospores of P. infestans strains JH19 and HB1501. As a result, up to 61 and 22 G418 resistant
transformants were obtained for JH19 and HB1501, respectively, in three independent trans-
formation experiments (Table 1). The localization of the GFP signal in the transformants T5
(JH19) and T6 (HB1501) was distinctly nuclear as visualized by confocal microscopy (Fig 4B).
Table 1. Genetic transformations of P. infestans strains JH19 and HB1501 by A. tumefaciens EHA105 with or without the helper plasmid pV1F.
Binary plasmid
pLY40-gfp
pLY40-gfp
pLY40-gfp
pLY40-gfp
pLY40-Cas12a-
gfp
pLY40-Cas12a-
gfp
pLY40-Cas12a-
gfp
pLY40-Cas12a-
gfp
Binary plasmid
pLY40-PiMADS-
KO
pLY40-PiMADS
-KO
pLY40-Avr8-KO
pLY40-Avr8-KO
Helper
plasmida
pEV
pV1F
pEV
pV1F
pEV
pV1F
pEV
P. infestans
strain
JH19
JH19
HB1501
HB1501
JH19
JH19
HB1501
pV1F
HB1501
Helper
plasmid
pEV
pV1F
pEV
pV1F
P. infestans
strain
JH19
JH19
HB1501
HB1501
GFP+/G418R colonies in
attempt 1b
0/3
11/21
0/0
2/8
1/1
13/22
0/0
3/6
GFP+/G418R colonies in
attempt 2
GFP+/G418R colonies in
attempt 3
Average GFP/G418R
colonies
1/2
10/29
0/1
7/12
0/7
3/19
0/0
3/7
1/3
13/24
0/0
5/12
0/2
6/20
0/0
7/9
0.67/2.67
11.33*/24.67*
0/0.33
4.67*/10.67*
0.33/3.33
7.33*/20.33*
0/0
4.33*/7.33*
G418R colonies in attempt 1 G418R colonies in attempt
0
7
2
11
2
0
4
2
9
G418R colonies in attempt
3
Average G418R
colonies
1
5
1
8
0.33
5.33*
1.67
9.33*
a Helper plasmids used in this experiment are described in detail in S2 Table.
b As determined with GFP-observation by confocal microscopy (GFP).
As determined 14 days after acquired transformants transferred to another rye-sucrose medium with 5 or 10 μg/L geneticin (G418).
*The marked values indicate significantly different with the AMT process used same binary plasmid but pEV as the helper plasmid. Student’s t-test was used to
determine the differences.
https://doi.org/10.1371/journal.ppat.1011346.t001
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PLOS PATHOGENSModification of AMT for two oomycete species
Fig 3. Obtaining Plasmopara viticola BS5 stable transformant T1 using the modified AMT protocol. (a) P. viticola BS5 strain
was used for transformation assay and was obtained by AMT using A. tumefaciens carrying constructs pLY40-gfp and pV1F. Scale
bars = 40 μm. The confocal microscopy images were taken 7 days post inoculation with the zoospores from the third sub-generation
of T1; wild type BS5 was used as negative control. (b) Immunoblot of P. viticola BS5 transformant T1 expressing free GFP, probed
with an anti-GFP antibody. Protein extracted from N. benthamiana leaves transiently expressing gfp driven by the CaMV35s
promoter was used as positive control in lane 2. (c) Transformant T1 of P. viticola BS5 expresses detectable GFP signal when
infecting grapevine leaves (Zitian seedless, A17). Scale bars = 100 μm. Images were taken 7 days post inoculation and wild type BS5
was used as negative control. (d) Southern blot analysis of transformant T1 of P. viticola BS5. Genomic DNA (4 μg) was digested
with HindIII and all blots were probed with a fragment containing the nptII gene to detect the presence of T-DNA. Numbers on the
left indicate the positions of molecular weight markers (kb).
https://doi.org/10.1371/journal.ppat.1011346.g003
As shown in Fig 4C, the hlbCas12a-GFP fusion protein was successfully detected by western
blotting in both transformants T5 and T6 with hlbCas12a-gfp expressed in N. benthamiana
used as a positive control. These data suggest successful delivery of the Cas12a gene into P.
infestans using our modified AMT method, paving a way for an efficient genome editing
method for this species.
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PLOS PATHOGENSModification of AMT for two oomycete species
Fig 4. Integration of LbCas12a in P. infestans. (a) Schematic representation of the constructs used in the experiment. A. tumefaciens
EHA105 carrying pLY40-Cas12a-gfp and either pV1F or pEV was used for P. infestans transformation. (b) Confocal micrograph of T5 and
T6 transformants expressing PsNLS-lbCas12-GFP. The nuclear localization pattern of the fusion protein, indicated by white arrows,
revealed mycelia and sporangia. T3, an empty vector pLY40 transformed line, is used as negative control. Bright field and GFP channels are
presented. Scale bars = 40 μm. (c) Immunoblot of two representative P. infestans transformants expressing PsNLS-lbCas12-GFP. The gfp
tagged hlbCas12a driven by CaMV35S promoter was expressed in N. benthamiana as positive control. The expected size of the protein is
176.6 kDa. The protein blot was stained with Coomassie Blue to confirm equal loading. (d) Quantification of positive P. infestans
transformants expressing GFP tagged Cas12a (JH19 and HB1501 backgrounds) generated using the modified AMT procedure. A.
tumefaciens EHA105 carrying the helper plasmid pEV was used as control in this experiment. Statistical differences among the samples
were analyzed with Sˇı´da´k’s multiple comparisons test (P< 0.0021: **, P< 0.0001: ****).
https://doi.org/10.1371/journal.ppat.1011346.g004
Editing a MADS-box-encoding gene in P. infestans
To investigate the prospect of using the modified AMT method for CRISPR/Cas12a-mediated
P. infestans genome editing, a single-copy gene encoding a MADS-box transcription factor
(PITG_07059) was chosen as the first editing target in this study. The homologous MADS-box
genes play an essential role in asexual reproduction and zoosporogenesis in both P. infestans
and P. sojae [49, 50]. Two gRNAs, MADS-g1 and MADS-g2, targeting the 1332 nt MADS-box-
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PLOS PATHOGENSModification of AMT for two oomycete species
encoding sequence were designed using the procedure described by Ah-Fong et al. (Figs 5A
and S6) [12]. In the binary construct pLY40-MADS-box-KO, MADS-g1 and MADS-g2 were
flanked by 21-bp short direct repeats (DRs) and inserted in a tandem downstream of LbCas12a
and the 73-nt poly-adenine sequence (pA), which was added to promote translation of Cas12a
mRNA (S6C Fig). As a 3’ uridine-rich tail positively regulates CRISPR/Cas12a crRNA forma-
tion, four thymines were added at the 3’ends of sequences encoding the gRNAs (S6C Fig) [12,
51]. The editing events within the MADS-box gene in the transformants were detected by per-
forming PCR, with primers amplifying the full length of the gene, and sequencing the PCR
amplicons. In 2 out of 16 G418 resistant transformants (T8 and T16), shorter PCR amplicons
were observed suggesting presence of CRISPR/Cas12a-induced deletions (Fig 5B). Sequencing
analysis confirmed that T8 and T16 carried identical 993 bp deletions, between MADS-g1 and
MADS-g2 loci, resulting in a truncated MADS-box gene coding sequence (Figs 5C and S6E).
The MEF2-like domain of the MADS-box protein contributes to the DNA binding activity,
which is essential for a transcription factor. The MEF2-like domain was predicted to be located
at the 2–72 aa sites by InterproScan (version 5.52–86.0) (Fig 5A). The sequencing data pre-
sented in Figs 5C and S6E showed that both mutant MADS-box alleles, present in T8 and T16,
lack the majority of the sequence encoding the MEF2-like domain, suggesting loss of function
of the MADS-box proteins in these transformants.
As shown in Fig 5D and 5F, MADS-box-edited JH19 strains T8 and T16 showed merely no
sporangia output after 5 days of cultivation in PEA broth compared with untransformed wild
type JH19, which yielded 49.22 sporangia in 10 μL PEA broth culture. Another transformant
(T5) was selected as a non-edited control, in which no significant reduction of sporangia out-
put was detected (Fig 5D and 5F). To check whether the phenotype observed in mutant T8
and T16 strains was specific to sporangia production, we decided to measure the vegetative
mycelia growth rate in them. As a result, both T8 and T16 showed similar vegetative growth
rates, comparable to the controls, on the rye-sucrose medium at 18˚C (S8A and S8B Figs). In
addition, we performed an in planta test by inoculating potato leaves (Solanum tuberosum cv.
De´sire´e) with T5, T8, T16 and wild type JH19. As MADS-box-edited JH19 strains yielded no
sporangia, we selected mycelial discs instead of zoospores for inoculation assays in this experi-
ment. T5 and wild type JH19 strains caused complete infectious lesions and developed obvious
aerial mycelia. In contrast, T8 and T16 only showed partial watery lesions without formation
of aerial mycelia (Figs 5E, 5G and S8C). We further examined the disease area by microscopy:
both T5 and wild type JH19 strains produced sporangia in heavily diseased potato leaves, while
T8 and T16 only developed sparse mycelia without detectable sporangia (S8C Fig).
Editing Avr8-encoding gene in P. infestans HB1501
Phytophthora avirulence (Avr) genes are key determinant factors for gene-for-gene interaction
with host plants such as potato and soybean (Dong et al., 2011). We selected Avr8
(PITG_07558), known as an avirulence gene recognized by potato late blight resistance gene
R8 [52], as the second editing target. We selected P. infestans strain HB1501 for Avr8 editing
since JH19 naturally overcomes the R8-mediated resistance, as was previously established
using inoculation assays. As shown in S7A Fig, genome-wide single nucleotide polymorphism
(SNP) analysis revealed that HB1501 is diploid. Avr8 encodes a 245 aa RxLR effector and was
confirmed as a single-copy gene in strain HB1501 based on the read depth analysis (S7B Fig).
The Avr8 protein includes 3 LWY motifs (63–107, 105–162, 165–218 aa), which might con-
tribute to its novel activities as an RxLR effector during infection progress (Fig 6A) [53].
Cas12a guides RNAs Avr8-g1 and Avr8-g2 were designed to target Avr8 before the first LWY
motif to increase chances of introducing a frame-shift mutation before this motif due to
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Fig 5. Editing a MADS-box transcription factor coding gene in P. infestans strain JH19. (a) Target sites of two gRNAs in the MADS-box coding sequence.
The MEF2-like domain was predicted by InterproScan (version 5.52–86.0). The MEF2-like domain locates at 2–77 aa sites. (b) Detecting of editing events in
MADS-box in JH19 transformants. The PCR assay on T8 and T16 revealed two homozygous editing events. (c) Analysis of PCR amplicon sequencing results
from (b). The PAM sequences are marked in red, the target sequences are marked in blue, and the stop codons are indicated by red arrowheads. Each dash line
represents a deleted nucleotide. (d) Culture scrapings from 10 days Pea broth cultures of wild type JH19, T5, T8 and T16. Scale bars = 0.4 mm. (e) Infection
phenotypes of wild type JH19 (WT), transformants T5, T8 and T16 on leaves of susceptible cultivar potato cv. De´sire´e. Detached potato leaves were inoculated
with mycelia medium discs, and images were recorded 5 days post inoculation. Scale bars = 2 cm. (f) Quantification of sporangia numbers in 10 μL PEA broth
culture of wild type JH19, T5, T8 and T16 in (d). (g) Quantification of lesion size in detached leaves of potato cv. De´sire´e inoculated with wild type JH19 (WT),
T5, T8 and T16 in (e). All data represent average values from three independent experiments with the indicated standard deviations. Statistical differences
among the samples were analyzed with Sˇı´da´k’s multiple comparisons test (P< 0.0021: **, P< 0.0002: ***).
https://doi.org/10.1371/journal.ppat.1011346.g005
editing events (S7D Fig). The cartoon illustrating the design of the Avr8 CRISPR/Cas12a
knockout construct is shown in S7C Fig, with Avr8-g1 and Avr8-g2 targets shown in red in
S7D Fig.
The transformants were PCR-genotyped for edits in Avr8 using primers amplifying the
full-length gene, with PCR amplicons being subsequently sequenced. Out of 27 G418 resistant
transformants, variant bands were observed in two of them, T3 and T10, suggesting both Avr8
alleles were altered in them (Fig 6B). Sequencing of the PCR amplicons from the shifted T3
and T10 bands showed deletions spanning both Avr8-g1 and Avr8-g2 target sites within Avr8.
Unlike the editing events detected in MADS-box, edits in the Avr8 gene in T3 and T10 resulted
in frame-shift mutations predicted to cause early termination of protein translation before the
first LWY motif (Fig 6C).
As a following step, we performed virulence assays by inoculating detached leaves of R8
transgenic potato (De´sire´e R8) with transformants T3, T10, T22 (unedited) and wild type
HB1501 strain. We recorded the infection phenotypes 5 days post zoospore inoculation. Com-
pared with unedited T22 and wild type HB1501, T3 and T10 caused lesions of significantly
larger size upon infection of R8 transgenic potato leaves. Importantly, both T3 and T10 caused
infection symptoms similar to T22 and wild type HB1501 when using detached leaves from
susceptible wild type potato (De´sire´e WT) lacking the R8 gene (Fig 6D and 6E). We therefore
reason that creating a loss-of-function Avr8 allele enables P. infestans to evade R8-mediated
host resistance.
Discussion
As a widely used approach for transient and stable expression of exogenous genes, AMT has
been set up for a broad spectrum of biological categories, including plants, microorganisms
and even human cells [20, 54–56]. The AMT protocols for oomycete species, the majority of
which are classified as destructive plant pathogens, have been reported, including Phy-
tophthora palmivora, Phythium ultimum and Phytophthora infestans [57]. Although these
AMT methods have been utilized for years, they require optimization due to generally low
transformation efficiencies. Arabidopsis bZIP family transcription factor AtVIP1, known as a
binding partner of A. tumefaciens effector VirE2, facilitates VirE2 nuclear import and A. tume-
faciens infectivity [43, 58]. Moreover, significant improvement of transformation was observed
in an A. tumefaciens transformation assay using AtVIP1-overexpressing tobacco plants [42].
Until now, utilization of AtVIP1 as a factor boosting the AMT efficiency required two steps:
(1) generating a stable AtVIP1 transgenic line; (2) transforming a gene of interest into the
AtVIP1 transgenic line. Overexpressing AtVIP1 in a stable transgenic line might cause an
unpredictable pleiotropic phenotype as well as limit the range of selectable markers available
for transformation of a gene of interest. In addition, when applying AtVIP1 the way described
above, one is presented with a chicken-and-egg problem in the case of plant genotypes, which
are not amenable to AMT to start with. A recent study in wheat reported that co-
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PLOS PATHOGENSModification of AMT for two oomycete species
Fig 6. Editing an avirulence gene Avr8 in P. infestans strain HB1501. (a) Target sites of two gRNAs in the Avr8 coding sequence. The LWY motifs were
predicted by InterproScan (version 5.52–86.0). The LWY1 domain locates at 63–107 aa sites, the LWY2 domain locates at 105–162 aa sites, and the LWY3
domain locates at 165–218 aa sites. (b) Detecting editing of Avr8 in HB1501 transformants. The PCR assay in T3 and T10 revealed two homozygous editing
events. (c) Analysis of PCR amplicon sequencing results from (b). The PAM sequences are marked in red, the target sequences are marked in blue, and stop
codons are indicated by red arrowheads. Each dash line represents a deleted nucleotide. (d) Infection phenotypes of wild type HB1501 (WT), T3, T10 and T22
on detached leaves of R8 transgenic potato. Detached potato leaves were inoculated with zoospores of selected strains, and images were taken 5 days post
inoculation. Scale bars = 2 cm. (e) Quantification of lesion sizes in (d). All data represent average values from three independent experiments with the indicated
standard deviations. Statistical differences among the samples were analyzed with Sˇı´da´k’s multiple comparisons test (P< 0.0002: ***).
https://doi.org/10.1371/journal.ppat.1011346.g006
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PLOS PATHOGENSModification of AMT for two oomycete species
transformation of the wheat gene TaWOX5 from the WUSCHEL family with a gene of interest
dramatically increases transformation efficiency, resulting in a lower genotype dependency, in
29 wheat varieties. The latter was similar to our original idea of modifying AMT for oomycete
species [59]. Here, we present an alternative method utilizing AtVIP1 to optimize AMT for
two oomycete species using prokaryotic expression of AtVIP1 fused with a sequence encoding
a T4SS translocation tag in A. tumefaciens.
In addition to utilizing AtVIP1, we have done additional modifications to the procedure
while developing our modified AMT protocol for P. infestans (S3 Fig). Murashige and Skoog
(MS) medium is commonly used for co-cultivation of A. tumefaciens and the explant material
[60, 61]. Considering that A. tumefaciens shows a better growth rate in MS medium than in
induction medium (IM), we used MS medium instead of IM for co-culturing A. tumefaciens
and P. infestans zoospores. The germination of zoospores and transformation efficiency were
not affected by this medium substitution. We used geneticin G418 as a selection agent in this
study, while different P. infestans wild-type strains showed variation in G418 tolerance. For
the JH19 strain, we used 5 μg/mL of G418 for selection of positive transformants, while for the
HB1501 strain—10 μg/mL.
In previously reported PEG-mediated P. infestans transformation or genome-editing proce-
dures, several different situations might occur upon plasmid introduction: (a) the plasmid
might integrate into an unstable site in the transformant’s genome; (b) the plasmid DNA
might be later degraded by enzymes inside P. infestans cells [62]. The modified AMT proce-
dure presented in this study has the advantages of the previously described AMT protocol,
including no need to produce protoplasts, no need for a large amount of high-quality plasmid
DNA, and, in addition, the integrated T-DNA fragment in the genomic DNA might be more
stable than plasmid DNA [63]. The AMT method also comes with its issues e.g. during the
T-DNA integration step: (a) some transgene instability might be observed, probably due to
rearrangement of the T-DNA region, and/or due to homologous recombination between cop-
ies of the transgene inserted into the DNA in the same nucleus; (b) only part of the T-DNA
might integrate into genomic DNA [64].
Importantly, during PEG-mediated transformation, the plasmid DNA might not integrate
straightaway in protoplasts but at a later stage, during cell differentiation. During the AMT
process, T-DNA integration also potentially occurs in encysted zoospores that is followed by
emergence of germ tubes. Both of the described above situations would result in chimeric
mycelia in resulting transformants, although there are currently no data to indicate that this is
the case with AMT [65].
In this study, each AMT experiment started with approximately 8 × 105 zoospores, and 9 of
18 experiments, conducted using our modified AMT method, produced at least 10 G418-resis-
tant colonies; 5 of 18 attempts produced at least 20 G418-resistant colonies (Table 1). However,
further characterization of acquired transformants revealed that part of the isolates, trans-
formed with gfp, that showed resistance to G418, did not show a GFP signal during confocal
microscopy analysis or expressed a GFP-size protein detectable by western blotting (Table 1
and S4 Fig). The Southern blot analysis of representative transformants of the HB1501 back-
ground suggested that the T-DNA segments with the nptII gene were integrated into all six
selected isolates, which were positive for the GFP signal, and one transformant (T1) with no
GFP signal (Fig 2F). The latter could be due to the issue (b) of the AMT protocol that was men-
tioned above.
During the Southern blot analysis, we observed bands of similar small size (< 4.3 kb) in
lanes 2, 3, 4, 7 and 8 (Fig 2F). These results might be caused by non-specific hybridization or,
possibly, partial T-DNA integration events in selected HB1501 transformants. The above-
mentioned observations are consistent with a similar phenomenon observed during plant
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PLOS PATHOGENSModification of AMT for two oomycete species
transformation [66]. To characterize better the integration events in transformants of oomy-
cete species, we would like to perform next generation sequencing (NGS), that represents a
highly sensitive approach to detect T-DNA insertions in transgenic isolates.
There are few more differences between the PEG-mediated transformation and AMT
methods, e.g. the different recipient cell types. Importantly, many protoplast cells used for
PEG-mediated transformation are coenocytic, while most zoospores used for AMT are single-
nucleated and wall-less [63, 67]. However, we have no sufficient evidence to suggest that AMT
of P. infestans zoospores could eliminate the issue of potential heterokaryoteyotic transfor-
mants, particularly because it was reported that a certain fraction of P. infestans zoospores had
been observed to be multinucleate [68]. Additionally, the conditions used in our modified
AMT method could not eliminate the possibility of encystment of the zoospores followed by
emergence of a germ tube during co-cultivation of zoospores and Agrobacterium cells. To illus-
trate such scenario, we included the potential situation of T-DNA integration in multinucleate
cells in Fig 1B. We also performed a comparison between the published PEG-mediated trans-
formation and AMT protocol, and our modified AMT protocol for P. infestans (S4 Table). As
a result, we would define our modified AMT protocol as an option to be considered, rather
than top choice, for P. infestans transformation, as transformation efficiencies associated with
different protocols are difficult to compare due to different standards used.
In addition to P. infestans, genetic transformation methods have not been set up for many
biotrophic oomycetes. Martı´nez-Cruz et al. has reported an AMT method for Podosphaera
xanthii, a biotrophic fungus that causes cucurbit powdery mildew [48]. Based on the AMT
method for P. xanthii, we extended our modified AMT protocol to Plasmopara viticola and
successfully obtained a positive transformant (Figs 3 and S5). There are a few more issues that
need to be addressed when it comes to AMT of P. viticola, including (a) transformation effi-
ciency might vary in different P. viticola isolates; (b) leaves from different grapevine varieties
may contribute differently to screening of resistant transformants; (c) it would be difficult to
recover P. vitcola transformants from infected grapevine leaves without aseptic conditions; (d)
stable expression of an exogenous gene needs further validation in subsequent generations of
obtained transformants [1]. Although we have acquired one positive stable transformant of P.
viticola based on our modified AMT method with AtVIP1, we still need to do more transfor-
mation attempts and analysis to draw a solid conclusion, in respect to the transformation effi-
ciencies, in the future. Surely, we know the importance of acquiring a stable transformant of P.
viticola, while our experimental procedure comes with a few shortcomings: (a) the transforma-
tion efficiency is not high enough as compared to other oomycete species; (b) we have not per-
formed a sufficient number of transformation assays with other P. viticola isolates.
Consequently, the extensibility of our strategy to P. viticola suggests that AtVIP1 could be con-
sidered for modifying AMT methods for other oomycete species, especially some hard-to-
transform biotrophic oomycetes, such as Bremia lactucae.
Unlike gene overexpression, integration of a CRISPR/Cas cassette in transformants does
not guarantee successful editing of a gene target. Previous reports have demonstrated that edit-
ing efficiency varies greatly, from 1% to 100%, among different eukaryotic pathogens [69]. The
editing frequency of CRISPR/Cas12a in P. infestans reached 13% by using the PEG transfor-
mation method [10, 12]. In this study, editing of the MADS-box gene resulted in two homozy-
gous mutants out of 16 transformants, and editing of Avr8 genes resulted in two homozygous
mutants out of 28 transformants (Table 1). Although introducing AtVIP1 does not seem to
increase the frequency of CRISPR/Cas12a-mediated genome editing events in P. infestans, our
modified AMT method still provides a valuable option for future related studies.
We selected two target genes for CRISPR/Cas12a-mediated genome editing in this study
based on two criteria. The first is avoiding multi-copy target genes to reduce the difficulty of
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PLOS PATHOGENSModification of AMT for two oomycete species
editing and transformant screening, and the second is that transformants with successful edit-
ing events should present explicit phenotypes. The cycle of aerial asexual sporangia dispersal
plays a crucial role in late blight development [70]. Thus, we selected MADS-box as our first
target gene that is reported to express only in sporulating mycelia and spores of P. infestans.
MADS-box (PITG_07059) was first identified by Leesutthiphonchai and Judelson in 2018 and
MADS-box transcription factors play significant roles in eukaryotes [50]. We utilized modified
AMT and CRISPR/Cas12a-mediated genome editing methods and obtained two edited
MADS-box mutants (Fig 5). Consistently with the results obtained using the RNAi approach,
our edited MADS-box mutants produced no sporangia and showed reduced ability to infect
potato leaves (Fig 5). RNAi is triggered by siRNAs whose silencing efficiency is not guaranteed
and varies widely in different transformants. In contrast to RNAi methods, genome editing
would provide more stable phenotypic data for further research on P. infestans. Since during
CRISPR/Cas12a-mediated genome editing, based on the AMT method, the Cas12a expression
cassette stably integrates into the P. infestans genome, an additional self-fertilization step could
be used to remove Cas12a from the original transformant, similarly to the situation in planta
[71].
Disrupting the recognition of phytopathogen avirulence (AVR) genes by plant resistance
(R) genes normally produces easily observable phenotypes. Thus, we selected Avr8 (also called
AVRSmira2 and PITG_07558), a single-copy AVR gene recognized by potato late blight resis-
tance gene R8, as our second genome editing target. We chose P. infestans strain HB1501 for
Avr8 gene editing because seemingly the JH19 strain broke down the R8-mediated resistance
in potato. Avr8 was identified by analysis of variance (ANOVA) using the average AUDPC val-
ues of both its responses to the R gene and field trials [72]. The broad spectrum late blight
resistance gene R8 that recognizes Avr8 was cloned from Solanum demissum, based on a previ-
ously published coarse map position on the lower arm of chromosome IX, and the correlation
between the expression levels of Avr8 and R8-mediated resistance had been proven in a previ-
ous study [73]. However, an inoculation assay of an Avr8 knockout P. infestans mutant on
potato carrying the R8 gene has not been reported yet. In our study, we produced two
genome-edited Avr8 mutants of P. infestans (strain HB1501), and both mutants induced infec-
tion lesions in leaves of the R8 transgenic potato line cv. De´sire´e (Fig 6D and 6E).
Collectively, generating P. infestans transformants or genome edited mutants via our modi-
fied AMT procedure is less laborious and results in an acceptable transformation rate as com-
pared with the previously reported AMT protocol and PEG-mediated protoplast
transformation method. Successfully acquiring a stable transformant of P. viticola gives a
strong hint of gaining a potential advantage by utilizing proteins, such as AtVIP1, that play an
important role in host cells during the AMT process. Although AMT has already been estab-
lished in plenty of phytopathogen species, it would be particularly interesting to investigate
whether our modified AMT protocol would increase the efficiency of transformation or that
of CRISPR/Cas-mediated genome editing in them or even extend the effect to other oomycete
or plant species.
Materials and methods
Growth conditions for P. infestans, P. viticola, bacteria and plants
P. infestans strains were cultured on rye-sucrose medium (agar 15g/L) at 18˚C. P. infestans
strain JH19 was isolated from infected tomato in San Diego Country, California in 1982 and
kindly provided by Howard S. Judelson lab [12]. P. infestans strain HB1501 was isolated from
Hebei Province in 2015 [74]. Plasmopara viticola isolate BS5 was kindly provided by Dr. Linfei
Shangguan at Nanjing Agricultural University and was isolated in Nanjing, China in 2017. A.
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PLOS PATHOGENSModification of AMT for two oomycete species
tumefaciens strains and E. coli strains were grown on Luria–Bertani (LB) agar (NaCl 10g/L,
Yeast extract 5g/L, Tryptone 5g/L, agar 15g/L) at 28˚C and 37˚C, respectively. Solanum tubero-
sum L. cv. De´sire´e (2n = 4x = 48) and trangenic lines were grown in soil or in MS medium
(MES 0.5 g/L, sucrose 20 g/L, agar 8 g/L, pH5.8), after seed surface sterilization, and main-
tained in vitro. Vitis vinifera (Cultivar grape, Zitian Seedless, A17) was used for culturing of P.
viticola isolate BS5. All plants were grown in environment-controlled growth chambers under
long-day conditions (16 h light/8 h dark cycle at 140 μE sec-1m-2 light intensity) at 22˚C.
Construction of plasmids
Primer sequences used in these cloning procedures are described in S1 Table, and plasmids
and cloning strategies are summarized in S2 Table. For AtVIP1 gene expression in A. tumefa-
ciens, the coding sequences of AtVIP1 (AT1G43700) and virF (NC_003065.2) without the N
terminal 42 amino acids (ΔN42virF) were PCR-amplified, using A. thaliana Col-0 cDNA
library and A. tumefaciens C58 gDNA, respectively, as templates and cloned into p533BL. A
pCB302B backbone construct with the virB1 promoter from A. tumefaciens C58 was used to
drive acetosyringone induced gene expression in A. tumefaciens.
To construct binary plasmid for P. infestans transformation, Bremia lactucae Ham34 pro-
moter and terminator were PCR-amplified and cloned into I-CeuI site of pPZP-RCS2, while
nptII expression cassette driven by Phytophthora sojae RPL41 promoter and B. lactucae Hsp70
terminator was inserted into AscI site of pPZP-RCS2, which resulted in pLY40. The coding
sequence of gfp was PCR-amplified and cloned into I-CeuI site of pLY40 separately to obtain
pLY40-gfp. The sequences of the RPL41 promoter from P. sojae, Ham34 promoter and termi-
nator, Hsp70 terminator from B. lactucae were all PCR-amplified from pYF515, a plasmid con-
struct used for genome editing in P. sojae [75].
To construct binary plasmids for CRISPR/Cas12a mediated P. infestans genome editing,
the coding sequences of NLS derived from a P. sojae bZIP transcription factor [10], human
codon-optimized LbCas12a from p33lb [76] and artificial synthetic polyA-crRNA-Ham34 ter-
minator segment (S6C and S7C Figs) were fused and cloned into I-CeuI/PacI sites in pLY40,
to obtain pLY40-MADS-box-KO and pLY40-Avr8-KO.
The plasmid sequences of pLY40, pLY40-gfp and pLY40-Cas12a-gfp are presented in
Appendix S1.
Transient transformation assays in wheat tissue
Transient expression assays in wheat tissue were performed as previously described for N.
benthamiana with some modifications [77]. A. tumefaciens overnight culture was diluted in
LB liquid medium without antibiotics, grown for 3–4 h and adjusted to OD600 = 0.5. Leaves
and roots from 4-weeks old in vitro wheat plant were collected and divided into 5 mm seg-
ments, then immersed for 10 min in Agrobacterium suspension, placed on MS medium at
22˚C for 3 days in growth chamber. Leaf and root segments were then rinsed by sterilized
water and transferred into GUS staining solution and incubated at 37˚C overnight [78].
Agrobacterium meditated transformation of P. infestans zoospores
AMT of P. infestans zoospores followed previous published method with few modifications
and summarized in S3 Fig [7]. Briefly, P. infestans strains were ready for zoospore-induction
after 14 days of growth on solid rye-sucrose medium (90mm petri dish plates). Approximately
5 mL of ice-cold sterilized water was used to flush and soak P. infestans culture and the culture
plates were plated at 4˚C for 2 hours, and zoospores will be released (100 zoospores counts/μL
for isolate JH19, 200 zoospores counts/μL for isolate HB1501). A. tumefaciens strains with
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PLOS PATHOGENSModification of AMT for two oomycete species
constructed plasmids for transformation was growing overnight with proper antibiotics
(25 μg/mL rifampicin, 50 μg/mL kanamycin, 100 μg/mL spectinomycin), 1 mL of Agrobacter-
ium culture was added into 50 mL LB liquid medium and grown for 3–4 h till OD600 reach 1.0.
Agrobacterium cells were centrifuged at 4000 rpm for 10 min to collect cells and resuspended
by MS liquid medium with 200 μM acetosyringone. Agrobacterium suspension was cultured at
room temperature for 1 h and then mixed with harvested fresh P. infestans zoospores (about
8 × 105 zoospores for both isolate JH19 and HB1501). The mixture was cultured at room tem-
perature for 45 min and zoospores were collected by centrifuge at 265 g for 5 min, each 200 μL
of zoospore culture was spread at a 5 cm × 5 cm Nytran membrane upon MS solid medium
plate (8 g/L agar), and the plates were cultured in dark at 22˚C for 4 d. The membrane was
then moved upside down on Plich medium (0.5 g/L KH2PO4, 0.25 g/L MgSO4.7H2O, 1 g/L
Asparagine, 1 mg/L Thiamine, 0.5 g/L Yeast extract, 10 mg/L β–sitosterol, 25 g/L Glucose, 15
g/L agar) with 1.5 mg/L G418 and 300 mg/L timentin, and plates were cultured at 18˚C for 4 d,
the membranes were then removed and germinated mycelia were supposed to be observed,
the plates were keep in 18˚C for 4 d. Melt rye-sucrose medium with 3 mg/L of G418 was then
covered on Plich medium plates for further selection, the G418 concentration could be
increased up to 5 mg/L at this stage.
Agrobacterium meditated transformation of P. viticola zoospores
AMT of P. viticola zoospores followed previous published method on cucurbit powdery mil-
dew pathogen Podosphaera xanthii and summarized in S5A Fig [48]. Briefly, culture of A.
tumefaciens strain EHA105 with pV1F and proper T-DNA construct was prepared following
the same methods that described in AMT of P. infestans. Separately, the sporangia from P. viti-
cola BS5 inoculated grape leaves were harvested by immersion of infected tissues in 30 mL of
sterilized water with 0.01% Tween-20 and keep in room temperature for 1 h until zoospores
released. About 10 mL (about 1 × 106 zoospores) P. viticola zoospores were gently mixed with
same volume of A. tumefaciens suspension and co-cultivated for 1 h at room temperature in
the dark in an orbital shaker at 65 rpm. Zoospores were then centrifuged for collection (265 g
for 5 min), and zoospores in 1 mL of residual were deposited in young detached grape leaves
(must be Zitian Seedless, A17 for the best inoculation rate). Two days after inoculation, the
grape leaves were rinsed with 5 mg/L G418 and 300 mg/L Timentin to kill A. tumefaciens and
select P. viticola transformants. To be noted, rinsing infection samples with G418 (5 mg/L)
and Timentin (300 mg/L) should have no visible negative effect on grape leaves during the
above-mentioned procedure. To acquire the stable transformant of P. viticola, the obtained
isolate was sub-inoculated at zoospore stage on young grape leaves without G418 treatment.
After at least three rounds of sub-inoculation, the P. viticola isolate that showed stable GFP sig-
nal, was defined as a stable transformant.
Virtualization of GFP
CLSM (Leica AF6000 modular microsystems) was used to take pictures of P. infestans. A
489-nm line from an argon ion laser were used to excite green fluorescent protein (GFP). For
each assay, six independent leaves were observed for each experiment and each experiment
has at least 3 repeats.
sgRNA design and cloning
CRISPR/Cas12a targets for MADS-box (PITG_07059) and Avr8 (PITG_07558) were designed
with overall consideration based on output data from EuPaGDT, CRISPOR and Deep-Cpf1
[79–81]. The used crRNAs were carefully inspected with sequencing data of P. infestans JH19
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PLOS PATHOGENSModification of AMT for two oomycete species
and 1501 to avoid off-target events. DNA oligonucleotides contains crRNAs and direct repeats
(DR) were artificial synthesized and cloned into pLY40 based strategy described above and in
S6C and S7C Figs.
Detection of target gene editing
Genomic DNA (gDNA) of P. infestans strain or relative transformants was first isolated from
liquid cultural mycelia. Specifically, 5 mycelia discs of each P. infestans strain from rye-sucrose
medium plates were cut and placed into 10 mL of PEA broth, and mycelia for gDNA extrac-
tion were harvested after 5 days growth in dark at 18˚C. Mycelia were then blot up by filter
paper and gDNA was extracted with Omega E.Z.N.A. Plant DNA Kit (HP). To confirm edit-
ing, primer pair F: 5’-ATGGGCCGCAAGAAGATCCAG-3’ and R: 5’-TCAAACAGCCACA
CGTTGACGCTTG-3’ were for checking MADS-box editing in P. infestans JH19 derived
transformants, and primer pair F: 5’-ATGCGCTCAATCCAACTTCTG-3’ and R: 5’-TTAC
GATGTTTTCGCTTCTTTAAAAAG-3’ was for checking Avr8 editing in P. infestans 1501
derived transformants.
Protein analysis
P. infestans protein assay referred to previously described method [12]. Briefly, mycelia were
collected from PEA broth culture and total protein was extracted with Beyotime RIPA P0013B
Lysis Buffer. Immunoblots were performed as described [78]. Total protein was eluted in
sodium dodecylsulfate (SDS) sampling buffer and proceed to western blot analysis. LbCas12a
was detected by immunoblotting with anti-LbCas12a (Cpf1) antibody (Sigma/SAB4200777,
dilution 1:4000), followed by a secondary antibody conjugated to FITC (ThermoFisher Scien-
tific, dilution 1:5000).
Southern blot analysis
For T-DNA integration analysis, we performed southern blot with genomic DNA obtained
from P. infestans transformants or wild-type (WT) isolates. Four μg genomic DNA was
digested with restriction enzyme HindIII (Takara), and separated on DNA agarose gel (1%)
and then blotted on positively charged nylon membranes. A nptII gene fragment was used as
probe. Further preparations of probes DIG-labeling, hybridization and chemiluminescent
detection were conducted according to the operation protocol of DIG-High Prime DNA label-
ing and Detection Starter Kit (ROCHE/11585614910).
Leaf inoculation with P. infestans
For zoospores inoculation assays, zoospores of P. infestans strains were collected from plates
followed by the same method described above. 10 μL drops with 200,000 to 400,000 zoospores
per mL were inoculated on detached leaves from 4 to 6 weeks old potato plants of wild type
De´sire´e and R8 trangenic potato lines. For mycelial disc inoculation assays, detached potato
leaves were inoculated with mycelial discs (5 mm diameter) taken from the edge of 7 days-old
rye-sucrose medium culture of P. infestans. Inoculated leaves were kept in a plastic tray
(30 × 44 × 8 cm) covered with polypropylene film at 22 ± 3˚C. Results were recorded 5 days
post inoculation. For each inoculation assay, 8 independent leaves were used for each experi-
ment and each experiment has at least 3 repeats.
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PLOS PATHOGENSModification of AMT for two oomycete species
Supporting information
S1 Table. Primers used in this study.
(XLSX)
S2 Table. Plasmids used in this study.
(XLSX)
S3 Table. Sequence similarity data used in Fig 1A.
(XLSX)
S4 Table. Comparisons of modified AMT protocol and previous reported transformation
protocols for P. infestans.
(XLSX)
S1 Fig. Translocating AtVIP1 from A. tumefaciens to host cells. (a) The expression cassette
used for translocating AtVIP1 fused with GFP (b) Confocal microscopy observation of N.
benthamiana leaves infiltrated with A. tumefaciens EHA105 carrying the construct described
in (a). Images were taken at 3 days post infiltration. Images are single confocal sections and are
representative of images obtained in three independent experiments. White arrows indicate
observed nuclei in tobacco cells. Scale bars = 40 μm. Three independent experiments were per-
formed for each assay with similar results.
(TIF)
S2 Fig. AtVIP1 enhances transient AMT efficiency in wheat tissues. (a) Schematic represen-
tation of plasmid constructs used in this experiment. The pWMB110-gus construct contains a
β-glucuronidase expression cassette, carrying the maize adh1 intron, in the T-DNA region.
(b-c) Transient transformation on wheat leaf and root segments. Dissected wheat tissue seg-
ments were inoculated with A. tumefaciens EHA105 carrying the binary plasmid pWMB110-
gus and either pV1F or the control plasmid pEV. At 3 days post inoculation, GUS activity was
analyzed by histochemical staining. Scale bars = 2 mm. At least 50 leaf or root segments were
recorded in each experiment. Each experiment was repeated 3 times and representative results
were presented. (d) Quantification of root segments that expressed the gus gene in (c). Statisti-
cal differences among the samples were analyzed with Sˇı´da´k’s multiple comparisons test (P<
0.0001: ****).
(TIF)
S3 Fig. Schematic outline of modified AMT for P. infestans.
(TIF)
S4 Fig. Western blot characterization of P. infestans HB1501 transformants obtained
using pLY40-gfp and pV1F. Total protein samples were purified from 14 transformants with
a GFP signal (up) and 14 transformants without a GFP signal (down). All blots were probed
with an anti-GFP antibody. The protein blot was stained with Ponceau S to confirm equal
loading.
(TIF)
S5 Fig. Obtaining Plasmopara viticola BS5 transformant T1, expressing gfp, using the opti-
mized AMT method. (a) Schematic outline of the optimized AMT method for P. viticola BS5.
(b) AMT with only pLY40-gfp produced no G418 resistant transformants of P. viticola BS5
(left), while AMT with pLY40-gfp and pV1F produced the transformant T1 (white arrow) that
is resistant to G418 (right). Scale bars = 2 mm.
(TIF)
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PLOS PATHOGENSModification of AMT for two oomycete species
S6 Fig. The gRNA target regions used for MADS-box genome editing in P. infestans. (a)
Genome-wide allele ratio analysis of P. infestans JH19. (b) Copy number of PITG_07059
(MADS-box) relative to single-copy control gene (= 1.0), determined based on read depth in
DNA library of JH19 strain. (c) Schematic representation of the constructs used in this experi-
ment. The pLY40-MADS-box-KO with either pV1F or pEV were used for P. infestans transfor-
mation in this experiment. Two gRNAs for MADS-box editing are named as g1 and g2. (d)
Gene sequence of PITG_07059 (MADS-box). Sequences marked in red are targeted by g1 and
g2. (e) Sequencing chromatograms of MADS-box in wild type JH19, T8 and T16. Both T8 and
T16 showed single peaks in either the g1 (left) or g2 (right) target sites. The wild type sequences
with gRNA targets are shown at the top of the panel; black arrows indicate the 5’ border of the
detected deletion.
(TIF)
S7 Fig. The gRNA regions used for Avr8 editing in P. infestans. (a) Genome-wide allele ratio
analysis of P. infestans HB1501. (b) Copy number of PITG_07558 (Avr8) relative to single-
copy control gene (= 1.0), determined based on read depth in DNA library of HB1501 strain.
(c) Schematic representation of the constructs used in this experiment. (d) Gene sequence of
PITG_07558 (Avr8). Two selected gRNA target regions are marked in red. (e) Sequencing
chromatograms of Avr8 in T3, T10 and T22 of HB1501. Both T3 and T22 showed single peaks
in both g1 and g2 target sites. The wild type sequences with gRNA targets are shown at the top
of the panel; black arrows indicate the 5’ border of the detected deletion.
(TIF)
S8 Fig. Vegetative growth of P. infestans strains. (a) Mycelia cultured on the rye-sucrose
medium were photographed at 5 days post inoculation. (b) Quantification of mycelium diame-
ter of P. infestans strains in (a). All data represent average values from three independent
experiments with the indicated standard deviations. (c) Microscopy images of the opposite
side of the inoculated region of detached potato leaves in Fig 5E show the details of mycelia
generated during infection. Images were taken at 5 days post inoculation. White arrowheads
indicate the observed sporangia. Scale bars = 1 mm.
(TIF)
S1 Appendix. Sequences of pLY40, pLY40-gfp, pLY40-Cas12a-gfp.
(DOCX)
Acknowledgments
We thank Dr. Howard Judelson (UCR, USA) and Prof. Yuanchao Wang (NAU) for the discus-
sion on Phytophthora genome editing. Potato R8 transgenic line was kindly provided by Dr.
Jack Vossen (WUR, Netherlands). The Plasmopara viticola BS5 was a kind gift from Prof. Lin-
fei Shangguan (NAU). We thank Dr. Vitaly Citovsky from Stonybrook University for support-
ive discussion on the original project design. We thank Ms. Ying Zheng (NAU) for confocal
microscopy. We thank Ms. Zhao Hu, Dr. Xinyu Liu and Dr. Changling Mou (NAU) for their
help with Southern blot analysis and constructive comments on this study.
Author Contributions
Conceptualization: Luyao Wang, Sanwen Huang, Suomeng Dong.
Data curation: Luyao Wang, Fei Zhao, Haohao Liu, Suomeng Dong.
Formal analysis: Luyao Wang, Fei Zhao, Haohao Liu, Suomeng Dong.
PLOS Pathogens | https://doi.org/10.1371/journal.ppat.1011346 April 21, 2023
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PLOS PATHOGENSModification of AMT for two oomycete species
Funding acquisition: Luyao Wang, Sanwen Huang, Suomeng Dong.
Investigation: Luyao Wang, Fei Zhao, Haohao Liu, Suomeng Dong.
Methodology: Luyao Wang, Fei Zhao, Haohao Liu, Han Chen, Fan Zhang, Vladimir
Nekrasov, Suomeng Dong.
Project administration: Luyao Wang, Sanwen Huang, Suomeng Dong.
Resources: Luyao Wang, Sanwen Huang, Suomeng Dong.
Software: Luyao Wang, Fan Zhang, Sanwen Huang, Suomeng Dong.
Supervision: Luyao Wang, Sanwen Huang, Suomeng Dong.
Validation: Luyao Wang, Sanwen Huang, Suomeng Dong.
Visualization: Luyao Wang, Suomeng Dong.
Writing – original draft: Luyao Wang, Sanwen Huang, Suomeng Dong.
Writing – review & editing: Luyao Wang, Han Chen, Fan Zhang, Suhua Li, Tongjun Sun,
Vladimir Nekrasov, Sanwen Huang, Suomeng Dong.
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PLOS PATHOGENS
| null |
10.1371_journal.pone.0269555.pdf
|
Data Availability Statement: All relevant data are
within the paper and its Supporting Information
files.
|
All relevant data are within the paper and its Supporting Information files.
|
RESEARCH ARTICLE
Grapevine trunk diseases of cold-hardy
varieties grown in Northern Midwest
vineyards coincide with canker fungi and
winter injury
David H. DeKreyID
1
1*, Annie E. Klodd2, Matthew D. Clark3, Robert A. BlanchetteID
1 Department of Plant Pathology, University of Minnesota, St. Paul, Minnesota, United States of America,
2 University of Minnesota Extension, Farmington, Minnesota, United States of America, 3 Department of
Horticultural Science, University of Minnesota, St. Paul, Minnesota, United States of America
* [email protected]
Abstract
Grapevine trunk diseases make up a disease complex associated with several vascular fun-
gal pathogenic species. Surveys to characterize the composition of grapevine trunk dis-
eases have been conducted for most major grape growing regions of the world. This study
presents a similar survey characterizing the fungi associated with grapevine trunk diseases
of cold-hardy interspecific hybrid grape varieties grown nearly exclusively in the atypical
harsh winter climate of Northern Midwestern United states vineyards. From the 172 samples
collected in 2019, 640 isolates obtained by culturing were identified by ITS sequencing and
represent 420 sample-unique taxa. From the 420 representative taxa, opportunistic fungi of
the order Diaporthales including species of Cytospora and Diaporthe were most frequently
identified. Species of Phaeoacremonium, Paraconiothyrium, and Cadophora were also
prevalent. In other milder Mediterranean growing climates, species of Xylariales and Botryo-
sphaeriales are often frequently isolated but in this study they were isolated in small num-
bers. No Phaeomoniellales taxa were isolated. We discuss the possible compounding
effects of winter injury, the pathogens isolated, and management strategies. Additionally,
difficulties in researching and understanding the grapevine trunk disease complex are
discussed.
Introduction
Grapevine trunk diseases (GTDs) make up a disease complex most often associated with sev-
eral wood-inhabiting fungal species [1] and more recently possibly some bacterial species [2].
Sub-groups of these diseases are frequently categorized by symptomology and or taxonomic
designation of causal fungal agents. Common names given to GTDs include Esca [3], folletage
or berry shrivel [4], Petri disease, young esca, young vine decline [5], hoja de malvo´n [6],
Botryosphaeria dieback, bot canker, black goo [7], slow stroke [8], eutypiosis, Eutypa dieback
[9], black dead arm, dying arm, dead arm [10], swelling arm [11], grapevine leaf stripe disease
a1111111111
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OPEN ACCESS
Citation: DeKrey DH, Klodd AE, Clark MD,
Blanchette RA (2022) Grapevine trunk diseases of
cold-hardy varieties grown in Northern Midwest
vineyards coincide with canker fungi and winter
injury. PLoS ONE 17(6): e0269555. https://doi.org/
10.1371/journal.pone.0269555
Editor: Hernaˆni Gero´s, Universidade do Minho,
PORTUGAL
Received: January 24, 2022
Accepted: May 23, 2022
Published: June 3, 2022
Copyright: © 2022 DeKrey et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: All relevant data are
within the paper and its Supporting Information
files.
Funding: MDC, RAB, AEK, DHD. This research was
funded by the Minnesota Agricultural Rapid
Response Fund and USDA Hatch Project MIN-22-
081 and MIN-22-089. The funders had no role in
study design, data collection and analysis, decision
to publish, or preparation of the manuscript.
Competing interests: The authors have declared
that no competing interests exist.
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
1 / 25
PLOS ONEGrapevine trunk diseases of the Northern Midwest
[12], Phomopsis dieback, black spot [13], black measles [14], and black foot disease [15]. These
diseases can be difficult to diagnose due to their sporadic symptom display and similarity of
external and internal symptoms. Such symptoms may include interveinal foliar chlorosis and
necrosis or tiger striping, generalized dieback, apoplexy or sudden death, gummosis, vascular
streaking, wedge- or V-shaped vascular discoloration, cankers, and wood decay (Fig 1) [16].
GTDs cause serious grapevine health and economic problems and can be found in all grape
growing regions of the world [17–19]. In the Northern Midwest United States (NMW), grow-
ers often struggle with unproductive cordon sections commonly referred to as “skips in the
cordon” or “blind wood” (Fig 1A and 1B). Cordon skips come at the cost of vineyard managers
with lower yields and require retraining new cordons. In the past, chemicals such as sodium
arsenate was used to control GTDs but health [20] and environmental concerns [21] have
eliminated its widespread use. Often the dramatic increase in the incidence of GTDs in the last
two decades is associated with the 2003 ban on sodium arsenate [22]. However, the increasing
incidence of GTDs in countries which have never used sodium arsenate points to other factors
being involved [22]. To date, very few chemical options are available to growers but recent
research in the use of biological control agents has shown some promise for controlling spe-
cific fungal GTD pathogens [23]. In most situations, development of best practices for GTD
management remains the best option for growers. Management strategies can include prac-
tices such as variety selection, rootstock selection, training system, pruning timing, double-
pruning, wound-protection, multi-trunking, trunk renewal, trunk surgery, debris removal,
tool sterilization, and other practices [24]. Management options of GTD pathogens tend to be
region specific with considerations to climate, weather, cultural practices, and varieties grown.
In the NMW, wine grape growing is a relatively new industry that is increasing at a consider-
able pace. According to the 2016 University of Minnesota Extension vineyards and grapes sta-
tus report, planted cold-hardy grapevine varieties increased from 5900 acres to 7580 acres
from 2011 to 2015 [25]. However, Tuck et al. also reported an average decrease in yield of 3.5
to 3.2 tons per acre from 2011 to 2015 which indicates a need for better-informed, variety and
region-specific GTD management practices. To accomplish this, it is important to identify the
GTDs responsible for the problems.
Traditional European Vitis vinifera cultivars are not often grown in the NMW due to diffi-
culties brought on by harsh winters and a short growing season. Instead, own-rooted cold-
hardy interspecific hybrid grape (CIHG) varieties are widely and often exclusively grown in
the region. The genetic contribution of the native riverbank grape (V. riparia) provide CIHG
varieties developed in Minnesota their cold-hardiness (rated down to -30˚C) [26, 27] and
some resistance to endemic diseases and insect pests like phylloxera [28, 29]. Over the past
four decades, the University of Minnesota has become a leader in the development of several
CIHG wine and table grape varieties. The varieties most produced in the region include Mar-
quette, Frontenac blanc, Frontenac, La Crescent, Petite Pearl, Brianna, and Frontenac Gris
[30].
As many NMW vineyards are now reaching a decade in age since their first vines were
planted, the characteristic cordon skip (Fig 1A and 1B) and dieback (Fig 1D) symptoms of
GTDs have begun to appear. In addition, the compounding effect that GTDs and winter injury
have on vines is becoming a major concern (Fig 1L). In many other parts of the world where
grapes are grown, surveys have been conducted to characterize the region-specific composi-
tion of GTD pathogens. In Europe and nearby Mediterranean countries where GTDs were
first reported, major causal agents include fungal species of the genera Eutypa, Diplodia,
Botryosphaeria, and Phaeomoniella [19]. Similar fungal species have also been identified as
major causal agents of GTDs in Australia, New Zealand [31], South Africa [32], China [33–
35], and Chile [36, 37] as well as southern US and west coast US [38, 39]. Species of
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
Fig 1. Symptoms of grapevine trunk diseases in Northern Midwest vineyards. Cankers were often associated with skips in the cordons but had
rarely wedge-shaped discoloration (A). Cankers more often had irregular shaped xylem reactions (B). Pycnidia were sometimes observed fruiting
from cankers (B) and bleached canes (C). Dieback symptoms are common and the result of successive skips starting from tips of cordons (D).
Pruning wounds were associated with minor (E), moderate (F), and severe (G) vascular streaking symptoms. Near completely healthy vascular
tissue observed in wild Vitis riparia vines (H). Infrequent shallow cracks (I), several shallow cracks (J), and deep cracks (K and L) were associated
with minor to moderate (I), moderate to severe (J), and severe (K) vascular symptoms. Winter injury often results in deep cracks on the trunk (L).
Observations included cankers (ck), skips in the cordons (sk), bleached canes (bc), dieback (db), pruning wounds (pw), shallow cracks (sc), deep
cracks (dc), black spotting (bs), black lines (bl), brown-red wood streaking (br), brown to black necrotic streaking (bn), discolored xylem (dx),
sometimes healthy tissue (h), and white rot (wr). Bars = 1 cm.
https://doi.org/10.1371/journal.pone.0269555.g001
Fomitiporia are often the main white-rot pathogen found in older vines in most of these
regions as well [19]. Species of Phaeoacremonium have been identified in grapevines and other
woody hosts in several countries around the world [40]. Species of Cadophora are on occasion
identified as well notably found in Canada [41]. Species of Diaporthe and Cytospora have also
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
3 / 25
PLOS ONEGrapevine trunk diseases of the Northern Midwest
been identified in most of these regions though often to a lesser extent and usually in more
humid growing regions [32].
However, no surveys have been conducted in the NMW or exclusively on CIHG cultivars.
The objective of this study was to identify the major GTD species throughout the grape-grow-
ing regions of Minnesota and Wisconsin. Three hypotheses were explored in this study. First,
NMW GTDs will have a regionally distinct composition compared to other grape-growing
regions of the world given the harsh growing climate and CIHG varieties grown. Second, die-
back symptoms and internal vascular streaking can be associated with pruning wounds and
winter injury. Third, isolation frequency of fungal genera will significantly differ compared to
sample variety, variety berry color, sample section type, and sample county origin.
Methods
Sample collection
Our sample collection was targeted towards symptomatic grapevines showing skips in the cor-
dons, generalized dieback, reduced productivity, vascular discoloration, vascular decay, or
apoplexy (Fig 1). A few externally asymptomatic vines were also collected for comparison. In
2019, a total of 172 samples were collected and brought to the laboratory. Samples were col-
lected throughout both the dormant and growing season of 2019. Some samples were shipped
by priority mail. Most samples collected were woody sections of grapevines, especially of cor-
dons and trunks. It is important to note that regular re-trunking is frequently practiced in
NMW vineyards and therefore main woody trunks of vines rarely, if ever, exceed ten years in
age. Samples were stored at -20˚C until processed. Samples were acquired from 34 vineyards
in Minnesota and Wisconsin from a total of 21 counties (Fig 2). However, data reported in this
study is down to the county level to conserve anonymity of contributing vineyards. Primarily
named CIHG varieties were collected as well as a few wild vines and genetically unique breed-
ing lines.
Sample processing
Large diameter vine samples were cut and 3–5 mm3 chips excised from the margins of discol-
ored or decayed internal vascular wood tissue or from the edge of cankers. For smaller diame-
ter vine samples, the bark was peeled off and 3–5 mm thick discs were cut. Some disks were
kept whole while others cut in half or in fourths depending on diameter of the sample. Excised
chips where surface sterilized for 30 sec in an aqueous 10% sodium hypochlorite solution, fol-
lowed by two washes in sterile distilled H2O, and one wash in 70% EtOH then left to dry in a
clean air cabinet prior to plating. Between 3–5 chips per plate were then semi-embedded into 3
different culturing medias including malt extract agar (MEA; 15 g of Difco Bacto-agar, 15 g of
Difco Bacto malt extract, and 1 L of deionized water with 0.1 g streptomycin sulphate dissolved
in a small amount of 95% EtOH added post-autoclaving once cooled to 50˚C), basidiomycete
semi-selective agar (BSA; same as MEA recipe plus 2 g of Difco yeast extract and 0.06 g Aldrich
benomyl dissolved in a small amount of 95% EtOH added pre-autoclaving with 2 mL 85% lac-
tic acid added post-autoclaving once cooled to 50˚C, adapted from Worrall, 1991) [42], and
sabouraud dextrose agar (SDA; same as MEA recipe with 0.1 g Aldrich cycloheximide dis-
solved in a small amount of deionized water added post-autoclaving once cooled to 50˚C,
adapted from Harrington, 1981) [43]. Plates were left to incubate at 20–23˚C in darkness and
checked daily. Emerging fungi were transferred onto fresh MEA. All cultures were maintained
and stored in plastic bins at 20–23˚C.
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
Fig 2. Map of counties sampled. Grapevine wood samples collected from Minnesota and Wisconsin counties traced in yellow included Blue
Earth (BE), Carver (C), Crow Wing (CW), Douglas (D), Fillmore (F), Goodhue (G), Jackson (J), Kanabec (K), Lac Qui Parle (LQP), Le Sueur
(LS), Meeker (Mk), Mower (Mw), Murray (Mr), Pine (Pn), Polk (Pl), Trempealeau (T), Vernon (V), Wabasha (Wb), Walworth (Wl),
Washington (W), and Winona (Wn). Color scale indicates elevation in meters. Pink points denote locations of the University of Minnesota
(UMN) St. Paul campus and the UMN Horticultural Research Center (HRC) where the grape breeding program is located and where several
samples were collected. Map constructed in R with the public domain map collections Natural Earth (https://www.naturalearthdata.com/) and
Terrain Tiles (https://registry.opendata.aws/terrain-tiles/).
https://doi.org/10.1371/journal.pone.0269555.g002
Isolate selection
Fungal isolates for each sample were selected by culture macro-morphology on MEA and
genetic identification by sequencing the internal transcribed spacer (ITS) genomic region. The
primary macro-morphological characteristics considered included isolate color, growth rate,
hyphal branching, hyphal depth, hyphal extension, hyphal margin, fruiting, sporulation, and
metabolite staining of media. At the start of this study all unidentified cultures with unique
morphologies isolated from a single sample were selected for sequencing. Isolates were later
selected by macro-morphology in a more targeted manner as the study progressed by choosing
unique cultures or cultures similar to known pathogens we previously identified in the isolate
collection. Any isolates with questionable, non-descript, or similar culture macro-morphology
were sequenced to be sure of their identity.
DNA extraction and amplification
The DNA of select isolates was extracted using the NaOH protocol according to Osmundson
et al. (2013) [44]. Hyphae were scraped using a sterile scalpel from cultures of select isolates on
MEA that had grown out larger than 2.5 cm in diameter. Hyphal tissue was transferred to a 1.7
mL microcentrifuge tube with 300 μL of 5 mM NaOH and 3 to 5 3.5 mm glass beads. The sam-
ples where then vortexed for 1 to 5 min and centrifuged for 30 sec at 10,000 rpm. Then 5 μL of
supernatant was transferred to new tubes containing 495 μL Tris-HCL 5 mM, pH 8.0.
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
The ITS region of the isolated DNA was targeted for PCR amplification using the ITS1F/4
primer pair [45] according to Blanchette et al. (2016) [46]. Each PCR had a final volume of
25.5 μL consisting of 12.5 μL GoTaq1 Green Master Mix, 9.5 μL molecular grade water, 1 μL
of each primer at 10 μM, and 0.5 μL bovine serum albumin. The ITS locus was amplified using
a Bio-Rad T100™ Thermal Cycler following a program of 94˚C for 5 min, 35 cycles of 94˚C for
1 min, 50˚C for 1 min, and 72˚C for 1 min, followed by a final extension step of 72˚C for 5
min. Locus amplification was confirmed by gel electrophoresis of SYBR stained PCR products
prior to sequencing. Crude PCR products were Sanger sequenced by ABI 3730xl DNA
sequences, Applied Biosystems, Foster City, CA.
Molecular identification
Sequences were processed using Geneious v9.0. The processed sequences where then identified
with the basic local alignment search tool algorithm program for nucleotide sequences
(BLASTn) initially against the TrunkDiseaseID.org [47] database and also against the standard
complete NCBI GenBank. Best sequence identity match was selected for by consideration of
highest score for published data as denoted in GenBank at the time of BLASTn searches. Iden-
tity of isolates were matched to published sequences from taxonomic studies and identified to
the species level whenever possible. Isolates with greater than 97% sequences identity match
were considered homologous. Pathogenicity of identified fungal species on grapevines were
denoted according initially to TrunkDiseaseID.org [47] and then confirmed and expanded by
an assortment of grapevine pathogenicity trials found in published literature. However, most
pathogenicity trials for these fungi were conducted on traditional V. vinifera grapevine culti-
vars. Samples were scored as GTD+ upon sequence confirmation of at least one known patho-
genic species. Additional isolation and sequencing was discontinued once a sample was
designated GTD+.
Data analysis
Data were analyzed using the R statistical programming language in the RStudio integrated
development environment using an assortment of packages but most notably the collection of
Tidyverse Packages (v1.3.0) [48], the iNEXT package (v2.0.20) [49] to analyze sample coverage,
and the vcd package (v1.4–9) for multivariant analysis. The vcd package was used to explore
potential differences in isolation frequencies of genera-level taxa compared to a few variables
of interest that are descriptive of the 168 collected woody samples. In brief, Hill numbers are
used in the iNEXT package to estimate and then visualized sample completeness [50]. Addi-
tionally, diversity Pearson residuals statistics were used to analyze the measure of discrepancy
between observed and expected values within the vcd package. For each statistical comparison,
a p-value is returned from a corresponding Chi-square test and a residual shaded mosaic plot
was produced. Mosaic plots are graphs used for visualizing the comparison of multi-categori-
cal data where both the x- and y-axis are sized proportionally to the input data, i.e. the sum
area of the blocks represent 100% of the data and individual blocks are size proportionally to
the frequency with which the categories are observed.
Results
Internal symptoms of GTDs following the terminology of Mugnai et al. 1999 [16] included
brown-red wood streaking in a clearly defined wedge-shape from the cambium to pith which
is indicative of canker fungi were observed in few of our samples. Cankers more often
occurred in irregular forms and were associated with skips in the cordons (Fig 1A and 1B).
Centrally diffuse brown-red wood as well as brown to black necrotic streaking originating
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
from the pith was often associated with pruning wounds (Fig 1E–1G) and cracks (Fig 1I–1L).
All samples collected had discolored xylem to some extent and nearly completely healthy vas-
cular tissues were only observed in some cross-sections of wild riverbank grapevines in forest
and urban environments not included in this survey (Fig 1H). Cross-sections near pruning
spurs often showed discolored wood symptoms without being preceded by diffuse brown-red
wood or brown to black streaking (Fig 1E). Concentric black spotting, the result of longitudi-
nal streaking, was also frequently observed, and in some cases, black spotting would begin to
coalesce into shorter black lines (Fig 1F). Most samples had severe mottled expression of vas-
cular symptoms especially for brown-red wood streaking, brown to black necrotic streaking,
and discolored xylem (Fig 1G). Severe symptoms were sometimes associated with several
points of origin from shallow cracking from winter injury or hail damage (Fig 1J). Rarely, if
ever, have GTD foliar symptoms been observed in the NMW which possibly may be the result
of our overall young vineyards or different climate. Foliar symptoms are more often observed
in older vines under particular seasonal conditions [51, 52]. Moreover, lack of foliar symptoms
may also be the result of regular re-trunking, a common cultural practice in the NMW. It is
uncommon in the NMW for grapevine trunk wood to exceed ten years in age.
All wood samples collected had some degree of internal vascular symptoms including exter-
nally healthy samples (Fig 1). From 172 samples with various symptoms that included cankers
and vascular discoloration, dieback as well as pruning wounds and cracks from cold injury or
other environmental stresses yielded 640 isolates. These isolates represented 420 species-level
taxa unique to individual samples. Rarefication using the 420 representative taxa estimate a
sample coverage of 83% that reached to 90% by doubling the number of representative taxa
(Fig 3).
We found 32 of the 34 sampled vineyard locations, 20 of 21 counties, in this survey to have
at least one GTD+ sample. Of the 172 samples we collected, 142 (83%) had taxa reported as
pathogens associated with GTDs. Most samples were cordon sections and of the Marquette
variety (Tables 1 and 2). Most taxa are of the phylum Ascomycota (398 isolates, 94.76%) which
encompass 19 different orders, 38 genera, and potentially 89 species (Table 3).
The most frequently isolated genera obtained in this study that were known to be associated
with GTDs from previous reports included Cytospora, Phaeoacremonium, Diaporthe,
Fig 3. Rarefaction sample coverage curve. Observed sample coverage reaches 83% for the 420 sample representative
taxa. Extrapolated sample coverage reaches 90% by doubling the number of sample representative taxa.
https://doi.org/10.1371/journal.pone.0269555.g003
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
Table 1. Type of samples collected from the Northern Midwest in 2019. The majority of the 172 samples included
woody sections of cordon, trunk, root, sucker, shoots, and unknown.
Type
cordon
trunk
root
sucker
shoot
unknown
slime flux
bark
basidiocarp
Sample no.
113
32
11
5
4
3
2
1
1
Percent
66%
19%
6%
3%
2%
2%
1%
1%
1%
https://doi.org/10.1371/journal.pone.0269555.t001
Cadophora, Pestalotiopsis, Diatrypella, Diplodia, and Botryosphaeria, respectively (Fig 4). Of
these genera the most frequent species level sequence matches associated with GTDs included
Cy. viticola, Ph. fraxinopennsylvanicum, Ph. minimum, Dpr. ampelina, Cd. luteo-olivacea, Ps.
neglecta, Dt. verruciformis, Dpl. seriata, and Bt. dothidea (Table 3).
Table 2. Varieties of the 172 samples collected in the Northern Midwest in 2019.
Variety
Marquette
La Crescent
Frontenac
St. Pepin
Frontenac Blanc
Brianna
Frontenac Gris
Edelweiss
Itasca
Marechal Foch
unknown
Petite Pearl
Prairie Star
Valiant
MN1069
MN1016
Sabrevois
slime flux
St. Croix
MN43765
basidocarp
Millot
MN1005
Osceola Muscat
Riverbank Grape
Sauvignon
Virginia Creeper
Sample no.
42
28
20
Percent
24%
16%
12%
9
8
7
7
6
6
6
6
3
3
3
2
2
2
2
2
1
1
1
1
1
1
1
1
5%
5%
4%
4%
3%
3%
3%
3%
2%
2%
2%
1%
1%
1%
1%
1%
1%
1%
1%
1%
1%
1%
1%
1%
https://doi.org/10.1371/journal.pone.0269555.t002
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PLOS ONETable 3. Taxonomy, isolation frequency, and pathogenicity of fungi identified by ITS with greater than 97% homology match.
Grapevine trunk diseases of the Northern Midwest
Family (n)
Genus (n)
Isolate Host variety
Origin
GenBank
Phylum (n)
Order (n)
Ascomycota (398)
Diaporthales (98)
Valsaceae (61)
Diaporthaceae (37)
Togniniales (40)
Togniniaceae (40)
Pleosporales (99)
Didymosphaeriaceae (31)
Didymellaceae (28)
Pleosporaceae (26)
Astrosphaeriellaceae (3)
Coniothyriaceae (3)
Phaeosphaeriaceae (3)
undefined family (3)
Cucurbitariaceae (1)
Species (n) [pathogenicity studies]
Cytospora (60)
Cy. viticola (57) [53]
Cy. piceae (2)
Cy. mali (1)
GI-174
Frontenac Gris
Blue Earth, MN
OM307727
GI-847 Virginia Creeper
Carver, MN
GI-89 Marquette
Meeker, MN
OM307728
OM307729
Frontenac
Crow Wing, MN
OM307730
Frontenac Gris
Douglas, MN
OM307731
GI-31
GI-75
GI-384
GI-856
GI-413
GI-347
GI-741
GI-212
Valsa (3)
Vl. sordida (2)
Vl. salicina (1)
Diaporthe (38)
Dpr. ampelina (31) [54–56]
Dpr. eres (7) [54]
Phaeoacremonium (41)
Ph. fraxinopennsylvanicum (22) [41]
Ph. minimum (15) [3, 38]
Ph. amstelodamense (1)
Ph. angustius (1) [57]
Ph. canadense (1) [41]
Ph. hungaricum (1)
Paraconiothyrium brasiliense (30) [58, 59] GI-516
Paraphaeosphaeria sporulosa (1)
GI-157
Didymella (16)
Dd. pinodella (11)
Dd. glomerata (2)
Dd. pomorum (2)
Dd. bellidis (1)
Epicoccum (10)
Ep. nigrum (9)
Ep. sorghinum (1)
Nothophoma spiraeae (2)
Alternaria (26)
Al. alternata (19)
Al. tenuissima (5)
Al. arborescens (1)
Al. infectoria (1)
Pithomyces chartarum (3)
Coniothyrium palmicola (3)
GI-162
GI-389
GI-885
GI-879
GI-190
GI-837
GI-882
GI-878
Frontenac
Carver, MN
GI-236 Marquette
GI-422 Marquette
St. Pepin
Edelweiss
Goodhue, MN
Goodhue, MN
Douglas, MN
Goodhue, MN
La Crescent
Carver, MN
St. Pepin
Pine, MN
Osceola Muscat Wabasha, MN
Frontenac
Edelweiss
Douglas, MN
Wabasha, MN
GI-257 Marquette
GI-116 MN43765
GI-787 MN1016
Wabasha, MN
Carver, MN
Carver, MN
La Crescent
Walworth, WI
La Crescent
Carver, MN
GI-223 Marquette
Blue Earth, MN
Riverbank Grape Carver, MN
La Crescent
La Crescent
Frontenac
GI-829 Marquette
Carver, MN
Blue Earth, MN
Wabasha, MN
Blue Earth, MN
Frontenac Gris
Blue Earth, MN
La Crescent
Blue Earth, MN
OM307732
OM307733
OM307734
OM307735
OM307736
OM307737
OM307738
OM307739
OM307740
OM307741
OM307742
OM307743
OM307744
OM307745
OM307746
OM307747
OM307748
OM307749
OM307750
OM307751
OM307752
OM307753
OM307754
OM307755
OM307756
Sclerostagonospora (2)
Sc. cycadis (1)
Sc. lathyri (1)
Neosetophoma cerealis (1)
Microsphaeropsis olivacea (3) [60]
Neocucurbitaria quercina (1)
GI-141 Marquette
Meeker, MN
GI-140 Marquette
Blue Earth, MN
GI-480
Frontenac Blanc
Crow Wing, MN
OM307757
GI-505 Marquette
Lac Qui Parle, MN
OM307758
GI-37 Marquette
Meeker, MN
OM307759
(Continued )
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
9 / 25
PLOS ONEGrapevine trunk diseases of the Northern Midwest
Family (n)
Genus (n)
Isolate Host variety
Origin
GenBank
Table 3. (Continued)
Phylum (n)
Order (n)
Hypocreales (49)
Nectriaceae (29)
Bionectriaceae (17)
Hypocreaceae (2)
Xylariales (25)
Sporocadaceae (11)
Diatrypaceae (9)
Hypoxylaceae (2)
Apiosporaceae (1)
Xylariaceae (2)
Helotiales (21)
undefined family (18)
Dermateaceae (1)
Porodiplodiaceae (1)
Sclerotiniaceae (1)
Dothideales (14)
Saccotheciaceae (14)
Botryosphaeriales (10)
Botryosphaeriaceae (10)
Species (n) [pathogenicity studies]
Fusarium (26)
Fs. acuminatum (5)
Fs. equiseti (3)
Fs. solani (3)
Fs. culmorum (1)
Ilyonectria liriodendri (1) [61–63]
Scolecofusarium ciliatum (1)
Thyronectria austroamericana (1)
Clonostachys (18)
Cln. rosea (16) [60]
Cln. byssicola (1)
Trichoderma (2)
Trc. atroviride (1)
Trc. deliquescens (1)
Pestalotiopsis (10)
Ps. neglecta (6)
Ps. uvicola (2) [38, 56]
Ps. brassicae (1)
Ps. chamaeropis (1)
Neopestalotiopsis mesopotamica (1)
Seimatosporium lichenicola (1)
Seiridium rosarum (1)
Diatrypella
Dt. verruciformis (8) [64, 65]
Dt. pulvinata (1)
Diatrype stigma (1) [65]
Hypomontagnella submonticulosa (1)
Hypoxylon invadens (1)
Arthrinium arundinis (1)
Rosellinia corticium (1)
Cadophora (16)
Cd. luteo-olivacea (13) [41, 66–68]
Cd. melinii (2) [68]
Cd. ferruginea (1)
Discohainesia oenotherae (1)
Porodiplodia vitis (1)
Botrytis cinerea (1)
Aureobasidium pullulans (14)
Diplodia (7)
Dpl. seriata (6) [38, 56, 58, 64, 69]
Dpl. corticola (1) [38, 56]
Botryosphaeria dothidea (2) [38, 56, 70]
Phaeobotryon negundinis (1)
GI-820
Frontenac
GI-95 MN1005
Fillmore, MN
Carver, MN
OM307760
OM307761
GI-376
Frontenac
Crow Wing, MN
OM307762
GI-151
La Crescent
Carver, MN
GI-322 Marechal Foch
Goodhue, MN
GI-149
La Crescent
GI-796
slime flux
Carver, MN
Carver, MN
OM307763
OM307764
OM307765
OM307766
GI-870
La Crescent
Polk, MN
OM307767
GI-874 Marquette
Trempealeau, WI
OM307768
GI-795
slime flux
Carver, MN
GI-351
Frontenac Blanc
Fillmore, MN
OM307769
OM307770
GI-491
Edelweiss
Trempealeau, WI
OM307771
GI-738
Edelweiss
Trempealeau, WI
OM307772
GI-403 Marquette
Lac Qui Parle, MN
OM307773
GI-231
St. Pepin
Goodhue, MN
GI-220
Frontenac Gris
Blue Earth, MN
GI-99 Marquette
GI-352
La Crescent
Carver, MN
Murray, MN
OM307774
OM307775
OM307776
OM307777
GI-464 Marquette
GI-416 Valiant
GI-895 Valiant
Carver, MN
Douglas, MN
OM307778
OM307779
Crow Wing, MN
OM307780
GI-817
Frontenac Blanc
Blue Earth, MN
GI-350
La Crescent
Blue Earth, MN
GI-70
GI-62
Frontenac
St. Croix
Carver, MN
Wabasha, MN
GI-370
La Crescent
Mower, MN
GI-316 Marechal Foch
Goodhue, MN
GI-328
La Crescent
Goodhue, MN
GI-442
Frontenac Gris
Winona, MN
GI-269
Frontenac
Blue Earth, MN
GI-386
Frontenac
Walworth, WI
GI-886
La Crescent
Blue Earth, MN
OM307781
OM307782
OM307783
OM307784
OM307785
OM307786
OM307787
OM307788
OM307789
OM307790
OM307791
GI-408
La Crescent
Blue Earth, MN
OM307792
GI-373
Petite Pearl
Crow Wing, MN
OM307793
GI-225 Marquette
Blue Earth, MN
GI-131 MN1005
Carver, MN
OM307794
OM307795
(Continued )
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
10 / 25
PLOS ONETable 3. (Continued)
Phylum (n)
Order (n)
Family (n)
Genus (n)
Isolate Host variety
Origin
GenBank
Species (n) [pathogenicity studies]
Grapevine trunk diseases of the Northern Midwest
Cladosporiales (11)
Cladosporiaceae (11)
Eurotiales (8)
Aspergillaceae (4)
Trichocomaceae (4)
Sordariales (6)
Chaetomiaceae (4)
Sordariaceae (1)
Trichosphaeriales (3)
Trichosphaeriaceae (3)
Chaetomellales (1)
Chaetomellaceae (1)
Chaetothyriales (1)
Herpotrichiellaceae (1)
Coniochaetales (1)
Coniochaetaceae (1)
Glomerellales (1)
Glomerellaceae (1)
Saccharomycetales (1) Dipodascaceae (1)
Thelebolales (1)
Thelebolaceae (1)
Valsariales (1)
Valsariaceae (1)
Basidiomycota (15)
Polyporales (9)
Phanerochaetaceae (3)
Irpicaceae (2)
Polyporaceae (2)
Cerrenaceae (1)
Meruliaceae (1)
Russulales (2)
Peniophoraceae (1)
Stereaceae (1)
Agaricales (2)
Physalacriaceae (1)
Schizophyllaceae (1)
Hymenochaetales (1)
Hymenochaetaceae (1)
Cystofilobasidales (1) Mrakiaceae (1)
Mucoromycota (7)
Mucorales (7)
Mucoraceae (7)
Cladosporium (11)
Cld. cladosporioides (9)
Cld. anthropophilum (1)
Cld. westerdijkiae (1)
Talaromyces amestolkiae (4)
Penicillium (5)
Pn. pulvillorum (2)
Pn. raistrickii (1)
Pn. simplicissimum (1)
Pn. sumatraense (1)
Ovatospora (3)
Ov. brasiliensis (2)
Ov. mollicella (1)
Chaetomium concavisporum (1)
Sordaria fimicola (1)
Nigrospora oryzae (3)
Chaetomella raphigera (1)
Rhinocladiella quercus (1)
Coniochaeta velutina (1)
Colletotrichum acutatum (1)
Geotrichum candidum (1)
Thelebolus microsporus (1)
Valsaria spartii (1)
Bjerkandera adusta (2)
Hyphodermella rosae (1)
Irpex lacteus (2)
Trametes versicolor (2)
Cerrena unicolor (1)
Phlebia radiata (1)
Peniophora cinerea (1)
Stereum complicatum (1)
Cylindrobasidium laeve (1)
Chondrostereum purpureum (1)
Phellinus conchatus (1)
Tausonia pullulans (1)
Mucor (7)
Mucr. circinelloides (6)
Mucr. moelleri (1)
GI-866 Marquette
GI-209 Marquette
GI-194 Marquette
GI-801 Vitis spp.
Blue Earth, MN
Blue Earth, MN
Blue Earth, MN
Carver, MN
GI-337 Marquette
Blue Earth, MN
GI-309
St. Pepin
Goodhue, MN
GI-210 Marquette
Blue Earth, MN
GI-36 Marquette
Meeker, MN
GI-828 Marquette
Blue Earth, MN
GI-881
La Crescent
Blue Earth, MN
GI-865 Marquette
Blue Earth, MN
GI-848 Virginia Creeper
Carver, MN
GI-846
Edelweiss
GI-217 Marquette
Winona, MN
Goodhue, MN
GI-486 Marquette
Blue Earth, MN
GI-472
Brianna
GI-287
La Crescent
GI-164
Edelweiss
Winona, MN
Goodhue, MN
Goodhue, MN
GI-88
Frontenac Blanc
Pine, MN
GI-43 Marquette
Meeker, MN
OM307796
OM307797
OM307798
OM307799
OM307800
OM307801
OM307802
OM307803
OM307804
OM307805
OM307806
OM307807
OM307808
OM307809
OM307810
OM307811
OM307812
OM307813
OM307814
OM307815
GI-417 Marquette
Trempealeau, WI
OM307816
GI-823
Frontenac
GI-806 Vitis spp.
GI-68
La Crescent
GI-198
Prairie Star
GI-798 Vitis spp.
GI-342
La Crescent
GI-200 Marquette
GI-263
Itasca
GI-444
Itasca
GI-805 Vitis spp.
slime flux
GI-61
Fillmore, MN
Carver, MN
Wabasha, MN
Carver, MN
Carver, MN
Blue Earth, MN
Goodhue, MN
Wabasha, MN
Le Sueur, MN
Carver, MN
Carver, MN
OM307817
OM307818
OM307819
OM307820
OM307821
OM307822
OM307823
OM307824
OM307825
OM307826
OM307827
GI-71
La Crescent
GI-365 Marquette
Vernon, WI
Mower, MN
OM307828
OM307829
Taxonomic rankings from order to species are denoted followed by isolation frequency in parenthesis. The isolation frequency is the count of samples each taxa was
isolated from a possible 172 samples. Representative isolates deposited to GenBank are listed for each species along with the sample variety and county origin of that
isolate. Pathogenicity studies conducted for each species are listed in brackets following species. See references for complete citations. Highlighted species have
associated pathogenicity studies. Highlighted isolates pictured in Fig 4.
https://doi.org/10.1371/journal.pone.0269555.t003
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
11 / 25
PLOS ONEGrapevine trunk diseases of the Northern Midwest
Fig 4. Fungal genera isolated from more than one grapevine sample. Individual culture image areas are relatively proportional to the number of samples
each fungal genus was isolated from. All pictured fungal isolates grown on MEA. Cytospora (Cy = 60, GI-174, 80 dpi); Phaeoacremonium (Ph = 41, GI-422, 94
dpi); Diaporthe (Dpr = 38, GI-449, 47 dpi); Paraconiothyrium (Pr = 30, GI-516, 47 dpi); Alternaria (Al = 27, GI-879, 36 dpi); Fusarium (Fs = 27, GI-151, 17 dpi);
Clonostachys (Cln = 18, GI-870, 27 dpi); Cadophora (Cd = 16, GI-370, 94 dpi); Didymella (Dd = 16, GI-257, 21 dpi); Aureobasidium (Ar = 14, GI-886, 21 dpi);
Cladosporium (Cld = 11, GI-866, 21 dpi); Epicoccum (Ep = 10, GI-837, 19 dpi); Pestalotiopsis (Ps = 10, GI-491, 40 dpi); Diatrypella (Dt = 9, GI-464, 15 dpi);
Diplodia (Dpl = 7, GI-408, 20 dpi); Mucor (Mucr = 7, GI-71, 20 dpi); Talaromyces (Tl = 6, GI-801, 55 dpi); Penicillium (Pn = 5, GI-337, 14 dpi); Coniothyrium
(Cn = 3, GI-882, 21 dpi); Microsphaeropsis (Mcrs = 3, GI-505, 20 dpi); Nigrospora (Ng = 3, GI-846, 14 dpi); Ovatospora (Ov = 3, GI-828, 19 dpi); Pithomyces
(Pt = 3, GI-162, 28 dpi); Valsa (Vl = 3, GI-384, 35 dpi); Bjerkandera (Bj = 2, GI-417, 28 dpi); Botryosphaeria (Bt = 2, GI-225, 35 dpi); Irpex (Ir = 2, GI-806, 55
dpi); Nothophoma (Nt = 2, GI-878, 31 dpi); Sclerostagonospora (Sc = 2, GI-140, 17 dpi); Trametes (Trm = 2, GI-68, 9 dpi); and Trichoderma (Trc = 2, GI-795, 14
dpi).
https://doi.org/10.1371/journal.pone.0269555.g004
There were 15 taxa of Basidiomycota (3.57%) which encompass 5 orders, 11 genera, and 12
species. Bjerkandera adusta, Irpex lacteus, and Trametes versicolor where the most frequently
identified Basidiomycota isolated. These fungi were present in 5 samples but were found in
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
counties not adjacent to one another. Very few taxa of Mucoromycota (7 isolates, 1.68%) were
identified. Mucor circinelloides, not considered associated with GTD, was isolated from 6 sam-
ples which originated from different vineyards in nonadjacent counties.
There were no significant differences in isolation frequencies of genera based on sample
berry color (S1 Fig). There is some indication of significant isolation frequency differences of
genera by sample variety (S2 Fig) or sample county origin (S3 Fig). For most genera not
enough sample representative taxa were obtained to be sure these isolation frequency differ-
ences between counties are truly significant. However, Cadophora obtained in this study nota-
bly had significant differences in isolation frequency between sample section types with a p-
value of 0.013. Cadophora spp. were less often isolated from cordons with a Pearson residual of
-2.9 and more frequently isolated from root, trunk, and sucker sections with Pearson residuals
between 2.2 to 3.9 (S4 Fig).
Discussion
The vast majority of the fungal taxa isolated in this study are of the phylum Ascomycota, sev-
eral of which are considered pathogenic to grapevines (references cited in Table 3). Cytospora
spp. and Diaporthe spp. of the order Diaporthales as well as Phaeoacremonium spp. make up
the largest majority of isolates identified and are known to be pathogenic on grapevines. Fre-
quent species identification of Phaeoacremonium in this study aligns similarly with most other
GTD surveys. However, the other major results confirm our first hypothesis that the composi-
tion of GTDs for the NMW is different in comparison to most other studied grape growing
regions. These fungi in the Diaporthales typically are considered a minor or secondary group
of causal agents in other regions were GTD surveys were completed [55, 71–74] but in the
study presented here they are the most commonly found GTD fungi in the NMW. The GTD
species genera of Diaporthe was previously named Phomopsis by some other investigators [55,
75]. Species of Cytospora have been reported previously as prevalent in cold climate regions
[74] and areas of high humidity [32].
The etiology of these Diaporthales pathogens on grapevines has been previously well char-
acterized [76]. In addition to symptoms of internal wood discoloration, pathogenic species of
Cytospora and Diaporthe can induce symptoms of cane bleaching (Fig 1C). They also produce
asexual fruiting bodies known as pycnidia which can be found on all affected tissues (Figs 1B,
1C and 4). On succulent green tissue, pycnidia may be surrounded by a halo or half halo of
chlorotic tissues or may reside hidden just under the bark of infected vines. Conidio-spores
that ooze out from pycnidia serve as a major source of inocula that can re-infect the same host
or infect other nearby hosts. Conidia are most often disseminated by rain or irrigation splash
but also by contaminated tools and more rarely by wind alone. These species overwinter in col-
onized wood of canes, spurs, pruning debris, and dormant buds [77]. However, symptoms
appear to differ from locations of sample collection and isolation particularly for Diaporthe
spp. [11, 55, 78, 79]. Symptom differences may be explained by genetic differences of local fun-
gal populations due to the result of horizontal gene transfer of transposable elements for the
acquisition or loss of pathogenicity [80, 81]. However, horizontal gene transfer has never been
studied in fungal GTD pathogens. Many of the Diaporthales are assumed opportunistic patho-
gens, causing disease only in stressed or weakened hosts or may live endophytically without
causing disease [82]. Since these fungi can colonize wounds, the prevalence of these fungi
found may be a result of wounds caused by cold injury.
In January of 2019, an atypical polar vortex occurred in the NMW. In Minnesota on Janu-
ary 30, 2019, the temperature dropped to -33˚C (-48˚C with wind chill) for the Minneapolis-
St. Paul area while the lowest temperature recorded in the state was -39˚C (-53˚C with wind
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
13 / 25
PLOS ONEGrapevine trunk diseases of the Northern Midwest
chill) [83]. The polar vortex temperatures were well below the lowest ratings for most of the
CHIG varieties in many counties. Winter injury was most apparent on Marquette variety
grapevines and in vineyards with little wind protection. Exposure of grapevines to these
extreme weather conditions resulted in frost cracks of woody tissues and damage to dormant
buds. However, winter injury of grapevines more typically occurs by means of sun exposure.
Injury occurs when both direct and snow reflected sunlight warms trunks to above freezing
during the day followed by a rapid decrease in temperature to below freezing at night. The sud-
den drop in temperature ruptures just the outer most layer of phloem cells for mild cases while
more serious cases kill cambial cells and damage xylem tissues. When this occurs on trees in
the NMW it is often referred to as sunscald. On grapevines this could be considered “winter
sunscald”, not to be confused with sunscald of grape berries in the summer. Like extreme cold
weather exposure, winter sunscald can also result in both shallow and deep frost cracks
depending on severity (Fig 1I–1L). Additionally, winter sunscald of grapevines results in a
blackened appearance of the bark on the south to southwest facing side of the vine (Fig 1L). In
either case of winter injury often the roots and the lower trunk of vines are protected by the
insulating snow covering. Thus, trunk replacement by sucker is a viable and common manage-
ment strategy in the NMW [84]. Regardless, associated observations of winter injury, vascular
discoloration, and identification of fungi suggests our second hypothesis is true and that the
polar vortex likely predisposed grapevines to these opportunistic canker pathogens.
Wounds, perhaps from winter injury or mechanical pruning, serve as portals for infection
by GTD pathogens under conducive weather conditions such as cool spring or fall rains [32,
85–87]. Fungal spores then colonize and spread through the vascular tissue either by hyphal
growth or additional sporulation. Many canker pathogens secrete cell wall degrading enzymes
or other compounds to spread laterally through xylem tissues eventually circumnavigating and
killing the entire cambium. However, the grapevine host produces tyloses, gels, phenolics, and
suberin to compartmentalize the damaged tissues and invading microorganisms [88]. How-
ever, restricted balanced production of these defensive structures and compounds is essential.
Overproduction of occlusions in response to pathogenic infections can lead to extensive
hydraulic failure resulting in external foliar symptoms and often vine death [89, 90]. In cross
sections the defense response of the grapevine host is seen as a continuum of brown-red wood
to brown-black necrotic tissue (Fig 1). Lighter vascular discoloration indicates more recent
responding tissues and likely the front of pathogen spread. Darker vascular discoloration indi-
cates long responding tissues and the probable point of pathogen entry [91]. Alternatively, pri-
marily pectinolytic active pathogens degrade gels in xylem vessels and spread longitudinally by
spores through the small spaces between tyloses partially occluding xylem conduits [92]. Lon-
gitudinal spread of these pathogens is seen in cross section by the host defense response as
black spotting and black lines (Fig 1F) [16]. Genomes of Cytospora spp. and Diaporthe spp.
reveal these fungi employ an abundance of cell wall degrading enzymes [93, 94].
Xylem vessel anatomy likely influences host resistance, pathogen spread, and environmen-
tal resilience. In the Dutch elm disease pathosystem, smaller diameter xylem vessels appeared
to confer some level of resistance to the causal fungal agents Ophiostoma ulmi and O. novo-
ulmi [95]. Reduced vessel diameter permits a more energetically conserved faster occlusion of
tissues adjacent to damaged or infected xylem tissues. Pouzoulet et al. (2014; 2017; 2020) con-
ducted histological and pathogenicity studies comparing a few V. vinifera grapevine cultivars
that had varying susceptibility to GTDs and showed cultivars with smaller diameter xylem ves-
sels may likely confer some resistance [88, 96, 97]. Unfortunately, histological pathogenicity
studies of grapevines against vascular pathogens are few and completely lacking for hybrid
varieties. However, hybrid varieties as well as traditional cultivars have been studied and show
links between vessel anatomy and environmental resilience against freezing and drought
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
conditions, though more research is needed [98, 99]. Interestingly, developmental histological
studies of grapevine xylem tissues have shown plasticity of vessel diameter even within a vari-
ety or individual based on early season precipitation [100]. Therefore, abundant early irriga-
tion influence vines to develop larger xylem vessels that can allow for vigorously growing
higher yielding grapevines but may also render vines more susceptible to biotic vascular patho-
gens and abiotic environmental stresses. Moreover, environmental stresses, including extreme
weather events, will be more frequent due to climate change which may provide more oppor-
tunities for some vascular pathogens [101]. However, the effects of climate change are likely
dependent on the pathogens, cultivars, and environments in question. For example, intensive
drought conditions have shown both positive [102] or negative [103] effects for grapevines suf-
fering from GTDs.
Species of Phaeoacremonium are found in many grape growing countries and often associ-
ated with GTDs of young vines. Phaeoacremonium spp. are often found to spread through
wounds, nursery propagation and grafting [104–112], see review by Gramaje et al. (2015) [40].
Ph. fraxinopennsylvanicum is widespread throughout the world on other hosts and has been
found in many other investigations in the Midwestern United States [113] but Ph. minimum
appears to be the most widespread Phaeoacremonium spp. throughout grape growing
countries.
Cd. luteo-olivacea has been isolated from many substrates including soils [114], decaying
wood [115–117], and grapevines [68] as well as from various grafting tools [118] and pruning
shears [119]. Cd. luteo-olivacea is often referred to as a weak pathogen and this fungus was not
recognized as pathogenic on grapevine until extended grapevine inoculation studies were con-
ducted (see Table 3). Interestingly, Cadophora was the only genus in this study that showed
some differences in isolation frequency in comparison with four tested criteria of hypothesis
three. No significant differences were observed for any fungal genera isolated compared to
variety berry color (S1 Fig). Some researchers have indicated suspicions that red cultivars are
more susceptible to GTD pathogens, although much more research is needed [120]. Some sig-
nificant differences were observed for a few genera compared to sample variety (S2 Fig) or
sample county origin (S3 Fig). However, the residuals were only slight for the variety and
county origin comparisons and more research is needed to be sure of these correlations. Yet,
Cadophora spp. were found to be significantly less isolated from cordon sample sections and
significantly more isolated from woody sections of trunk, roots, and suckers (S4 Fig).
Increased isolation of Cadophora spp. from the more central main trunk of the vine may be an
indication that infection occurs from the soil or possibly the infection was acquired prior to
planting. Additional research of vineyard soils and nursery stock materials would better eluci-
date the origin of Cadophora spp. in NMW grapevines. Additionally, Ilyonectria liriodendri,
isolated just once in this study, is another weak pathogen often associated with GTDs of roots
and often found in nurseries [121, 122].
Fungi considered nonpathogenic to grapevines according to TrunkDiseaseID.org [47]
included Penicillium, Alternaria, Didymella, Epicoccum, and Paraconiothyrium which were
some of the more frequently isolated genera in this study. However, few GTD pathogenicity
studies have tested Pleosporales fungi. Paraconiothyrium spp. have been demonstrated to be
pathogenic on fruit trees and other woody species [105] and potentially pathogenic on grape-
vines [59]. In the NMW, Paraconiothyrium spp. could be a potential pathogen. This fungus
was recently found associated with the emerald ash borer and found to cause small cankers on
healthy ash trees [113, 123]. Further investigation of the pathogenesis of Pleosporales may
prove interesting considering the persistence in isolation and sequencing of these fungi.
Basidiomycota have been also found to play a role in GTDs [124–126]. Often the presence
of these wood decay fungi are found mainly in older vines following the colonization of faster
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
growing host detoxifying pioneering ascomycota [16]. In many parts of the grape growing
regions of the world, the primary Basidiomycota associated with GTDs are Fomitporia medi-
terriana [127] and Stereum hirsutum [128]. However, in our study no species of Fomitporia
were isolated but a different species of Stereum was one of the more frequently isolated Basi-
diomycota. Additionally, Trametes versicolor and Cerrena unicolor were also isolated. These
fungi are commonly found on forest and shade trees locally (personal observations). Fruiting
bodies of these fungi have been found on trunks of grapevines that had advanced stages of
GTD symptoms. These Basidiomycota have not been tested for pathogenicity on grapevines
but Trametes versicolor causes cankers and decay on fruit trees [129] and Cerrena unicolor is
well characterized on hardwoods where it is an aggressive canker rot pathogen [130].
GTD fungi in the Xylariales, Botryosphaeriales, and Phaeomoniellales are of concern in
many grape growing countries and this includes fungi in the families Diatrypaceae, Botryo-
sphaeriaceae, and Phaeomoniellaceae [73]. In our study, only 10 Diatrypaceae, and 10 Botryo-
sphaeriaceae isolates were identified. No Phaeomoniellaceae isolates were identified. No
species of Eutypella or Eutypa (both Diatrypaceae), common in some other grape growing
regions, were isolated. However, a few isolates not included in analysis closely matched with
Eutypa but with less than 97% and may prove to be new species following additional detailed
taxonomic studies (See S1 Table). Pestalotiopsis spp., Neopestalotiopsis spp., Diatrypella verru-
ciformis, and Diatrype stigma of the Xylariales as well as Diplodia seriata, Botryosphaeria dothi-
dea, Diplodia corticola, and Phaeobotryon negundinis of the Botryosphaeriales represented a
minority of the GTD pathogens isolated in our study (Table 3).
At the start of our research project, many grape growers expressed concerns about GTDs in
their young vineyards. There was also considerable concern about Botryosphaeriaceae GTD
often called “Bot-rot” or otherwise known as Bot canker. Grape growers in the NMW regularly
associate any wedge-shaped discoloration of cross-sections of grapevines as Bot-rot. Based on
this survey, Botryosphaeriaceae GTD is rare in the NMW. Confusion and concerns of growers,
viticultural professionals, and even fellow researchers is understandable given the complexity
of GTDs in addition to the many various names used in an attempt to sub-categorize GTDs.
Many of these sub-categorized GTDs have been associated with irregular generalized symp-
toms of grapevines influenced by the cultivar or variety, climate, and environmental condi-
tions [32, 118, 131]. Moreover, many GTD designations rapidly become obsolete with each
taxonomic recategorization of fungal species. Fungal taxonomy will likely continue to change
as more genetic information is gathered into databases and mycologist strive to dissolve the
two-name system for fungi [132].
The isolation frequency differences of these typically important GTD groups in other grape
growing regions is especially notable. Such differences could possibly be correlated with the
different climate of the NMW as compared to the many other grape growing regions which
typically have more seasonally mild, often Mediterranean climates. Several spore trapping
studies from various countries have attempted to characterize sporulation events of various
GTD pathogens in correlation with varying weather measurements [87, 133–135]. Given the
drastically different GTDs composition of the NMW, additional studies using spore trapping
would prove insightful to obtain a better understanding of the GTD pathogens in the NMW.
Notably, culturing methods may present bias as some faster growing fungal species such as
those of Cytospora, Diaporthe, Diplodia, and Botryosphaeria may outgrow slower growing spe-
cies such as those of Phaeoacremonium, Phaeomoniella, and many basidiomycota. This bias of
culture-based studies would benefit being paired with modern metagenomic techniques to
characterize all potential microorganismal species present in a substrate. However, many
metagenomic techniques also present bias such as detection of non-viable organisms or unin-
tended preferential over-identification. Thus, metagenomic techniques also benefit being
PLOS ONE | https://doi.org/10.1371/journal.pone.0269555 June 3, 2022
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
paired with classical culture-based techniques. Additionally, inclusion of culture-based meth-
ods allows for the curation of live microbial collections for use in future pathogenicity or char-
acterization studies. Therefore, future studies which use both classical culturing and
metagenomic techniques would better elucidate the NMW GTD complex. This combination
of classical and modern techniques has been demonstrated effective in recent local studies of
Heterobasidion Root Rot [136]. Regardless, in the study we present here the sample coverage
curve (Fig 3) was observed to have reached a plateau providing confidence all major fungal
species were identified in this study. Moreover, the use of three types of media allowed for fre-
quent isolation of slow growing fungal species such as those of Phaeoacremonium as well as
infrequent isolation of fast growing fungal species such as those of the Botryosphaeriales.
Therefore, confidence is assured that the isolation frequency of these fungi identified is repre-
sentative for grapevines of the NMW.
In this study we revealed a large diversity of fungal species associated with cold-hardy
hybrid grapevines in the NMW. A handful of these isolates (those with less than 97% sequence
match provided in S1 Table) could potentially be revealed as new species following additional
detailed taxonomic studies. However, the majority of fungal species we identified show Dia-
porthales predominate GTDs in the NMW. Diaporthales GTD species, Cytospora and Dia-
porthe, are generally opportunistic fungi and largely spread to new hosts within short distances
by asexual conidia via rain splash or contaminated tools. Basic understanding of these oppor-
tunistic pathogens lifecycles emphasizes the benefit growers would gain from more intentional
phytosanitary practices such as prompt removal and destruction of pruning debris as well as
the regular sanitization of tools. Pruning debris and diseased canes left unpruned have recently
been shown to be a major source of Diaporthe GTD Inoculum [135]. Our current recommen-
dation for grape growers in the NMW is to prune in the dormant winter season during a
period of cold and dry weather. Recommendations on pruning timing could be fine-tuned by
epidemiological spore trapping studies in NMW vineyards and may possibly allow for some
degree of GTDs forecasting. Vineyard spore trapping could also provide the opportunity for
broader biosurveillance of invasive pathogenic microbial species of forest, shade, and orchard
trees.
Knowing the prevalence of GTDs in the NMW provides insight for the development of
improved management practices. Similar studies of GTD pathogens spread from nurseries of
cold-hardy grapevine hybrid varieties would also provide insight to improved propagation
practices as well as yield less stressed, higher quality, and more vigorous growing nursery stock
plants for growers. Assessment of these hybrid varieties against a panel of GTD pathogens may
reveal novel evidence of resistance or susceptibility that would be useful for grape breeders.
The development of cost-effective rapid molecular assays for the most prevalent GTDs in the
NMW would be a useful tool to measure the effectiveness of practices or the variability of vari-
ety susceptibility to GTDs.
Supporting information
S1 Table. Isolates with less than 97% homology match. Taxonomic rankings from order to
species are denoted followed by isolation frequency in parenthesis. The isolation frequency is
the count of samples each taxa was isolated from a possible 172 samples. Isolates deposited to
GenBank are listed for each species along with the sample variety and county origin of that iso-
late. Pathogenicity studies conducted for each species are listed in brackets following species.
See references for complete citations. Highlighted species have associated pathogenicity stud-
ies.
(DOCX)
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PLOS ONEGrapevine trunk diseases of the Northern Midwest
S1 Fig. Mosaic plot of genus level taxa isolated from sample varieties.
(TIF)
S2 Fig. Mosaic plot of genus level taxa isolated from sample variety berry color.
(TIF)
S3 Fig. Mosaic plot of genus level taxa isolated from sample section types.
(TIF)
S4 Fig. Mosaic plot of genus level taxa isolated from counties.
(TIF)
Acknowledgments
We thank Owen Geier and Brian Prior for technical support and the staff and management of
all the contributing Northern Midwestern vineyards that provided samples for this study.
Author Contributions
Conceptualization: David H. DeKrey.
Data curation: David H. DeKrey.
Formal analysis: David H. DeKrey.
Funding acquisition: Matthew D. Clark.
Investigation: David H. DeKrey.
Methodology: David H. DeKrey.
Project administration: David H. DeKrey.
Resources: David H. DeKrey, Robert A. Blanchette.
Software: David H. DeKrey.
Supervision: Matthew D. Clark, Robert A. Blanchette.
Validation: David H. DeKrey.
Visualization: David H. DeKrey.
Writing – original draft: David H. DeKrey.
Writing – review & editing: David H. DeKrey, Annie E. Klodd, Matthew D. Clark, Robert A.
Blanchette.
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PLOS ONE
| null |
10.1038/s41467-022-29297-2
|
Data availability
The microbial growth data generated in this study are provided in the Supplementary
Table S2.
Code availability
The model code is deposited on GitHub (https://github.com/LevineLab/POMmodel) and
citable using https://doi.org/10.5281/zenodo.6015020.
|
Data availability The microbial growth data generated in this study are provided in the Supplementary Table S2 . Code availability The model code is deposited on GitHub ( https://github.com/LevineLab/POMmodel ) and citable using https://doi.org/10.5281/zenodo.6015020 .
|
ARTICLE
https://doi.org/10.1038/s41467-022-29297-2
OPEN
Microbes contribute to setting the ocean carbon
flux by altering the fate of sinking particulates
Trang T. H. Nguyen
Kapil Amarnath
Otto X. Cordero
3, Uria Alcolombri
2 & Naomi M. Levine
1✉
1, Emily J. Zakem1, Ali Ebrahimi
2, Julia Schwartzman
2, Tolga Caglar3,
4, François J. Peaudecerf
4, Terence Hwa
3, Roman Stocker
4,
;
,
:
)
(
0
9
8
7
6
5
4
3
2
1
Sinking particulate organic carbon out of the surface ocean sequesters carbon on decadal to
millennial timescales. Predicting the particulate carbon flux is therefore critical for under-
standing both global carbon cycling and the future climate. Microbes play a crucial role in
particulate organic carbon degradation, but
the impact of depth-dependent microbial
dynamics on ocean-scale particulate carbon fluxes is poorly understood. Here we scale-up
essential features of particle-associated microbial dynamics to understand the large-scale
vertical carbon flux in the ocean. Our model provides mechanistic insight into the microbial
contribution to the particulate organic carbon flux profile. We show that the enhanced
transfer of carbon to depth can result from populations struggling to establish colonies on
sinking particles due to diffusive nutrient loss, cell detachment, and mortality. These
dynamics are controlled by the interaction between multiple biotic and abiotic factors.
Accurately capturing particle-microbe interactions is essential for predicting variability in
large-scale carbon cycling.
1 Department of Biological Sciences, University of Southern California, Los Angeles, CA 90089, USA. 2 Ralph M. Parsons Laboratory for Environmental
Science and Engineering, Department of Civil and Environmental Engineering, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
3 Department of Physics, University of California at San Diego, La Jolla, CA 92093, USA. 4 Institute of Environmental Engineering, Department of Civil,
Environmental and Geomatic Engineering, ETH Zurich, 8093 Zurich, Switzerland.
email: [email protected]
✉
NATURE COMMUNICATIONS |
(2022) 13:1657 | https://doi.org/10.1038/s41467-022-29297-2 | www.nature.com/naturecommunications
1
ARTICLE
NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-022-29297-2
The vertical flux of particulate organic carbon (POC) in the
ocean has been the subject of numerous field campaigns,
laboratory experiments, and modeling studies over the past
four decadese.g.,1–25. Ultimately,
the vertical flux of POC is
determined by the rate of POC production in the surface ocean
where de novo particle production takes place, the sinking speed
of particles, and the rate of POC consumption in the subsurface
ocean. Previous carbon cycle modeling studies aimed at under-
standing basin-scale fluxes out of the upper ocean have focused
primarily on physical and chemical processes5,7,8,26 and have
shown that differences in particle size spectra5,9,16,17, lability6,
and temperature8,27 play important roles in determining the
efficiency of POC transfer, consistent with observations4,28,29.
However, these large-scale models have not explicitly included
microbial ecological dynamics. This is problematic as many of the
aforementioned physical and chemical mechanisms shown to
impact the vertical flux of POC are controlled by microbial and
grazer dynamics22–25,30. For example, lability as represented by
these models is inherently related to microbial activity (as we
demonstrate below). Even the size of particles and thus their
sinking speed is strongly influenced by the rate of degradation by
microbes and consumption by zooplankton31–33.
Organisms alter the POC flux through a variety of processes.
Heterotrophic microbes directly consume organic carbon
within particles with an estimated contribution of 70-92% of
POC remineralization25. Grazers such as zooplankton con-
tribute to the aggregation, disaggregation, and consumption of
particles23,25,30,34–40 with small particles (0.7-53 μm) acting as
a primary food source for zooplankton in the mesopelagic ocean
through flux feeding36. However, rather than explicitly capturing
these dynamics, current biogeochemical models rely on low and
invariant rates of POC consumption (typically using bulk remi-
neralization terms) tuned in order to match observed POC flux
profiles5,6,8. Here we focus on the mechanisms behind the per-
sistence of particulate organic carbon in the deep ocean and the
role that heterotrophic microbes play in decreasing the vertical
flux of particulate carbon out of the surface ocean. Additional
work is needed to understand the coupled impact of microbial and
grazer dynamics on the POC flux and the relative contribution of
these processes to the shape of the POC flux profile (see Discus-
sion below).
Particle-associated heterotrophic microbial communities are
incredibly dynamic41–44 and able to achieve relatively rapid growth
rates (order of 1 to 10 day −1)32,42,43,45,46 even on seemingly
‘recalcitrant’ organic carbon compounds41,44. As a result, microbes
are capable of consuming particles on the timescales of days32,41–44.
This contrasts with observations of ‘labile’ particles in the bath-
ypelagic and epibenthic zones21,47. Previous work suggests that
temperature and pressure limitation on microbial activity might
allow for the persistence of particles in the deep ocean16,48–50. In
addition, microbial dynamics such as enzyme production, attach-
ment, detachment, and mortality have been shown to play a key
role in the rate of POC degradation31,41–43,46,51–53. Laboratory
studies suggests that, for successful colonization of a particle to
occur, particle-associated microbes must surpass a critical popula-
tion size46,54. This critical population size or density of cells (cells
per surface area) is necessary for countering the diffusive losses of
both extracellular enzymes that are used to break down polymers
(the main component of POC) and the resulting low-molecular-
weight degradation products42,46,54–56. These micro-scale observa-
tions suggest that the rate of POC consumption in the ocean is
highly variable and can vary as a function of microbial processes, in
contrast
representation in carbon cycle
models45,46,53,57,58. Therefore, to mechanistically understand the
vertical flux of carbon in the ocean and generate robust predictions
of future changes, we must account for particle-associated microbial
to the conventional
behavior22,24,59, in addition to other dynamics such as particle size
distribution and zooplankton activity.
is
Here we present a water-column model
that explicitly
accounts for micro-scale observations, reconciles rapid microbial
growth rates with slow POC remineralization timescales (order
of 10−3 to 10−1 day−1) in the upper ocean (<2,500 m)3,4,29,60,
and determines the impact of shifts in microbial dynamics on
the rate of POC flux attenuation. Specifically, we identify key
aspects of particle-associated microbial community dynamics
that contribute to setting the shape of the POC flux attenuation
profile. We also predict that changes in microbial community
dynamics can rapidly shift rates of POC remineralization. This
work demonstrates that the assumption of low constant POC
incorrect5,61,62, and that microbial
consumption rates
dynamics alone can generate significant variability in the POC
flux. Our results challenge the classic idea of particles being
inherently labile or recalcitrant and propose that lability is an
emergent ecosystem property and a function of the microbial
community, organic matter chemistry, and environmental
conditions.
One of the difficulties in studying the vertical POC flux in the
ocean is that POC flux observations provide a poor constraint on
models13—in fact only 2 free parameters are needed to represent
the classic POC flux curve while mechanistic carbon-cycle models
rely on many more parameters. Thus, capturing observed POC
flux profiles is not in of itself sufficient validation of a proposed
mechanism. Our model allows for targeted hypotheses that can be
tested in the field—the results of which will provide enhanced
constraints on global carbon-cycle models allowing for more
robust predictions of future changes in carbon export out of the
surface ocean.
Results
Scaling-up micro-scale dynamics to the water-column. Our
mechanistic model captures the colonization of particles by free-
living microbes and conversion from polymeric
to low-
molecular-weight organic matter (LMWOM) compounds as the
particles sink (Methods and Supplementary Material 1). To
represent the complexity of the interactions between diverse
particle-associated microbial communities and a chemically
diverse organic carbon pool, we use lability as an ecosystem
property that specifies the conversion rate of polymeric material
to LMWOM of a specific POC pool by a specific microbial
group63. As lability is poorly constrained by observations, we test
a wide range of POC lability values assuming a log-normal
distribution63, though the modeled POC fluxes at the ocean-scale
are found to be independent of the specific form of the dis-
tribution chosen (Supplementary Fig. 1). We represent
the
organic carbon content of each model particle using a single,
stochastically assigned, lability value and represent the particle-
associated microbial community using a single microbial group
per particle (in all we resolve 18 microbial types with different
enzyme kinetics and growth rates). Sensitivity tests with complex
particles, multiple microbial groups per particle, and greater
numbers of microbial groups show that these simplifications do
not impact the overall POC flux profiles (Supplementary Figs. 2
and 3). The model is initialized using a particle export depth
between 50 and 100 m (with a default value of 100 m) with
particle size distributions spanning the observed range (power law
with exponent s = −2, −3, or −4; Supplementary Table 1). For
simplicity, we do not include any additional particle formation
below the export depth.
Each particle is stochastically assigned an initial radius at the
export depth and type of microbial degrader. The microbial groups
are defined by their enzyme kinetics (i.e., POC degradation rate),
2
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Fig. 1 Micro-scale model dynamics. a Illustration showing micro-scale model dynamics occurring on sinking particles. Primary degraders (red microbes)
convert polymeric organic matter (dark blue sphere) into low molecular weight organic matter (LMWOM, light blue) using extracellular enzymes (yellow).
The particle-associated community experiences loss due to mortality (gray microbes) and detachment (purple microbes). b Illustration of water column
model dynamics with an emphasis on a single particle (blue sphere) falling through the water column. Each particle is stochastically assigned an initial
radius, lability, and set of biological parameter values at the depth of formation (see Methods). The particle-associated microbial dynamics then evolve
prognostically for each particle as it sinks through the water column and is consumed by microbial activity. The total particulate organic carbon flux
throughout the water column is obtained by summing across all sinking particles.
maximum growth rate, and abundance in the free-living microbial
pool, which is set to decrease exponentially with depth64 (Fig. 1, see
Methods and Supplementary Material 1 for more details). The
particle is initialized with a stochastically assigned initial microbial
biomass and is continually colonized by the free-living microbial
pool as it sinks through the water column. The sinking speed of
size and specific
each particle is calculated based on its
gravity5,16,28,65 (Supplementary Material 1 eqs. s13–s15). As each
particle sinks through the water column, microbial growth on the
particle evolves prognostically, and organic carbon is consumed or
lost
to the surrounding water column due to diffusion and
advection55. The microbially-catalyzed degradation of the particle
causes the radius to shrink and the sinking speed to decrease.
Temperature dependence of microbial growth rates is applied
using a typical water column temperature profile66 (Supplementary
Figs. 4 and 5).
The model captures the observed density-dependent growth of
particle-associated microbial populations, where the population
density (cells per surface area) must surpass a critical threshold in
order for successful particle colonization to occur46 (Fig. 2). This
critical threshold is a consequence of mortality and population-
size dependent per capita growth rate (the ‘Allee effect’54); see
Supplementary Figs. 6–9, Supplementary Material 3. Specifically,
microbial populations must overcome multiple sources of loss
including mortality (e.g., viral lysis or bacterivory), detachment,
and the diffusive and advective loss of LMWOM away from the
loss
particle
processes). Model populations below a critical threshold cannot
establish a colony on the particle due to these loss processes,
consistent with laboratory observations46 (Fig. 2 and Supple-
mentary Fig. 10). Using a simplified mathematical model of POC
degradation, we show that the population-dependent growth rate
arises naturally as an interplay of simple microbial dynamics (e.g.,
saturating (Monod) growth kinetics, uptake kinetics, and yield)
and particle chemical and physical properties (e.g., particle size
and monomer diffusivity leading to nutrient loss) (Supplementary
Material 4, Supplementary Fig. 11).
referred to collectively as
(hereafter
surface
Ebrahimi et al 2019
Our Model
2.5
2
1.5
1
0.5
s
s
a
m
o
B
n
i
i
e
g
n
a
h
C
d
o
F
l
0
100
102
Initial population (cells/particle)
104
Fig. 2 Density-dependent growth validation. The model captures observed
density-dependent growth of particle-associated communities. Fold change
in microbial population biomass after 10 hours of growth is shown for
the model simulations (red asterisks) and experimental data (open circles,
Ebrahimi et al. (2019)). Error bars on the open circles represent standard
error of measurement from at least three measurements of particle
colonization density from Ebrahimi et al. (2019).
Role of microbes in setting water-column POC fluxes. Multiple
biotic and abiotic factors control the rate of particle-associated
microbial growth and therefore the microbial consumption of
POC. Critically, the emergent particle consumption rates that
result from interactions between these factors (e.g., particle labi-
lity and particle-microbe encounter rate) are not predictable from
one factor alone (Fig. 3b). For example, with an initial radius of
−1 day−1, half of
500 μm and lability of 32 mmol CPOC mmol Ccell
the time the particle is consumed in the upper 1,000 m (50% of
particles) and half of the time the particle will persist into the
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a)
3
2.5
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1.5
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2
-
m
m
s
l
l
e
c
104
b)
100
80
60
40
i
s
u
d
a
r
i
i
g
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n
a
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e
r
0
50
100
Time (hour)
150
%
20
0
0
50
100
Time (hour)
150
c)
500
)
m
(
h
t
p
e
D
1000
1500
2000
0
100
50
% remaining of initial radius
d)
% particle persisting to 1,000 m
0.005
17
17
17
17
0
0.01
50
34
17
17
17
0.02
100
59
25
17
17
0.05
100
84
50
25
17
0
0
9
9
0.1
100
92
59
34
25
12
0.2
100
100
75
42
25
12
)
m
c
(
i
s
u
d
a
r
l
e
c
i
t
r
a
P
0
0
7
9
9
9
0.4
100
100
92
67
41
21
10
0
0
0
0
5
5
6
0
0
0
0
0
0
2
102
101
100
(A) struggling community: low lability
(B) struggling community: slow growth
(C) rescued community
(D) exponential growth: long lag
(E) exponential growth: small particle
(F) exponential growth: large particle
(G) exponential growth: high lability
10 18 32 56
100
180
315
Lability (mmol C
mmol C
POC
560
1000
-1 day-1)
cell
Fig. 3 Particle-associated microbial growth dynamics. Example degradation dynamics are shown for rapidly growing particle-associated microbial
populations (curves E, F, G), ‘rescued’ populations (C, D), and ‘struggling’ populations (A, B). Parameter values are given in Supplementary Fig. 14. For each
simulation, the change in microbial density on the particle surface over time (a), percentage changes in the particle radius over time (b) and depth (c) are
shown. To quantify the impact of microbial growth dynamics on POC persistence at depth, the fraction of particles within a given lability class and radius at
formation that persist below 1,000 m is calculated (d). The colors and values in each grid correspond to the percentage of model parameter combinations
for a given lability and initial radius (n = 72) that persist past 1,000 m depth (see Supplementary Material 1).
deep ocean (>2,000 m). The timescale for particle degradation
by the microbial community varies from ~5 days to >200 days,
with most particles lasting for a few weeks below the export
depth (~30 days,
lognormally distributed), consistent with
observations67,68. The degradation timescale for each particle is
determined by the duration of the lag phase for the particle-
associated microbial populations: once populations reach expo-
nential growth, the particle is consumed rapidly. When popula-
tion density at particle formation (100 m in the default
simulations) is high, encounter rates are high, and/or lability is
high,
the population quickly overcomes loss processes and
reaches exponential growth (Fig. 3, E-G curves). This results in
the complete consumption of particles within the upper 500 m of
the water column. When the population density at formation is
low, encounter rates are low, and/or the lability of the particle is
low, loss rates can exceed the particle-associated microbial growth
rates. This results in a particle-associated community that is
unable to successfully colonize the particle and reach exponential
growth (here termed a “struggling” community). This in turn
results in slow microbially mediated POC remineralization rates,
and a higher transfer of carbon into the deep ocean (Fig. 3, A-B
curves). A struggling particle-associated population can be “res-
cued” by recruitment from the free-living microbial pool as the
particle sinks if the encounter rates are sufficiently high, resulting
in shallower particle consumption (Fig. 3, e.g., A vs. C curve). The
depth over which a particle sinks before it is completely con-
sumed by the particle-associated microbial community thus
depends on multiple biotic and abiotic factors that determine
microbial population behavior (Fig. 3d, see Supplementary
Material 3): the conversion rate of POC to LMWOM, particle size
(which determines diffusive loss and sinking speed), microbial
biomass at particle formation,
temperature, and exchange
between the particle and free-living community (encounter rate).
The dichotomy between particle-associated populations that
successfully colonize particles and populations that struggle to
colonize particles provides a mechanistic explanation for the
commonly used approximation of two labilities of POC6 or the
double exponential representation of the POC flux10. Here we
show that this dichotomy emerges mechanistically as a result of
lability cannot be defined
microbial dynamics. Furthermore,
solely as a chemical property of
the particle but must be
considered an ecosystem property63,69–71 defined by both the
organic carbon composition and the enzyme systems of the
colonizing microbial community. The result of these dynamics is
that particle remineralization rates for a single particle type (e.g.,
radius and lability) can vary by several orders of magnitude across
particles with different microbial dynamics and over depth
(Supplementary Figs. 12 and 13). This dichotomy also emerges
when a modified version of the model is used where the particle-
associated populations are able to directly consume POC and so
are not subjected to diffusive loss (Supplementary Material 3 and
Supplementary Fig. 15). In this direct-uptake formulation, the
rate of particle degradation is limited by the rate at which the
microbes can incorporate carbon into their biomass. We
demonstrate that both models produce similar dynamics and
rates of particle remineralization (Supplementary Fig. 16). Our
4
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model mechanistically captures these particle-associated micro-
bial dynamics and their impacts on particle consumption. This
provides insight into how micro-scale processes might drive
geographic variations in POC flux attenuation and allows for the
generation of testable hypotheses for experimentalists.
The model predicts a shift in particle-associated microbial
community composition with depth. Fast growing microbes
associated with high-lability particles are abundant in the upper
water column, whereas slower-growing microbes associated with
low-lability particles are relatively more abundant at depth
(Supplementary Fig. 17). This pattern emerges because popula-
tions growing on labile particles and populations with faster
maximum growth rates can more easily surpass the critical
threshold necessary for successful colonization and so thrive in
the upper water column. In contrast, slower-growing commu-
nities take longer to build up biomass on particles and so are
more abundant at depth. Since slow growing populations are also
present in the surface ocean, the model predicts a more diverse
particle-associated microbial community in the surface waters
compared to the deeper ocean (Supplementary Fig. 17). These
findings are consistent with documented changes in particle-
communities with depth18,57,58,72,73:
associated prokaryotic
particle associated communities tend to be more homogenous
at depth and community richness is positively correlated with the
rate of POC remineralization.
The ocean is associated with strong vertical gradients in
temperature which have been hypothesized to play an important
role in POC flux attenuation8,60,74. We investigate the role that
temperature plays in our modeled microbial dynamics using a
suite of model simulations with varied temperature profiles and
two temperature limitation functions, which span the observed
temperature-growth rate
relationship for marine microbial
heterotrophs (Supplementary Fig. 5). Temperature does play an
important role in the loss processes described above as decreased
growth rates due to temperature limitation makes it more difficult
to overcome loss processes and
for microbial populations
successfully colonize particles. However, our results suggest that
temperature limitation is not the primary driver of the observed
dynamics (Supplementary Material 3, Supplementary Figs. 18–20).
Specifically, if a population is able to grow exponentially, the
impact of temperature becomes secondary. Temperature becomes
important for the struggling communities which are associated
with slow microbial growth rates and low particle consumption
rates, consistent with previous work48,50. The global relationships
observed between POC flux attenuation rates and temperature
may be partially explained by co-varying factors such as shifts in
POC lability and microbial community function4,64,75,76.
(cid:1)
Variability in microbially mediated POC flux attenuation. The
explicit representation of micro-scale dynamics on particles in
our model generates water-column-scale estimates of bacterially
mediated POC fluxes (Fig. 4). To compare across large numbers
of model simulations and with observed POC flux profiles, we
quantify the rate of POC flux attenuation using the commonly
(cid:3)(cid:2)b; where b is the attenua-
used power law function F ¼ F100
tion exponent, which is inversely related to the vertical carbon
transfer rate, F100 is the flux at 100 m, and z is depth in meters1–3.
The model reproduces known relationships. For example, higher b
values in the model output are associated with higher abundance of
small particles (flatter particle size spectra) and higher lability. Thus,
the model predicts that oligotrophic regions with flatter particle size
spectra would coincide with higher b values, consistent with pre-
vious studies5–9,16 In addition, the model results suggest that shifts
in the depth of particle formation within the euphotic zone play
z
100
a key role in the attenuation rates observed in the upper water
column (<500 m) (Supplementary Fig. 21).
The observed range in the POC flux across different oceanic
regions is large (i.e., 1–30% of the initial flux remains at 1,000 m)1,3.
We demonstrate that variable microbial dynamics is sufficient to
generate the observed mean, range, and distribution of observed
POC flux profiles from across the global oceans (n = 897)3 (Fig. 4).
While other processes not included in the model (e.g., zooplankton
dynamics) are also critical for setting the POC flux attenuation
profile, our results suggest
that variations in microbial POC
consumption rates may play a significant role in determining spatial
and temporal changes in the POC flux profile. For example, we
show that particle-associated microbial community dynamics such
as shifts in maximum growth rate or particle lability can alter the
POC flux to the same extent as a change in particle size spectra
(Fig. 4). These model dynamics (from rapidly growing populations
to those struggling to survive) emerge as a result of stochastic
interactions between biological, chemical, and physical controls on
microbial growth.
Discussion
Our results suggest that the stochastic assembly of communities on
particles frequently results in communities struggling to overcome
losses, thereby generating the long tail of persistent POC at depth
(>1000 m). Furthermore, for particles that persist at depth due to
sub-optimal growth of the particle-associated communities, rela-
tively small changes in microbial dynamics can rescue these
communities, allowing them to rapidly reach exponential growth
and generating large changes in POC flux. For example, while a
given particle type (e.g., size and lability) might persist below 1000
m in one region of the ocean due to low initial biomass or low
microbial encounter rates, that same particle might be consumed
rapidly in a different region where microbial encounter rates are
higher (Fig. 3). Our model provides an alternative hypothesis for
pulsed export of carbon from oligotrophic regions77–79. In addi-
tion to a shift
in particle size associated with these export
eventse.g.,77,80,81, the microbial community in oligotrophic regions
is typically associated with picoplankton dominated communities
and so may not be adapted to consume particles generated by
larger phytoplankton groups. These differences in microbial
dynamics, represented as lower biomass at formation and lower
encounter rates in our model, will yield greater transfer efficiency
of carbon to depth than would occur if the same type and quantity
of particles were released in more productive regions where the
microbial community is primed to consume POC generated by
larger phytoplankton groups.
This work suggests that shifts in microbial communities both
in surface waters and at depth can result in significantly dif-
ferent POC fluxes and that the magnitude of microbial driven
variations in the POC flux is similar to other previously pro-
posed processes (e.g., particle size spectrum). This is not to say
that other processes do not also impact the POC flux. Dynamics
not explicitly represented in the model such as particle aggre-
gation and disaggregation32,35,39, zooplankton grazing on
particles30,36,37,40,82, phytoplankton dynamics83–85, and the
formation of new particles within the water column83–85 also
play an important role. An exciting avenue of future work is to
investigate the extent to which complex ecological interactions
between the microbial communities and zooplankton dynamics
impact the POC flux, the relative importance of these different
processes for determining the rate of organic carbon export, and
how these dynamics may vary geographically. Our model
provides a unique framework for understanding the carbon
cycle impact of zooplankton bactivory on particle-associated
communities42, and the direct consumption of sinking particles
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a) Size spectra
b) Lability
e) Attenuation
)
m
(
h
t
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500
1000
1500
2000
)
m
(
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500
1000
1500
2000
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1500
2000
s=-4
s=-3
s=-2
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=50
=200
=500
avg
avg
avg
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c) Max growth
d) Encounter
500
1000
1500
2000
High Enc
Low Enc
Martin 1987
0
0.5
1
1.5
=7.2 d -1
=1.2 d -1
max
max
0
0.5
1
1.5
POC flux (mol C m -2 year-1)
Global UVP
Our model
Avg. b
1.5
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q
e
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f
d
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i
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0
1
2
Attenuation exponent (b)
Fig. 4 Microbial contribution to large-scale particulate organic carbon (POC) fluxes. Shifts in POC fluxes over depth are shown as a function of varying
particle and microbial dynamics. Each gray line is the integrated flux over 2,256 to 763,615 stochastically initialized particles (depending on the particle size
spectra). For each parameter set, 1,000 stochastic simulations were conducted (1,000 gray lines of different shades). The average for each parameter set is
shown with the thick colored line. The data from Martin et al (1987) (in open circles) are also shown. POC transfer efficiency decreases (larger attenuation
−1 day−1) (b), higher
exponent b) with more negative particle size spectra power law exponent s (a), higher mean particle lability (β
maximal growth rate (μmax, day−1) (c), and higher particle-microbe encounter rate (Enc) (d). The distribution of attenuation exponent (b) for all
10,000 stochastic simulations from panels a-d (gray bars) are compared against observed attenuation coefficients from 897 global Underwater Video
Profiler (UVP) measurements compiled by Guidi et al. (2015) (open bars) (e).
avg, mmol Cpoc mmol Ccell
by zooplankton (e.g., exploring preferences for different types of
POC and particle sizes). Direct inclusion of dynamics such as
zooplankton disaggregation of particles and zooplankton
vertical migration would allow for further mechanistic con-
straints on spatial and temporal variability of organic carbon
export.
This work takes a first step towards explicitly integrating micro-
scale dynamics into large-scale models to generate predictions of
organic carbon fluxes in the ocean. We show that microbial
growth dynamics can generate temporal and spatial variability in
POC consumption rates, suggesting that current parametrizations
for POC degradation are inadequate (Supplementary Mate-
rial 1–3). Our model generates hypotheses as to the relative
importance of particle-associated microbial dynamics throughout
the water column that can be tested by targeted field and
laboratory studies. These studies will in turn improve the model
parameterizations and generate more robust estimates of the POC
vertical flux. For example,
incubation experiments could test
whether a significant fraction of particle-associated populations at
depth are below the critical density threshold. Many aspects of
particle-associated microbial dynamics are currently poorly con-
strained (e.g., encounter rates, bacterial growth efficiencies). Our
results highlight the need for better in situ measurements of these
key biological processes such as loss processes for microbial
communities, microbial abundance on particles, enzyme activities,
growth rates on particles, and encounter and detachment rates for
dominant particle-associated marine species. Ultimately, robust
predictions of future shifts in carbon cycle dynamics require
accurate, mechanistic representation of the primary processes in
global climate models. Here we demonstrate that particle-
associated microbial dynamics are one of these processes.
Methods
This model captures key micro-scale dynamics occurring on particulate organic
carbon (POC) in a manner scalable to the water column. For the results presented
in the main text, we represent particle-associated microbial diversity using 18
groups of heterotrophic microbes, defined based on their enzyme kinetics and
growth rates. Supplementary Material 2 presents a sensitivity test with a continuum
of microbial classes and demonstrates that this discretization does not impact our
results. We also make the simplifying assumption that each particle type consists of
a single lability of organic carbon colonized by a single type of microbial primary
degrader, though the conclusions of this work are not dependent on this
assumption (Supplementary Fig. 2 and Supplementary Material 2). Here we track
each unique particle type i, which is defined based on radius at formation and
lability (β
i). We include enzymatic degradation of polymer into low molecular
weight organic matter (Clmwom), density dependent growth of the particle-
associated microbial community (Bi), and the attachment (Ei;z) and detachment
(Li) of heterotrophic microbes to/from the particles. This model can be coupled to
a full ecosystem model such that the generation of each particle type can be
calculated prognostically. However, here we focus on the degradation of POC
below the export depth and so simply include a source term to represent net
particle formation above the export depth (default 100 m, see Supplementary
Material 2 for simulations with alternative formation depths). For simplicity, we
also do not allow for aggregation or disaggregation to occur within the water
column. An extended model description is provided in Supplementary Material 1.
The change in the carbon content of particle i (Cpoc;i, mmol CPOC particle−1)
over time is defined as:
iBi
¼ (cid:2)β
i (mmol CPOC mmol Ccell
dCpoc;i
dt
−1 day−1) represents the polymer degradation
where β
rate of Cpoc;i by microbial group Bi (mmol Ccell particle−1) similar to59. Specifically,
β
i captures differences in ‘lability’ of particles, which is a function the organic
carbon itself, the microbial enzymes specific to group Bi, and production rate of
= 0), the particle-
those enzymes by Bi. When the particle is fully consumed (Cpoc
associated microbial community detaches and so consumption stops.
ð1Þ
The enzymatic degradation of POC results in the production of low molecular
weight organic matter (LMWOM) (Clmwom, mmol C m−3 particle−1) which sup-
ports microbial growth. We assume that there is no loss of carbon during the
enzymatic cleavage from POC to LMWOM such that 1 mmol Cpoc degraded = 1
6
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mmol Clmwom produced. There is however diffusive loss of LMWOM away from
the particle as described in Eq. 2. Specifically, the LMWOM concentration is cal-
culated assuming steady state dynamics as:
Clmwom
(cid:4)
¼ β
(cid:5)
iBi
(cid:2)
μ
iBi
ylmwom
=dloss
ð2Þ
i is the growth rate of microbial group Bi on the particle (day−1), ylmwom is
−1), and dloss is
where μ
the aerobic microbial growth efficiency (mmol Ccell mmol Clmwom
the diffusion loss rate of the LMWOM (m3 day−1) (Supplementary Material 1
eq. s3 and Supplementary Material 4 for full calculation).
Microbial dynamics on each particle are defined as:
(cid:6)
¼ μ
i
dBi
dt
(cid:7)
(cid:2) Li
(cid:2) mlin;i
Bi
þ Ei;z
ð3Þ
where mlin;i is the microbial mortality rate (day−1) and Li is the detachment rate
(day−1). The microbial encounter rate (Ei;z, mmol Ccell day−1 particle−1) repre-
sents the rate of colonization of the particle by the free-living microbial pool.
Ei;zvaries with depth based on particle size, sinking speed, and the abundance of
free-living, motile microbes in group i51,64 (eq. s11 in Supplementary Material 1).
The free-living abundance is assumed to decrease exponentially with depth64.
Microbial growth rate, μ
the particle surface and is represented with the Monod equation:
i (day−1) is dependent on the LMWOM concentration at
μ
i
¼ V max;i
Clmwom
Clmwom
þ km;i
γ
T;z
ð4Þ
;
i;z
ω
Fpoc;z
where V max;i, km;i, and γ
T;z represent the maximum LMWOM uptake rate, the half
saturation of LMWOM uptake by microbial group Bi, and the temperature lim-
itation at depth z (eq. s11 in Supplementary Material 1), respectively. Model
parameter values are given in Supplementary Table 1 and sensitivity tests are
described in Supplementary Material 2.
The total POC flux at a certain depth z (Fpoc
z in mmol CPOC m−2 day−1), is
calculated as the sum of the vertical fluxes of each individual particle as they sink
;
through the water column, where Fpoc
z is:
¼ ∑Cpoc;i;zN i;z
ð5Þ
where N i;z is the number of particles of type i per m3 water column at depth z.
To test the impact of particle-associated microbial dynamics on the POC vertical flux
through the water column, we perform a set of stochastic simulations in which para-
meters are randomly chosen from within a reasonable range. Here we simulate a single
2.24 m ´ 2.24 m water column initialized between 50 and 100 m with an observed
particle size distribution yielding a total flux of 1.5 mol m−2 yr−1 1,5,13. Specifically, we
simulate 2,256 particles (particle size spectra with power law exponent s = −2), 69,000
particles (s = −3), or 763,615 particles (s = −4) ranging from 50 μm to 0.4 cm in radius
as they fall through the water column. For each particle, the following model para-
meters are stochastically assigned within a reasonable range (Supplementary Table 1)
using a uniform distribution, except for lability for which a log-normal distribution is
used: maximum growth rate V max (1.2 or 7.2 day−1), particle lability β (10–1,000 mmol
−1 day−1), initial cell density (400–2,800 cell mm−2), and density of
CPOC mmol Ccell
free-living community of microbes in group i (Fi) (10–285 cell mm−3). The stochastic
simulations are conducted 1,000 times for each particle size distribution. Simulations
are run for 600 days which is sufficient for all particles to be fully consumed or exported
to >4,000 m. The attenuation exponent b for the modeled POC flux is calculated using a
least square fit of the power law function.
Reporting summary. Further information on research design is available in the Nature
Research Reporting Summary linked to this article.
Data availability
The microbial growth data generated in this study are provided in the Supplementary
Table S2.
Code availability
The model code is deposited on GitHub (https://github.com/LevineLab/POMmodel) and
citable using https://doi.org/10.5281/zenodo.6015020.
Received: 29 June 2021; Accepted: 2 March 2022;
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Acknowledgements
This work was supported by a grant from the Simons Foundation (542387 to NML,
542395 to RS and OC, 542389 to TH). We thank N. Norris and E. Lee for assistance with
model development.
8
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ARTICLE
Author contributions
TTHN and NML designed the study, developed the full model, and conducted the
numerical analysis; TC and TH developed and analyzed the mathematical model in
Supplementary Material 4; KA and TC performed measurements of bacterial parameters
for Vibrio sp. 1A01; EJZ, OXC, AE, JS, UA, FJP, TH, and RS contributed data and to
model development; all authors contributed to the writing.
Competing interests
The authors declare no competing interests.
Additional information
Supplementary information The online version contains supplementary material
available at https://doi.org/10.1038/s41467-022-29297-2.
Correspondence and requests for materials should be addressed to Naomi M. Levine.
Peer review information Nature Communications thanks Jacob Cram, Philip Boyd and
the other, anonymous, reviewer for their contribution to the peer review of this work.
Peer reviewer reports are available.
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10.1073_pnas.1913292117.pdf
|
Data Availability Statement. All data discussed in the paper are available
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Data Availability Statement. All data discussed in the paper are available to readers through Harvard Dataverse, https://doi.org/10.7910/DVN/RFGT4S .
|
B cells migrate into remote brain areas and support
neurogenesis and functional recovery after focal
stroke in mice
Sterling B. Ortegaa,b,c,1, Vanessa O. Torresb,c,1, Sarah E. Latchneyd,e, Cody W. Whooleryd, Ibrahim Z. Noorbhaib,c,
Katie Poinsatteb,c, Uma M. Selvarajb,c, Monica A. Bensonb,c, Anouk J. M. Meeuwissenb,c, Erik J. Plautzb,c,
Xiangmei Kongb,c, Denise M. Ramirezb,c, Apoorva D. Ajayb,c, Julian P. Meeksb,c,f, Mark P. Goldbergb,c,
Nancy L. Monsonb,c, Amelia J. Eischd,g,h, and Ann M. Stoweb,c,i,2
aDepartment of Pathology, University of Iowa, Iowa City, IA 52242; bDepartment of Neurology and Neurotherapeutics, UT Southwestern Medical Center,
Dallas, TX 75390; cPeter O’Donnell Jr. Brain Institute, UT Southwestern Medical Center, Dallas, TX 75390; dDepartment of Psychiatry, UT Southwestern
Medical Center, Dallas, TX 75390; eDepartment of Biology, St. Mary’s College of Maryland, St. Mary’s City, MD 20686; fDepartment of Neuroscience, UT
Southwestern Medical Center, Dallas, TX 75390; gDepartment of Neuroscience, Perelman School of Medicine, University of Pennsylvania, Philadelphia, PA
19104; hDepartment of Anesthesiology and Critical Care, Children’s Hospital of Philadelphia, Philadelphia, PA 19104; and iDepartment of Neurology,
University of Kentucky, Lexington, KY 40506
Edited by Lawrence Steinman, Stanford University School of Medicine, Stanford, CA, and approved January 16, 2020 (received for review August 1, 2019)
Lymphocytes infiltrate the stroke core and penumbra and often
exacerbate cellular injury. B cells, however, are lymphocytes that
do not contribute to acute pathology but can support recovery. B
cell adoptive transfer to mice reduced infarct volumes 3 and
7 d after transient middle cerebral artery occlusion (tMCAo), in-
dependent of changing immune populations in recipient mice.
Testing a direct neurotrophic effect, B cells cocultured with mixed
cortical cells protected neurons and maintained dendritic arbori-
zation after oxygen-glucose deprivation. Whole-brain volumetric
serial two-photon tomography (STPT) and a custom-developed
image analysis pipeline visualized and quantified poststroke B cell
diapedesis throughout the brain, including remote areas support-
ing functional recovery. Stroke induced significant bilateral B cell
diapedesis into remote brain regions regulating motor and cogni-
tive functions and neurogenesis (e.g., dentate gyrus, hypothalamus,
olfactory areas, cerebellum) in the whole-brain datasets. To confirm
a mechanistic role for B cells in functional recovery, rituximab was
given to human CD20+ (hCD20+) transgenic mice to continuously
deplete hCD20+-expressing B cells following tMCAo. These mice
experienced delayed motor recovery, impaired spatial memory,
and increased anxiety through 8 wk poststroke compared to wild
type (WT) littermates also receiving rituximab. B cell depletion re-
duced stroke-induced hippocampal neurogenesis and cell survival.
Thus, B cell diapedesis occurred in areas remote to the infarct that
mediated motor and cognitive recovery. Understanding the role of
B cells in neuronal health and disease-based plasticity is critical for
developing effective immune-based therapies for protection against
diseases that involve recruitment of peripheral immune cells into
the injured brain.
B lymphocytes | focal stroke | serial two-photon tomography | adaptive
immunity | neurogenesis
Stroke leads to central nervous system (CNS) damage, which
results in functional deficits (1) and is exacerbated by an
inflammatory immune response derived from both the innate and
adaptive immune systems (2). Mechanistic studies using murine
stroke models show a significant infiltration of innate immune
cells, including monocytes, macrophages, and neutrophils, pre-
dominantly in the area of ischemic injury (i.e., infarct, periinfarct
regions) (3). The role of the adaptive immune system is also
pivotal to stroke recovery, as it can both exacerbate and amelio-
rate long-term neuropathology, depending on the lymphocyte
population, location, and timing of activation (4–10). Location and
timing are particularly relevant, as recovery of lost function in
stroke patients depends on functional plasticity in areas outside of
the infarct (i.e., remote cortices) to subsume lost function (11).
Neurons in remote cortical areas that are interconnected to the
infarct up-regulate growth factors and plasticity-related genes af-
ter stroke (12, 13), but it is unknown if neuroinflammation is
concomitant with remote genetic and proteomic responses to is-
chemic injury and subsequent reorganization.
B cells, critical effector cells for antibody production and an-
tigen presentation, are one adaptive immune cell subset with the
capacity to also produce neurotrophins to support neuronal
survival and plasticity (14–16). Prior work found that the loss of
B cells increases stroke-induced infarct volumes,
functional
deficits, and mortality in immunodeficient μMT
mice, which
lack B cells (17). Polyclonal activated and nonactivated B cell
−/−
E
C
N
E
I
C
S
O
R
U
E
N
Significance
Neuroinflammation occurs immediately after stroke onset in
the ischemic infarct, but whether neuroinflammation occurs in
remote regions supporting plasticity and functional recovery
remains unknown. We used advanced imaging to quantify
whole-brain diapedesis of B cells, an immune cell capable of
producing neurotrophins. We identify bilateral B cell diapede-
sis into remote regions, outside of the injury, that support
motor and cognitive recovery in young male mice. Poststroke
depletion of B cells confirms a positive role in neurogenesis,
neuronal survival, and recovery of motor coordination, spatial
learning, and anxiety. More than 80% of stroke survivors have
long-term disability uniquely affected by age and lifestyle
factors. Thus, identifying beneficial neuroinflammation during
long-term recovery increases the opportunity of therapeutic
interventions to support functional recovery.
Author contributions: S.B.O., S.E.L., C.W.W., K.P., M.P.G., N.L.M., A.J.E., and A.M.S. de-
signed research; S.B.O., V.O.T., S.E.L., C.W.W., I.Z.N., K.P., U.M.S., M.A.B., A.J.M.M., E.J.P.,
X.K., D.M.R., A.D.A., J.P.M., M.P.G., A.J.E., and A.M.S. performed research; N.L.M. contrib-
uted new reagents/analytic tools; S.B.O., V.O.T., S.E.L., C.W.W., D.M.R., A.D.A., J.P.M., and
A.M.S. analyzed data; and S.B.O., V.O.T., S.E.L., C.W.W., N.L.M., A.J.E., and A.M.S. wrote
the paper.
The authors declare no competing interest.
This article is a PNAS Direct Submission.
This open access article is distributed under Creative Commons Attribution-NonCommercial-
NoDerivatives License 4.0 (CC BY-NC-ND).
Data deposition: All raw data have been uploaded to Harvard Dataverse, https://doi.org/
10.7910/DVN/RFGT4S.
1S.B.O. and V.O.T. contributed equally to this work.
2To whom correspondence may be addressed. Email: [email protected].
This article contains supporting information online at https://www.pnas.org/lookup/suppl/
doi:10.1073/pnas.1913292117/-/DCSupplemental.
First published February 12, 2020.
www.pnas.org/cgi/doi/10.1073/pnas.1913292117
PNAS | March 3, 2020 | vol. 117 | no. 9 | 4983–4993
−/−
transfer into syngeneic mice also ameliorates stroke pathology
and functional deficits within the first 96 h after stroke via in-
terleukin (IL)-10–mediated up-regulation (9, 10). Reconstitution
of Rag
(i.e., B- and T cell-knockout) mice with B cells does
not exacerbate infarct volume, confirming a nonpathological role
in acute stroke (18, 19). Others confirmed a nonpathological role
for B cells after stroke in several other strains (20). However,
additional studies do not extend the neuroprotective and/or
nonpathological role beyond 4 d after stroke onset, with the only
investigation into the long-term role of B cells in stroke recovery
finding that B cells contribute to cognitive decline weeks after
stroke in multiple strains of mice across various stroke models
(21). These data, coupled with human data associating self-
reactive antibodies with cognitive decline (8), underscore the
importance of additional studies to clarify the contribution of B
cells to poststroke injury and repair. This includes the impor-
tance of timing, location, and function of B cells recruited into
the injured brain in defining the role in either injury or repair.
The goal of this series of experiments is to elucidate the en-
dogenous role of B cells, including localization of B cell diape-
desis after stroke using advanced volumetric imaging strategies
(e.g., serial two-photon tomography), and the behavioral rele-
vance of B cells using refined neurological motor and cognitive
assessments. In this work, we show that poststroke B cell re-
pletion reduces neuropathology via an IL-10–dependent mech-
anism that is independent of immune modulation. Second, we
show that B cells exert a direct neuroprotective effect on neurons
and preserve neuronal dendritic arborization following oxygen-
glucose deprivation in vitro. We find that B cells diapedese bi-
laterally into remote areas of the brain that associate with long-
term motor and cognitive function following a transient middle
cerebral artery occlusion (tMCAo), while long-term depletion of
B cells after stroke exacerbates motor and cognitive deficits and
reduces poststroke neurogenesis. In summary, we show that B
cells play a prominent role in stroke recovery beyond the first
4 d after stroke by directly protecting neurons and promoting
recovery within the injured and reorganizing brain.
Results
B Cells Use IL-10 to Reduce Stroke-Induced Neuropathology. Pre-
viously published studies found that B cells exhibit conflicting
roles in stroke recovery dependent on the state of activation:
acute in vitro activation benefits (i.e., 1 to 4 d) versus long-term
in vivo activation detriments (i.e., months) (10, 21). Further-
more, the use of antibody-mediated B cell depletion in wild type
and transgenic mice revealed no change in the neuropathology
or functional deficits at the acute phase of stroke (days 1 and 3
post induction) (20). Thus, to further dissect the role of B cells in
subacute to long-term stroke recovery, we investigated the en-
dogenous function of B cells by adoptive transfer of naïve,
wild type B cells into stroke-induced recipient mice, measuring
neuropathology and motor coordination at time points up to 2
wk following stroke induction. We purified unstimulated B cells
from naïve mice and injected them i.v. into recipient mice 7 h
after stroke onset (60-min tMCAo; Fig. 1A). On all mice, suc-
cessful tMCAo induction was qualified as a 20% reduction for
60 min followed by reperfusion to at least 50% of baseline
(pretMCAo induction) cerebral blood flow. We measured motor
function using rotarod (days 2, 6, and 14 poststroke), forearm
strength (force grip), neuropathology via T2-weighted MRI (days
3 and 7), and cytotoxicity via standard histology (day 15). Rela-
tive to PBS controls, B cell recipients exhibited reduced infarc-
tions identified by serial MRI at both 3 d (P < 0.01) and 7 d (P <
0.05; Fig. 1 B and C) post tMCAo. Interestingly, the rotarod and
force grip assays did not detect differences between the two
cohorts, even though all groups initiated acute deficits con-
firming similar degree of initial stroke-induced neuropathology
(SI Appendix, Fig. S1 A and B). We sought to determine if naïve
B cells, without in vitro activation, caused reduced infarct vol-
umes via an IL-10–mediated mechanism. Adoptive transfer of
wild type B cells from naïve mice reduced infarct volume, and
this protection was lost with IL-10–deficient B cells (Fig. 1D).
As protection was absent in both IL-10–deficient (Fig. 1D) and
“preconditioned” (22) B cells (SI Appendix, Fig. S1 B and C),
these data show that naïve B cells provide an endogenous
neuroprotective function (22). In contrast to other studies (9),
Fig. 1. B cell adoptive transfer reduces infarct volumes via IL-10 but independently of immunomodulation. (A) Experimental timeline for B cell adoptive
transfer 7 h after tMCAo. (B) Infarct volumes quantified from (C) serial MR images show that naïve B cells (green upward triangles) significantly decrease
infarct volumes 3 and 7 d poststroke as compared to PBS control (black circles). (D) B cells isolated from wild type (WT) B6 mice (solid green triangles, white
bar) and IL-10 KO mice (open green triangles, gray bar) show that only WT B cells reduced infarct volumes 3 d after tMCAo compared to PBS controls (black
T cells in the spleen, nor did they (F) induce a
circles; determined by one-way ANOVA). (E) WT B cell treatment did not differentially activate CD4
regulatory T cell population in the spleen. Significance determined by two-way repeated-measure ANOVA or Student’s t test (*P < 0.05, **P < 0.01 vs. PBS
control unless indicated by bracket).
CD25
+
+
4984 | www.pnas.org/cgi/doi/10.1073/pnas.1913292117
Ortega et al.
+
CD25
protection by naïve B cells was indicated neither by peripheral
+
T cells (Fig. 1E), nor by
suppression of activated CD4
the induction of splenic regulatory T cell population (Fig. 1F).
Together with prior studies showing no induction of regula-
tory T cells in the CNS by B cell adoptive transfer (10), our
data suggest a previously unreported and distinct mechanism
employed by the adoptive transfer of naive B cells during stroke
recovery.
B Cells Directly Promote Neuronal Viability and Dendritic Arborization
In Vitro. One regulatory immune cell-independent mechanism of
poststroke neuroprotection that could be induced by B cells is a
direct neurotrophic effect of B cells on neurons at risk for cell
death (14). Using an in vitro approach to determine a direct role
in neuronal protection, mixed cortical cells were subjected to
2 h of oxygen-glucose deprivation (OGD) followed immedi-
ately by addition of naïve B cells to the culture for 4 d (Fig. 2 A
and B). In the mixed cortical culture condition without B cells,
+
OGD caused loss of microtubule-associated protein (MAP)2
neurons (P < 0.001) and loss of arborization (P < 0.01; Fig. 2 C
+
and D). Addition of naïve B cells to cortical cells (0.1:1.0 ratio)
reduced both neuronal death (P < 0.05) and loss of dendritic
arborization (P < 0.05). In the absence of ischemic injury, the
addition of naïve B cells increased the number of surviving
neurons (P < 0.05; Fig. 2C) and increased dendritic
MAP2
arborization (P < 0.05, 0.1:1.0 ratio; P < 0.01, 1:1; Fig. 2D)
compared to cultures without B cells. Replication of these ex-
periments with naïve IL-10–deficient B cells showed no dose–
response effect on neuronal cell loss either with or without OGD
(Fig. 2E). In contrast, IL-10–deficient B cells still preserved
dendritic arborization after OGD, albeit at a higher concen-
tration (P < 0.05; Fig. 2F and SI Appendix, Fig. S2). Increased
dendritic arborization also occurred in the absence of OGD with
IL-10–deficient B cells (P < 0.05), suggesting that IL-10 is a re-
dundant mechanism that supports maintenance of mature neu-
rons with dendrites. In summary, these data confirm the
capability of naïve B cells for direct neuronal protection in vitro
by an IL-10 mechanism within the context of neuronal ischemic
injury.
E
C
N
E
I
C
S
O
R
U
E
N
Fig. 2. B cells induce a neurotrophic effect in mixed cortical cultures. (A) Experimental timeline for the placement of naïve B cells on culture after oxygen-
+
glucose deprivation (OGD) and prior to immunocytochemistry (ICC). (B) Images at 10× of microtubule-associated protein (MAP2)
neurons (red) for treatment
(txn) groups; higher-magnification image is also shown (Inset). (Scale bar, 50 μm.) (C) Increasing ratio of B cells to mixed cortical (MC) cells increased the
number of MAP2+ neurons, as well as (D) the number of MAP2+ neurons with dendrites, in the non-OGD experiments. OGD decreased overall numbers, with
only a 0.1:1.0 B cell:mixed cortical cell ratio preserving neuronal survival and dendritic arborization. (E and F) Experiments were replicated with IL-10–deficient
B cells (images shown in SI Appendix, Fig. S2). IL-10–deficient B cells (E) did not preserve cell survival after OGD, but (F) a 1:1 ratio did preserve dendritic
arborization after OGD. Replicate, independent experiments (each with interexperimental replicates) are shown by red circles for total n. Nonparametric one-
way ANOVA (Kruskal–Wallis) determined within-group significance, and t test was used for untreated non-OGD:OGD comparisons. Data graphed as mean ±
SD, and significance determined by nonparametric one-way ANOVA or Student’s t test (*P < 0.05, **P < 0.01, ***P < 0.001 vs. untreated control unless
otherwise indicated by brackets).
Ortega et al.
PNAS | March 3, 2020 | vol. 117 | no. 9 | 4985
B Cells Are Present within the Parenchyma of the Poststroke Brain. At
the whole-brain level, B cells are an abundant leukocyte pop-
ulation within the stroke-injured brain 48 h after stroke onset
(22, 23). In fact, the cortical and subcortical brain vascular en-
dothelium exhibits an up-regulation of CXCL13, a B cell homing
chemokine (22). Recent advances in volumetric whole-brain
imaging methods including serial two-photon tomography (STPT)
have enabled automated, unbiased methods to visualize and
computationally detect signals of interest, including fluorescently
labeled cell populations as well as neuronal substructures in the
entire brain (24–26). We established a custom pipeline including
STPT, supervised machine learning-based pixel classification, and
image registration to visualize and quantify adoptively transferred
immune cells labeled with the fluorophore e450 throughout the
whole mouse brain. We verified this methodology to accurately
+
T cell diapedesis into the whole brain after
quantify labeled CD8
tMCAo in Poinsatte et al., 2019 (27). The output of our machine
learning-based pixel classification step is visualized as a probability
map of pixels automatically detected by the trained algorithm as B
cells (Fig. 3A) (28). The brighter the area in the probability map,
the more likely the trained algorithm identified the fluorescence
as a B cell.
To quantify whole brain neuroinflammation, we used two
mice or
B cell donor littermate controls, with all
cohorts of mice: (i) B cell-depleted recipient hCD20
wild type (WT) hCD20
+
−
+
−
+
recipient mice receiving rituximab prior to tMCAo to target
B cells for depletion (29) (Fig. 3B); and (ii) B cell-
hCD20
sufficient C57BL/J6 mice with unaltered B cell populations. In
order to account for endogenous poststroke autofluorescence
secondary to ischemic injury and cell death, we included PBS
+
recipient cohorts. STPT detected signal from fluorescent e450
donor hCD20
B cells in both the ipsilesional and contralesional
hemispheres (Fig. 3C) of B cell-depleted recipient mice (P < 0.05
for both hemispheres vs. PBS; Fig. 3D). We also observed bi-
lateral e450
B cell signal in the B cell-sufficient cohort, albeit
with larger group variation (Fig. 3E). B cell recipients in both
B cells identified by flow
cohorts of mice exhibited e450
cytometry in both the cervical lymph nodes and spleen 4 d after
tMCAo (SI Appendix, Fig. S3), confirming the presence of live B
cells following adoptive transfer. The surprising increase of B
cells in the contralesional hemisphere indicates that B cell di-
apedesis is not only localized to infarct and periinfarct areas with
high cytokine and chemokine up-regulation, but there is also an
active recruitment from the periphery in brain regions remote
from the ischemic core.
+
Adoptively Transferred B Cells Localize to CNS Motor Nuclei and Areas
of Neurogenesis. We previously observed B cell infiltration into
the brain following stroke (22, 30). Now, understanding that B
cells could exert in vitro neuroprotection (Fig. 2), we wanted to
Fig. 3. Establishing whole-brain quantification of neuroinflammation using STPT. (A) Representative coronal section image acquired via STPT shown as a
multichannel raw fluorescence merged image. (Magnification: Left, 16×.) (Inset) e450
B cells present in the hippocampus (blue). (Right) Corresponding 2D
probability map from the same coronal section in which the trained machine-learning algorithm classified pixels likely to represent brain parenchyma (gray)
and e450+ B cells (magenta). A 3D rendering of the B cell and parenchyma probability maps for each section in the whole brain are shown (Right). (B) Timeline
for B cell depletion immediately prior to a transient middle cerebral artery occlusion (tMCAo), with adoptive transfer (AT) of e450+ B cells. (C) Whole-brain
images show a representative brain from the PBS- (Left) and B cell-treated (Right) cohorts. The probability maps of e450+ B cells are shown in green and
fluorescence
overlaid onto the average template from the atlas shown in grayscale. Ipsilesional (ipsi) hemisphere is identified. (D) Whole-hemisphere e450
(in pixels per cubic millimeter) is shown for hCD20
-depleted mice that received PBS (black squares) or B cells (red squares). Dashed lines show mean PBS
fluorescence that is used for normalization. (E) Similar to D, showing fluorescence in C57BL/6J mice that received PBS or B cells but without depletion of
endogenous B cells. Significance determined by two-way ANOVA (*P < 0.05 vs. respective PBS-treated control).
+
+
+
4986 | www.pnas.org/cgi/doi/10.1073/pnas.1913292117
Ortega et al.
determine if B cells were infiltrating bilateral brain areas favor-
able to poststroke functional recovery. To achieve specific lo-
calization of neuroinflammation, raw fluorescent STPT images of
every coronal section were registered with the corresponding
sections in the CCFv3.0 atlas (Fig. 4A) in order to assess cellular
+
B cells across brain regions of interest (Fig. 4B). Quantifi-
e450
cation of e450-labeled B cells in whole-brain STPT datasets
revealed brain regions with significant B cell diapedesis, including
ipsilesional cerebral cortex, olfactory areas, and hypothalamus
(Table 1). Contralesional areas with significant B cell diapedesis
included olfactory areas, dentate gyrus, and hypothalamus, creat-
ing a bilateral diapedesis of B cells into brain regions typically
spared in tMCAo-induced injury and that mediate motor and
cognitive recovery, as well as active neurogenesis. To determine if
endogenous B cells have an effect on adoptively transferred B
+
cells, we also adoptively transferred naive WT e450
B cells into
+
donor B
poststroke WT mice that were not B cell-depleted. e450
cells were again localized to the spleen and CLN after stroke (SI
Appendix, Fig. S3E). STPT detected e450
B cells throughout
+
B cell signal was not
the poststroke brain, even though e450
significantly elevated over PBS controls due to more within-group
fluorescent variation.
+
B cell diapedesis was elevated in five brain regions associated
with motor function (i.e., cerebral cortex, cortical subplate,
midbrain [sensory-related], cerebellum, and substantia nigra
[reticular]) in B cell-depleted mice, which are highlighted in 3D
surface renderings created by the Allen Institute for Brain Science
Brain Explorer application (Fig. 4C). All areas demonstrated a
+
B cell signal (100- to 200-fold higher
similar magnitude of e450
than PBS fluorescence), with ipsilesional signals significant in
E
C
N
E
I
C
S
O
R
U
E
N
Fig. 4. B cells show diapedesis into remote motor areas after stroke. (A) Serial two-photon tomography images are coregistered to the Allen Institute CCF3.0
+
to allow identification of region-specific fluorescence in 3D whole-brain probability maps. (Magnification: A, 16×.) (B) Representative areas classified as e450
B cells via machine learning (punctate magenta dots [Insets], identified by white arrows) that show B cell diapedesis in cortex and hippocampus (enlarged
areas indicated by white squares). (C) Three-dimensional surface renderings created with the Brain Explorer application (Allen Institute for Brain Science)
show regions with bilateral B cell diapedesis after stroke, with areas labeled to the letter corresponding to the data graphs. (D–H) Quantification of e450+ B
cell fluorescence in both B cell-depleted mice (red squares) and mice with endogenous B cells at time of stroke (black circles). Ipsilesional (ipsi, white bars) and
contralesional (contra, hatched bars) brain regions show predominantly ipsilesional B cell diapedesis for (D) cerebral cortex, (E) cortical subplate, (F) midbrain,
(G) cerebellum, and (H) substantia nigra with percent change (y-axes, pixels per cubic millimeter). Significance determined by paired t tests (*P < 0.05, **P <
0.01 vs. PBS controls unless indicated by brackets).
Ortega et al.
PNAS | March 3, 2020 | vol. 117 | no. 9 | 4987
Table 1. STPT data for e450
+
pixels for each brain region
Brain region
Gray matter
Cerebral cortex
Olfactory areas
Dentate gyrus
Cerebral nuclei
Striatum
Striatum ventral region
Cortical subplate
Hypothalamus
Midbrain, sensory related
Cerebellum
White matter
Corpus callosum
Ipsilesional, mm3
Contralesional, mm3
Allen Brain Atlas
abbreviation
PBS control
(n = 3)
B cells (n = 4)
P value
PBS control
(n = 3)
B cells
(n = 4)
P value
Laterality index
CTX
OLF
DG
CNU
STR
STRv
CTXsp
HY
MBsen
CB
CC
8.6
8.05
26.55
4.25
3.88
5.26
2.5
11.85
28.09
10.32
1.29
22.44
33.5
67.45
10.62
9.27
13.52
5.46
32.21
75.47
24.14
0.025*
0.019*
0.073
0.061
0.06
0.06
0.066
0.039*
0.056
0.061
11.64
10.1
30.2
8.09
8.16
12.18
6.45
12.35
35.38
12.96
26.62
32.46
55
18.78
18.34
21.09
9.15
36.1
85.27
22.32
0.155
0.041*
0.028*
0.202
0.227
0.17
0.514
0.020*
0.136
0.128
4.41
0.313
1.98
6.44
0.242
0.9
1.1
1.2
0.7
0.6
0.6
0.8
0.9
0.9
1.1
0.8
STPT, serial two-photon tomography. Significance between PBS and B cell recipients per hemisphere was analyzed by unpaired, parametric. Student’s
t test: *P < 0.05; bolded text, P ≤ 0.06.
+
cerebral cortex (P < 0.05). Ipsilesional B cell diapedesis was also
significantly higher compared to the contralesional hemisphere in
the cerebellum (P < 0.05; Fig. 4G). In contrast, B cell-sufficient
mice exhibited higher laterality for ipsilesional diapedesis, with
B cell signal localized to the ipsilesional cortical
more e450
subplate (P < 0.01; Fig. 4E) and midbrain (P < 0.05; Fig. 4F).
Interestingly, one motor region, the substantia nigra pars retic-
ulata, had much higher B cell diapedesis (1,000- to 2,000-fold vs.
PBS) in the mice with endogenous B cells versus B cell-depleted
mice (Fig. 4H), with highest values in the contralesional hemi-
sphere. In summary, these data show that, in a mouse devoid of B
cells, adoptively transferred B cells migrate to the motor areas to
a similar magnitude in both the ipsi- and contralesional hemi-
spheres, possibly exerting a supportive role in functional recovery.
B Cells Contribute to Long-Term Motor Function Recovery. As several
motor areas remote from the tMCAo-mediated infarction exhibi-
ted B cell diapedesis, we hypothesized that long-term depletion of
poststroke B cells could impede motor recovery. We tested this
mice or WT
with prestroke depletion of B cells in hCD20
−
littermate controls receiving rituximab, with continuous
hCD20
depletion for 2 wk after tMCAo (Fig. 5A and SI Appendix, Fig.
S4A). While an effect of B cell depletion on infarct volumes
between cohorts (Fig. 5B) was observed, there was no geno-
type effect on motor skill acquisition during rotarod training
(SI Appendix, Fig. S4B). WT mice exhibited a motor deficit at 2 d
after tMCAo (P < 0.001; Fig. 5C) that recovered by 4 d relative
to prestroke baseline. In contrast, B cell-depleted mice exhibited
a significant loss in poststroke motor function at 2 d (P < 0.01;
+
Fig. 5. B cells support motor recovery after stroke. (A) Experimental timeline for motor testing after transient middle cerebral artery occlusion (tMCAo).
Rituximab treatment in wild type (WT; black circles) and B cell-depleted (red squares) mice show (B) infarct volumes that were similar between cohorts. Cresyl
violet images for animals closest to the mean are shown. (Magnification: B, 20×, whole brain images.) (C) WT mice exhibited a motor deficit on a rotarod
2 d poststroke compared to prestroke baseline (horizontal gray bar) that (D) correlated to infarct volume. (E) B cell-depleted mice exhibited a loss in motor
performance 2, 4, and 14 d poststroke compared to prestroke baseline (red horizontal bar), an observation (F) independent of infarct volume. Significance
determined by Student’s t test, one-way repeated-measure ANOVA, or linear correlation (*P < 0.05, **P < 0.01, ***P < 0.001 vs. prestroke baseline). Dotted
lines indicate 95% confidence interval.
4988 | www.pnas.org/cgi/doi/10.1073/pnas.1913292117
Ortega et al.
Fig. 5E), 4 d (P < 0.01), and 14 d (P < 0.05) relative to prestroke
baseline. There were no significant between-group differences.
These data suggest that the absence of B cells after stroke could
potentially impede plasticity in the motor network(s), located
outside of the area of infarction, that support recovery of motor
coordination. B cell depletion, however, did not affect the muscle
strength, as analyzed by force grip analysis (SI Appendix, Fig. S4C).
Infarct volumes only in WT mice negatively correlated with motor
performance (Fig. 5D), with larger infarct volumes associated with
poorer motor performance but lost with B cell depletion (Fig. 5F).
With the observed bilateral B cell migration into brain regions
associated with motor function, combined with the behavioral
deficits in B cell-depleted mice, these data suggest that the pres-
ence of B cells may affect remote brain regions required for motor
recovery (11).
Poststroke B Cell Depletion Increases General Anxiety and Spatial
B
Memory Deficits. Initially, we observed significant e450
cell signal
in several brain regions (e.g., olfactory areas,
dentate gyrus, substantia nigra, and hypothalamus) also asso-
ciated with cognitive function (Fig. 6A) (31, 32). These areas,
with the exception of the substantia nigra, show high bilateral
e450
B cell signal. In the olfactory areas and the hypothalamus,
+
+
+
diapedesis of adoptively transferred B cells in B cell-depleted
mice was significant (P < 0.05) for both the ipsi- and con-
tralesional hemispheres (both P < 0.05 vs. PBS; Fig. 6 B and C).
The dentate gyrus is unique in that e450
B cell signal was sig-
nificant in the contralesional hemisphere (P < 0.05; Fig. 6D).
Both the olfactory areas and the hypothalamus also exhibit in-
creased signal in ipsi- vs. contralesional hemispheres, though the
latter, surprisingly, is in the B cell-sufficient cohort. Thus, we
sought to determine any associated poststroke cognitive deficits
(e.g., locomotor activity, anxiety, learning, and memory) with B
cell depletion extended through 8 wk after tMCAo (Fig. 6E).
Interestingly, while rituximab maintained B cell depletion for 8
cohorts (SI Appendix,
wk in both uninjured and tMCAo hCD20
Fig. S5A), WT poststroke mice also exhibited reductions in
splenic B cell representation compared to uninjured WT mice
(P < 0.05).
+
As with the 2-wk motor recovery cohort shown in Fig. 5,
there was no effect of long-term B cell depletion on infarct
volumes (Fig. 6F). For the cognitive tests, we first measured lo-
comotor activity using open field and found that the total distance
traveled decreased between day 1 and day 2 for both poststroke WT
(P < 0.01) and B cell-depleted (P < 0.05) cohorts (Fig. 6G).
E
C
N
E
I
C
S
O
R
U
E
N
Fig. 6. B cell depletion increases general anxiety and spatial memory deficits independent of infarct volume. (A) Brain Explorer surface rendering shows
brain regions with B cell diapedesis related to cognitive function, including (B) olfactory areas, (C ) hypothalamus, and (D) dentate gyrus, as indicated by
letter in the figure. Both B cell-depleted mice (red squares) and mice with endogenous B cells at time of stroke (black circles) show B cell diapedesis in
ipsilesional (ipsi, white bars) and contralesional (contra, hatched bars) brain regions. Fold change (y-axes) and significance vs. PBS controls shown unless
indicated by brackets. (E) Experimental timeline for behavior testing in uninjured mice (white bars) or after transient middle cerebral artery occlusion
(tMCAo; gray bars). (F ) B cell depletion did not affect infarct volumes or (G) total movement in the open field. (H) Both uninjured and poststroke B cell-
depleted mice spent more time in the periphery (“P”) of the open field compared to the center (“C”) of the field. (I) On the first day of cued and
contextual fear-conditioning, poststroke B cell-depleted mice exhibited prolonged freezing during the training tones/shocks. (J) The next day, these
same mice exhibited a worse spatial memory. (K) On the last day, B cell-depleted mice again exhibited more freezing during cued memory. Data graphed
as mean ± SD. Significance determined by paired t test, Student’s t test, or repeated-measures ANOVA (*P < 0.05, **P < 0.01 vs. nondepleted control or
D1 unless indicated by brackets).
Ortega et al.
PNAS | March 3, 2020 | vol. 117 | no. 9 | 4989
Interestingly, though all cohorts traveled similar distances, B
cell-depleted mice, regardless of injury, exhibited a preference
to travel in the periphery of the open field compared to WT
uninjured (P < 0.05) or stroke-injured mice (P < 0.01; Fig. 6H).
Subsequent nonaversive cognitive assessment by novel object
and novel location (33) failed to show differences between
cohorts based on either genotype or stroke (SI Appendix, Fig.
S5 C–F). Finally, we assessed hippocampal-dependent and
-independent forms of learning and memory using a contextual
and cued fear-conditioning paradigm, respectively. During the
training phase, there was a significant effect of genotype for
poststroke mice (P < 0.001), as B cell-depleted mice froze for
longer durations during the second, third (both P < 0.05; Fig.
6I), and final (P < 0.05; SI Appendix, Fig. S5G) tones. The next
day, evaluation of contextual, hippocampal-dependent memory
showed that B cell-depleted poststroke mice had worse recall
compared to WT mice (P < 0.05; Fig. 6J). In contrast, hippocampal-
independent (i.e., amygdala-mediated) cued memory recall was
exaggerated in B cell-depleted mice (P < 0.01; Fig. 6K). These
data suggest that long-term B cell depletion independently in-
fluences both hippocampal- and amygdala-dependent cognitive
functions after stroke.
B Cell Support of Poststroke Neurogenesis. Adult neurogenesis
occurs in the subventricular zone (SVZ) and the subgranular
zone (SGZ) of the dentate gyrus, within the hippocampus (34).
Stroke is also a potent inducer of neurogenesis (35, 36), al-
though the mechanism is still poorly understood. Interestingly,
of the 40 brain regions assessed for B cell migration in the
poststroke brain, the two associated with neurogenesis were
significant: olfactory areas, including the lateral olfactory tract,
and the dentate gyrus (Fig. 6 B and D). In fact, a greater mag-
nitude of e450
B cell signal over PBS controls occurred in the
dentate gyrus of mice with endogenous B cell populations, again
with an almost equivalent bilateral signal similar to the B cell-
depleted cohort. These data demonstrate that B cells exhibit sig-
nificant migration patterns into areas associated with neurogenesis
yet outside of the ischemic injury. We thus quantified hippocampal
+
neurogenesis 2 wk after tMCAo. Doublecortin-expressing (DCX
)
cells are immature neuroblasts generated in the inner granular cell
+
layer (GCL) of the hippocampal dentate gyrus (37), and DCX
cell
bodies are an index of neurogenesis. Two weeks of B cell depletion
+
+
cell numbers (Fig. 7B) and GCL volume (SI
did not affect DCX
Appendix, Fig. S6A) in otherwise healthy mice. Two weeks after
+
tMCAo, however, WT mice had more DCX
neuroblasts in the
dentate gyrus of the ipsilesional hemisphere compared to the
contralesional hemisphere (P < 0.01; Fig. 7C), consistent with
other studies (35, 38). In contrast, the B cell-depleted mice did not
exhibit increased poststroke neurogenesis (P < 0.001 vs. WT).
+
Changes (or lack thereof) in DCX
cell number were not asso-
ciated with changes in GCL volume (Fig. 7D). In combination
with the in vivo data (Fig. 6), these data suggest that B cells
contribute to both stroke-induced neurogenesis and poststroke
cognitive recovery, although removal of B cells does not affect
basal (i.e., homeostatic) neurogenesis. Next, we quantified hip-
pocampal cell survival via bromodeoxyuridine (BrdU) injection
prior to the first rituximab treatment in the cognitive cohorts
shown in Fig. 6. BrdU birthdates new neurons, and we determined
long-term (i.e., 8 wk) cell survival in the hippocampus following
continued poststroke B cell depletion. Basal cell survival in the
uninjured mice was unaffected by long-term rituximab treatment
+
(SI Appendix, Fig. S6B), similar to the DCX
population data.
+
Stroke induced an increase in the ipsilateral BrdU
neurons of
adult-generated hippocampal cells in the ischemic hemisphere of
WT mice 8 wk after tMCAo (P < 0.05 vs. contralesional hemi-
sphere), but not B cell-depleted mice (Fig. 7 E and F). As all mice
received rituximab to control for off-target drug effects, this con-
firms a role for B cells in sustaining neuronal cell survival in areas
outside of the ischemic injury.
Discussion
Under physiological conditions, neuroplasticity occurs through-
out life in cortical, subcortical, and cerebellar brain regions [e.g.,
olfactory areas (34), motor cortex (39, 40), hippocampus (34,
41), and cerebellum (42, 43)]. These areas are responsible for
brain development, neurogenesis, learning, and memory forma-
tion. Following stroke, the spinal cord and brain, including the
brain regions regulating motor and cognitive function, undergo
significant neuroplasticity to reinnervate injured areas and re-
organize neural networks supporting recovery (44–49). While
neuroplasticity occurring within the ipsilesional hemisphere can
improve functional outcome (46, 50–52), bihemispheric plasticity
in the contralesional hemisphere also supports recovery (53–57).
Fig. 7. B cells support poststroke neurogenesis. (A) Brain Explorer surface rendering shows neurogenic regions with bilateral B cell diapedesis after stroke. (B)
cells)
B cell depletion did not alter basal neurogenesis in the dentate gyrus in the absence of stroke. (C) Stroke induced neurogenesis (i.e., doublecortin [DCX]
in the ipsilesional (ipsi) hemisphere of wild type (WT; black circles) mice but not B cell-depleted (red squares) mice (D) independent of changes in granule cell
layer (GCL) volume. (E) Stroke increased bromodeoxyuridine (BrdU)
cells in the dentate gyrus over contralesional (contra) numbers only in WT mice, (F) as
shown by immunohistochemical detection of BrdU-positive cells, that was lost with long-term B cell depletion of healthy mice. Significance determined by
one-way ANOVA (*P < 0.05; **P < 0.01; ***P < 0.001 vs. ipsilesional hemisphere unless indicated by brackets).
+
+
4990 | www.pnas.org/cgi/doi/10.1073/pnas.1913292117
Ortega et al.
While our understanding of whole-brain neuroplasticity following
stroke is ever-evolving, few studies investigate neuroinflammation
in reorganizing brain regions. We previously found a high diape-
desis of B cells into the poststroke brain, with a concomitant up-
regulation of CXCL13 in cortical and subcortical brain areas (22,
23). Here, our advanced whole-brain imaging and analysis meth-
ods highlight significant bilateral migration of B cells to select
brain regions, including the aforementioned regions undergoing
poststroke plasticity, that are outside of the area of infarction and
thus distant to the epicenter of poststroke neuroinflammation.
B cells are part of the adaptive immune system, and are re-
sponsible for many immunological functions, including antibody
production, modulation of T cell responses, and antigen pre-
sentation (14). However, what is becoming increasingly apparent
in animal studies of stroke is that not only the location, but also
the timing and type, of B cell activation is critical in determining
the contribution to stroke injury and/or repair (10, 21). B cells
lack an acute (day 1 to 3 post stroke) physiological role in stroke
pathology, indicating that their effector function is irrelevant to
stroke etiology or innate immune modulation (20). B cells can
produce several neurotrophins capable of supporting plasticity
and neurogenesis, including brain-derived neurotrophic factor
(BDNF) and nerve growth factor (NGF), in addition to IL-10
(15, 58, 59). Our in vitro data confirm a neurotrophic effect of B
cells on the survival and health of neurons, as well as dendritic
arborization, in mixed cortical cultures. Interestingly, treatment
of mixed cortical cultures with IL-10–deficient B cells was not
neuroprotective for total neuronal counts, but a 1:1 ratio of IL-
10–deficient B cells to mixed cortical cells still protected arbor-
ization. This suggests that IL-10 is not the only neuroprotective
effector produced by B cells following oxygen-glucose depriva-
tion that should be addressed in future studies.
The neurotrophic effect of B cells is also reflected in our long-
term hippocampal neurogenesis and cell survival data, wherein
increases in both cellular processes require the active presence of
B cells after stroke. The adult brain has the capacity to induce
neurogenesis within the SGZ of the dentate gyrus and the SVZ
of the lateral ventricle (60). Ischemic insult significantly in-
creases neurogenesis in the SGZ and SVZ (61), with several
studies also suggesting that neuroblasts migrate from the SVZ
and SGZ to areas of ischemia, with the potential to adapt a
neuronal phenotype and integrate into existing circuitry (35, 62).
Others found that Copaxone (i.e., glatiramer acetate), which
promotes the development of regulatory T (63) and B (Breg)
cells (64, 65), induced both ipsi- and contralesional neurogenesis
in a murine model of stroke concomitant with improved recovery
(66), even though a specific B cell response was not investigated.
However, we did not see an effect of B cell depletion on basal
levels of neurogenesis or neuronal survival in otherwise healthy
young mice. Other forms of neuroinflammation, particularly the
microglial response (67), can modulate induction of poststroke
neurogenesis. However, microglia do not play a role in the age-
related decline of basal levels of neurogenesis in rats (68). Thus,
future studies should investigate whether a natural, age-related
decline in B cell lymphopoiesis, and thus declining circulating B
cells and their neurotrophic capacity (69), contributes to lower
basal neurogenesis with age. Of course, our study does not exclude
other neuronal regeneration mechanisms, and future studies could
use additional methods such as electrophysiology in order to more
fully elucidate the neurotrophic function of B cells.
Our data suggest several future directions for study. While
skilled motor rehabilitation improves motor function concomi-
tant with neurogenesis (70), we used several additional cognitive
tests to assess hippocampal-related recovery. Long-term B cell
depletion increased anxiety with a concomitant decrease in con-
textual fear memory, suggesting both hippocampal and amygdala-
related deficits, though these deficits were only present under
stressful testing conditions and not during nonaversive testing.
Additional tests should augment our cognitive testing, especially in
light of prior conflicting studies showing an active role of B cells in
the development of poststroke cognitive decline in mice (21). We
also previously identified that preconditioning down-regulated B
cell antigen presentation and antibody production (22) and that
poststroke B cell diapedesis in preconditioned mice correlated
with fewer CD4 T cells and macrophages in the ipsilesional
hemisphere (30). It was therefore understandably surprising to
find that the adoptive transfer of this novel B cell subset did not
reduce infarct volumes and, in fact, inhibited long-term motor
recovery. B cell adoptive transfer into Rag
mice did not show
evidence of poststroke neuroprotection either, indicating that B
cell neuroprotection may be dependent on multiple lymphocyte
subset synergism (18). It must be noted that our study used mature
adult mice, and further understanding would necessitate the in-
corporation of female and aged (>18 mo) mice. This interaction
with resident cells or, more intriguingly, the possibly detrimental
inability of interaction from anergic B cells suggests a complicated
poststroke immune response that potentially may be manipulated
for a much longer window of time to induce neuroprotection.
−/−
Several clinical studies confirm a role for the B cell immune
response in stroke, evident by the presence of immunoglobulins
in the CSF of stroke patients (71–73) and the presence of anti-
body deposits in the brain of individuals with poststroke dementia
(21). However, whether these are epiphenomena or represent an
active role of B cells in neuropathology and/or functional recovery
remains to be determined. Recovery occurs for months following
stroke onset in patients, with better recovery associated with an-
atomical and functional plasticity (74, 75) and angiogenesis (76) in
the ipsilesional hemisphere. Even though neuroplasticity occurs
rapidly and robustly within an acute time window after stroke,
neuroplasticity can last for years after stroke and support the long-
term improvement of functional outcomes (11, 77). As stroke
remains a leading cause of adult disability (1), it is vital to
identify mechanisms that can contribute to neuroplasticity in
neural networks. This includes new studies into long-term neu-
roinflammatory mechanisms that could be either detrimental or
beneficial to stroke recovery depending on the timing of activa-
tion, the responding leukocyte subset, and now also the remote
brain region(s) in which the responding immune cells migrate.
Materials and Methods
Mice. All experiments used male mice that were 2 to 4 mo old at the start of
experimentation and maintained in accordance to NIH guidelines for the care
and use of laboratory animals. UT Southwestern Medical Center approved all
procedures according to AAALAC accreditation and current PHS Animal Wel-
fare Assurance requirements. Transgenic human CD20+ expressing (hCD20+/−)
mice were obtained from Mark Shlomchik (University of Pittsburgh, Pittsburgh,
PA). C57BL/6J mice and B6.Cg-Tg(Thy1-YFP)16Jrs/J mice were purchased from
Jackson Laboratory, and Swiss Webster mice were purchased from Harlan.
Mice were group-housed in cages of 2 to 4 mice in standard animal housing
with cob bedding, a 12/12-h light cycle with lights on at 6:00 AM, and food and
water ad libitum. A total of 125 mice were used in experiments, with 84 un-
dergoing tMCAo surgery. A total of 23 were excluded (73% success), including
6 for failure to meet blood flow criteria, 16 for death during or after surgery,
and 1 for a lack of B cell depletion.
E
C
N
E
I
C
S
O
R
U
E
N
−/−
+/+
and hCD20
B Cell Depletion and Repletion. Rituximab (Micromedex) was given to
(littermate controls) at a standard dose of 100 μg i.p.
hCD20
for three consecutive days before tMCAo (29). Each mouse was administered
a weekly additional dose of rituximab thereafter to target the turnover of B
cells. Successful and sustained B cell depletion was confirmed by isolating
lymphocytes from spleen 2 or 8 wk post tMCAo that were stained with a
general antibody panel and quantified by flow cytometry (78–80). B cells
were purified from the splenocyte population using magnetic bead sepa-
ration (Stem Cell Technologies). Purity was verified by flow cytometry. A
total of 5 × 106 B cells were transferred i.v. in 0.2 mL 0.1 M PBS. B cells for
imaging were labeled with eFluor 450 (e450) proliferation dye (eBioscience
65–0842-85). Hemocytometer counts were not collected for one cohort of B
Ortega et al.
PNAS | March 3, 2020 | vol. 117 | no. 9 | 4991
cell-depleted mice in the long-term cognitive studies, so percent represen-
tation of CD45
cells is shown SI Appendix, Fig. S4A.
+
Statistical Analysis. Power analysis based on previous results and published
data determined the approximate number of animals given an expected 30%
stroke-induced mortality rate (80). Statistical differences were analyzed using
unpaired parametric two-sample Student’s t test, ratio paired Student’s t test,
one-way repeated-measures ANOVA, or two-way ANOVA where appropriate
and as indicated in the text (Graph Pad Prism 6.0). Values of P < 0.05 were
considered significant. All experimenters were blinded to condition, and all
animals were randomly assigned to group.
All detailed protocols for tMCAo induction, imaging (Tissuecyte, MRI),
histology, stereology, flow cytometry, motor and cognitive assays, and in vitro
culture assays are available in SI Appendix, Methods.
Data Availability Statement. All data discussed in the paper are available
to readers through Harvard Dataverse, https://doi.org/10.7910/DVN/RFGT4S.
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ACKNOWLEDGMENTS. The authors acknowledge Drs. Abhijit Budge,
Shanrong Zhang, and Shari Birnbaum for their technical expertise for imaging
and behavioral analyses and data acquisition. The authors also acknowl-
edge UT Southwestern’s Flow Cytometry Core, the Moody Foundation Flow
Cytometry Facility at the Children’s Research Institution, the Advanced Imaging
Research Center (Shared Instrumental Grant NIH1S10OD023552-01), Rodent Be-
havior Core Facility, the Whole Brain Microscopy Facility, and the Neuro-Models
Facility with Laura Ingle. This study was funded by grants to A.M.S. from the
American Heart Association (14SDG18410020), NIH/NINDS (NS088555), the Dana
Foundation David Mahoney Neuroimaging Program, and The Haggerty Center
for Brain Injury and Repair (UTSW); to S.B.O. from the American Heart Associa-
tion (14POST20480373) and NIH/NINDS (3R01NS088555-03S1); to V.O.T. from the
NIH/NIAID (5T32AI005284-40) and NIH/NINDS (3R01NS088555-02S1); to U.M.S.
from the American Heart Association (17PRE33660147); and to A.J.E. from the
NIH (DA023701, DA023555, MH107945) and the US National Aeronautics and
Space Administration (NNX15AE09G). S.E.L. and C.W.W. were funded by an NIH
institutional training grant (DA007290, Basic Science Training Program in the
Drug Abuse Research, Principal Investigator A.J.E.). The UT Southwestern Whole
Brain Microscopy Facility and the Neuro-Models Facility are supported by the
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10.1371_journal.pntd.0010231.pdf
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Data Availability Statement: De-identified data is
available online via the COR-NTD Research
Dataverse: https://dataverse.unc.edu/dataset.
xhtml?persistentId=doi:10.15139/S3/WOYRUW.
|
De-identified data is available online via the COR-NTD Research Dataverse: https://dataverse.unc.edu/dataset. xhtml?persistentId=doi:10.15139/S3/WOYRUW .
|
RESEARCH ARTICLE
Positive-case follow up for lymphatic filariasis
after a transmission assessment survey in Haiti
1☯*, Alain JavelID
Marisa A. HastID
1, Tara A. BrantID
Keri RobinsonID
Aurèle Telfort5, Christine Dubray1
2☯, Eurica Denis2, Kira BarbreID
1, Ryan WiegandID
1, Katherine GassID
3, Jonas RigodonID
3, Marc
4,
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
OPEN ACCESS
Citation: Hast MA, Javel A, Denis E, Barbre K,
Rigodon J, Robinson K, et al. (2022) Positive-case
follow up for lymphatic filariasis after a
transmission assessment survey in Haiti. PLoS
Negl Trop Dis 16(2): e0010231. https://doi.org/
10.1371/journal.pntd.0010231
Editor: Peter Steinmann, Swiss Tropical and Public
Health Institute, SWITZERLAND
Received: October 21, 2021
Accepted: February 1, 2022
Published: February 25, 2022
Copyright: This is an open access article, free of all
copyright, and may be freely reproduced,
distributed, transmitted, modified, built upon, or
otherwise used by anyone for any lawful purpose.
The work is made available under the Creative
Commons CC0 public domain dedication.
Data Availability Statement: De-identified data is
available online via the COR-NTD Research
Dataverse: https://dataverse.unc.edu/dataset.
xhtml?persistentId=doi:10.15139/S3/WOYRUW.
Funding: This work received financial support from
the Coalition for Operational Research on
Neglected Tropical Diseases, which is funded at
The Task Force for Global Health primarily by the
Bill & Melinda Gates Foundation, by the United
States Agency for International Development
through its Neglected Tropical Diseases Program,
1 Centers for Disease Control and Prevention, Atlanta, Georgia, United States of America, 2 IMA World
Heath, Port-au-Prince, Haiti, 3 Neglected Tropical Diseases Support Center (NTD-SC), Task Force for
Global Health, Atlanta, Georgia, United States of America, 4 Centers for Disease Control and Prevention
Country Office, Port-au-Prince, Haiti, 5 Ministry of Public Health and Population (MSPP), Port-au-Prince,
Haiti
☯ These authors contributed equally to this work.
* [email protected]
Abstract
Background
Lymphatic filariasis (LF) has been targeted for global elimination as a public health problem
since 1997. The primary strategy to interrupt transmission is annual mass drug administra-
tion (MDA) for �5 years. The transmission assessment survey (TAS) was developed as a
decision-making tool to measure LF antigenemia in children to determine when MDA in a
region can be stopped. The objective of this study was to investigate potential sampling
strategies for follow-up of LF-positive children identified in TAS to detect evidence of ongo-
ing transmission.
Methodology/Principle findings
Nippes Department in Haiti passed TAS 1 with 2 positive cases and stopped MDA in 2015;
however, 8 positive children were found during TAS 2 in 2017, which prompted a more thor-
ough assessment of ongoing transmission. Purposive sampling was used to select the clos-
est 50 households to each index case household, and systematic random sampling was
used to select 20 households from each index case census enumeration area. All consent-
ing household members aged �2 years were surveyed and tested for circulating filarial anti-
gen (CFA) using the rapid filarial test strip and for Wb123-specific antibodies using the
Filaria Detect IgG4 ELISA. Among 1,927 participants, 1.5% were CFA-positive and 4.5%
were seropositive. CFA-positive individuals were identified for 6 of 8 index cases. Positivity
ranged from 0.4–2.4%, with highest positivity in the urban commune Miragoane. Purposive
sampling found the highest number of CFA-positives (17 vs. 9), and random sampling found
a higher percent positive (2.4% vs. 1.4%).
Conclusions/Significance
Overall, both purposive and random sampling methods were reasonable and achievable
methods of TAS follow-up in resource-limited settings. Both methods identified additional
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1 / 18
PLOS NEGLECTED TROPICAL DISEASESand with UK aid from the British people. The
funders had no role in study design, data collection
and analysis, decision to publish, or preparation of
the manuscript. The authors received no specific
funding or salary for this work.
Competing interests: The authors have declared
that no competing interests exist.
Lymphatic filariasis follow-up in Haiti
CFA-positives in close geographic proximity to LF-positive children found by TAS, and both
identified strong signs of ongoing transmission in the large urban commune of Miragoane.
These findings will help inform standardized guidelines for post-TAS surveillance.
Author summary
Lymphatic filariasis (LF) is a debilitating parasitic disease that has been targeted for global
elimination. The transmission assessment survey (TAS) is a tool used to determine if LF
transmission has reached low enough levels that prevention activities can be stopped. This
study aimed to identify methods to investigate positive LF cases found during TAS. The
investigation was conducted in Nippes Department, Haiti, where 8 positive cases were
found in TAS in 2017. Participants were recruited through two methods: purposive selec-
tion of the closest 50 households to the positive case, and random selection of 20 house-
holds in the census enumeration area of the case. Participants completed a survey and
were tested for LF antigen, indicative of current infection, and parasite-specific antibody,
indicative of current or past infection. A total of 1,927 people participated in the study;
1.5% of these were antigen-positive, and 4.5% were antibody-positive. Purposive sampling
found a higher number of antigen-positive individuals, and random sampling found a
higher percent positive. Both sampling methods were feasible to use in this setting, and
both methods identified signs of ongoing transmission in a large urban area. Additional
research is needed to help standardize guidance for post-TAS surveillance to best identify
ongoing transmission.
Introduction
Lymphatic filariasis (LF) is a mosquito-borne parasitic disease caused by the filarial worms
Wuchereria bancrofti, Brugia Malayi, and B. timori, and is endemic to tropical areas in 72
countries [1]. The debilitating clinical disease caused by LF can result in fluid accumulation in
the extremities, resulting in lymphedema, hydrocoele, and acute adenolymphangitis. LF is one
of the leading causes of chronic disability worldwide, and it is estimated that LF was responsi-
ble for over 5 million disability-adjusted life years prior to the implementation of disease con-
trol programs [2]. Due to this high global burden, LF has been targeted for global elimination
as a public health problem since 1997 [3].
The primary strategy for LF control and elimination is the use of annual mass drug admin-
istration (MDA) for the entire population at risk for at least five consecutive years or until
local transmission is interrupted [4]. In order to define when this criteria has been reached
and MDA can be stopped in a region, the transmission assessment survey (TAS) was devel-
oped as a decision-making tool to determine when prevalence of LF has reached low enough
levels that transmission cannot be sustained, even in the absence of active control measures
[5].
The current World Health Organization (WHO) criteria states that TAS can be initiated
once pre-TAS sentinel site and spot checks show <2% LF antigenemia among the population
over 5 years old in a given evaluation unit (EU), which is typically a district or a combination
of districts [4]. As part of TAS, antigenemia in children aged 6–7 is systematically measured,
typically using a cluster survey of at least 30 schools, although some variations exist globally.
Measuring infection in children this age is relevant for LF since they are of sufficient age to
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
develop a mature parasite but young enough for a current infection to indicate recent trans-
mission. WHO guidelines then state that MDA can be stopped in the EU if prevalence of LF
antigenemia among children this age in the first TAS (TAS 1) is below 2% in regions where
Anopheles or Culex mosquitoes are the main vectors or below 1% where Aedes mosquito spe-
cies are the main vectors [4]. Once antigenemia falls below the appropriate threshold and
MDA is stopped, the EU must then pass 2 additional TAS (TAS 2 and TAS 3) over a period of
4–6 years. Once all EUs in a country successfully pass three TAS, the country is eligible to sub-
mit a dossier to the WHO to receive formal acknowledgement of validation of the elimination
of LF as a public health problem, indicating that prevalence in the population is below the
threshold to support onward transmission [6].
Since its inception in 2011, TAS has been widely integrated into national elimination pro-
grams worldwide, with over 1,000 EUs having already passed TAS 1 [7]. However, a continu-
ing challenge for LF programs is how to interpret and respond to antigen-positive children
identified in a TAS 2 or 3 survey that passes the overall threshold. Although a passing result
suggests that transmission has been interrupted, any positive result in young children without
travel to other regions is cause for concern regarding ongoing transmission, particularly if
those cases are clustered geographically or if the number of cases increases between surveys
[8]. Furthermore, there is some concern that a cluster-based survey might not be sensitive
enough to detect all hotspots of transmission, particularly in large or environmentally hetero-
geneous EUs [9,10].
Due to these concerns, the WHO currently encourages program managers to conduct fol-
low-up surveys in communities where antigen-positive children are detected [4]. However, lit-
tle guidance exists on how follow-up should be conducted, what threshold should trigger a
programmatic response, or what this response should entail. Given the recent evidence of
residual LF transmission or resurgence in Sri Lanka and American Samoa following multiple
passed TAS, additional research is needed to help guide these programmatic decisions and bet-
ter determine the utility of TAS for measuring interruption of transmission [11–13]. Addi-
tional research is also needed to determine the role of emerging tools, including the use of
antibody testing which may detect both current and past infection, and how these complement
antigen detection in the context of identifying ongoing transmission.
Haiti is one of only four countries in the Americas where transmission of W. bancrofti still
occurs [7]. In 2001, it was determined that LF endemicity was widespread throughout the
country, and the decision was made to conduct MDA nationwide. By 2012, MDA was con-
ducted in all 140 communes (equivalent to districts) [14]. As of 2020, 122 of these communes
had reached the WHO criteria to stop MDA, many of which had low or moderate LF transmis-
sion at baseline. However, the remaining 18 communes have had persistent LF transmission
despite more than 10 years of MDA, and other communes have had an increase in antigen-
positive children despite continuing to pass their TAS. In the context of potential continuing
transmission, it is critical to follow-up positive cases from TAS 2 and TAS 3 to identify any
areas where targeted MDA may be warranted to sustain the gains made towards LF elimina-
tion. The objective of this study was to identify potential sampling strategies for positive case
follow-up after a TAS using antigen and antibody detection that optimizes the chances of cor-
rectly identifying evidence of ongoing transmission in Haiti, while saving program resources.
Methods
Ethics statement
This study was approved by the National Bioethical Committee in Haiti (1718–84) and the Sci-
entific Internal Review Board at the CDC (2018–430). Formal informed consent was obtained
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
by all participants or parents/guardians of children <18 years old. All study participants were
read a consent form in Haitian Kreyol by the survey team and provided verbal informed con-
sent or parental consent, and children aged 7–17 years provided verbal informed assent. A
written copy of the consent form in Haitian Kreyol and the study investigator’s phone number
was left with each household. Consent for collecting geographic coordinates was obtained
from the head of household. All data were stored on secure servers and password-protected
computers. Results of biological testing were kept confidential and only were shared with the
study participant or their guardian. Individuals with positive test results were offered treat-
ment with the standard of care in Haiti.
Study site
The site for this study was the department of Nippes, Haiti, which has a population of approxi-
mately 342,000 and is comprised of 11 communes [15]. The most populous commune is Mira-
goane, which has more than 62,000 residents and contains the department capital. Due to a
low baseline prevalence of <5%, all communes were combined into one EU for the LF elimi-
nation program, so the whole department is evaluated for TAS together. The department suc-
cessfully received five consecutive rounds of MDA from 2009–2013 with sufficient coverage,
defined as �65% of the population. TAS 1 was conducted in 2015 using a cluster survey of 30
primary schools, and two children were identified as antigen-positive using the rapid filariasis
test strip (FTS) (Alere, Scarborough, ME), which detects circulating filarial antigenemia (CFA)
for adult worms. This was below the critical cutoff of 2% for regions with Culex vectors, and
MDA in the department was stopped. Nippes underwent TAS 2 in 2017 and passed again,
however the number of CFA-positive children had increased to eight. Of these, four came
from the commune of Miragoane, with two residing across the street from each other in a
dense urban area. The four other CFA-positive children were located in the communes of
Anse-a-Veau, L’Asile, Petit-Trou de Nippes, and Plaisance du Sud.
Study design and sampling
Each CFA-positive child identified in TAS 2 was considered an index case. The residential
locations of the index cases were plotted in ArcGIS Version 10.7 (ESRI, Redland, CA), and
each case was mapped to an Enumeration Area (EA) for follow-up (Fig 1). EA boundaries
were previously determined by the Haitian Ministry of Health and Ministry of Statistics for
use with the census and the Demographic Health Survey and range from 0.02–30.8 square
kilometers. The index case in Anse-a-Veau had moved recently from a more rural area, so
both the case’s current location and previous residence were mapped to their respective EAs
for follow-up. Purposive and random sampling methods were used to select participants for
this study.
Purposive sampling
For each index case, the location of the index case household was identified by the field team
using global position system (GPS) coordinates. The index household and the 50 closest house-
holds by straight-line distance were selected for inclusion in the sample. Fifty was chosen since
it was the maximum deemed to be feasible and sustainable using this method. In all selected
households, head of household consent was obtained, and household coordinates were col-
lected on electronic mobile devices. If any of the 50 nearest households declined, it was
replaced with the next nearest household until 50 had been enrolled.
To identify the 50 nearest households to each index case, structures surrounding index case
households were enumerated using high-definition satellite images (DigitalGlobe, Denver,
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Fig 1. Locations of antigen-positive lymphatic filariasis cases identified in TAS 2, Nippes Department, Haiti 2017. Exact locations are
jittered for participant confidentiality. Shapefiles for administrative boundaries are from the Centre National d’Information Geo-Spatiale
and are available at https://data.humdata.org/dataset/hti-polbndl-adm1-cnigs-zip.
https://doi.org/10.1371/journal.pntd.0010231.g001
CO), and the proportion of inhabited structures in that EA was calculated using geo-linked
census data. Using a projected non-response/refusal rate of 10%, an approximate radius was
calculated around each index household to encompass the 50 households anticipated to partic-
ipate. A buffer of the appropriate radius was developed in ArcGIS for each index case, and
these shapefiles were loaded onto Garmin GPSMAP 64 handheld GPS devices (Olathe, KS)
and Locus Map software (Prague, Czech Republic) for use by the field team. Once the index
household was identified, field teams started at the index house and proceeded outwards in
concentric circles until 50 households had been enrolled, using the buffer shapefile as a guide.
Due to their close proximity, the two Miragoane index cases in the same EA were treated as a
unit and a purposive circle was drawn around the midpoint between the two houses.
Random sampling: Index EA
In each index case EA, field teams conducted a comprehensive census in the EA to identify
and number all occupied households. The boundaries of the EA were determined using maps
and GPS tools, and every structure in the EA was categorized as a household or non-house-
hold. Each occupied household was given a number, and 20 households were selected for
inclusion using systematic random sampling, which was the maximum deemed to be feasible
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
and sustainable using this method. A sampling interval was determined by dividing the total
number of households by 20 and rounding down to the nearest whole number. A random
start was selected between 1 and the sampling interval using random number generating soft-
ware. A list of selected households was developed by serially adding the sampling interval to
the random start until 20 households had been selected. At each selected house, head of house-
hold consent was obtained, and household coordinates were collected on electronic mobile
devices. If any of the selected households declined to participate, it was not replaced.
Random sampling: Neighbor EA
If any participant in a selected household from either purposive or random sampling tested
CFA-positive for LF (methods to follow), additional random sampling of 20 households was
conducted in each of the two neighboring EAs nearest to the positive case. For these neighbor-
ing EAs, sampling methods were identical to random sampling conducted in index case EAs,
including conducting the census, household numbering, identification of a sampling interval
and random start, listing of selected households, and head of household consent.
Field methods and sample collection
Field data collection occurred from July to August 2019. In selected households, all household
members aged 2 years and older were invited to participate in the sample. Adults provided
informed consent or parental permission for their children under 18 years, and children aged
7–17 years provided informed assent. Exclusion criteria included age under 2 years, having
another primary residence, and inability to provide informed consent due to physical or men-
tal incapacity. All consenting household members were given a unique barcode and adminis-
tered an electronic questionnaire using Secure Data Kit software (Atlanta, GA). The
questionnaire collected information on participant demographics, time living in the EA, his-
tory of travel, participation in the most recent MDA, and use of bed nets.
All consenting participants provided approximately 250μl of blood, which was collected by
finger stick into heparinized collection tubes. Collection tubes were marked with a matching
barcode to the participant and were not otherwise marked with any personally identifying
information.
Antigen testing was done at point-of-collection with FTS using standardized methods [16].
In brief, 75 μL of blood were pipetted from the heparinized tubes onto the test sample pad and
allowed to flow through the strip. After exactly 10 minutes, the result window was read for a
positive, negative or invalid CFA result. Any positive or invalid FTS were repeated with a sec-
ond confirmatory FTS. Individuals with two positive FTS were counted as CFA-positive, and
individuals with one or more negative FTS were counted as CFA-negative. Tubes with the
remainder of the blood samples were then transported to the field laboratory in a portable
cooler, where dried blood spots (DBS) were prepared for each participant. Ten μL of heparin-
ized blood were pipetted onto each of six extensions of Trop Bio filter paper (Cellabs, Sydney,
Australia) for a total sample of 60 μL. Filter paper was labeled with the unique barcode for the
participant, allowed to dry, and packed with desiccant in labelled bags until transport to the
National Laboratory of Public Health in Port au Prince, where they were stored at -20˚C.
Individuals with two positive FTS were treated with the standard combination of albenda-
zole and diethylcarbamazine (DEC), with dosage calculated based on the age of the participant
following standard procedure in Haiti. Pregnant women were eligible for participation in the
study; however, due to the unknown effects of these medications in utero, pregnant partici-
pants who tested CFA-positive were advised to seek treatment for LF a week after delivery.
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Laboratory analysis
Preserved DBS were transported to the Centers for Disease Control and Prevention (CDC) in
Atlanta, GA where they were tested for IgG4 antibodies against the recombinant Wb123 anti-
gen using the Filaria Detect IgG4 ELISA kit (InBios, Seattle, WA), a direct enzyme immunoas-
say. The assay was performed according to the standard operating procedure provided by the
manufacturer with minor modifications, as described previously [17]. In brief, blood spot
extensions of DBS and positive and negative controls were diluted 1:50 in kit-provided sample
buffer and stored overnight at 4˚C. Samples and controls were added to plate wells, sealed, and
incubated at 37˚C for 30 minutes, washed using an automated plate washer and kit-provided
wash buffer, incubated again with mouse anti-human IgG4 conjugated with horseradish per-
oxidase for another 30 minutes, and washed again. Plates were developed at room temperature
in the dark for 13 minutes with an added 100 μL of tetramethylbenzidine substrate in each
well, stopped using kit-provided stop solution, and incubated for one minute. Plates were read
on a microplate reader at 450 nm. To compare optical density (OD) values across plates the
OD values were normalized by dividing the mean OD of the sample by the mean OD of the
H3-positive control from the same plate. Additional details are described in Supplementary
Materials S1 Text.
Data analysis
Cutoff determination for ELISA OD values.
In order to analyze the ELISA OD values as
a dichotomous variable, a fixed finite mixture model (FMM) [18] was fit to the serology OD
dataset to determine a cutoff using the flexmix, mixtools, mixsmsn and sn packages in R version
4.0.2 (R Core Team, Vienna, Austria). These models use maximum likelihood estimation to fit
a two-component FMM to the data to estimate the parameters of “seropositive” and “seroneg-
ative” distributions [19,20]. Each component was fitted with a normal or skew-normal distri-
bution to log-transformed OD values and assumed to be independent of age. The ELISA value
at which the probability of positive was greater than 0.5 was used as the cutoff, which is also
the point where the two distributions intersect [21]. Values above the cutoff were determined
to be seropositive and values below were considered seronegative.
Statistical analysis. All analyses were done in Stata 13.1 (Stata Corporation, College Sta-
tion, TX) and R version 4.0.2 statistical software. Frequencies of demographic and behavioral
characteristics of the study population were calculated. Both CFA and serology results are
described by participant characteristics and sampling method, and bivariate comparisons were
conducted using chi-squared and Fisher’s exact tests. For purposively sampled households, the
proportion and number CFA positive were compared by increasing number of sampled
households from the index case house (e.g., closest 10, closest 20, etc.). To better visualize their
distribution, the natural log of serology OD values were plotted against participant characteris-
tics in scatterplots.
Exploratory analyses were conducted both by index case and by geographic zone. Index
cases were defined by number as cases 1–8. The two index cases in the same EA in Mira-
goane, designated as 1a and 1b, were analyzed together as index case 1 due to their close
proximity and resulting inability to differentiate in sampling. Geographic zones were defined
as Miragoane (containing index cases 1a, 1b, 2, and 3), L’Asile (index case 4), Plaisance du
Sud (index case 5), Petit-Trou de Nippes (index case 6), Anse-a-Veau rural (index case 7),
and Anse-a-Veau urban (index case 8). As described above, index cases 7 and 8 were the
same individual but were analyzed separately since he or she resided in the two zones at dif-
ferent times.
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Results
Study population
A total of 1,927 participants from 786 unique households completed the survey and FTS test-
ing. Of these, nearly 40% were male and 18% were under age 10 years (Table 1). Nearly half of
participants resided in the commune of Miragoane, with 8–14% residing in each of the other 5
geographic zones. Forty percent of participants were students, 20% listed commerce as their
primary occupation, and 15% did not have a stated occupation. Approximately one fifth of
participants reported sleeping under a bed net the previous night, and a quarter reported travel
outside their commune in the past year. Among participants aged 12 and above who would
have been eligible to take MDA during the last administration, 65% reported ever taking medi-
cations for LF as part of MDA in the past.
By mode of sampling, 63% of participants were selected by purposive sampling, 20% were
selected by random sampling in the index case EA, and 26% were selected by random sam-
pling in a neighboring EA. Nine percent of participants (175) were selected for both purposive
and either index case EA or neighbor EA random sampling, and thus these numbers add to
more than 100%.
Antigen results (CFA)
Of the 1,927 participants who completed FTS testing, 29 were CFA-positive, for a total positivity
rate of 1.5% (Table 2). Of these, 21 (72%) were from Miragoane, and each index case in this
commune led to the identification of CFA-positive participants, with the number found per
index case ranging from 6 to 8 (Fig 2). An additional 3 and 4 CFA-positive participants were
found in Anse-a-Veau rural and urban zones, respectively, 1 was found in L’Asile, and no CFA-
positive participants were found in Plaisance du Sud or Petit-Trou de Nippes (S1 Table). Over-
all, 6 of the 8 original index cases (75%) were linked to at least one CFA-positive participant.
Miragoane also had the highest rate of CFA positivity, with 2.4% of participants testing positive
compared to the range of 0.0%–1.8% in other geographic zones (Chi squared P value = 0.03).
Two CFA positives were found among participants aged <10 years (positivity 0.8%), both
of which resided in Miragoane and were between the ages of 4 and 6 years. CFA positivity
rates were slightly higher among participants aged 20–44 years (2.4%) compared to other age
bands; however, this difference was not statistically significant (P = 0.08). Positivity was slightly
higher among participants who did not sleep under a bed net (1.6% vs. 1.0%) or did not take
MDA in past (2.3% vs. 1.5%) compared to those who did; however, these differences also were
not statistically significant (P = 0.4 and 0.3, respectively). Rates of positivity were similar by
participant sex and history of travel.
Purposive sampling identified 17 CFA-positive participants for a positivity rate of 1.4%, ran-
dom sampling in the index case EA identified 9 positive participants for a positivity rate of
2.4%, and random sampling in a neighboring EA identified only 3 positive participants for a
positivity rate of 0.6% (Table 2). Thereby, purposive sampling identified the highest number of
CFA-positive participants, but random sampling in the index case EA returned the highest per-
cent positive. Among the 6 index cases that yielded any CFA-positive cases in this investigation,
purposive sampling found positives for 5 index cases in 3 geographic zones (Miragoane, rural
and urban Anse-a-Veau), and random sampling in the index EA found positives for 4 index
cases in 3 geographic zones (Miragoane, L’asile, urban Anse-a-Veau) (S1 Table). Both of these
sampling methods missed cases in one zone each. Positivity rate by geographic zone ranged
from 1.3–2.7% for purposive sampling and 2.0–9.6% for random sampling. Random sampling
in a neighboring EA found one additional CFA-positive participant for 3 of the 6 index cases.
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PLOS NEGLECTED TROPICAL DISEASESTable 1. Demographics and participant characteristics among survey respondents in Nippes Department, Haiti,
July-August 2019. N = 1,927.
Lymphatic filariasis follow-up in Haiti
Sex
Male
Female
Age in years
<10
10–19
20–44
�45
Commune of residence
Miragoane
L’Asile
Plaisance du Sud
Petit-Trou de Nippes
Anse-a-Veau rural
Anse-a-Veau urban
Occupation
Student
Commerce
Agriculture1
Manual labor
Public sector
Private sector
None
Other
Missing
Slept under bed net last night
Yes
No
Traveled outside commune past year
Yes
No
Have taken MDA in past2
Yes
No
Don’t know
Sampling method3
Purposive
Random (index)
Random (neighbor)
Total
n
742
1,185
351
461
702
413
861
268
158
152
268
220
776
378
157
71
32
19
288
86
120
392
1,535
500
1,427
943
488
26
1,221
381
500
1927
%
38.5%
61.5%
18.2%
23.9%
36.4%
21.5%
44.7%
13.9%
8.2%
7.9%
13.9%
11.4%
40.3%
19.6%
8.1%
3.7%
1.7%
1.0%
15.0%
4.5%
6.2%
20.3%
79.7%
26.0%
74.0%
64.7%
33.5%
1.8%
63.4%
19.7%
25.9%
100%
1 Includes farming or fishing
2among participants aged 12 years and above
3 adds to more than 100% because 175 participants were from households selected for both purposive and random
sampling; MDA = mass drug administration
https://doi.org/10.1371/journal.pntd.0010231.t001
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PLOS NEGLECTED TROPICAL DISEASESTable 2. Filariasis test strip (FTS) and serology results by participant characteristic, Nippes Department, Haiti, July-August 2019. FTS N = 1927; Serology
N = 1,914.
CFA Positive n (%)
P value�
Serology Positive n (%)
P value�
Lymphatic filariasis follow-up in Haiti
Sex
Males
Females
Age in years
<10
10–19
20–44
�45
Slept under bed net last night
Bed net
No bed net
Travel outside commune past year
Yes
No
Have taken MDA in past
Yes
No
Geographic zone
Miragoane
L’Asile
Plaisance du Sud
Petit-Trou de Nippes
Anse-a-Veau rural
Anse-a-Veau urban
Sampling method
Purposive sampling
Random (index)
Random (neighbor)
Total
0.7
0.08
0.4
0.8
0.3
0.03
0.08
12 (1.6%)
17 (1.4%)
2 (0.8%)
5 (1.1%)
17 (2.4%)
5 (1.2%)
4 (1.0%)
25 (1.6%)
8 (1.6%)
21 (1.5%)
14 (1.5%)
11 (2.3%)
21 (2.4%)
1 (0.4%)
0 (0.0%)
0 (0.0%)
3 (1.1%)
4 (1.8%)
17 (1.4%)
9 (2.4%)
3 (0.6%)
29 (1.5%)
43 (5.8%)
44 (3.7%)
11 (3.1%)
14 (3.0%)
35 (5.0%)
27 (6.6%)
9 (2.3%)
78 (5.1%)
27 (5.4%)
59 (4.2%)
42 (4.5%)
22 (4.6%)
43 (5.1%)
9 (3.4%)
6 (3.8%)
9 (6.0%)
13 (4.8%)
6 (2.7%)
62 (5.1%)
15 (4.0%)
16 (3.2%)
87 (4.5%)
0.02
0.06
0.02
0.2
0.9
0.5
0.2
�P values were Chi squared tests or Fisher’s Exact tests as appropriate; CFA = circulating filarial antigen
https://doi.org/10.1371/journal.pntd.0010231.t002
Among purposively sampled households, average CFA positivity was highest in the closest
10 households to the index case at 1.6%, declined to 1.4% in the 20 closest households, and
then remained relatively stable at 1.3%, 1.3%, and 1.4% in the closest 30, 40, and 50 households
respectively. However, these differences were not statistically significant, and there was sub-
stantial variation by index case and geographic zone (Figs 3 and S2). For 4 of 5 index cases
with purposively identified CFA-positive participants, the majority of these were found within
the 20 closest households to the index household, and prevalence in these households was
higher than random sampling for 3 of 5 index cases (S1 Table and S1 Fig). The primary excep-
tion to this was for Miragoane index case 2, which had >9% positivity among randomly sam-
pled participants compared to 2.4% positivity among purposively sampled households.
Serology results (ELISA OD values)
Of the 1,927 participants who received FTS testing, 1,914 (99.3%) also provided DBS for serol-
ogy analysis. Normalized mean OD values from ELISA testing ranged from 0.04 to 4.5, with a
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Fig 2. Locations of individuals positive for circulating filarial antigen (CFA) identified through purposive or random sampling in
relation to their index case, Nippes Department, Haiti July-August 2019. Exact locations are jittered for participant confidentiality.
Shapefiles for administrative boundaries are from the Centre National d’Information Geo-Spatiale and are available at https://data.
humdata.org/dataset/hti-polbndl-adm1-cnigs-zip.
https://doi.org/10.1371/journal.pntd.0010231.g002
mean of 0.11. The cutoff for serology positivity determined by FMM methods was 0.18. Using
this cutoff, there were 87 serology-positive participants, for a seropositivity rate of 4.5%. Con-
cordance with CFA antigen results was 95%, with 6 participants positive by both methods,
1,813 negative by both methods, 23 CFA-positive only, and 81 seropositive only.
Seropositivity was higher than CFA positivity across every category, however the size of the
difference varied (Table 2). Seropositive participants were found for all 8 index cases, with pos-
itivity rates ranging from 2.7–6.0% (S2 Table). The distribution of log-transformed OD values
across participant characteristics can be seen in Fig 4. The highest number of seropositive par-
ticipants was found in Miragoane (43, 5.1% positive), but the highest percent seropositive was
found in Petit-Trou de Nippes (6.0% positive), which had no CFA positives. There were no sig-
nificant differences in seropositivity by index case or geographic zone (Table 2 and Fig 4).
Eleven seropositive results were found in participants <10 years (3.1%), and seropositivity
increased by age to 6.6% in participants aged �45 years, although this increase was not statisti-
cally significant (Table 2). Seropositive children were aged 4–9 years and were located in Mira-
goane, rural Anse-a-Veau, and Petit-Trou de Nippes. Seropositivity was higher among male
(5.8%) than female (3.7%) participants (P = 0.02) and was higher among participants who did
not sleep under a bed net (5.1%) than those who did (2.3%) (P = 0.02) (Table 2 and Figs 4 and
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Fig 3. Circulating filarial antigen (CFA) prevalence by geographic zone, index case, and number of purposively sampled households by
increasing distance from index case household, Nippes Department, Haiti, July-August 2019.
https://doi.org/10.1371/journal.pntd.0010231.g003
S3). Seropositivity was similar among participants who did or did not participate in MDA for
LF in the past. By sampling method, seropositivity was 5.1% by purposive sampling, 4.0% by
random sampling in the index case EA, and was 3.2% by random sampling in neighboring
EAs. Purposive sampling found at least one seropositive participant for all 8 index cases, ran-
dom sampling in the index EA found seropositive participants for 7 of 8, and random sam-
pling in neighboring EAs found seropositive participants for 4 of 8 index cases.
Discussion
This investigation describes findings for several methods of follow-up for CFA-positive chil-
dren identified in TAS 2 in the Department of Nippes, Haiti. From 8 initial index cases in 6
geographic zones, a total of 29 additional CFA-positive individuals were identified out of 1,927
tested, and CFA-positives were found during follow-up for 6 of the 8 index cases. High rates of
CFA positivity were found in the commune of Miragoane (2.4%).
Overall, both purposive and random sampling methods detected additional CFA-positive
persons in the vicinity of most index cases, and both methods identified a high positivity rate
in Miragoane. Purposive sampling tested, found, and treated the highest number of CFA-posi-
tives, and this method found follow-up CFA-positive participants for a higher number of
index cases. Correspondingly, random sampling in the index case EA returned the highest per-
cent positive and was therefore most efficient at identifying additional cases. Random sam-
pling in neighboring EAs returned both a low number and percent positivity, indicating that
this additional element may be of limited usefulness in the future.
Considering use of these sampling methods in the resource-limited context of Haiti, purpo-
sive sampling tested a higher number of households (50 per index case compared to 20) and
therefore was more resource-intensive for both field staff hours and study materials, but
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Fig 4. Log normalized mean optical density (OD) values for IgG4 antibodies against the recombinant Wb123 antigen by participant characteristics. Red
line indicates cutoff for seropositivity.
https://doi.org/10.1371/journal.pntd.0010231.g004
random sampling was more time-consuming overall due to the need for a census of the index
EA in order to select a random sample, which took 2.2 days per EA on average. Interestingly,
purposive testing of only the closest 20 households to the index case yielded a similar percent
positivity as the closest 50 households in sub-analyses, which corresponds to previous findings
in Haiti that additional LF cases may be clustered close to the index case [22]. Purposive sam-
pling of fewer households may therefore be an option in the future to save resources, although
more research is needed to confirm this across settings and species of LF. Random sampling
might also not be as time intensive if countries have already performed the appropriate census
in advance, if satellite mapping could be used to enumerate households, or if alternatives to
random sampling such as segmentation could be used. As a whole, both random and purpo-
sive sampling had merits and continue to be potential methods for TAS follow-up.
In this setting, having a higher number of index cases was also correlated with a higher per-
cent positivity. Four of the original index cases were found in Miragoane, and percent positiv-
ity in this geographic zone was 2.4% compared to 0.0–1.8% in the other 4 zones where only
one index case was found. Despite this result, sample sizes were too small to draw definitive
conclusions, and percent positivity approached the 2% cutoff in the urban zone of Anse-a-
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Veau despite having only one index case. These observations indicate that, although having
multiple index cases in an area might suggest heightened chance of ongoing transmission, at
this time the conservative choice still would be to follow up every positive case found in TAS.
Of importance for the LF elimination effort in Haiti, the CFA prevalence of 2.4% in Mira-
goane was higher than the 2% cutoff typically needed in pre-TAS sentinel checks to initiate the
TAS process and stop MDA in regions with Culex vectors [4]. The two CFA-positive children
under 7 years were also found in Miragoane, which is concerning since MDA was stopped in
Nippes eight years prior and might be a further indication of ongoing transmission. This is a
change from historical data, as Miragoane had no positive LF cases during initial mapping; how-
ever, the dramatic urbanization of the commune and influx of people from rural areas might have
resulted in a higher concentration of cases and thereby allowed low levels of transmission despite
the pressure of MDA. As shown in previous research, urban areas can have unique barriers to LF
elimination, including high community mobility and lower compliance with MDA [23,24]. As a
result of this study’s findings, the Haiti National Program to Eliminate LF has decided to adjust
the practice of combining all the Nippes Department communes for the upcoming TAS 3 and
will evaluate Miragoane separately from the rest of the department. This will likely provide a more
sensitive result and will identify whether the commune needs to resume MDA.
This study was also enriched by antibody testing, which provide a more thorough picture of
LF in Nippes. As seen in other studies [25,26], a higher proportion of participants were sero-
positive than CFA-positive since antibody responses may be seen in both past and present LF
infection [27]. Seropositivity was not significantly different by geographic zone and was not
correlated with number of index cases, but was higher among males, older adults, and among
participants who reported not sleeping under a bed net. This might indicate higher prevalence
of lifetime infection in these groups, consistent with other studies [28]. Of note, seropositivity
in this population was approximately 3% in both children under 10 years and children aged
10–19 years. Seropositivity in the youngest age group could indicate persistent or recurrent LF
transmission since infection was likely acquired after MDA was stopped eight years prior to
the study and it takes approximately three years to develop antibodies after initial infection
[29]. Antibody response to Wb123 has also been correlated with molecular xenomonitoring
results in prior studies, further suggesting that ongoing transmission may be occurring [25].
However, this could also indicate residual seropositivity following interruption of transmission
in the older children. Continuing vigilance in this population is warranted to determine if anti-
body responses are indicative of ongoing transmission.
Similar to previous investigations [30–32], individual-level concordance of Wb123-specific
antibody and CFA antigen was poor in this investigation. Eighty-one participants (4%) were
antibody positive only, which can be explained by past infection and persistent antibody
response. However, 23 participants (1%) were CFA-positive only, which constituted a high
proportion of the total 29 CFA-positives. This could potentially be due to recent infection or a
less durable antibody response in some individuals [27,29], but further research is needed to
characterize the relationship between LF antibody and antigen response to better understand
the utility of these markers during post-MDA surveillance. Therefore, antibody results appear
to primarily be useful at the population level to describe patterns and trends in transmission
but may not be appropriate for individual diagnosis, while antigen detection remains the gold
standard for both diagnosis and surveillance.
This study had several limitations. Individuals in sampled households could have been
missed if they were away during household visits, and responses to the survey could have been
inaccurate if respondents did not sufficiently recall their history or provided answers they
thought interviewers preferred. Due to the small sample size of positive participants and high
number of zero cells, there was insufficient power to conduct multivariate analyses, including
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
more complex analyses comparing sampling methods or antigen vs. antibody results. Further-
more, due to varying household density in urban vs. rural zones, the distance of the 50 closest
household to the index case varied greatly during purposive sampling. In urban areas, the
diameter of the purposive circle was as small as 135 m, but it ranged up to 2 km in rural areas,
so an ideal minimum distance for sampling could not be established. This issue was also seen
to a lesser extent in random sampling, since the size of the census EA also varied by household
density and was as small as 0.02 square kilometers in urban settings. Future studies could sam-
ple all households within a set diameter in order to determine a minimum sampling distance.
Another limitation of this study is the possibility that the cutoff values for the ELISA OD
values were inaccurate. Due to the absence of well-characterized panels for neglected tropical
diseases, it is often challenging to determine cutoffs for serological assays. The method used in
this study represents fitting two distributions to the OD data with the assumption that there is
limited overlap between the results for true positive and negative samples. Although this
method is becoming standard in neglected tropical disease research, it is unknown to what
extent the assumptions are met, particularly given the unknown duration of antibody
responses to these pathogens. Future studies and meta-analyses can better confirm the appro-
priateness of this method.
Despite these limitations, this study provides some of the first systematic analyses on fol-
low-up of LF CFA-positive children identified by TAS. Two sampling methods were demon-
strated to be achievable in resource-limited settings, and both identified strong signs of
ongoing transmission in the large urban commune of Miragoane. This area of potential trans-
mission after the cessation of MDA has the potential to disrupt the local program to eliminate
LF in Haiti and further demonstrates the importance of TAS follow-up for the Global Program
to Eliminate Lymphatic Filariasis. While this study will help inform standardized guidelines
for post-TAS surveillance, more research is needed, and additional results including cost-effi-
cacy analyses from forthcoming post-TAS surveillance analyses from the Philippines, Burkina
Faso, and Nepal will continue to explore best methods for TAS follow up.
Supporting information
S1 Text. Detailed methods for ELISA antibody testing.
(DOCX)
S1 Table. Number and percent of participants who tested positive for circulating filarial
antigen by index case and sampling method, Nippes Department, Haiti, July-August 2019.
Purposive sampling N = 1,221; random sampling index case enumeration area (EA) N = 381;
random sampling neighbor EA N = 500.
(DOCX)
S2 Table. Number and percent of participants who tested serology positive by index case
and sampling method, Nippes Department, Haiti, July-August 2019. N = 1,914.
(DOCX)
S1 Fig. Circulating filarial antigen (CFA) prevalence by geographic zone, index case, and
number of purposively sampled households by increasing distance in meters from index
case household in comparison to households random sampled in the index case enumera-
tion area (EA) where available, Nippes Department, Haiti, July-August 2019.
(TIF)
S2 Fig. Circulating filarial antigen (CFA) prevalence by geographic zone and index case by
increasing 10-house band of increasing distance from index case household, Nippes
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PLOS NEGLECTED TROPICAL DISEASESLymphatic filariasis follow-up in Haiti
Department, Haiti, July-August 2019. Each band comprised only the 10 households in that
distance band (e.g. 1–10, 11–20, 21–30, etc.)
(TIF)
S3 Fig. Log normalized mean optical density (OD) values for IgG4 antibodies against the
recombinant Wb123 antigen by participant characteristics and circulating filarial antigen
(CFA) results. Navy color indicates CFA-negative participants, and pink color indicates CFA-
positive participants. Red line indicates cutoff for seropositivity.
(TIF)
Acknowledgments
The findings and conclusions in the article are those of the authors and do not necessarily rep-
resent the views of the US Centers for Disease Control and Prevention.
The authors would like to thank the field study teams for their hard work and dedication to
this project and would especially like to thank the participants in Nippes Department of Haiti
for their time and cooperation with the study. We would also like to thank Amber Dismer,
Kim Won, Paul Cantey, and Mary Kamb at CDC, and Patrick Lammie at the Task Force for
Global Health for their expertise and advice.
Author Contributions
Conceptualization: Marisa A. Hast, Alain Javel, Kira Barbre, Tara A. Brant, Katherine Gass,
Marc Aurèle Telfort, Christine Dubray.
Data curation: Marisa A. Hast, Keri Robinson.
Formal analysis: Marisa A. Hast, Ryan Wiegand.
Funding acquisition: Kira Barbre, Katherine Gass, Christine Dubray.
Investigation: Marisa A. Hast, Alain Javel, Eurica Denis, Keri Robinson, Christine Dubray.
Methodology: Marisa A. Hast, Alain Javel, Eurica Denis, Kira Barbre, Keri Robinson, Ryan
Wiegand, Katherine Gass, Christine Dubray.
Project administration: Marisa A. Hast, Alain Javel, Eurica Denis, Jonas Rigodon, Tara A.
Brant, Katherine Gass, Christine Dubray.
Resources: Alain Javel, Eurica Denis, Kira Barbre, Jonas Rigodon, Keri Robinson, Katherine
Gass, Marc Aurèle Telfort.
Supervision: Alain Javel, Eurica Denis, Jonas Rigodon, Katherine Gass, Marc Aurèle Telfort,
Christine Dubray.
Visualization: Marisa A. Hast, Ryan Wiegand.
Writing – original draft: Marisa A. Hast.
Writing – review & editing: Alain Javel, Eurica Denis, Kira Barbre, Jonas Rigodon, Keri Rob-
inson, Tara A. Brant, Ryan Wiegand, Katherine Gass, Marc Aurèle Telfort, Christine
Dubray.
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| null |
10.1371_journal.pmed.1002934.pdf
|
Data Availability Statement: A minimal dataset
and STATA DO file are included as Supporting
information files to enable readers to replicate our
analysis.
|
A minimal dataset and STATA DO file are included as Supporting information files to enable readers to replicate our analysis.
|
RESEARCH ARTICLE
Mortality and recovery following moderate
and severe acute malnutrition in children
aged 6–18 months in rural Jharkhand and
Odisha, eastern India: A cohort study
1,2*, Nirmala Nair2, Andrew Copas1, Hemanta Pradhan2, Naomi SavilleID
1,
Audrey ProstID
Prasanta Tripathy2, Rajkumar Gope2, Shibanand Rath2, Suchitra Rath2, Jolene SkordisID
Sanghita BhattacharyyaID
4
2, Harshpal S. SachdevID
3, Anthony CostelloID
2,
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
OPEN ACCESS
Citation: Prost A, Nair N, Copas A, Pradhan H,
Saville N, Tripathy P, et al. (2019) Mortality and
recovery following moderate and severe acute
malnutrition in children aged 6–18 months in rural
Jharkhand and Odisha, eastern India: A cohort
study. PLoS Med 16(10): e1002934. https://doi.
org/10.1371/journal.pmed.1002934
Academic Editor: Zulfiqar A. Bhutta, The Hospital
for Sick Children, CANADA
Received: January 28, 2019
Accepted: September 9, 2019
Published: October 15, 2019
Copyright: © 2019 Prost et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: A minimal dataset
and STATA DO file are included as Supporting
information files to enable readers to replicate our
analysis.
Funding: This study used data collected as part of
a trial funded by a Global Health Trial grant funded
by UK Medical Research Council (https://mrc.ukri.
org; MR/K007270/1), Wellcome Trust (https://
wellcome.ac.uk; 099708/Z/12/Z), and UK
Department for International Development (https://
1 University College London, Institute for Global Health, London, United Kingdom, 2 Ekjut, Chakradharpur,
Jharkhand, India, 3 Public Health Foundation of India, New Delhi, India, 4 Sitaram Bhartia Institute of
Science and Research, New Delhi, India
* [email protected]
Abstract
Background
Recent data suggest that case fatality from severe acute malnutrition (SAM) in India may be
lower than the 10%–20% estimated by the World Health Organization (WHO). A contempo-
rary quantification of mortality and recovery from acute malnutrition in Indian community set-
tings is essential to inform policy regarding the benefits of scaling up prevention and
treatment programmes.
Methods and findings
We conducted a cohort study using data collected during a recently completed cluster-ran-
domised controlled trial in 120 geographical clusters with a total population of 121,531 in
rural Jharkhand and Odisha, eastern India. Children born between October 1, 2013, and
February 10, 2015, and alive at 6 months of age were followed up at 9, 12, and 18 months.
We measured the children’s anthropometry and asked caregivers whether children had
been referred to services for malnutrition in the past 3 months. We determined the incidence
and prevalence of moderate acute malnutrition (MAM) and SAM, as well as mortality and
recovery at each follow-up. We then used Cox-proportional models to estimate mortality
hazard ratios (HRs) for MAM and SAM. In total, 2,869 children were eligible for follow-up at
6 months of age. We knew the vital status of 93% of children (2,669/2,869) at 18 months.
There were 2,704 children-years of follow-up time. The incidence of MAM by weight-for-
length z score (WLZ) and/or mid-upper arm circumference (MUAC) was 406 (1,098/2,704)
per 1,000 children-years. The incidence of SAM by WLZ, MUAC, or oedema was 190 (513/
2,704) per 1,000 children-years. There were 36 deaths: 12 among children with MAM and
six among children with SAM. Case fatality rates were 1.1% (12/1,098) for MAM and 1.2%
(6/513) for SAM. In total, 99% of all children with SAM at 6 months of age (227/230) were
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1002934 October 15, 2019
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Mortality and recovery following acute malnutrition in rural India
www.gov.uk/government/organisations/
department-for-international-development; MR/
K007270/1), for which NN and AP were Co-PIs.
The funders had no role in study design, data
collection and analysis, decision to publish, or
preparation of the manuscript.
Competing interests: The authors have declared
that no competing interests exist.
Abbreviations: aOR, adjusted odds ratio; CMAM,
community-based management of acute
malnutrition; HR, hazard ratio; ICDS, Integrated
Child Development Services; IQR, interquartile
range; LiST, Lives Saved Tool; MAM, moderate
acute malnutrition; MTC, malnutrition treatment
centre; MUAC, mid-upper arm circumference;
RUTF, ready-to-use therapeutic food; SAM, severe
acute malnutrition; SD, standard deviation;
STROBE, Strengthening the Reporting of
Observational Studies in Epidemiology; TEM,
technical error of measurement; UR, uncertainty
range; WASH, water sanitation and hygiene; WHO,
World Health Organization; WHZ, weight-for-height
z score; WLZ, weight-for-length z score.
alive 3 months later, 40% (92/230) were still SAM, and 18% (41/230) had recovered (WLZ �
−2 standard deviation [SD]; MUAC � 12.5; no oedema). The adjusted HRs using all anthro-
pometric indicators were 1.43 (95% CI 0.53–3.87, p = 0.480) for MAM and 2.56 (95% CI
0.99–6.70, p = 0.052) for SAM. Both WLZ < −3 and MUAC � 11.5 and < 12.5 were associ-
ated with increased mortality risk (HR: 3.33, 95% CI 1.23–8.99, p = 0.018 and HR: 3.87,
95% CI 1.63–9.18, p = 0.002, respectively). A key limitation of our analysis was missing
WLZ or MUAC data at all time points for 2.5% of children, including for two of the 36 children
who died.
Conclusions
In rural eastern India, the incidence of acute malnutrition among children older than 6
months was high, but case fatality following SAM was 1.2%, much lower than the 10%–20%
estimated by WHO. Case fatality rates below 6% have now been recorded in three other
Indian studies. Community treatment using ready-to-use therapeutic food may not avert a
substantial number of SAM-related deaths in children aged over 6 months, as mortality in
this group is lower than expected. Our findings strengthen the case for prioritising prevention
through known health, nutrition, and multisectoral interventions in the first 1,000 days of life,
while ensuring access to treatment when prevention fails.
Author summary
Why was this study done?
• Moderate acute malnutrition (MAM) and severe acute malnutrition (SAM) increase a
child’s risk of dying. The World Health Organization (WHO) estimates that 10%–20%
of children die following SAM, but this range comes from studies conducted over 15
years ago, mostly in African nations, and does not discriminate between children with
and without medical complications.
• Recent studies from India have suggested that acute malnutrition may carry a lower risk
of mortality than estimated by WHO, with substantial implications for the number of
lives that could be saved by treating children as outpatients with ready-to-use therapeu-
tic food. Unfortunately, most Indian studies conducted to date have been cross-sec-
tional, small, or did not examine mortality risk with mid-upper arm circumference
(MUAC), a commonly used anthropometric indicator to identify children with MAM
or SAM.
What did the researchers do and find?
• We conducted a cohort study as a secondary data analysis nested within a recently com-
pleted cluster-randomised controlled trial in 120 geographical clusters of Jharkhand and
Odisha, two states of eastern India with a high prevalence of child undernutrition.
• We determined the incidence and prevalence of MAM and SAM, mortality, and recov-
ery among 2,869 children followed up from 6 to 18 months of age.
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1002934 October 15, 2019
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Mortality and recovery following acute malnutrition in rural India
• We found that SAM carried a lower case fatality rate (1.2%) than expected from WHO
estimates (10%–20%), echoing results from three other Indian studies, which found case
fatality rates ranging from 2.7% to 5.2% among children older than 6 months. We also
found that over 40% of children with MAM and SAM remained acutely malnourished
for over 3 months.
What do these findings mean?
• Our data add to the accruing evidence that, in India, high rates of acute malnutrition in
children over 6 months old are accompanied by lower case fatality rates than those
reported in older, largely African studies.
• Overall, our findings suggest a need to prioritise the prevention of undernutrition by
supporting known health, nutrition, and multisectoral interventions in the first 1,000
days of life.
Introduction
In 2017, around 50 million children under 5 years globally were acutely malnourished [1].
Severe acute malnutrition (SAM) is defined as weight-for-height z score (WHZ)/weight-for-
length z score (WLZ) < −3 standard deviation (SD) of the World Health Organization
(WHO) 2006 Growth Standards, or mid-upper arm circumference (MUAC) < 11.5 cm [2].
Moderate acute malnutrition (MAM) is defined as WHZ/WLZ � −2 and < −3 or
MUAC � 11.5 cm and < 12.5 cm [2]. Both MAM and SAM increase children’s risk of dying: a
pooled analysis of 10 longitudinal studies from Asia, Africa, and South America found that
children with moderate and severe wasting had 3- and 9-fold increased mortality rates, respec-
tively, compared with children with WHZ > −1 [3]. Drawing on data collected mostly from
hospitalised children before the advent of community-based management of acute malnutri-
tion (CMAM), WHO estimated that between 10% and 20% of children with SAM generally
die within 2–3 months without treatment, without discriminating between children with and
without medical complications [4–6].
Nearly 18% of all children under 5 years globally live in India (121 out of 679 million), as do
half of all children under 5 years affected by wasting (around 25.5 million out of 50.5 million)
[1,7]. Indian policy makers, scholars, and activists relentlessly call for increased public funding
to support the health, nutrition, sanitation, and social protection interventions that could
reduce undernutrition [8–10]. Despite these efforts, scaling up preventive supplementary
nutrition and detecting children with acute malnutrition has proved challenging. The Inte-
grated Child Development Services’ (ICDS) Anganwadi (nutrition) workers should normally
give supplementary food to pregnant and breastfeeding women, children under 3 years, and
adolescent girls. They should also measure children’s WHZ monthly and refer severely wasted
children to malnutrition treatment centres (MTCs) [10]. In 2014, however, a nationally repre-
sentative survey found that only 21% of children aged 6–35 months received supplementary
food at least 21 days per month [11]. When children with SAM were found and referred to
MTC, families often feared the length and cost of hospital care [12]. There are currently no
national-level data on the proportion of children with SAM who are identified and treated and
few data on mortality following acute malnutrition in the community [9].
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Mortality and recovery following acute malnutrition in rural India
Using the Lives Saved Tool (LiST), the 2013 Lancet Commission on Maternal and Child
Undernutrition estimated that scaling up outpatient feeding with ready-to-use therapeutic
foods (RUTFs) for MAM and SAM at 90% coverage could save an estimated 435,210 children
under 5 years every year [13,14]. Previous studies have suggested that mortality from acute
malnutrition may be lower in India than in other settings [15–17]. Measuring actual mortality
rates from MAM and SAM for children in India is critical to understand how many deaths
could be prevented by scaling up treatment.
In this analysis, we estimated the prevalence and incidence of MAM and SAM, referrals,
mortality, and recovery in a cohort of children aged 6–18 months in Jharkhand and Odisha,
two Indian states with high levels of undernutrition, in the context of ordinary detection and
treatment protocols from the ICDS, and with no ongoing CMAM programme.
Methods
Design
We conducted a cohort study as a secondary data analysis nested within a cluster-randomised
controlled trial conducted between 2013 and 2016. The original trial tested a community inter-
vention to improve linear growth among children under 2 years in rural eastern India through
a participatory learning and action cycle of meetings with women’s groups and monthly visits
for all mothers from the third trimester of pregnancy until a child’s second birthday. The trial
was registered as ISCRTN 51505201 and Clinical Trials Registry of India number 2014/06/
004664 [18]. This cohort study is reported in accordance with the Strengthening the Reporting
of Observational Studies in Epidemiology (STROBE) guideline (S1 STROBE Checklist).
Setting
The trial from which our cohort data are drawn took place in two districts: West Singhbhum,
in Jharkhand, and Kendujhar, in Odisha. Both districts had high levels of child undernutrition:
in 2015–2016, 38% of children under 5 years in West Singhbhum were wasted (13.5% severely
wasted), as were 19% of children in Kendujhar (5% severely wasted) [7]. Over 75% of the pop-
ulation in the trial study areas belonged to Adivasi communities (Hindi: original inhabitants—
i.e., indigenous), also known as Scheduled Tribes. Most families were engaged in agricultural
labour, and 46% of women could read [18]. In total, 61% of households had electricity, and 1%
had an improved toilet [18]. ICDS had unequal coverage in the study areas: we witnessed mul-
tiple interruptions in the provision of iron and folic acid, deworming tablets, and supplemen-
tary nutrition between 2013 and 2016. In the study clusters, village-based Anganwadi workers
weighed children whose mothers attended monthly Village Health and Nutrition Days, offered
supplementary nutrition to moderately underweight children, and referred those who were
severely underweight to the MTC. Three treatment centres served the study communities: two
in West Singhbhum and one in Kendujhar. They admitted children with WHZ < −3 SD or
MUAC < 11.5 cm for inpatient treatment.
Participants
In the trial that provided data for this study, 120 clusters were purposively created to approxi-
mate Anganwadi worker catchment areas of 1,000 people each [19]. Community-based infor-
mants identified all women in the third trimester of pregnancy residing in these clusters and
invited them to participate in the study. All women who agreed were visited again within 72
hours of the birth, as well as 3, 6, 9, 12, and 18 months after the birth. For this cohort study, eli-
gible participants were all singleton children born to pregnant women recruited between
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Mortality and recovery following acute malnutrition in rural India
October 1, 2013, and February 10, 2015 (the trial recruitment period), and who were alive at 6
months of age. Data collectors made a minimum of three attempts to find children at each fol-
low-up. We excluded data from infants younger than 6 months for three reasons. First, these
infants are not currently targeted by community-based detection, referral, and treatment pro-
grammes for acute malnutrition in India. Second, other studies on mortality and recovery fol-
lowing MAM and SAM in India included children older than 6 months, and we wanted our
analyses to be comparable with these. Finally, we had substantial missing data for WLZ or
MUAC within 72 hours of birth (39.6%, or 1,188/3,001) because many mothers and infants
were still in hospital or away from their homes; these missing data made it challenging to
explore the association between birth anthropometry and mortality.
Variables
We defined an episode of SAM as being newly identified with WLZ < −3, MUAC < 11.5 cm,
and/or bilateral pitting oedema at 6, 9, or 12 months after not being SAM or missing at the pre-
vious follow-up. Similarly, we defined an episode of MAM as being newly identified with WLZ
between −3 and −2 and/or MUAC between 11.5 and 12.5 cm at 6, 9, or 12 months after not
being MAM or missing at the previous follow-up. Children could be acutely malnourished at
two or more consecutive follow-ups; we reported such cases as a single episode of acute malnu-
trition. For example, a child found with SAM at both 6 and 9 months was counted as having a
single episode of SAM. A child with SAM at 6 months who recovered at 9 months but was
SAM again at 12 months was counted as having two episodes. Recovery was defined as
WLZ � 2 SD, MUAC � 12.5, and no oedema. We considered a child to have died from acute
malnutrition if they were acutely malnourished at the last follow-up before death (e.g., if a
child was acutely malnourished at 6 months and died before the next follow-up at 9 months).
If a child was SAM at 6 months, recovered at 9 months, and died at 10 months, the child was
not considered to have died from SAM. The case fatality rate was calculated from among inci-
dent cases of MAM/SAM only.
Measurement
Data collectors received 5 days of training on anthropometry, followed by 7 days of field prac-
tice. They measured children’s length using Shorr boards with a precision of 0.1 cm, their
weight using Tanita BD-590 scales with 10-g graduations, and MUAC using UNICEF tapes
with a precision of 0.1 cm. Data collectors also took part in three technical error of measure-
ment (TEM) exercises: two before and one during the trial. In the first TEM, reliability coeffi-
cient values (R) were consistently over 0.95 for weight but below 0.5 for length and MUAC,
which led to retraining and two further TEM exercises for length and MUAC. In the second
and third TEMs, the average R was 0.98 for length and 0.78 for MUAC [20]. The third TEM
took place in November 2014—i.e., nearly halfway through data collection. At each follow-up,
data collectors checked whether the child was alive and asked whether they had ever been
referred to an Anganwadi worker or MTC since the last visit. In total, 11% of interviews and
measurements were conducted with a supervisor present. We had information on whether the
children were alive at the last visit before migration. Data collectors sought to find each mother
at least three times at each follow-up. Data collectors referred all children with WLZ < −3,
oedema, or MUAC < 11.5 cm to local Anganwadi workers. This method was chosen to ensure
that we did not create a parallel system for referrals to onwards facility-based treatment in
MTC or bypass supplementary nutrition programmes.
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Mortality and recovery following acute malnutrition in rural India
Statistical methods
We had no formal written analysis plan but took key decisions and drafted dummy tables
prior to the analysis. All children recruited in the original trial were included in the analysis.
We described the mothers’ and children’s socioeconomic characteristics and then examined
differences between children retained in the cohort and those lost to follow-up using chi-
squared tests for categorical variables and t tests for continuous variables. We used the
zscore06 macro in Stata 14 to generate z scores of 2006 WHO Growth Standards and excluded
WLZ values < −5 and > 5 as implausible, as recommended in WHO guidance [21]. We
checked and flagged any cases in which height and weight did not increase over an interval of
3 months. We then calculated the prevalence and incidence of MAM and SAM at 6, 9, 12, and
18 months. Within each time period (6–9 months, 9–12 months, 12–18 months), we checked
whether surviving children remained SAM, became MAM, or recovered from acute malnutri-
tion at the next follow-up.
We used Cox-proportional models to estimate minimally and fully adjusted hazard ratios
(HRs) with 95% CIs for mortality following MAM and SAM by WLZ, MUAC, and oedema (as
relevant) combined and then for individual indicators [22]. The variables indicating MAM
and SAM were time varying and updated at each follow-up time to reflect their impact on the
risk of death only during an episode. In this analysis, we included the effect of prevalent MAM
and SAM. We used multiple imputation by chained equations to account for missing measure-
ments of WLZ or MUAC for children who had measurements from at least one follow-up.
Thirty imputations sets were created, with missing values imputed conditional on values for
the same variable at other times and also on whether the child subsequently died and the time
of death or censoring. In all Cox-proportional models, we used robust standard errors to
account for correlation within clusters (villages). We included data from both the intervention
and control arms of the trial to maximise power and present HRs both adjusted and unad-
justed for trial allocation. The intervention reduced infant mortality (adjusted odds ratio
[aOR]: 0.63; 95% CI 0.39–1.00, p = 0.05) and underweight at 18 months (aOR: 0.81; 95% CI
0.66–0.99, p = 0.04) but did not reduce wasting (aOR: 0.88; 95% CI 0.71–1.08, p = 0.22) or
increase mean MUAC at 18 months (adjusted difference: 0.05; 95% CI −0.08 to 0.186,
p = 0.44). Adjusted analyses included variables for child sex, trial allocation arm, and district.
A minimal data set and STATA DO file are included to enable readers to replicate our analyses
(S1 Data and S1 DO File).
Ethical considerations
We sought women’s individual informed consent in writing or by thumbprint during the
enrolment interview in pregnancy and verbally before all subsequent interviews. The trial was
reviewed and approved by the research ethics committee of the Public Health Foundation of
India (June 2013, TRC-IEC-163/13), an independent ethics committee linked to Ekjut (May
2013, reference IEC/EKJUT/01), and University College London’s Research Ethics Committee
(June 2013, reference 1881/002). The independent ethics committee linked to Ekjut approved
this secondary data analysis after the completion of the trial.
Results
Retention and participants’ characteristics
Fig 1 shows the retention of participants in the study. In total, 2,869 singleton infants were eli-
gible at 6 months, of which 36 died between 6 and 18 months, and 56 migrated permanently.
We found 93% (2,669/2,869) of all children eligible at 6 months.
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Mortality and recovery following acute malnutrition in rural India
Fig 1. Flowchart describing the retention of children in the study. MUAC, mid-upper arm circumference; WLZ,
weight-for-length z score.
https://doi.org/10.1371/journal.pmed.1002934.g001
Table 1 describes mothers’ and children’s characteristics by follow-up status. Around half
of infants were born in Kendujhar District in Odisha, and the other half were born in West
Singhbhum, Jharkhand. Over two-thirds were born in Adivasi families. In total, 50.5% of
infants were female, and 49.5% were male. Mothers’ mean height was 1.50 m (SD: 0.07), and
children’s mean birth weight was 2.57 kg (SD: 0.4). We compared the characteristics of chil-
dren with known vital status at 18 months with those of children lost to follow-up at 18
months. Children lost to follow-up were more likely to be from Jharkhand (72% of children
lost to follow-up versus 48% of children with known status), female (59% of children lost to
follow-up versus 50% of children with known status), and from poorer households (median
multidimensional poverty score: −0.90 interquartile range [IQR]: −1.69, 0.63 for children lost
to follow-up versus −0.56, IQR: −1.64, 1.39 for children with known status at 18 months).
Case fatality and mortality incidence following MAM and SAM
Children had 1,098 episodes of MAM beginning between 6 and 18 months and a MAM inci-
dence rate of 406 per 1,000 children-years (1,098/2,704 children-years). In all, 12 children died
during an incident MAM episode, five within 6 months of the start of the episode, and seven
after 6 months. The case fatality from MAM was 0.4% (5/1,098) within 6 months and 1.1%
(12/1,098) overall.
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Mortality and recovery following acute malnutrition in rural India
Table 1. Characteristics of participants.
Characteristics
N
District (state), n (%)
West Singhbhum (Jharkhand)
Kendujhar (Odisha)
Class or caste status, n (%)
Scheduled Tribe
Scheduled Caste
Other Backward Class
Other
Multidimensional poverty scorec, median
(interquartile range)
Mother’s age, mean (SD)
Maternal height in m, mean (SD)
Parity, mean (SD)
Child sex
Female
Male
Children eligible at 6
months
2,869
Children with known status at 18
monthsa
2,669
Children lost to follow-up at 18
monthsb
200
1,425 (49.7)
1,444 (50.3)
2,192 (76.4)
188 (6.5)
484 (16.9)
5 (0.2)
1,281 (48.0)
1,388 (52.0)
2,033 (76.2)
178 (6.7)
453 (17.0)
5 (0.2)
144 (72.0)
56 (28.0)
159 (79.5)
10 (5.0)
31 (15.5)
0 (0)
−0.63 (−1.64,1.23)
−0.56 (−1.64,1.39)
−0.90 (−1.69, 0.63)
24.0 (4.6)
1.50 (0.07)
2.4 (1.6)
1,450 (50.5)
1,419 (49.5)
24.0 (4.6)
1.50 (0.07)
2.4 (1.6)
1,332 (49.9)
1,337 (50.1)
23.7 (4.5)
1.50 (0.07)
2.5 (1.5)
118 (59.0)
82 (41.0)
aChildren with known status at 18 months include those found alive at 18 months and those who died during follow-up.
bLost to follow-up is defined as not found at 18 months and not dead.
cThe Multidimensional Poverty Index comprised data on household assets, roof and floor materials, any deaths to a child under 5 years in the household, and any
school-age children out of school, following the methodology described by Alkire and colleagues, which involves principal component analysis [22].
Abbreviation: SD, standard deviation
https://doi.org/10.1371/journal.pmed.1002934.t001
Children had 513 episodes of SAM beginning between 6 and 18 months and a SAM inci-
dence rate of 190 per 1,000 children-years (513/2,704 children-years). In total, six children
died during an incident SAM episode, four within 6 months of the start of the episode, and
two after 6 months. The case fatality for SAM was 0.8% (4/513) within 6 months and 1.2%
overall (6/513).
Table 2 shows the mortality incidence rates for MAM and SAM, as well as unadjusted and
adjusted associations between MAM and SAM incidence and short-term (i.e., within the epi-
sode) mortality. A total of 68 children could not be included in analyses with multiple imputa-
tion: 10 had no WLZ measurement at any follow-up, 55 had no MUAC measurement at any
follow-up, and three were immediately censored at the 6 months’ visit. S1 Table shows the
number of missing values for each WLZ, MUAC, and oedema variable. The mortality inci-
dence rate for MAM was 19.1 per 1,000 children-years. The mortality incidence rate for SAM
was 20.1 per 1,000 children-years. The adjusted HR for MAM using all anthropometric indica-
tors was 1.43 (95% CI 0.53–3.87, p = 0.480) and 2.56 (95% CI 0.99–6.70, p = 0.052) for SAM
(overall p = 0.073). Lower MUAC, lower WLZ, and the presence of oedema were associated
with increased risk of mortality (p = 0.003, p = 0.060, and p = 0.059, respectively).
Nutritional status among survivors
S2 Table describes the prevalence of MAM and SAM at the start of each follow-up period (i.e.,
at 6, 9, and 12 months), along with the vital and nutritional status of children at the next fol-
low-up. In total, 99% of all children with SAM at 6 months (227/230) were alive after 3 months,
40% (92/230) were still SAM, and 18% (41/230) had ‘recovered’ (WLZ � −2 SD;
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1002934 October 15, 2019
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Mortality and recovery following acute malnutrition in rural India
Table 2. Associations between anthropometric indicators of MAM or SAM and short-terma mortality.
Anthropometric
indicators
Mortality incidence
per 1,000 children-
years
Minimally adjusted
hazard ratios (95% CI),
by categoryb
p
Minimally adjusted
hazard ratios (95%
CI), overallb
p
Fully adjusted
hazard ratios (95%
CI) by categoryc
p
Fully adjusted
hazard ratios (95%
CI), overallc
p
All indicators
No acute
MAM
SAM
WLZ
�−2
�−3 and <−2
<−3
MUAC
�12.5
�11.5 and <12.5
<11.5
Oedema
No
Yes
9.2
19.1
19.7
9.3
21.1
25.0
10.3
24.4
11.3
12.2
67.4
1
1.40 (0.52–3.77)
2.23 (0.80–6.19)
1
1.14 (0.46–2.83)
2.80 (0.94–8.37)
1
3.81 (1.57–9.24)
1.95 (0.24–15.5)
1
0.508
1.43 (0.53–3.87)
0.480
0.124 1.47 (0.89–2.43)
0.128 2.56 (0.99–6.70)
0.052 1.57 (0.96–2.55)
0.070
1
0.773
1.20 (0.47–3.04)
0.702
0.064 1.53 (0.88–2.65)
0.131 3.33 (1.23–8.99)
0.018 1.65 (0.98–2.78)
0.061
1
0.003
3.87 (1.63–9.18)
0.002
0.527 2.13 (1.25–3.62)
0.005 1.89 (0.23–15.2)
0.551 2.10 (1.25–3.53)
0.005
1
1
4.79 (0.61–37.6)
0.136
5.87 (0.94–36.5)
0.058
aHazard ratios reflect the impact of a malnutrition indicator until its value is updated at a subsequent follow-up visit.
bAdjusted for clustering using robust standard errors.
cAdjusted for child’s sex, trial allocation, district, and clustering using robust standard errors.
Abbreviations: MAM, moderate acute malnutrition; MUAC, mid-upper arm circumference; SAM, severe acute malnutrition; WLZ, weight-for-length z score
https://doi.org/10.1371/journal.pmed.1002934.t002
MUAC � 12.5; no oedema). Only 5% (32/584) of children with SAM at 6, 9, or 12 months
were ever referred to an MTC. The coverage of preventive nutrition services was also unequal:
for example, 66% (1,917/2,869) of children aged 6 months were weighed by an Anganwadi
worker, but only 13% (382/2,869) had mothers who received nutrition counselling.
Outcomes up to 12 months after MAM and SAM
Fig 2 shows outcomes at 9, 12, and 18 months for children who were not undernourished or
had MAM or SAM at 6 months. These were derived after multiple imputation for missing
WLZ, MUAC, and oedema data. The proportions of children with MAM or SAM at 6 months
who had died by 18 months were 1.3% and 1.1%, respectively. These were not very different,
in absolute terms, to the proportion of non-acutely malnourished children who died (0.8%).
Recovery from MAM and SAM was relatively low and stable over time. Recovery out of acute
undernutrition was similar for MAM or SAM, particularly by 18 months.
Discussion
We found a high incidence of MAM and SAM among rural, largely tribal communities of
Jharkhand and Odisha. A substantial proportion (>40%) of children with MAM and SAM
remained acutely malnourished for over 3 months, and 99% of children with SAM at 6 months
survived for 3 months or more, suggesting that, in this context, MAM and SAM are persistent.
WLZ < −3 was associated with increased mortality risk, as expected, but MUAC � 11.5
and < 12.5 was associated with a greater mortality risk than MUAC < 11.5. The finding that
children with MUAC � 11.5 and < 12.5 had a higher mortality risk is counterintuitive and
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Mortality and recovery following acute malnutrition in rural India
Fig 2. Long-term outcomes for children with and without acute malnutrition at 6 months, using a data set with multiple imputation.
MAM, moderate acute malnutrition; SAM, severe acute malnutrition.
https://doi.org/10.1371/journal.pmed.1002934.g002
deserves further investigation. Anganwadi workers referred only 5% of SAM cases to MTC,
highlighting a considerable treatment gap.
Our most salient finding is that SAM carried a much lower case fatality rate (1.2%) than
expected from older, largely African studies and WHO estimates (10%–20%). If the two
deceased children for whom we did not have any anthropometry data had died following
SAM, the case fatality rate would have been 1.5% (8/513), still much below 10%–20%.
Three other Indian studies with different designs but broadly similar inclusion criteria offer
data for comparison. The first was a follow-up study of children initially screened as having an
MUAC < 11.5 cm as part of a multicentric trial in poor urban and rural communities in New
Delhi, Udaipur, and Vellore [23]. Case fatality among children aged 6–23 months with
MUAC < 11.5 cm was 4.3% (6/140) after 12 months [24]. A second study conducted in rural
Uttar Pradesh found a case fatality of 2.7% among 409 children aged 6 months to 5 years fol-
lowed up between 0.6 and 17.8 months after severe wasting [25]. In a third study from Bihar,
Burza and colleagues followed up defaulters from a WHO-standard RUTF programme who
had MUAC < 11.5 cm [26]. Case fatality among these defaulters—who tended to be younger
children and girls—was 5.2% within 18 months (36/692). All of these case fatality rates, with
varying durations of follow-up, are below WHO estimates (10%–20%) and closer to the 4%
(range: 2%–7%) case fatality rate that a 2013 expert panel considered normal in the context of
a CMAM programme [27].
There are at least four possible explanations for the considerable difference between case
fatality rates in these recent Indian studies and the 10%–20% estimates drawn from older,
largely African studies. First, the studies upon which WHO estimates are based included
mostly hospitalised children who were more likely to have SAM with medical complications
and, therefore, higher mortality rates [6].
A second possible explanation is that the most vulnerable children in our rural study areas
died before reaching 6 months. In the trial’s control clusters, the infant mortality rate was 64
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Mortality and recovery following acute malnutrition in rural India
per 1,000 live births; 64% (116/181) of all infant deaths across both trial areas occurred in the
first month of life, and 86% (157/181) occurred in the first 6 months [18]. In 2015, the preva-
lence of low birth weight per 100 births was greater in southern Asia than in sub-Saharan
Africa (26.4%; uncertainty range [UR]: 18.6–35.2 versus 14.0%, UR: 12.2–17.2) [28]. Around
half of neonatal deaths in India (370,000 of 698,000 neonatal deaths in 2015) are caused by pre-
maturity or low birth weight, and these factors also accounted for 46.1% of all under-5 deaths
in 2017 (95% uncertainty interval: 44.5–47.6) [29,30]. In rural India, undersize is probably tak-
ing its heaviest toll in the first 6 months of life, before treatment with RUTF becomes relevant.
A third source of variation in case fatality rates may lie in differences in infection burdens
between South Asian and African settings. In 2017, the disability-adjusted life years rate for
communicable maternal, neonatal, child, and nutritional diseases was 26,492 per 100,000 in
sub-Saharan Africa, roughly double that in South Asia (13,197 per 100,000) [31]. HIV preva-
lence is 4.1% among 15–49-year-olds in sub-Saharan Africa versus 0.2% in South Asia, includ-
ing India, and several studies have demonstrated that HIV infection interacts with
undernutrition to increase the risk of death [31–33].
A final explanation may lie in the developmental origins of adult health and disease. Moth-
ers in our study areas had an average height of 1.5 m [17]. During pregnancy, half of them had
an MUAC < 23 cm, and one-third of them did not have diets with minimum diversity [17].
Around one-third (33%) of infants were low birth weight, and over 65% were stunted by 18
months [18]. These data reflect intergenerational, chronic undernutrition inflicted by poverty
[34]. Indian infants often have a ‘thin-fat’ phenotype: they have small abdominal viscera and
low muscle mass but preserve body fat in utero that can track into birth and young adulthood,
depending on the nutritional environment [35]. Studies have found that body fat–related mea-
surements such as skinfold thickness, abdominal circumference, and MUAC are often similar
between Indian babies and Western infants, despite low birth weight [36].The hidden adipos-
ity of Indian infants may give small infants a survival advantage by acting as a form of energy
reserve available to maintain body temperature and brain development in times of nutritional
deprivation, albeit with adverse consequences for noncommunicable disease risk in later life
[37]. It is therefore possible that thinness in infancy and early childhood does not carry the
same mortality risk in this setting as in others. The interplay between undernutrition, immune
dysfunction, and mortality risk is complex, as summarised in recent reviews [38–40]. Integrat-
ing longitudinal immune assessments into ongoing trials of nutrition and water sanitation and
hygiene (WASH) interventions will help elucidate when and how immune dysfunction and
undernutrition interact and help better target public health interventions to lower mortality
risk.
Our study had several strengths. To our knowledge, it is the largest Indian community-
based longitudinal study of mortality following MAM and SAM in the absence of management
of uncomplicated SAM with RUTF for children older than 6 months. The three TEM exercises
undertaken by the data collection team enhance our trust in the accuracy of anthropometry
data. We had information about vital status for 93% of infants eligible for follow-up at 6
months by the end of the study period.
Our study had three main limitations. We had missing anthropometry data for some chil-
dren, including fully missing data for two of the 36 children who died. We attempted to
address possible bias caused by missing data by using multiple imputation to provide more
accurate estimates of mortality risk but were not able to use imputation for 68 children who
had no WHZ or MUAC measurements at any time point. A second limitation is that we did
not follow children up until 59 months of age. The study from Uttar Pradesh by Kapil and col-
leagues found a case fatality rate of 2.7% among children aged 6–60 months; this is higher than
among the younger children in our study but still not within WHO’s estimated range [25].
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Mortality and recovery following acute malnutrition in rural India
Our results are therefore likely to be generalisable to young children aged 6–24 months in
other rural, underserved Indian settings and may provide a modest underestimate of case fatal-
ity for children aged 6–59 months. Finally, monitoring and referral systems for SAM in the
original trial differed from those available in the general population, and this may have con-
tributed to lowering mortality. We have little evidence to support this hypothesis, however:
infant mortality in the trial’s control area (63 per 1,000 live births) was similar to that reported
in the 2011–2012 Annual Health Surveys for our two study districts (56 per 1,000 live births in
Kendujhar and 58 in West Singhbhum), suggesting that the trial monitoring systems did not
lead to large reductions in mortality in and of themselves [41].
If data from poor urban and rural communities in Delhi, Bihar, Uttar Pradesh and our own
data from Jharkhand and Odisha are representative of the contemporary Indian situation,
then case fatality rates following SAM in Indian children older than 6 months are substantially
lower than those estimated from earlier studies conducted in African countries. In other
Indian studies assessing progress following inpatient and/or community care for SAM, rates of
recovery were often lower than recommended in SPHERE guidance, and relapse was common
[42–44]. For example, in a recent follow-up study of 150 children discharged from MTCs in
Jharkhand, 52% of children had relapsed into severe wasting 2 months after discharge [45]. In
light of these findings, scaling up outpatient RUTF treatment for children over 6 months with-
out concurrently strengthening ICDS, WASH, and the social protection interventions that
support the intergenerational prevention of undernutrition may not have the large effects on
mortality predicted by the 2013 Lancet Maternal and Child Nutrition Series in India and other
South Asian contexts [17]. Prevention can work: a recent intervention combining crèches, par-
ticipatory meetings with women’s groups, and home visits reduced wasting, underweight, and
stunting among children under 3 years old in Jharkhand and Odisha [46]. A recent UNICEF-
led consultation aptly called for a new approach to wasting in South Asia, one that positions
prevention as the ‘first priority’ and ensures access to treatment when prevention fails [47].
Our findings support such a strategy.
In conclusion, we found a high incidence of acute malnutrition among children older than
6 months in rural eastern India but a lower than expected case fatality rate following SAM.
This finding has been replicated in at least three other Indian studies. Given that the risk of
mortality is lower than expected among children older than 6 months and that many deaths
occur because of prematurity or low birth weight during the neonatal period, outpatient treat-
ment for SAM using RUTF for children over 6 months may be too late to avert a substantial
number of deaths from undernutrition in Indian children. This further strengthens the case
for prioritising prevention through known health, nutrition, and multisectoral interventions
in the first 1,000 days of life.
Supporting information
S1 STROBE Checklist. STROBE, Strengthening the Reporting of Observational Studies in
Epidemiology.
(DOCX)
S1 Data.
(CSV)
S1 DO File.
(DO)
S1 Table.
(DOCX)
PLOS Medicine | https://doi.org/10.1371/journal.pmed.1002934 October 15, 2019
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Mortality and recovery following acute malnutrition in rural India
S2 Table.
(DOCX)
Acknowledgments
We thank the mothers and children who took part in the study, as well as the SPKs, ANMs,
ASHAs, and Anganwadi workers in participating clusters. We thank Dr Hembrom, who sup-
ported referrals for severely acutely malnourished children. We thank Professor Clive
Osmond, from the University of Southampton, for comments on the statistical methods, and
Kripa Harper, UCL MSc class of 2017, for sharing her literature review on SAM in India.
Author Contributions
Conceptualization: Audrey Prost, Andrew Copas, Harshpal S. Sachdev.
Data curation: Audrey Prost, Hemanta Pradhan, Shibanand Rath.
Formal analysis: Audrey Prost, Andrew Copas, Hemanta Pradhan, Harshpal S. Sachdev.
Funding acquisition: Audrey Prost, Nirmala Nair, Andrew Copas, Naomi Saville, Jolene Skor-
dis, Sanghita Bhattacharyya, Harshpal S. Sachdev.
Investigation: Audrey Prost, Nirmala Nair, Andrew Copas, Prasanta Tripathy, Rajkumar
Gope, Shibanand Rath, Suchitra Rath, Sanghita Bhattacharyya, Harshpal S. Sachdev.
Methodology: Audrey Prost, Nirmala Nair, Andrew Copas, Prasanta Tripathy, Rajkumar
Gope, Shibanand Rath, Suchitra Rath, Harshpal S. Sachdev.
Project administration: Audrey Prost, Rajkumar Gope, Shibanand Rath.
Resources: Audrey Prost, Nirmala Nair, Prasanta Tripathy.
Supervision: Audrey Prost, Hemanta Pradhan, Rajkumar Gope, Shibanand Rath, Suchitra
Rath, Anthony Costello, Harshpal S. Sachdev.
Visualization: Audrey Prost.
Writing – original draft: Audrey Prost.
Writing – review & editing: Audrey Prost, Nirmala Nair, Andrew Copas, Naomi Saville, Pra-
santa Tripathy, Jolene Skordis, Anthony Costello, Harshpal S. Sachdev.
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10.1088_1361-6552_ad001a.pdf
|
Data availability statement
The data cannot be made publicly available upon
publication due to legal restrictions preventing
unrestricted public distribution. The data that sup-
port the findings of this study are available upon
reasonable request from the authors.
|
Data availability statement The data cannot be made publicly available upon publication due to legal restrictions preventing unrestricted public distribution. The data that support the findings of this study are available upon reasonable request from the authors.
|
P A P E R
iopscience.org/ped
Phys. Educ. 59 (2024) 015001 (12pp)
Einsteinian gravitational
concepts throughout
secondary school
∗
Corey McInerney
and Phil Sutton
University of Lincoln, School of Mathematics and Physics, Lincoln LN6 7TS, United
Kingdom
E-mail: [email protected]
Abstract
Einstein’s theory of relativity is largely thought of as one of the most
important discoveries of the 20th century and continues to pass observational
tests over 100 years later. Yet, it is Newtonian gravity, a 350 year old
formalism proven to be less accurate than relativity, which is taught in
schools. It has been shown that Einsteinian gravitational concepts can be
well understood by students in both primary and secondary education. In this
paper, a cross-section of students from Yr 7 to 13 enrolled in an English
secondary school took part in an intervention designed to introduce the idea
of gravity from spacetime curvature. The overall aim of this work is to assess
the viability of including relativity in the secondary curriculum and to
ascertain which year this material would be best placed in. We determine that
all year groups where able to appreciate the effects of curvature to some
extent. Visual demonstrations aided conceptual understanding at Yr 7–8
level, but this does not have a strong effect on their ideas around the source
of the gravitational force. Participants in Yr 9–13 were able to understand
concepts beyond those introduced in the demonstrations. However, a deeper
understanding of curvature as the source of the gravitational force is not seen
until years 12 and 13. We find that those in Yr 13 have the best overall
understanding of the concepts introduced during our intervention.
Keywords: Einsteinian gravity, relativity, secondary school, conceptual understanding
1. Introduction
In 1687, Isaac Newton published his law of uni-
versal gravitation [1]; it is commonly taught in
schools because it combines the concept of mass
∗
Author to whom any correspondence should be addressed.
and weight with everyday phenomenon like fall-
ing objects [2]. Gravity is regarded as being one
of the key threshold concepts in education used
as an indicator of a students understanding of
wider physics topics [3, 4]. However, research
suggests that a large number of misconceptions
about gravity are held by students. These include
issues surrounding the direction of gravitational
1361-6552/24/015001+12$33.00
1
© 2023 IOP Publishing Ltd
C McInerney and P Sutton
force, gravity outside of the Earth and the role of
the Sun in celestial dynamics [5–7]. These issues
are tied to students not being able to fully grasp
where the gravitational force comes from, with
some students believing that objects only have a
gravitational pull if they are heavy and spherical,
or that air is needed in order for gravity to act
between objects [8, 9]. Misconceptions can stay
with students throughout their schooling, impact-
ing confidence, ability and thus students overall
enjoyment of science [10].
A new approach pioneered by the Einstein-
First project could eliminate some of the con-
ceptual issues faced by students. The idea is to
introduce principals from modern physics, such
as Einstein’s theory of general relativity (GR)
into the Australian curriculum at primary and
secondary level. A similar project, ReleQuant,
in Norway also pioneers the teaching of relativ-
ity and quantum mechanics at secondary school
[11, 12].
Einstein’s theory of GR provides a mathem-
atical description of gravity and offers a qualitat-
ive description of how gravity works [13]. A key
feature of GR is the non-Euclidean geometry of
space and the interplay between time and space.
The sophisticated mathematics involved in GR
are seen as a barrier to students below degree
level. The ReleQuant project bypasses this math-
ematical rigor by placing conceptual language
at the forefront of the learning process, explor-
ing concepts via thought experiments and visual
demonstrations.
This study explores the impact of a one-
off intervention on students’ understanding of
Einsteinian gravitational concepts. Similar studies
have been performed in Lebanon [14], Australia
[15, 16], Indonesia [17] and Italy [18, 19].
Each of those works report that students have
a better understanding of gravity from a GR
stand point after being introduced to concepts
such as curvature, time dilation and spacetime
diagrams.
The intervention used for this study was
designed to fit
into a standard 50 min lesson
period at a single English state funded secondary
school. Within that period, students were taught
about how spacetime curvature produces the
gravitational force with the help of two hands on
activities. The host school is a fully government
funded, selective, mixed grammar school located
the town of Gainsborough, County Lincolnshire,
England. This study took place during February
and March 2023 and at that time a total of 1237
students were enrolled at the school.
An identical intervention was delivered to all
age groups (years 7–13) at this school. Students
were issued with questionnaires before and after
the intervention and by comparing the results
across year groups, we hope to identify the
optimum place for GR to be introduced into the
secondary science curriculum.
In the following section we describe the
research methodology in comparison with other
works, as well as the content and application
method of our intervention. In section 3, we
present the results of our research, which are also
discussed and analysed.
2. Method
2.1. The host school
The school where this research was performed
is a fully government funded, selective, mixed
grammar school located in England. At the time
of this study, a total of 1237 students were
enrolled at the school. The UK government web-
site (www.find-school-performance-data.service.
gov.uk) shows that in 2022, the school was ranked
in the top 25% in the UK for academic perform-
ance at GCSE level and that 82% of pupils at
∗
the school achieved A-level grades between A
and C.
2.2. Comparison with other works
In other works, interventions range from short,
to full 20 session
one off workshops [20],
programmes [21, 22]. The offering a longer syl-
labus means more content and concepts can be
covered, students can learn at their own pace and
there are opportunities for deeper learning experi-
ences. Nonetheless, it has been shown that one-off
interventions have a significant impact on students
engagement with science topics and consequently,
their future career choices [23, 24].
The intervention used in this paper was
designed as a single, one-off session to introduce
January 2024
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Phys. Educ. 59 (2024) 015001
Einsteinian gravitational concepts throughout secondary school
Table 1. Number of participants in this study by year group.
Key stage
Year group
Number of students
7
8
9
10
11
12
13
KS3
KS4
A-level
Total
59
41
24
20
13
12
14
183
Table 2. An outline of the different topics and concepts covered during our intervention.
Topic
Details
Newton’s law of universal gravitation
Gravitational field lines
E = mc2
General relativity
Every particle attracts every other particle in the Universe.
Field lines on the surface of and around celestial bodies.
Relation between mass and energy in special relativity, leading to
relation between mass and gravity in GR.
Space, time and spacetime curvature.
Spacetime simulator
Gravitational force in GR
Force increase with curvature.
Triangles on balloons
Geometry in GR
GPS corrections for Earth’s curvature. Positive and negative
curvature. The curvature of the Universe.
students to the subject of GR and to explore grav-
itational phenomena in the realm of GR. While
other works have used participants from a single
class, a single year group or a particular key stage
(KS), we offered this intervention to all physics
students in the school. A total of 183 students from
years 7 to 13, choose to take part in this study, the
breakdown of which is shown in table 1.
Surveying students from one single school
allows us to see how students understanding of
gravity changes throughout the educational years
via this cross-sectional study and offers the oppor-
tunity for longitudinal studies in the future follow-
ing specific cohort(s). Gravity is taught in England
at KS3 (11–14 years old), KS4 (14–16 years old)
and A-level (16–18 years old), therefore, any mis-
conceptions picked-up at KS3 have the potential
to carry forward and impact a students under-
standing at A-level.
2.3. The intervention
The intervention implemented in this work
consisted of 33 identical 50 min workshops in
the presence of 8–30 students from a single year
group. The same researcher conducted all ses-
sions, covering the same material and activities.
The intervention began with students being
asked to describe gravity in their own words
before GR was introduced. Table 2 shows the
order that topics were introduced, the material
spoken about and where any hands-on activities
involved tie-in (highlighted in blue).
A common
2.3.1. The spacetime simulator.
analogy for the curvature of spacetime uses a
sheet of stretchy, elastic material such as Lycra,
and some different massed objects. This particular
analogy is commonly referred to as ‘the spacetime
January 2024
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Phys. Educ. 59 (2024) 015001
C McInerney and P Sutton
Figure 1. The stretched sheet of Lycra used as a space-
time simulator. Three 1 kg masses placed in the centre
of the sheet provide curvature.
simulator’ [25] and has proven to be effective at
dispelling misconceptions around gravity [26].
For our demonstration, a large Lycra sheet
was stretched flat across a plastic frame as seen in
figure 1. Three students were then invited forward
to hold the sheet in the air and it was explained to
the group that the sheet represents spacetime in the
flat Euclidean plane (as per the Newtonian model).
Students were then invited forward to roll tennis,
squash, and golf balls across it, perceiving that
they travel in straight lines and that mass does not
affect motion in flat space. A mass heavy enough
to deform the sheet was then placed on it and
students observed that the balls now roll towards
the central mass much like a ball rolling towards
the bottom of a hill. By adding more mass to the
centre of the sheet and increasing the curvature,
students observe that the balls roll towards the
central mass much quicker than before. This opens
up a discussion around mass, curvature and grav-
itational attraction.
Additionally, while the sheet is deformed,
squash balls were given some sideways velocity.
Here, students observe the ball circling around the
central mass with motion analogous to an orbit.
It was important here to draw attention to the
fact that the orbital motion decays due to the loss
of energy from friction between the ball and the
sheet, whereas orbits in the Universe conserve
energy in general and will be continuous.
To explore this further, students were shown a
plot akin to figure 1(b) from Kaur et al [16] which
Figure 2. An example of some of the balloons used
by students to demonstrate the effects of curvature on
geometry.
illustrates that increasing curvature (adding mass
to the sheet) changes the distance between two
points in spacetime, thus influencing the geometry
of the surrounding spacetime.
Following the
2.3.2. The geometry of GR.
introduction to curvature, the intervention moved
to exploring the geometry of spacetime.
Pairs of students were issued with differ-
ent sized balloons. Each balloon had a triangle
drawn on it and the students were tasked with
carefully measuring the internal angles of the tri-
angles by placing protractors on the balloons sur-
face. An example is shown in figure 2. Students
of a tri-
then compared their results to the 180
angle in Euclidean space to that of one with
increased curvature and how that changes the
internal angles. These results were then related
to applications of non-Euclidean geometry such
as the spherical curvature of Earth, it is effect on
lines of longitude (such as their convergence at
the poles), GR corrections to GPS and the poten-
tial geometries of the Universe (hyperbolic, flat,
parabolic).
◦
2.4. Pre/post intervention questionnaire
Two sets of questionnaires were used in this
research. One disseminated 2 weeks before the
intervention (pre-), and one given to students
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Phys. Educ. 59 (2024) 015001
Einsteinian gravitational concepts throughout secondary school
Table 3. Questions from the pre/post intervention questionnaire.
Questions
Q1 Can parallel lines meet?
Q2 Can the sum of the angles in a triangle be different from 180
Q3 What is gravity?
Q4 How do objects move in gravitational fields?
Q5
Q6 Does space have a shape? What about the space around heavy objects like stars and planets?
Q7 Do you prefer to learn about physics by listening to your teacher, watching demonstrations or doing
Isaac Newton is famous for his laws of motion and his law of gravity. What is Albert Einstein famous for?
?
◦
practical work?
Q8 Did you enjoy learning about this topic? What did you like/not like?
Q9 Are you interested in learning more about gravity and general relativity?
Q10 Should Einsteinian physics, like general relativity be included in the curriculum?
2 weeks after the intervention (post-). Following
the format of related studies [15, 20, 21], the open-
ended questions in the questionnaires examined
conceptual understandings and attitudes towards
GR.
The pre-questionnaire comprised seven ques-
tions exploring students’ understanding of grav-
ity, its origins, workings, their perspectives on
space shape, and opinions on physics teaching
methods.
The post-questionnaire was nearly identical
to the pre-questionnaire, allowing direct compar-
ison. It included three additional questions to gain
insight into students’ views on the intervention
and Einsteinian gravity itself.
The questions themselves are open-ended and
can be found in table 3.
3. Results and discussion
Figure 3 and table 4 show the responses to Q1.
The majority of participants (93.8%) said that
parallel lines cannot meet. Of the ten that said
they can (three from Yr 7, four from Yr 10 and
one each from Yr 11, 12 and 13), five of these
responses (three Yr 10, one Yr 11 and one Yr
13) used the phrase ‘non-Euclidean’ or ‘not on
flat space’, thus showing good knowledge before
the intervention. It is likely that these participants
have had previous exposure to curved geomet-
ries. The total number of ‘yes’ responses moves
from 6.2% to 44.2% after the intervention. This
is not as much as the 11.3% to 83.6% rise in
correct responses to Q2, shown in figure 4 and
table 5. The intervention design contributed to this
as Q2 relates to the balloon activity, whereas the
information about parallel lines also being influ-
enced by curved geometry was presented after
this activity as part of the slideshow presentation.
As such, participants had to pay more attention
to grasp this information. Nonetheless, all year
groups showed an increase in ‘yes’ responses for
both Q1 and Q2 with Yr 9, 11, and 12 having
the highest increase in percentage. This is per-
haps expected as these cohorts have studied more
geometry than younger students and so are better
prepared for discussion’s around non-Euclidean
geometry.
These
that participants
indicate
comprehend information better through visual
and hands-on activities. Well-designed prac-
tical activities are reported to increase students
levels of understanding [27], with practical work
seen by students as more interesting and enga-
ging than listening to their teacher or watching
demonstrations [28].
results
Q3 is more open to predisposed misconcep-
tions than Q1 or Q2. As seen in figure 5, there were
many different responses to this question. We have
categorised responses into those which described
gravity as a force versus those which did not. It
was expected that post-intervention, participants
would shift their answers towards describing grav-
ity as the ‘bending/warping of spacetime’. 82%
of the pre-questionnaire responses described grav-
ity as a force, with responses ranging from ‘the
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Phys. Educ. 59 (2024) 015001
C McInerney and P Sutton
Figure 3. Responses to Q1. Can parallel lines meet?
Table 4. Difference in pre- and post-questionnaire responses to Q1 by year group.
Pre
Post
No
93.62%
100.00%
100.00%
78.95%
91.67%
91.67%
90.91%
Yes
8.51%
0.00%
0.00%
21.05%
8.33%
8.33%
9.09%
No
79.66%
75.76%
33.33%
6.25%
20.00%
0.00%
11.11%
Yes
20.34%
21.21%
61.11%
75.00%
80.00%
100.00%
88.89%
Yr 7
Yr 8
Yr 9
Yr 10
Yr 11
Yr 12
Yr 13
force that keeps us on Earth’, ‘the force that stops
us from floating/keeps us on the ground’ and ‘the
force between objects/masses’.
Only 1.8% of participants specified that
gravity was the cause of spacetime curvature
pre-intervention, increasing to only 8.9% post-
intervention. Similar studies [26] also struggled
to fully influence descriptions of gravity using
the spacetime simulator. However looking at
table 6 which shows the breakdown of Q3 by
year group, reveals that responses related to
spacetime curvature increased notably in years
10 (up 17.52%), 12 (up 20.24%), and 13 (up
35.35%).
One positive result from table 6 is that par-
ticipants associating gravity as an Earth-bound
force decreased across all year groups (except
Yr 10), particularly in Yr 8 and 11. The data
indicates that the KS4 and A-level groups best
understood the concept of gravity from space-
time curvature. The majority of participants how-
ever either did not grasp the concepts introduced
(not indicated by the results to Q1 and Q2),
or the intervention’s influence was limited by
their pre-existing classroom-based learning and
opinions.
Q4 assess participants understanding of how
gravity influences the motion of objects. Presented
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Phys. Educ. 59 (2024) 015001
Einsteinian gravitational concepts throughout secondary school
◦
Figure 4. Responses to Q2. Can the sum of the angles in a triangle be different from 180
?
Table 5. Difference in pre- and post-questionnaire responses to Q2 by year group.
Pre
Post
No
93.48%
88.89%
87.50%
84.21%
83.33%
83.33%
90.91%
Yes
6.52%
11.11%
12.50%
15.79%
8.33%
16.67%
9.09%
No
13.79%
33.33%
16.67%
6.25%
0.00%
0.00%
11.11%
Yes
86.21%
63.64%
83.33%
75.00%
100.00%
100.00%
88.89%
Yr 7
Yr 8
Yr 9
Yr 10
Yr 11
Yr 12
Yr 13
in figure 6, the responses to this question are
extremely varied, ranging from high level answers
like ‘conic sections’ and ‘along geodesics’ to less
descriptive responses such as ‘they float’ or ‘fast’.
Many responses show an understanding of the
attractive powers of gravity, as well as know-
ledge of other aspects of physics such as kinetic
and gravitational potential energy. While many of
these descriptions are not wholly incorrect, they
fail to properly describe the motion of objects
in gravitational fields. This is likely due to par-
ticipants lack of formal education on gravitational
orbits, a topic not covered in detail until Yr 13. It
is possible that responses such as ‘around’ and ‘in
circles’ are consequences of this as those in lower
year groups attempt to describe orbits without
knowledge of the correct scientific terminology.
This is supported by the fact that we see a slight
increase in these descriptors post-intervention as
participants watched objects circle around masses
on the spacetime simulator sheet.
such as
Positively, phrases
‘they fall’,
‘towards ground/source’ and ‘pushed/pulled’
decrease post-intervention, whereas the number
of participants describing orbital motion doubles.
Those describing motion in gravitational fields
January 2024
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Phys. Educ. 59 (2024) 015001
C McInerney and P Sutton
Figure 5. Pre- (a) and post-questionnaire (b) responses to Q3. What is gravity? Responses in which gravity is
described as a force are shown in the right-hand charts, with other opinions of gravity being shown in the left-hand
charts.
Table 6. Difference in pre- and post-questionnaire responses to Q3 by year group.
Pre
Force
Post
Force
Earth
Other
Spacetime curvature
Earth
Earth
Other
Spacetime curvature
Earth
Yr 7
Yr 8
Yr 9
Yr 10
Yr 11
Yr 12
Yr 13
25.53% 48.94%
35.14% 54.05%
29.17% 87.50%
5.56% 72.22%
58.33% 41.67%
16.67% 75.00%
0.00% 81.82%
0.00%
0.00%
0.00%
5.56%
0.00%
8.33%
9.09%
6.38% 17.24% 48.28%
2.70% 25.81% 51.61%
0.00% 38.89% 38.89%
0.00% 15.38% 53.85%
0.00% 30.00% 40.00%
0.00% 0.00% 42.86%
0.00% 0.00% 44.44%
1.72%
3.23%
5.56%
23.08%
10.00%
28.57%
44.44%
6.90%
6.45%
0.00%
0.00%
0.00%
0.00%
0.00%
January 2024
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Phys. Educ. 59 (2024) 015001
Einsteinian gravitational concepts throughout secondary school
Figure 6. Responses to Q4. How do objects move in gravitational fields?
Figure 7. Responses to Q6. Does space have a shape? What about the space around heavy objects like stars and
planets?
as attractive also sees a significant increase post-
intervention. This again is likely due to the use
of the spacetime simulator demonstration where
it was observed that objects on the sheet moved
towards the source of curvature. This is also evid-
enced by the added uses of terms such as ‘oval’
and ‘spirals’ which appear in post-questionnaire
responses only.
58.2% of
Pre-intervention,
participants
thought that space had no shape, often saying
it
is infinite or expanding (‘no because it
is
infinite/expanding’) to justify their response. This
number decreases to 42.4% post-intervention,
the intervention had limited
indicating that
success in conveying the geometry of space
around celestial objects. Nonetheless, figure 7
reveals an increase in responses other than ‘yes’
or ‘no’ post-intervention with the addition of
more conceptualised answers like ‘the shape
changes with gravity’ or ‘it stretches’ demon-
strating an understanding of the ideas presen-
ted using the spacetime simulator. 9.2% of post-
intervention participants shown deeper under-
standing by correctly noting that space is curved
around masses but flat otherwise. Coupling these
responses with the other ‘yes’ responses gives a
total percentage of conceptually correct answers
of 58.9%.
January 2024
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Phys. Educ. 59 (2024) 015001
C McInerney and P Sutton
Figure 8. Responses to Q9. Are you interested in learning more about gravity and general relativity?
Figure 9. Responses to Q10. Should Einsteinian physics, like general relativity be included in the curriculum?
Figure 8 shows responses to Q9, where 77.1%
of participants said they would like to learn more
about gravity and GR.
The last question in our questionnaires
addresses the main research question of this work
and asked: should Einsteinian physics, like GR be
January 2024
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Einsteinian gravitational concepts throughout secondary school
included in the curriculum? results are shown in
figure 9. A resounding 82.5% of participants said
that it should be included. Of those, 10% indic-
ated that, if added to the curriculum, it should be
included at a specific level. 41% of those respond-
ents said that this content should not be taught
before A-level. The rest thought that it should not
be covered before KS4.
that
4. Conclusion
In this work, 183 students from a state-funded
English secondary school participated in a one-
off intervention introducing them to GR and the
concept
the gravitational force is caused
by the curvature of spacetime. This theory was
introduced visually using the spacetime simulator
demonstration. Once this idea was established,
participants performed an experiment using bal-
loons and triangles to investigate what happens to
these shapes in curved spaces.
The aim was to gauge students’ reception to
GR and to investigate where these concepts would
be best placed into a school curriculum.
Results showed that 77.1% of our participants
overall would like to delve further into the sub-
ject. This is consistent with the opinions of teach-
ers and the public who also encourage the addi-
tion of Einsteinian physics into the curriculum
[29, 30]. Noting that the largest percentage of our
participants come from Yr 7 shows how eager
young students are for opportunities to learn about
cosmology.
KS4 and A-level students demonstrated bet-
ter understanding of the presented ideas through
their responses to Q1–3 in the questionnaires.
Years 11, 12 and 13 had the best improvement
from pre- to post-questionnaire for Q1 and Q2,
with Yr 10 also showing a good increase in under-
standing for Q3. While many participants from the
other year groups liked the material covered, their
responses to Q3 showed little grasp of spacetime
curvature. Years 7, 8 and 9 all showed good aware-
ness of the deformation of triangles in curved
spaces after the intervention, only Yr 9 parti-
cipants showed a grasp of the curving of initially
parallel lines.
While Einsteinian gravitational concepts are
taught completely distinct from the Newtonian
gravity, it has been shown by other studies that
students can understand the ideas of GR even at
primary level [2, 15, 16, 18]. While the results
to Q1 and Q2 show that participants were able
to appreciate the effects of curvature, the results
of Q3 demonstrate that it would take more than
a one-off intervention to imbue a deeper under-
standing of GR. This result aligns with that of
other works [31]. Additionally, our intervention
was not successful at dispelling misconceptions
around the gravitational force. A multi-stage inter-
vention may prove more beneficial for this [32].
Regarding GR and its associated geometry,
our results show that this material is better suited
to the A-level curriculum rather than lower year
groups. Therefore, we conclude that introducing
GR in the English secondary curriculum at Yr 13
aligns with students’ ability to recognise curvature
as the source of gravitational force and matches
the current placement of gravity study in the
curriculum.
Further insights into the effects of teaching
GR could be obtained through a longitudinal study
that follows a group or groups of students through
late primary/early secondary school to KS4 and
A-level.
Data availability statement
The data cannot be made publicly available upon
publication due to legal restrictions preventing
unrestricted public distribution. The data that sup-
port the findings of this study are available upon
reasonable request from the authors.
Acknowledgments
The authors would like to thank the staff and
students of the science department at Queen
Elizabeth’s High School for their support with and
participation in this work.
Ethical statement
This study has been reviewed and given favour-
able opinion by a University of Lincoln Research
Ethics Committee. Reference Number: 12146.
January 2024
11
Phys. Educ. 59 (2024) 015001
C McInerney and P Sutton
ORCID iDs
Corey McInerney https://orcid.org/0000-0002-
2452-7259
Phil Sutton https://orcid.org/0000-0003-3936-
4170
Received 5 June 2023, in final form 4 September 2023
Accepted for publication 4 October 2023
https://doi.org/10.1088/1361-6552/ad001a
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Phys. Educ. 59 (2024) 015001
| null |
10.1371_journal.pone.0296688.pdf
|
Data Availability Statement: All data files are
available from the OpenBU database (https://hdl.
handle.net/2144/45321).
|
All data files are available from the OpenBU database ( https://hdl. handle.net/2144/45321 ).
|
RESEARCH ARTICLE
Flanged males have higher reproductive
success in a completely wild orangutan
population
Amy M. ScottID
Wahyu Susanto6, Tatang Mitra Setia6, Cheryl D. Knott1,7
1,2*, Graham L. Banes3,4, Wuryantari Setiadi5, Jessica R. Saragih5, Tri
1 Department of Anthropology, Boston University, Boston, Massachusetts, United States of America,
2 Department of Natural Resources and the Environment, University of New Hampshire, Durham, New
Hampshire, United States of America, 3 Wisconsin National Primate Research Center, University of
Wisconsin–Madison, Madison, Wisconsin, United States of America, 4 The Orang-Utan Conservation
Genetics Project, Madison, Wisconsin, United States of America, 5 Eijkman Research Center for Molecular
Biology, National Agency for Research and Innovation (BRIN), The Science and Technology Center of
Soekarno, Cibinong, West Java, Indonesia, 6 Departemen of Biology, Faculty of Biology and Agricultural,
Universitas Nasional, Kota Jakarta Selatan, Daerah Khusus Ibukota Jakarta, Indonesia, 7 Department of
Biology, Boston University, Boston, Massachusetts, United States of America
* [email protected]
Abstract
Male orangutans (Pongo spp.) exhibit bimaturism, an alternative reproductive tactic, with
flanged and unflanged males displaying two distinct morphological and behavioral pheno-
types. Flanged males are larger than unflanged males and display secondary sexual char-
acteristics which unflanged males lack. The evolutionary explanation for alternative
reproductive tactics in orangutans remains unclear because orangutan paternity studies to
date have been from sites with ex-captive orangutans, provisioning via feeding stations and
veterinary care, or that lack data on the identity of mothers. Here we demonstrate, using the
first long-term paternity data from a site free of these limitations, that alternative reproductive
tactics in orangutans are condition-dependent, not frequency-dependent. We found higher
reproductive success by flanged males than by unflanged males, a pattern consistent with
other Bornean orangutan (Pongo pygmaeus) paternity studies. Previous paternity studies
disagree on the degree of male reproductive skew, but we found low reproductive skew
among flanged males. We compare our findings and previous paternity studies from both
Bornean and Sumatran orangutans (Pongo abelii) to understand why these differences
exist, examining the possible roles of species differences, ecology, and human intervention.
Additionally, we use long-term behavioral data to demonstrate that while flanged males can
displace unflanged males in association with females, flanged males are unable to keep
other males from associating with a female, and thus they are unable to completely mate
guard females. Our results demonstrate that alternative reproductive tactics in Bornean
orangutans are condition-dependent, supporting the understanding that the flanged male
morph is indicative of good condition. Despite intense male-male competition and direct sex-
ual coercion by males, female mate choice is effective in determining reproductive out-
comes in this population of wild orangutans.
a1111111111
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OPEN ACCESS
Citation: Scott AM, Banes GL, Setiadi W, Saragih
JR, Susanto TW, Mitra Setia T, et al. (2024)
Flanged males have higher reproductive success in
a completely wild orangutan population. PLoS ONE
19(2): e0296688. https://doi.org/10.1371/journal.
pone.0296688
Editor: Honnavalli Nagaraj Kumara, Salim Ali
Centre for Ornithology and Natural History, INDIA
Received: August 21, 2023
Accepted: December 17, 2023
Published: February 9, 2024
Copyright: © 2024 Scott et al. This is an open
access article distributed under the terms of the
Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: All data files are
available from the OpenBU database (https://hdl.
handle.net/2144/45321).
Funding: This research was supported by
Adventure Travel Conservation Fund:
adventuretravelconservationfund.org; Arcus
Foundation (G-PGM-1708- 2235, G-PGM-1506-
1327, G-PGM- 1104-36, 1104-36/PID-01853,
0902-30): www.arcusfoundation.org; Association
of Zoos and Aquariums Conservation Endowment
Fund (13-1159, 11-1063) and Conservation Grants
PLOS ONE | https://doi.org/10.1371/journal.pone.0296688 February 9, 2024
1 / 20
PLOS ONEFund (15-1296): www.aza.org/conservation-
funding; Balikpapan Orangutan Society-Canada:
orangutan.ca; Conservation, Food and Health
Foundation: cfhfoundation.grantsmanagement08.
com; Disney Conservation Fund: impact.disney.
com/environment/conservation; Focused on
Nature: focusedonnature.org; Hollomon Price
Foundation: hollomonpricefoundation.org; Houston
Zoo: www.houstonzoo.org; Indonesia Climate
Change Trust Fund: www.icctf.or.id; Keidanren
Nature Conservation Fund: www.keidanren.net/
kncf/en; The Leakey Foundation: leakeyfoundation.
org; Nacey Maggioncalda Foundation: formerly:
www.naceymaggioncalda.org, currently:
leakeyfoundation.org; National Geographic Society
(ECO690-14, GEFNE68-13, 8564-08, C113-07):
www.nationalgeographic.org/society; National
Science Foundation (BCS-1638823, BCS-
0936199): nsf.gov; Ocean Park Conservation Fund:
www.opcf.org.hk/en; Orangutan Conservancy:
orangutan.com; Phoenix Zoo: www.phoenixzoo.
org; Primate Conservation International; Sea World
Busch Gardens Conservation Fund; swbg-
conservationfund.org; Tides Foundation: tides.org;
US Fish and Wildlife Service (F19AP00798,
F18AP00898, F15AP00812, F13AP00920,
F12AP00369, 96200-0-G249, 96200-9-G110,
98210-8-G661, 98210-7-G185): www.fws.gov;
Wenner-Gren Foundation: wennergren.org; Whitley
Fund for Nature: whitleyaward.org; Wildlife
Conservation Network: wildnet.org; Woodland Park
Zoo Partners for Wildlife: zoo.org; Zoo New
England: www.zoonewengland.org; and Zoo
Atlanta: zooatlanta.org grants to CDK. This
research was supported by Boston University
Graduate Research Abroad Fellowship: www.bu.
edu/cas/admissions/phd-mfa/fellowship-aid/aid-
for-phd-students; Boston University Graduate
Student Organization Research Grant: www.bu.
edu/gso/travelgrants; Boston University Women’s
Guild: www.bu.edu/womensguild; Cora Du Bois
Charitable Trust: library.harvard.edu/cora-du-bois-
fellowship; The Leakey Foundation:
leakeyfoundation.org/; and National Science
Foundation Graduate Research Fellowship (Grant
DGE-1247312): nsf.gov grants to AMS. The
funders had no role in study design, data collection
and analysis, decision to publish, or preparation of
the manuscript.
Competing interests: The authors have declared
that no competing interests exist.
Flanged male orangutans have higher reproductive success
Introduction
Alternative reproductive tactics (ARTs) are the existence of two distinct phenotypes within
one sex in the context of reproduction [1]. ARTs occur throughout the animal kingdom and
are expected to evolve when there is strong sexual selection [1,2], specifically intra-sexual com-
petition [2]. There are two primary explanations for the existence of ARTs. The two pheno-
types may be either frequency-dependent evolutionary stable strategies, where the relative
fitness of each morph depends on its frequency in the population [3] or condition-dependent,
due to difference in the quality (i.e. age, body condition, experience, nutritional state and/or
genes) of individuals where one morph is ‘making the best of a bad lot’ [4].
Male orangutans (Pongo spp.) display two ARTs with males exhibiting distinct morphologi-
cal (Fig 1) (expressed as bimaturism) and behavioral phenotypes [5–8]. Flanged males (50–90
kg) are up to twice the size of unflanged males, but some unflanged males reach flanged male
body size (30–59 kg) [9,10]. Flanged males possess secondary sexual characteristics, including
an enlarged throat sac and cheek flanges [6,7,11], and are the only morph capable of producing
long calls [5,6]. Flanged males are intolerant of each other, either avoiding or fighting and
wounding each other [5,12], but they are typically more tolerant of unflanged males [5]. Con-
versely, unflanged males are generally tolerant of each other and tend to avoid flanged males
[5,6]. Flanged males are dominant to unflanged males and displace unflanged males in con-
sortships with females [5,6,12–14]. It has been suggested that flanged males use consortships to
mate guard females, as a means to keep other males from mating with a female [12,15,16]. The
male morphs also differ in activity patterns, with unflanged males traveling further per day
than flanged males [14,17,18]. Due to these differences, the flanged male mating strategy has
been described as “sit, call, and wait” and the unflanged male strategy described as “go, search,
and find” [7,14].
For male orangutans, ARTs are plastic and sequential—an immature male first develops the
unflanged male phenotype and may develop the flanged male phenotype later, but this transi-
tion is irreversible [7,19]. There is tremendous variation in the age of flange development, with
wild males reportedly developing flanges from ages 14 to 30, and some males never developing
flanges [11,16,20]. Flanged males in poor condition exhibit shriveled flanges and are referred
to as past-prime males [21]. Past-prime males are not regularly seen, suggesting that this phase
is not reached by all males, and is likely short for the males who do become past-prime. Addi-
tionally, the presence of past-prime males indicates that the flanged morph is so costly to
maintain that some flanged males that cannot continue to maintain it enter the past-prime
state [11].
Understanding how sexual selection acts on traits, such as ARTs, requires considering mul-
tiple mechanisms of sexual selection simultaneously [22]. Both male and female reproductive
strategies are expected to impact the relative reproductive success of each morph [22], and this
is especially true for primates, where male and female strategies are closely tied [23]. Orangu-
tans are semi-solitary with large home ranges and adults primarily range alone or adult females
range with dependent offspring [11,16,24,25], so reproduction first requires finding a mate. It
has been suggested that one function of flanged male long calls is to attract females [26,27],
and it may also play a role in male-male competition [26,28,29]. Across study sites, female
orangutans prefer flanged males [5,6,21,30,31]. Orangutans also have slow life histories,
including the longest interbirth interval of any mammal (7.6 years) [32,33]. Slow life histories
push the potential for sexual conflict to an extreme [34]. Both male morphs employ sexual
coercion in the form of forced copulations [30,35]. Sexual coercion can override female mate
choice, but it is unknown if it increases male reproductive success. Female orangutans do not
display overt signals of ovulation, such as the sexual swellings typical of many cercopithecoids
PLOS ONE | https://doi.org/10.1371/journal.pone.0296688 February 9, 2024
2 / 20
PLOS ONEFlanged male orangutans have higher reproductive success
Fig 1. Example of male orangutans displaying the two alternative reproductive tactics. An unflanged male (left) lacks cheek pads and a
throat sac and has a smaller body size. A flanged male (right) has secondary sexual characteristics including large cheek pads (flanges), a large
throat sac, and larger body size. Photos by Tim Laman.
https://doi.org/10.1371/journal.pone.0296688.g001
[21,36] and ovulatory status appears to be effectively hidden from males [36,37]. Females pref-
erentially mate with prime flanged males when they are ovulating and show increased willing-
ness to mate with unflanged and non-prime males when the risk of conception is low [21].
Across primates this mating pattern—mating preferentially with preferred males when the
likelihood of conception is highest and mating with non-preferred males when the likelihood
of conception is lowest—is argued to be a paternity confusion strategy that reduces the likeli-
hood of infanticide [21,38,39].
Quantifying the reproductive success of each morph is essential for testing hypotheses
about the evolutionary pressures that resulted in orangutan ARTs. Previous studies of pater-
nity in both Bornean (Pongo pygmaeus) and Sumatran (Pongo abelii) orangutans are limited
by incomplete maternity data [40–43], the inclusion of ex-captive orangutans who may not
display natural mating behaviors, or by provisioning from feeding stations and from veterinary
care [13,20,44,45] (Table 1). The first orangutan (P. abelli) paternity study found that the two
morphs had similar reproductive success and therefore concluded that the two morphs repre-
sent alternative mating strategies that coexist as evolutionary stable strategies [20]. The subse-
quent three orangutan (P. pygmaeus) paternity studies all concurred that flanged males had
much higher reproductive success than unflanged males [13,44,45]. Each of these studies has
unique limitations (Table 1). There are also important island or species differences to consider.
P. abelii live in habitats with higher food availability, exist at higher densities, and are more
social compared to P. pygmaeus [24,46]. We present paternity data from Cabang Panti
Research Station in Gunung Palung National Park, Borneo, Indonesia (GPNP), the first from
completely wild orangutans with known mothers. We compare our results against others to
discern how study limitations and habitat differences explain contrasting results across sites.
Orangutan paternity studies also differ in the degree of male reproductive skew—the degree
to which reproduction is monopolized versus shared (Table 1). Characterizing male
PLOS ONE | https://doi.org/10.1371/journal.pone.0296688 February 9, 2024
3 / 20
PLOS ONEFlanged male orangutans have higher reproductive success
Table 1. Paternity determination and paternity skew across study sites.
Study Site
No. offspring
sired by
flanged
males
No. offspring
sired by
unflanged
males
Ketambe Research
Station, Gunung Leuser
National Park [18]
Kinabatangan Orang-
utan Conservation
Project, Lower
Kinabatangan Wildlife
Sanctuary [37]
Camp Leakey, Tanjung
Puting National Park
[36]
Sepilok Orangutan
Rehabilitation Center
[12]
Cabang Panti Research
Station, Gunung Palung
National Park
4
9
10
4
5
6
1
3c
1
0
Total
32
11
Total no.
offspring
with father
assigneda
10
10
14
6c
6c
46
Total no.
offspring
tested
Total no.
candidate
sires testeda
Study
Periodb
11
16
25
8
11
16
17
4
1983–
1997
(11)
1985–
2000 (8)
1993–
2009
(13)
2010–
2014 (1)
Most
successful
male’s share
(mean)
48.18
Most
successful
male’s share
(range)
33.33–100
33.32
18.18–50
56.57
14.29–100
57.14
NA
13
20
2008–
2014 (3)
33.33
20–40
Limitation
Ex-captives in study
population
Limited population
knowledge;
Mothers genetically
assigned
Feeding station; Ex-
captives in study
population;
veterinary care
Feeding station; Ex-
captives in study
population; Only
one flanged male
sampled
Gray background = P. abelii.
White background = P. pygmaeus.
a = Number of offspring and candidate sires tested are likely an underestimate of the total number of offspring born or candidate sires in the study site due to sampling
difficulties.
b = Number in parentheses is the number of 5-year periods during the study period.
c = Number of offspring sired by flanged males and unflanged males do not add up to the total because there was a male of unknown morph who sired an offspring.
https://doi.org/10.1371/journal.pone.0296688.t001
reproductive skew is important for understanding the evolution of ARTs in orangutans.
Across primates, the degree of male reproductive skew in multi-male groups is best explained
by the degree of female reproductive synchrony and the number of males in the group [47,48].
The orangutan social system, with a high fission-fusion dynamic (social associations vary in
size, composition, and cohesion) [11,24,49], and a lack of group formation, makes defining the
number of males in a "group" difficult. However, there is clearly a male biased operational sex
ratio, with many males competing for a few conception opportunities, due in part to the long
interbirth interval [16]. In terms of female reproductive synchrony, reproduction is asynchro-
nous, although some sites do see increases in births following periods of high fruit availability
[50]. Even without female reproductive synchrony, in a dispersed social system, low male
reproductive skew is expected [47]. Additionally, male dominance can lead to higher repro-
ductive success through priority-of-access [51], but this is not the case for all species [52]. Here
we compare male reproductive skew across sites and use long-term behavioral data to test the
ability of flanged males or a single dominant flanged male to mate guard females.
We combine long-term behavioral observations and genetic paternity determination from
a completely wild orangutan population at Cabang Panti Research Station in Gunung Palung
National Park, Borneo, Indonesia, to investigate the evolution of male ARTs in Bornean
orangutans. If male ARTs are frequency-dependent evolutionary stable strategies, we would
expect the frequency of each morph to be stable and relative fitness of each morph to depend
PLOS ONE | https://doi.org/10.1371/journal.pone.0296688 February 9, 2024
4 / 20
PLOS ONEFlanged male orangutans have higher reproductive success
on its frequency in the population [1,3], i.e. if 20% of males are flanged then 20% of offspring
will be sired by flanged males. Conversely if the male morphs are condition-dependent strate-
gies, then we would expect unequal fitness benefits for each morph, where the morph in ‘poor
condition’ has lower reproductive success and takes advantage of alternative tactics [1,4]. First,
we determine the relative reproductive success of the two morphs and measure male reproduc-
tive skew. Second, we test the ability of flanged males to mate guard females. We then compare
our results to those from prior studies in other populations to discern how study limitations
and habitat differences might explain contrasting results across studies. Finally, we discuss the
implications of these results for our understanding of the evolution of ARTs in orangutans and
the interaction between male and female reproductive strategies.
Materials and methods
Study site and population
Orangutans (Pongo pygmaeus wurmbii) were studied in Gunung Palung National Park
(GPNP), West Kalimantan, Indonesia, based out of the Cabang Panti Research Station (CPRS)
(1˚13´S, 1107´E) (3400 ha), as part of a study that began in 1994 [53]. Most orangutans
encountered and followed were habituated and individually identifiable, but unknown and
unhabituated individuals were also encountered, due to male dispersal and large home ranges
[11,24,54,55]. Each month, phenology data were collected to characterize food availability of
orangutan foods from 60 plots (totaling 9 ha) spread across 6 habitat types in the study site
[56,57]. Fruit availability was calculated from the top 25 genera of plants that orangutans are
known to consume most often at GPNP which represented 80% of fruit in their diet [57,58].
We then normalized that data by calculating modified Z scores from the percentage of stems
that had mature or ripe fruits. Food availability was used as a control variable in our statistical
models.
Behavioral data collection
We used long-term data (2008–2019) from orangutans in CPRS collected during focal follows
[59] to assess the ability of the two male morphs to effectively mate guard females and to create
a male dominance hierarchy. During orangutan follows, an association was recorded when-
ever another orangutan came within 50 meters of the focal [60,61]. The identity and age-sex
class of all orangutans was recorded. Males were classified by morph—flanged or unflanged.
For this analysis, males who had small, developing flanges were classified as unflanged males.
We used long-term follow data to tally the number of flanged and unflanged males that were
seen in the study site one year prior to and following conception for each offspring, where we
were able to identify a father and determine his morph. Females were classified as ‘sexually
active’ or ‘non-sexually active’ based on the likelihood that they were fecund and actively mat-
ing. The ‘sexually active’ category included nulliparous females, parous females without depen-
dent offspring, mothers with offspring over age six, and pregnant females in the first trimester.
Females in this population are most proceptive to mating during the first trimester of preg-
nancy [21]. The non-sexually active category included parous females with dependent off-
spring under age six and pregnant females in the second and third trimester. Since orangutans
have a gestation period of approximately eight months [62] and an average interbirth interval
of 7.6 years [32], females will on average conceive when a dependent offspring is 6.8 years old
and will begin mating 6–12 months before she conceives. Therefore, we used six years as a cut-
off because we expected females to begin mating again at approximately that time. Addition-
ally, we have previously shown that male-female interactions change when the dependent off-
spring reaches age six [63].
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We analyzed all adult male-female associations from 2008–2019 (N = 759), noting the
occurrence and outcome of an encounter with a second or ‘extra-pair male’ (EPM). If the asso-
ciation between the first male and female was terminated after the second male arrived, and
the second male stayed with the female, we defined this as male displacement. Displacement
did not necessarily involve agonism or aggression between the males, nor was it necessarily
immediate. For each male-female association, the length of the association (in minutes) and all
mating events were also recorded.
We analyzed all adult male-male interactions from 2008–2014, the period with both behav-
ioral data and with paternity determination data, to evaluate male dominance rank. Offspring
with known paternities were conceived from January 2010 to August 2014. During this period,
nine of the sampled flanged males (Bilbo was still unflanged), an additional three individually
recognizable flanged males, and up to seven unknown flanged males were observed in the
study site. We examined the outcome of all dyadic interactions between flanged males to eval-
uate dominance rank. Dominance was defined by the outcomes of dyadic agonistic interac-
tions [64]. We included avoidance, displacement, and chase interactions as dominance
interactions with a clear dominant and subordinate individual.
Sample collection
Fecal samples were collected after observed defecation from known and unknown orangutans
from 2008 through 2019. When possible, two samples were collected from one individual on
separate occasions. Samples from mother and dependent offspring were collected in the same
encounter. Samples were stored in either RNAlater, 70% ethanol, or dried using the two-step
ethanol alcohol-silica desiccation method [65,66]. Dried samples were stored at ambient tem-
perature (up to 40˚ C) until analysis. Samples stored in RNAlater or 70% ethanol were stored
at -20˚ C or -80˚ C.
Genotyping and paternity analysis
We collected fecal samples from 42 orangutans for genotyping: 13 offspring, their 10 mothers,
and 19 candidate fathers (8 unflanged, 10 flanged, and 1 observed as both unflanged and
flanged males) in GPNP. Genomic DNA was extracted 2–3 times from each fecal sample using
ChimerX stool DNA purification kits. Following Morin et al. [67], we quantified DNA content
through qPCR12. We amplified a panel of 12 autosomal tetranucleotide microsatellites
[20,44,68–71] (S1 Table). These were first co-amplified in an initial PCR reaction, with suffi-
cient replicates to maintain error rates of less than 1% when scoring homozygotes, per Ara-
ndjelovic et al. [72], before the products were re-amplified with labelled primers in panels of
3–5 loci.
Fragment analysis was performed by the DNA sequencing unit at Eijkman Institute for
Molecular Biology, using an Applied Biosystems 3130 Genetic Analyzer to size alleles against a
GeneScan™ 500 LIZ™ internal size standard. Peaks were manually scored by two different peo-
ple using GeneMapper (v3.7 and v4.0). Scores were concordant irrespective of software ver-
sion. Heterozygotes were called when the same two alleles were observed in at least two
independent amplifications, and homozygotes were called when only one allele was observed
in up to five independent amplifications, per Arandjelovic et al. [72].
Prior to downstream analysis, CERVUS 3.0 [42] and MICRO-CHECKER 2.2.3 [73] were
used to assess genotypes for null alleles, allelic dropout, and scoring errors due to stuttering,
and to confirm that all 12 microsatellites were in Hardy-Weinberg equilibrium (S2 Table).
Individual identity analysis was performed in CERVUS 3.0 to ensure that purported replicates
derived from the same individual. Individuals genotyped at a minimum of nine loci were
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PLOS ONEFlanged male orangutans have higher reproductive success
subsequently used in parentage analysis, having met the minimum number of loci needed to
tell full siblings apart (PID-sibs <0.001) for the mean observed heterozygosity in our panel of
microsatellites (sensu Waits et al. [74]).
Paternity analyses were performed in CERVUS 3.0 [42] and in COLONY 2.0.6.7 [75], using
both an exclusionary approach and a likelihood approach. In the exclusionary approach, off-
spring are required to share one allele at each locus with the known mother and the other allele
must be shared with the father. On the other hand, the likelihood approach in CERVUS 3.0
allows for genotyping errors, null alleles, and potential mutations. The advantage of COLONY
2.0.6.7 is that it uses a full-pedigree likelihood approach, rather than dyadic relationships,
when inferring both parentage and sibship.
Field observation of mother-offspring pairs was confirmed using exclusionary maternity
analysis CERVUS 3.0. Mothers were then used as known parents in CERVUS 3.0, increasing
the statistical power of paternity assignment. All sampled males were considered candidate
fathers for each offspring. Paternity was simulated using 100,000 offspring to obtain critical
values of Delta at confidence levels of 80% (relaxed) and 95% (strict), sensu Marshall et al.
[43]. For simulation in CERVUS 3.0, the proportion of candidate fathers sampled was
inferred at three different values: 0.2, 0.5, 0.65 to simulate the possibility that an unsampled
sire fathered offspring. The values 0.65 and 0.2 represent the upper and lower limits of
‘unknown’ males being entirely ‘known’ males or entirely ‘unknown, unique’ males, respec-
tively. Each value produced the same results, so we report values using 0.5 as the proportion
of candidate fathers.
In COLONY 2.0.6.7, analysis was run with the following parameters: female polygamy and
male polygamy without inbreeding or clones, ‘long’ length of run, ‘high’ likelihood precision,
no updating of allele frequency, and no sibship prior. Reported paternity results take known
maternal genotype into account. Again, all sampled males were considered candidate fathers
for each offspring.
Cross-site comparisons
We compared our paternity data from CBRS in GPNP to published paternity results from four
other orangutan study sites: Kinabatangan Orangutan Conservation Project, Lower Kinaba-
tangan Wildlife Sanctuary [45]; Ketambe Research Station, Gunung Leuser National Park [20];
Camp Leakey, Tanjung Puting National Park [44]; and Sepilok Orangutan Rehabilitation Cen-
ter [13].
Reproductive skew
We calculated male reproductive skew (2008–2014) using two measures: Nonacs B index
[76,77] and the most successful sire’s share as a percentage. We calculated both measures for
our study population and the most successful sire’s share for all published orangutan paternity
data. Due to the male dispersal and long lives, we were unable to accurately estimate adult
male ages required for the multinomial skew index [78], and Nonacs B index was calculated
with the Skew calculator 2013 (https://www.dropbox.com/home/2013%20Version, accessed
December 2021) [79]. The B index takes residency and number of offspring into account (see
S1 File for details of interpretation). We included only sampled males and the two unsampled
fathers (of the two offspring for whom we could not identify a father) in our calculation. For
the unsampled fathers, we used the average male residency time across this study period, 3
years.
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Statistical analysis
To test the ability of flanged and unflanged males to mate guard females, we used two-sided
Fisher’s exact tests to compare the rate at which the two male morphs are displaced by an EPM
in association with a female (N = 63). We additionally tested this hypothesis using two-sided
Fisher’s exact tests to compare the rate at which the two male morphs are displaced by an EPM
in association with only sexually active females (N = 36). Fisher’s exact tests are appropriate for
comparisons when values in some categories are less than five [80].
Further, we tested the possibility that flanged male presence alone acts as a deterrent pre-
venting EPM from encountering the flanged male-female pair using Chi-square tests of equal
proportions and a binomial generalized linear mixed model (GLMM). We used Chi-square
tests of equal proportions to compare the rate at which sexually active female (N = 486 associa-
tions), non-sexually active female (N = 201 associations), and total female associations
(N = 706 associations) with flanged versus unflanged males encounter an additional or EPM.
We also tested whether male-female association grouping (sexually active female-flanged male,
sexually active female-unflanged male, non-sexually active female-flanged male, and non-sexu-
ally active female-unflanged male) impacted the chance of encountering an EPM using a bino-
mial GLMM. Data exploration and model residuals revealed no violations of the assumptions
of the binomial GLMM [81]. The response variable was the occurrence of an encounter with
an EPM (yes/no). We used the length of a male-female association as an offset variable and
included the identity of the male and female as random effects. Fruit availability (see Study Site
and Population) was included as a fixed effect (control variable) because some study sites show
that orangutans are more social during periods of high fruit [82–84] (but see [85,86]). We
compared AIC values between models that excluded fixed effects to determine the best model
and how to code male morph and female reproductive class (S3 Table).
We performed all statistical procedures in R [87]. For the nonparametric post-hoc tests, we
used the package PMCMR [88]. For the binomial GLMMs, we used the packages lme4 [89]
and arm [90] to calculate confidence intervals. Graphs were made in the packages ggplot2 [91]
and cowplot [92].
This study followed the American Society of Primatologists’ ‘Ethical Treatment of Non-
Human Primates’ principles. It was non-invasive and observational. All protocols were
approved by The Eijkman Institute Research Ethics Commission, Boston University IACUC
(protocol no. 11–045 and 14–043) or deemed exempt by Boston University IACUC. All proto-
cols were approved by the Indonesian State Ministry for Research and Technology (RISTEK),
the Ministry of Home Affairs and the Indonesian Institute of Sciences (LIPI), the Center for
Research and Development in Biology (PPPB), and Balai Taman Nasional Gunung Palung
(BTNGP). Sample collection was approved by Balai Taman Nasional Gunung Palung
(BTNGP), permit numbers: 86/YPPN/SK/XII/2009-2019.
Results
Male reproductive success
Each of the three methods of paternity determination (exclusionary and likelihood approaches
in CERVUS and full-pedigree likelihood approach in COLONY) were concordant in paternity
assignment (Table 2). Paternity could be assigned for five out of seven offspring conceived
during the sampling period (2008–2019) and one individual conceived prior to the sampling
period. The flange-status of this sire at the time of conception (ca. 2005) is unknown, but he
was flanged at first observation in 2009. Over a six-year period (2009–2014), four flanged
males sired five offspring, indicating that male morph plays an important role in male
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Table 2. Paternity assignment at cabang panti research station in GPNP.
Offspring
Est. Birth Year
Mother
Trio mis-match
Pe
Next best mis-match
Delta
Assigned Father
CERVUS
Exclusion
Likelihood
COLONY
Prob.
Dagul
Rossa
Berani
Ijal
Telur
Uok
Januari
Benny
Dolia
Hannah
Vanna
Tawni
Bayasa
2002 Delly
2004 Veli
2005
Bibi
2005
Irmaa
2007
Tari
2007 Umi
2009
JT
2010
Beth
2011 Dewi
2012 Heraa
2012 Veli
2014
Tari
2015
Bibi
—
—
0
—
—
—
—
0
0
—
0
1
0
—
—
—
—
—
—
—
0.999
0.999
0.999
0.999
0.999
0.998
—
—
4
—
—
—
—
3
2
—
1
4
2
—
—
—
—
—
—
—
13.7
‡
7.76
4.30
6.50
4.08
5.29
‡
‡
‡
‡
‡
—
—
0.999
—
—
—
—
0.961
0.023
—
0.880
0.023
0.072
—
—
Codet
—
—
—
—
Prabu
Senjaa
—
Prabu
Mandab
Moris
Gray = conceptions within the sampling (fecal and behavioral data collected) period.
a = genotyped at 11 loci, not all 12 loci.
b = genotyped at 10 loci, not all 12 loci.
Bold = male is known to have been flanged at the time of conception. Non-bolded father means that his phenotype was unknown at the time of conception.
Trio mismatch = the number of loci that are a mismatch in the trio of offspring, mother and assigned father.
Pe = exclusion probability, calculated in CERVUS 3.0 using allele frequencies from all 48 individuals genotyped.
Next best mismatch = refers to the trio of offspring, mother, and the male with the closest match after the assigned father.
‡ = the trio delta value meets the strict (95%) confidence level.
https://doi.org/10.1371/journal.pone.0296688.t002
reproductive success (Table 2). During each of these conception periods, there were never
more flanged males than unflanged males observed in the study site (S4 Table). The mothers
of these five offspring were parous at the time of conception. For the two offspring for whom
fathers could not be determined, the COLONY pedigree results inferred different fathers.
Male reproductive skew
We found low reproductive skew in our study population. From 2008 to 2014, the period with
both behavioral data and offspring genetic sampling, the most successful sire’s share was
28.57% and Nonacs B index was 0.0004 (Npotential sires = 17, Noffspring = 6, P = 0.502, 95% CI =
-0.121–0.188) (Table 1). Our Nonacs B values indicated either a random or equal distribution
of male reproductive skew (equalB = 0.121, monopolyB = 0.922, see S1 File for details of inter-
pretation). Unfortunately, we were not able to construct a male dominance hierarchy because
only six interactions between flanged males were observed during this same period, with 3434
flanged male observation hours (S5 Table). Even with few observations, we did not find a strict
relationship between male dominance and reproductive success. For example, Senja, who
sired one known offspring during this period, was subordinate to Codet, who did not sire any
known offspring during this period (Tables 1 and S5).
Cross-site comparisons
Combining paternity assignment data across the five study sites showed that, overall, flanged
males sired a greater proportion of offspring (69.57%) than did unflanged males (23.91%)
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PLOS ONEFlanged male orangutans have higher reproductive success
(Table 1). This was especially true for Bornean sites, where flanged males sired 77.78% of off-
spring (Table 1). There was also variation in the degree of male reproductive skew across study
sites (Table 1). Across study sites, the mean most successful sire’s share (for 5-year periods)
ranged from 33.33%-57.57% (Table 1).
Mate guarding
Our paternity results demonstrated that a single male was unable to monopolize paternity
within our study site during any time period. To examine this from a behavioral perspective,
we examined the ability of males to mate-guard females. We tested whether the presence of a
male in association with a female served to deter a second or ‘extra-pair male’ (EPM) from
interacting with that female. Further, we examined the outcome of those interactions to deter-
mine if flanged males were able to displace unflanged males.
We observed no significant difference in the rate at which female associations with flanged
and unflanged males encountered an EPM (χ2 = 0.120, df = 1, P = 0.730, N = 706). On average,
an EPM was encountered every 56.65 hours of unflanged male-female associations, and every
54.08 hours of flanged male-female associations (S6 Table). Likewise, there was not a signifi-
cant difference in the rate at which sexually active female associations (χ2 = 2.412, df = 1,
P = 0.120, N = 486) or non-sexually active female associations (χ2 = 0.746, df = 1, P = 0.388,
N = 201) with flanged and unflanged males encountered an EPM. On average, sexually active
females in association with flanged males encountered an EPM every 95.85 hours and in asso-
ciation with unflanged males encountered an EPM every 70.78 hours (S6 Table). In contrast,
non-sexually active females in association with flanged males encountered an EPM every 15.28
hours and in association with unflanged males encountered an EPM every 43.08 hours, on
average (S6 Table). Our best binomial Generalized Linear Mixed Model (GLMM) found that
food availability and both male and female age-sex classes significantly impacted the likelihood
that a male-female association would encounter an EPM (S7 Table). Flanged males with non-
sexually active females were significantly more likely to encounter an EPM than were either
flanged or unflanged males with sexually active females (S7 Table and Fig 2).
However, after an EPM was encountered, there was a statistically significant difference
between male morphs in the proportion of encounters in which the first male associating with
a female was displaced (Fisher’s Exact Test, N = 50, P = 0.0004) (Fig 3A). Unflanged males
were displaced in 60% of encounters with an EPM. Of the 18 times that unflanged males were
displaced, 61% of the EPM were flanged. Flanged males were only displaced in 10% of encoun-
ters with an EPM and they were never displaced by unflanged males. This 10% represents one
instance in which one flanged male chased off another flanged male in the presence of two
non-sexually active females. When considering only sexually active females, flanged males
were statistically significantly less likely to be displaced than unflanged males (Fisher’s Exact
Test, N = 36, P = 0.003) (Fig 3B). Conversely, when considering only non-sexually active
females, there is no difference in the rate of displacement between male morphs (Fisher’s
Exact Test, N = 20, P = 0.379) (Fig 3C). Thus, both female reproductive state and male morph
are important determinants of orangutan mating behavior [21].
Discussion
Male reproductive success and skew
Our paternity results (6 assigned paternities over 10 years) most closely align with those of
Kinabatangan [45], finding low reproductive skew among flanged males. While Kinabatangan
inferred maternity from genetic data, our results confirm the same overall pattern. Only these
two studies are from wholly wild and unprovisioned orangutans in primary rainforest habitat
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Fig 2. The proportion of male-female associations in which the dyad encounters an ‘Extra-Pair Male’ (EPM) by
male-female association group type. FL-SA = flanged male/sexually active female association. FL-NSA = flanged
male/non-sexually active female association. UF-SA = unflanged male/sexually active female association.
UF-NSA = unflanged male/non-sexually active female association. N values at the top of each column show the
number of male-female associations in each group type. Dark gray represents encounters with an EPM and light gray
represents no encounter with an EPM. Significance values from the binomial GLMM (* = P < 0.05).
https://doi.org/10.1371/journal.pone.0296688.g002
without feeding stations, ex-captive orangutans, or veterinary care. This suggests that flanged
males have higher reproductive success than unflanged males in completely wild Bornean pop-
ulations, and that a single flanged male cannot monopolize paternity. In contrast, provisioning
from feeding stations at Tanjung Putting [44] and Sepilok [13], in conjunction with veterinary
interventions, may explain why a single flanged male was able to monopolize paternity at these
two sites. Feeding stations may create an unnaturally high concentration of female orangutans
in one area, increasing the ability of a single male to monopolize females. One unexpected out-
come of feeding stations may be a reduction in genetic diversity in subsequent generations due
to high male reproductive skew. It is likely that without feeding stations, either (1) dominant
males are unable to monopolize females across large areas or (2) male dominance hierarchies
are less strict when males are not competing over access to a feeding station. Due to the rarity
of interactions between flanged males (6 interactions in 7 years), we could not construct a
dominance hierarchy, but all observed interactions suggest a linear hierarchy with no
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PLOS ONEFlanged male orangutans have higher reproductive success
Fig 3. Male displacement in male-female associations. The proportion of (a) all male-female associations, (b) a subset of male-female
associations where the female is a sexually active, and (c) a subset of male-female associations where the female is a non-sexually active in
which the first male is displaced by an ‘extra-pair male’ (EPM). Male displacement is represented by darker shading. N values at the top of
each column show the number of male-female associations by male morph. Dark gray represents encounters with displacement and light
gray represents encounter with no displacement. Significance values from Fisher’s exact tests (* = P < 0.05, ns = P > 0.05).
https://doi.org/10.1371/journal.pone.0296688.g003
observations of rank reversals or rank instability. Continued study of paternity and male inter-
actions at GPNP and more orangutan study sites could differentiate between these two
possibilities.
Paternity results from Ketambe, Sumatra [20], starkly contrast with those from Borneo—
unflanged males at Ketambe had higher reproductive success than flanged males [20]. It is
unclear if this represents a species difference or unusual population parameters. The combina-
tion of male rank instability, first-time mothers, and ex-captive females in that study [20,93]
may have resulted in an inflated reproductive advantage for unflanged males. For instance,
Sepilok and Tanjung Puting also found that the offspring of first-time mothers were sired by
unflanged males [13,44], although in GPNP nulliparous females formed preferential mating
relationships with flanged males [94]. If there truly is a species difference between the relative
reproductive success of flanged and unflanged males, it is likely due to differences in the dura-
tion of the unflanged stage and variation in the relative proportions of each morph between
the islands [19,86].
However, it is important to note that orangutan paternity studies are limited by small sam-
ple sizes (Table 1) due to their long interbirth intervals and semi-solitary social structure.
Smaller samples are more subject to random stochasticity, which may also play a factor in
explaining the differences between sites, but comparison of data across five different sites adds
robustness to these comparisons. Small sample sizes may contribute to the finding of lower
reproductive skew. In this comparative perspective, the two Bornean sites with completely
wild orangutans (GPNP and Kinabatangan) agree that flanged males have higher reproductive
success than unflanged males and reproductive success is spread broadly across many flanged
males. But with only one Sumatran site in the sample [20], where there are also ex-captives, it
is unclear if that pattern holds for Sumatran orangutans. Half of the offspring (5 out of 10) in
Ketambe were born to matrilines with ex-captive mothers, and 4 of these 5 offspring were
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PLOS ONEFlanged male orangutans have higher reproductive success
sired by unflanged males [93]. If mating strategies are learned through the observation of the
mother, then ex-captive matrilines might not display the same mate choice preferences as wild
orangutans.
Orangutan reproductive strategies
Orangutans exhibit male-male competition, sexual coercion by males, and female mate choice.
Reproductive success is impacted by the interaction between each of these male and female
reproductive strategies. Due to the highly dispersed spatial distribution of female orangutans
[11,24,25], it is expected that a single male cannot monopolize females or conceptions, result-
ing in low male reproductive skew [47]. Our paternity data concluded that a single male can-
not monopolize paternity, and the behavioral data on male-female association encounter rates
with EPMs further addresses the inability of a single flanged male to monopolize females. Con-
sistent with other studies [6,16,30], we found that flanged males at GPNP were able to displace
unflanged males associating with females, specifically with sexually active females. However,
the mere presence of a flanged male with a female does not keep other males away. But once a
sexually active female is an association with a male, regardless of male morph, the pair is less
likely to encounter an EPM. Female orangutans at GPNP display a mixed mating strategy pref-
erentially associating with prime, flanged males when they are most likely to conceive and with
non-prime, unflanged males when they are less likely to conceive [21,38]. Thus, females may
be choosing who to associate with based on their probability of conception [21,38]. The limited
ability of flanged males to mate guard further highlights the importance of female choice in
facultative associations and mating. Therefore, female preference for flanged males, coupled
with the flanged male ability to displace unflanged males, operate in parallel leading to higher
reproductive success for flanged males, and flanged male inability to completely mate guard
females, leads to low reproductive skew among these flanged males. Because both flanged and
unflanged males perform forced copulations [11,35], our results cannot speak to the efficacy of
that form of sexual coercion in leading to reproductive success. Since unflanged males have
lower reproductive success, it appears that harassment by unflanged males is not a successful
reproductive strategy. Instead, female preference for flanged males and flanged male competi-
tive ability are operating in the same direction, leading to higher reproductive success for
flanged males.
Alternative reproductive strategies
Our results also have important implications for understanding ARTs in male orangutans.
ARTs have been hypothesized to be either frequency-dependent evolutionary stable strategies
[3] or due to difference in the quality of individuals [1,4]. The first published study of orangu-
tan paternity, and still the only study in Sumatran orangutans, found that the two morphs had
comparable reproductive success at Ketambe, and thus argued that the two morphs were evo-
lutionary stable strategies [7,20]. Now, 20 years later with data from an additional four Bor-
nean sites, it is clear, that at least in Borneo, flanged males have higher reproductive success
than unflanged males.
The relative numbers of flanged and unflanged males are pivotal to our interpretation of
paternity data, but accurate counts of the numbers of males in a study site are difficult to
obtain due to large home ranges and the difficulty of visually identifying orangutans who tran-
sition from unflanged to flanged males. Cross-site comparisons agree that in Sumatra there are
approximately twice as many unflanged males as flanged males, whereas in Borneo there is
more inter-site variation, but the morphs exist in approximately equal proportions [12,19].
Long-term demographic data at GPNP agrees with these approximations [35]. These
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PLOS ONEFlanged male orangutans have higher reproductive success
proportions indicate that males remain in the unflanged morph longer in Sumatra than in Bor-
neo [19]. Because the first paternity study found that unflanged males sired 60% of offspring in
a Sumatran population, it was argued that flanged and unflanged male morphs represent alter-
native mating strategies that coexist, representing evolutionary stable strategies [7,20]. If this
result is representative of all of Sumatra, it could explain why Sumatran males remain
unflanged for longer than Bornean males. In this case, unflanged males avoid the energetic
and competitive costs of becoming a flanged male [11], while achieving reproductive success.
However, the paternity data from Borneo does not support the understanding that male alter-
native reproductive strategies are frequency-dependent evolutionary stable strategies. In Bor-
neo, 77% of offspring are sired by flanged males while flanged males only represent
approximately 50% of all males, demonstrating that the flanged morph is absolutely and rela-
tively more successful. Because the reproductive success of the morphs is not related to their
proportion in the population, Bornean orangutan ARTs are not frequency-dependent.
For Bornean orangutans, ARTs are due to individual differences in quality, with the flanged
morph indicating higher quality and unflanged morph indicating lower quality. Our results
support the view that the unflanged morph is a transitional stage, where unflanged males are
in a ‘waiting room’, avoiding the costs associated with the flanged morph, and ‘making the
best of a bad situation’ until they are able to flange [7,93]. The variation in results at different
study sites highlights the dynamic nature of ARTs; the ability of each morph to attain repro-
ductive success is likely highly dynamic, depending on the relative proportions of each male
morph and density of orangutans, which is influenced by food availability [24,95]. More data
on the relative proportion of each male morph, male dominance hierarchies, and paternity
data from additional study sites of P. abelii in Sumatra will clarify if island differences are due
to ecological factors or if there are true species differences. Additionally, studies of the recently
described Tapanuli orangutan (Pongo tapanuliensis)—who live on Sumatra, south of Lake
Toba, but inhabit less productive forests, live at lower densities, and are less social and thus
more similar to Bornean orangutans than Sumatran orangutans [84]—will further help to clar-
ify the relative roles of ecology and species differences.
These combined paternity results across sites align with the model of developmental arrest
in male orangutans developed by Pradhan et al. [95] which explains differences in the ratio of
flanged to unflanged males across sites through ecology. According to this model, longer
delays in the development of flanges are expected when females are monopolizable by the
dominant male because, in this situation, non-dominant flanged males will have lower repro-
ductive success; thus, males should remain unflanged to avoid the costs of the flanged male
morph [24,46,95]. Dominant male monopolization of females is expected when orangutans
live at higher densities and are more gregarious, which is related to increased food availability
[24,46]. Thus, where orangutans live at higher densities (i.e., Ketambe, Sumatra), a dominant
flanged male is expected to be able to monopolize females, and a smaller proportion of flanged
males are expected. It is worth noting that at Ketambe, there are periods of both high repro-
ductive skew, where a single flanged male sires many offspring, and periods of low reproduc-
tive skew which correspond to times of rank instability. Conversely, where orangutan habitat
is less productive and orangutans live at lower densities (i.e., Borneo), a dominant flanged
male is not expected to be able to monopolize females, and a greater proportion of flanged
males are expected. Paternity results from the two Bornean sites with completely wild orangu-
tans agree with this model, showing that in the absence of feeding stations, a single male is not
able to monopolize females. And in the Bornean case, we also see short developmental arrest,
resulting in relatively more flanged males. In Borneo, with low reproductive skew among
flanged males, there is a reproductive benefit to flanging.
PLOS ONE | https://doi.org/10.1371/journal.pone.0296688 February 9, 2024
14 / 20
PLOS ONEFlanged male orangutans have higher reproductive success
Despite intense male-male competition [5,12,96] and sexual coercion [11,35], female choice
remains an important factor in determining orangutan reproductive outcomes. The impor-
tance of female choice may explain why it is that in all primate species with male ARTs, the
morphs are attributed to individual differences in quality [23]. In taxa where the costs of repro-
duction are disproportionately borne by one sex, we expect strong sexual selection, including
mate choice to evolve [97]. In the case of mammals where obligate female gestation and lacta-
tion mean that females must invest heavily in reproduction and parental care, we expect female
choice to evolve [98], and thus is not surprising that male ARTs in orangutans are signals of
male quality that are subject to female choice. We predict that in species with both strong mate
choice, driven by differential costs of reproduction, and ARTs, the ARTs will be condition-
dependent, rather than frequency-dependent.
This study of orangutan paternity determination in GPNP is the first study of orangutan
paternity from a completely wild population in a primary rainforest site, without feeding sta-
tions, rehabilitant orangutans, or veterinary care, and with known maternal-offspring relation-
ships. This enables us to better understand why previous orangutan paternity studies disagree
on which morph has higher reproductive success and the degree of male reproductive skew.
We show that the ARTs are condition-dependent. Flanged males have higher reproductive
success, and unflanged males are ‘making the best of a bad situation’.
Supporting information
S1 Table. Panel of microsatellite primers used for genotyping.
(DOCX)
S2 Table. Summary statistics for the 12 microsatellite loci used.
(DOCX)
S3 Table. GLMM comparisons.
(DOCX)
S4 Table. Ratio of flanged to unflanged males during each of the five conception periods
where paternity and male morph were determined.
(DOCX)
S5 Table. Flanged male-flanged male dyadic dominance interactions from 2008 to 2014.
(DOCX)
S6 Table. Rates at which male-female associations encounter an additional or Extra-Pair
Male (EPM), expressed as the average number of hours of association per encounter with
an EPM.
(DOCX)
S7 Table. GLMM testing the probability that a male-female pair encountered an EPM.
(DOCX)
S1 File. Reproductive skew calculation and nonac’s b interpretation.
(DOCX)
Acknowledgments
We thank the Universitas Nasional (UNAS), the Eijkman Research Center for Molecular Biol-
ogy, National Research and Innovation Agency–BRIN (Eijkman Institute for Molecular Biol-
ogy–EIMB), the Universitas Tanjungpura (UNTAN), the Directorate of Natural Resource
PLOS ONE | https://doi.org/10.1371/journal.pone.0296688 February 9, 2024
15 / 20
PLOS ONEFlanged male orangutans have higher reproductive success
Conservation and Ecosystems (KSDAE)–Ministry of Environment and Forestry, the Gunung
Palung National Park office (BTNGP), National Research and Innovation Agency (BRIN, for-
merly LIPI), the Center for Research and Development in Biology (PPPB), and the Ministry of
Research and Technology/National Research and Innovation Agency (RISTEK/BRIN) for
their sponsorship, collaboration, and permissions to conduct research in Gunung Palung
National Park. We are grateful to all the dedicated field assistants, research assistants, field
managers, and students who assisted with project maintenance and data collection. Thank you
to the Genome Diversity and Disease Laboratory and DNA Sequencing Unit at EIMB and
Hannah Gorman, Morgana Haub, and Jay Coogan for help with genotyping. We would like to
thank Carolyn Hodges-Simeon, Christopher Schmitt, and Larissa Swedell for constructive sug-
gestions on the manuscript.
Author Contributions
Conceptualization: Amy M. Scott, Cheryl D. Knott.
Data curation: Amy M. Scott, Cheryl D. Knott.
Formal analysis: Amy M. Scott, Cheryl D. Knott.
Funding acquisition: Amy M. Scott, Cheryl D. Knott.
Investigation: Amy M. Scott, Jessica R. Saragih.
Methodology: Amy M. Scott, Graham L. Banes, Cheryl D. Knott.
Project administration: Amy M. Scott, Tri Wahyu Susanto, Cheryl D. Knott.
Resources: Wuryantari Setiadi, Tri Wahyu Susanto, Tatang Mitra Setia, Cheryl D. Knott.
Supervision: Wuryantari Setiadi, Tatang Mitra Setia, Cheryl D. Knott.
Validation: Amy M. Scott, Graham L. Banes.
Visualization: Amy M. Scott.
Writing – original draft: Amy M. Scott.
Writing – review & editing: Amy M. Scott, Graham L. Banes, Cheryl D. Knott.
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PHYSICAL REVIEW D 107, 023530 (2023)
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing
from SPT and Planck. II. Cross-correlation measurements
and cosmological constraints
C. Chang ,1,2 Y. Omori,1,2,3,4 E. J. Baxter,5 C. Doux,6 A. Choi,7 S. Pandey,6 A. Alarcon,8 O. Alves,9,10 A. Amon,4
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D. L. Burke,4,46 J. E. Carlstrom,1,2,8,61,62 J. Carretero,37 C. L. Chang,1,2,8 R. Chown,63,64 M. Costanzi,65,66,67
L. N. da Costa,10,68 A. T. Crites,1,2,69 M. E. S. Pereira,70 T. de Haan,71,72 J. De Vicente,50 S. Desai,73 H. T. Diehl,28
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J. D. Vieira,20,83 J. Weller,53,54 and R. Williamson104,1,2
(DES & SPT Collaborations)
1Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
2Kavli Institute for Cosmological Physics, University of Chicago, Chicago, Illinois 60637, USA
3Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305, USA
4Kavli Institute for Particle Astrophysics & Cosmology,
P. O. Box 2450, Stanford University, Stanford, California 94305, USA
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Philadelphia, Pennsylvania 19104, USA
7California Institute of Technology, 1200 East California Blvd,
MC 249-17, Pasadena, California 91125, USA
8Argonne National Laboratory, 9700 South Cass Avenue, Lemont, Illinois 60439, USA
9Department of Physics, University of Michigan, Ann Arbor, Michigan 48109, USA
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11Physics Department, 2320 Chamberlin Hall, University of Wisconsin-Madison,
1150 University Avenue Madison, Wisconsin 53706-1390
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13Department of Physics, Northeastern University, Boston, Massachusetts 02115, USA
14Laboratory of Astrophysics, École Polytechnique F´ed´erale de Lausanne (EPFL),
Observatoire de Sauverny, 1290 Versoix, Switzerland
15Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, Brazil
16Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15312, USA
17Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife, Spain
18Universidad de La Laguna, Dpto. Astrofísica, E-38206 La Laguna, Tenerife, Spain
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19Center for Astrophysical Surveys, National Center for Supercomputing Applications,
1205 West Clark St., Urbana, Illinois 61801, USA
20Department of Astronomy, University of Illinois at Urbana-Champaign,
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21Physics Department, William Jewell College, Liberty, Missouri, 64068
22Department of Physics, Duke University Durham, North Carolina 27708, USA
23Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, University of Manchester,
Oxford Road, Manchester, M13 9PL, United Kingdom
24Institut d’Estudis Espacials de Catalunya (IEEC), 08034 Barcelona, Spain
25Institute of Space Sciences (ICE, CSIC),
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26Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720, USA
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30Jet Propulsion Laboratory, California Institute of Technology,
4800 Oak Grove Drive, Pasadena, California 91109, USA
31Department of Physics & Astronomy, University College London,
Gower Street, London, WC1E 6BT, United Kingdom
32Center for Cosmology and Astro-Particle Physics, The Ohio State University,
Columbus, Ohio 43210, USA
33Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
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35Department of Astronomy, University of California,
Berkeley, 501 Campbell Hall, Berkeley, California 94720, USA
36Kavli Institute for Cosmology, University of Cambridge,
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Campus UAB, 08193 Bellaterra (Barcelona) Spain
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Scheinerstrasse 1, 81679 Munich, Germany
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Brighton, BN1 9QH, United Kingdom
43Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa,
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Cambridge CB3 0WA, United Kingdom
45Perimeter Institute for Theoretical Physics, 31 Caroline St. North, Waterloo, Ontario N2L 2Y5, Canada
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13083-859, Campinas, SP, Brazil
48Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo,
Kashiwa, Chiba 277-8583, Japan
49ICTP South American Institute for Fundamental Research Instituto de Física Teórica,
Universidade Estadual Paulista, São Paulo, Brazil
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56Cerro Tololo Inter-American Observatory, NSF’s National Optical-Infrared Astronomy
Research Laboratory, Casilla 603, La Serena, Chile
57Institute of Cosmology and Gravitation, University of Portsmouth,
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58CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014, Paris, France
59Sorbonne Universit´es, UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris,
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London Ontario N6A 3K7, Canada
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70Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany
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73Department of Physics, IIT Hyderabad, Kandi, Telangana 502285, India
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80Institute of Astronomy, University of Cambridge,
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81Department of Physics, University of Colorado, Boulder, Colorado, 80309, USA
82School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
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1110 West Green Street, Urbana, Illinois 61801, USA
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87Australian Astronomical Optics, Macquarie University, North Ryde, New South Wales 2113, Australia
88Lowell Observatory, 1400 Mars Hill Rd, Flagstaff, Arizona 86001, USA
89Department of Physics, University of California, Berkeley, California, 94720, USA
90Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo,
CP 66318, São Paulo, SP, 05314-970, Brazil
91Department of Astrophysical Sciences, Princeton University,
Peyton Hall, Princeton, New Jersey 08544, USA
92Department of Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois, 60637, USA
93Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
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99Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
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PHYS. REV. D 107, 023530 (2023)
100Liberal Arts Department, School of the Art Institute of Chicago, Chicago, Illinois USA 60603
101School of Physics and Astronomy, University of Southampton,
Southampton, SO17 1BJ, United Kingdom
102Harvard-Smithsonian Center for Astrophysics,
60 Garden Street, Cambridge, Massachusetts 02138, USA
103Computer Science and Mathematics Division, Oak Ridge National Laboratory,
Oak Ridge, Tennessee 37831
104Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA
(Received 4 April 2022; accepted 30 September 2022; published 31 January 2023)
Cross-correlations of galaxy positions and galaxy shears with maps of gravitational lensing of the
cosmic microwave background (CMB) are sensitive to the distribution of large-scale structure in the
Universe. Such cross-correlations are also expected to be immune to some of the systematic effects that
complicate correlation measurements internal to galaxy surveys. We present measurements and modeling
of the cross-correlations between galaxy positions and galaxy lensing measured in the first three years of
data from the Dark Energy Survey with CMB lensing maps derived from a combination of data from the
2500 deg2 SPT-SZ survey conducted with the South Pole Telescope and full-sky data from the Planck
satellite. The CMB lensing maps used in this analysis have been constructed in a way that minimizes
biases from the thermal Sunyaev Zel’dovich effect, making them well suited for cross-correlation studies.
The total signal-to-noise of the cross-correlation measurements is 23.9 (25.7) when using a choice of
angular scales optimized for a linear (nonlinear) galaxy bias model. We use the cross-correlation
measurements to obtain constraints on cosmological parameters. For our fiducial galaxy sample,
m ¼ 0.272þ0.032
which consist of four bins of magnitude-selected galaxies, we find constraints of Ω
−0.052
and S8 ≡ σ8
−0.028 ) when assuming linear
(nonlinear) galaxy bias in our modeling. Considering only the cross-correlation of galaxy shear with
−0.061 and S8 ¼ 0.740þ0.034
CMB lensing, we find Ω
−0.029 . Our constraints on S8 are consistent
with recent cosmic shear measurements, but
lower than the values preferred by primary CMB
measurements from Planck.
−0.044 and S8 ¼ 0.734þ0.035
m ¼ 0.245þ0.026
m ¼ 0.270þ0.043
¼ 0.736þ0.032
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
m=0.3
Ω
−0.028 (Ω
p
DOI: 10.1103/PhysRevD.107.023530
I. INTRODUCTION
Significant progress has been made recently in using
cross-correlations between galaxy imaging and cosmic
microwave background (CMB) surveys to constrain cos-
mological parameters. These developments have come
naturally as ongoing galaxy and CMB surveys collect
increasingly sensitive data across larger and larger over-
lapping areas of the sky. The Dark Energy Survey [DES, 1]
is the largest galaxy weak lensing survey today, covering
∼5000 deg2 of sky that is mostly in the southern hemi-
sphere. By design, the DES footprint overlaps with high-
resolution CMB observations
from the South Pole
Telescope [SPT, 2], enabling a large number of cross-
correlation analyses [3–12].
Although CMB photons originate from the high-redshift
Universe, their trajectories are deflected by low-redshift
structures as a result of gravitational lensing—these are the
same structures traced by the distributions of galaxies and
the galaxy weak lensing signal measured in optical galaxy
surveys. Cross-correlating CMB lensing with galaxy sur-
veys therefore allows us to extract information stored in the
large-scale structure.
t
κ
CMBi,
CMB, and hγ
In this work, we analyze both hδgκ
the cross
correlation of the galaxy density field δg and the CMB
CMBi,1 the
weak lensing convergence field κ
cross correlation of the galaxy weak lensing shear field γ
and κ
CMB. Notably, these two two-point functions correlate
measurements from very different types of surveys (galaxy
surveys in the optical and CMB surveys in the millimeter),
and are therefore expected to be very robust to systematic
biases impacting only one type of survey. Furthermore,
CMB lensing is sensitive to a broad range of redshift, with
peak sensitivity at redshift z ∼ 2; galaxy lensing, on the
other hand, is sensitive to structure at z ≲ 1 for current
surveys. As a result, the CMB lensing cross-correlation
functions, hδgκ
CMBi, are expected to increase in
signal-to-noise relative to galaxy lensing correlations as
one considers galaxy samples that extend to higher redshift.
Our analysis relies on the first three years (Y3) of galaxy
observations from DES and a CMB lensing map con-
structed using data from the 2500 deg2 SPT-SZ survey [13]
CMBi þ hγ
κ
t
1The “t” subscript denotes the tangential component of shear,
which will be discussed in Sec. IV.
023530-4
JOINT ANALYSIS OF …. II. CROSS-CORRELATION …
PHYS. REV. D 107, 023530 (2023)
t
κ
CMBi þ hγ
and Planck [14]. The combined signal-to-noise of the
hδgκ
CMBi measurements used in the present
cosmological analysis is roughly a factor two larger than in
the earlier DES þ SPT results presented in [11], which
used first year (Y1) DES data. This large improvement in
signal-to-noise derives from two main advancements:
(1) We have adopted a different methodology in con-
structing the CMB lensing map, which results in
much lower contamination from the thermal Su-
nyaev Zel’dovich (tSZ) effect, allowing small-scale
information to be used in the cosmological analysis.
This methodology is described in [15].
(2) Data from DES Y3 covers an area approximately
three times larger than DES Y1 and is slightly
deeper.
Along with the significant increase in signal-to-noise, we
have also updated our models for the correlation functions
to include a number of improvements following [16]. These
include an improved treatment of galaxy intrinsic align-
ments, inclusion of magnification effects on the lens galaxy
density, and application of the so-called lensing ratio
likelihood described in [17].
The analysis presented here is the second of a series of
three papers: In [15] (Paper I) we describe the construction
of the combined, tSZ-cleaned SPT þ Planck CMB lensing
map and the methodology for the cosmological analysis. In
this paper (Paper II), we present the data measurements of
the cross-correlation probes hδgκ
CMBi, a series
of diagnostic tests, and cosmological constraints from
this cross-correlation combination. In [18] (Paper III),
we will present the joint cosmological constraints from
hδgκ
CMBi and the DES-only 3 × 2 pt probes,2
and tests of consistency between the two, as well as
constraints from a joint analysis with the CMB lensing
auto-spectrum.
CMBi þ hγ
CMBi þ hγ
κ
κ
t
t
Suprime-Cam Subaru
Similar analyses have recently been carried out using
different galaxy imaging surveys and CMB data. [19]
studied the cross-correlation of the galaxy weak lensing
from the Hyper
Strategic
Program Survey [HSC-SSP, 20] and the Planck lensing
map [21]; [22] used the same HSC galaxy weak lensing
measurement to cross-correlate with CMB lensing from the
POLARBEAR experiment [23]; [24] cross-correlated gal-
axy weak lensing from the Kilo-Degree Survey [KiDS, 25]
and the CMB lensing map from the Atacama Cosmology
Telescope [ACT, 26]; and [27] cross-correlated the galaxy
density measured in unWISE data [28] with Planck CMB
lensing. Compared to these previous studies, in addition to
the new datasets, this paper is unique in that we combine
hδgκ
CMBi. Moreover, our analysis uses the
CMBi and hγ
κ
t
2The 3 × 2 pt probes refer to a combination of three two-point
functions of the galaxy density field δg and the weak lensing shear
field γ: galaxy clustering hδgδgi, galaxy-galaxy lensing hδgγti and
cosmic shear hγγi.
same modeling choices and analysis framework as in [16],
making it easy to compare and combine our results later
(i.e. Paper III).
The structure of the paper is as follows. In Sec. II we
briefly review the formalism of our model for the two cross-
correlation functions and the parameter inference pipeline
(more details can be found in Paper I). In Sec. III we review
the data products used in this analysis. In Sec. IV we
introduce the estimators we use for the correlation func-
tions. In Sec. V we describe out blinding procedure and
unblinding criteria. In Sec. VI we present constraints on
cosmological parameters as well as relevant nuisance
parameters when fitting to the cross-correlation functions.
Finally we conclude in Sec. VII.
II. MODELING AND INFERENCE
We follow the theoretical formalism laid out in Paper I
and [29] for this work. Here, we summarize only the main
equations relevant to this paper. Following standard con-
vention, we refer to the galaxies used to measure δg as lens
galaxies, and the galaxies used to measure γ as source
galaxies.
power
spectra: Using
Angular
Limber
approximation3
the cross-spectra between CMB
lensing convergence and galaxy density/shear can be
related to the matter power spectrum via:
[31],
the
Z
CκCMBXiðlÞ ¼
dχ
qκCMBðχÞqi
XðχÞ
χ2
(cid:3)
l þ 1=2
χ
(cid:4)
; zðχÞ
;
PNL
ð1Þ
where X ∈ fδg; γg, i labels the redshift bin, PNLðk; zÞ is the
nonlinear matter power spectrum, which we compute using
CAMB and HALOFIT [32,33], and χ is the comoving distance
to redshift z. The weighting functions, qXðχÞ, describe how
the different probes respond to large-scale structure at
different distances, and are given by
qκCMBðχÞ ¼
3Ω
mH2
0
2c2
χ
aðχÞ
χ(cid:2) − χ
χ(cid:2)
;
qi
δg
ðχÞ ¼ biðzðχÞÞni
δg
ðzðχÞÞ
dz
dχ
γðχÞ ¼
qi
3H2
0Ω
m
2c2
χ
aðχÞ
Z
χh
χ
dχ0ni
γðzðχ0ÞÞ
dz
dχ0
χ0 − χ
χ0
;
ð2Þ
ð3Þ
ð4Þ
3In [30], the authors showed that at DES Y3 accuracy, the
Limber approximation is sufficient for galaxy-galaxy lensing and
cosmic shear but insufficient for galaxy clustering. Given the
primary probe in this work, hδgκ
CMBi, are at much
lower signal-to-noise than galaxy-galaxy lensing and cosmic
shear, we expect that Limber approximation is still a valid choice.
CMBi þ hγ
κ
t
023530-5
C. CHANG et al.
PHYS. REV. D 107, 023530 (2023)
where H0 and Ω
m are the Hubble constant and matter
density parameters, respectively, aðχÞ is the scale factor
corresponding to comoving distance χ, χ(cid:2) denotes the
comoving distance to the surface of last scattering, bðzÞ is
the galaxy bias as a function of redshift, and ni
δg=γðzÞ are the
normalized redshift distributions of the lens/source galaxies
in bin i. We note that the above equations assumes linear
galaxy bias, which is our fiducial model. Modeling the
nonlinear galaxy bias involves changes to both Eq. (1) and
Eq. (3) (see below).
Correlation functions: The angular-space correlation
functions are then computed via
X
wδi
gκCMBðθÞ ¼
wγi
t
κCMBðθÞ ¼
l
X
l
2l þ 1
4π FðlÞPlðcosðθÞÞCδi
gκCMBðlÞ;
2l þ 1
4πlðl þ 1Þ
FðlÞP2
lðcosθÞCκi
γκCMBðlÞ;
ð5Þ
ð6Þ
where Pl and P2
l are the lth order Legendre polynomial
and associated Legendre polynomial, respectively, and
FðlÞ describes filtering applied to the κ
CMB maps. For
correlations with the κ
CMB maps, we set FðlÞ ¼
BðlÞHðl − l
− lÞ, where HðlÞ is a step
function and BðlÞ ¼ expð−0.5lðl þ 1Þσ2Þ with σ ≡
θ
FWHM=
FWHM describes the beam applied
to the CMB lensing maps (see discussion of l
max,
and θ
FWHM choices in Sec. III, and further discussion
in Paper I).
minÞHðl
ffiffiffiffiffiffiffiffiffiffiffi
8 ln 2
, and θ
min, l
max
p
Galaxy bias: We consider two models for the galaxy
bias. Our fiducial choice is a linear bias model where
bðzÞ ¼ bi is not a function of scale and is assumed to be a
free parameter for each tomographic bin i. The second bias
model is described in [34] and is an effective 1-loop model
with renormalized nonlinear galaxy bias parameters: bi
1
(linear bias), bi
2 (local quadratic bias), bi
s2 (tidal quadratic
bias) and bi
3nl (third-order non-local bias). The latter two
parameters can be derived from bi
1, making the total
number of free parameters for this bias model two per
tomographic bin i. To use this model, we replace the
combination of biPNL in Equation (1) with Pgm described
in [34].
Intrinsic alignment (IA): Galaxy shapes can be intrinsi-
cally aligned as a result of nearby galaxies evolving in a
common tidal field. IA modifies the observed lensing
signal. We adopt the five-parameter (a1,η1,a2,η2,bta) tidal
alignment tidal torquing model (TATT) of [35] to describe
galaxy IA. a1 and η1 characterize the amplitude and
redshift dependence of the tidal alignment; a2 and η2
characterize the amplitude and redshift dependence of
the tidal torquing effect; bta accounts for the fact that our
measurement is weighted by the observed galaxy counts.
In Sec. VI B, we will also compare our results using
the nonlinear alignment model
a simpler
IA model,
[NLA, 36]. The TATT model is equivalent to the NLA
model in the limit that a2 ¼ η2 ¼ bta ¼ 0.
Impact of lensing magnification on lens galaxy density:
Foreground structure modulates the observed galaxy den-
sity as a result of gravitational magnification. The effect of
magnification can be modeled by modifying Eq. (3) to
include the change in selection and geometric dilution
quantified by the lensing bias coefficients Ci
g:
qi
δg
ðχÞ → qi
δg
ðχÞð1 þ Ci
gκi
gÞ;
ð7Þ
where κi
in [29] and the values of Ci
to the values listed in Table I.
g is the tomographic convergence field, as described
g are estimated in [37] and fixed
Uncertainty in redshift distributions: We model uncer-
tainty in the redshift distributions of the source galaxies
with shift parameters, Δzi, defined such that for each
redshift bin i,
niðzÞ → niðz − Δi
zÞ:
ð8Þ
For the lens sample, we additionally introduce a stretch
parameter (σz) when modeling the redshift distribution, as
motivated by [38]:
niðzÞ → σi
zniðσi
z½z − hzi(cid:3) þ hzi − Δi
zÞ;
ð9Þ
where hzi is the mean redshift.
Uncertainty in shear calibration: We model uncertainty
in the shear calibration with multiplicative factors defined
such that the observed CκCMBγ is modified by
CκCMBγiðlÞ → ð1 þ miÞCκCMBγiðlÞ;
ð10Þ
where mi is the shear calibration bias for source bin i.
they can, however,
Lensing ratio (or shear ratio, SR): The DES Y3 3 × 2 pt
analysis used a ratio of small-scale galaxy lensing measure-
ments to provide additional information, particularly on
source galaxy redshift biases and on IA parameters. These
ratios are not expected to directly inform the cosmological
constraints;
improve constraints via
degeneracy breaking with nuisance parameters. The lensing
ratios can therefore be considered as another form of
systematic calibration, in a similar vein to, e.g., spectro-
scopic data used to calibrate redshifts, and image simulations
used to calibrate shear biases. In [17], it was demonstrated
that
the lensing ratio measurements are approximately
independent of the 3 × 2 pt measurements, making it trivial
to combine constraints from 3 × 2 pt and lensing ratios at the
likelihood level. Unless otherwise mentioned, all our analy-
ses will include the information from these lensing ratios. We
investigate their impact in Sec. VI B.
Angular scale cuts: The theoretical model described
above is uncertain on small scales due to uncertainty in our
understanding of baryonic feedback and the galaxy-halo
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TABLE I. Prior values for cosmological and nuisance param-
eters included in our model. For the priors, U½a; b(cid:3) indicates a
uniform prior between a and b, while N ½a; b(cid:3)
indicates a
Gaussian prior with mean a and standard deviation b. δðaÞ is
a Dirac Delta function at value a, which effectively means that the
parameter is fixed at a. Note that the fiducial lens sample is the
first 4 bins of the MAGLIM sample. The two high-redshift MAGLIM
bins and the REDMAGIC sample are shown in gray to indicate they
are not part of the fiducial analysis.
Parameter inference: We assume a Gaussian likelihood4
for the data vector of measured correlation functions, ⃗d,
given a model, ⃗m, generated using the set of parameters ⃗p:
ln Lð⃗dj ⃗mð ⃗pÞÞ ¼ −
1
2
XN
ij
ðdi − mið ⃗pÞÞTC−1
ij ðdj − mjð ⃗pÞÞ;
ð11Þ
Parameter
Ωm
As × 109
ns
Ωb
h
Ωνh2 × 104
a1
a2
η1
η2
bta
MAGLIM
b1(cid:4)(cid:4)(cid:4)6
b1(cid:4)(cid:4)(cid:4)6
1
b1(cid:4)(cid:4)(cid:4)6
2
C1(cid:4)(cid:4)(cid:4)6
l
Δ1…6
z × 102
σ1…6
z
REDMAGIC
b1(cid:4)(cid:4)(cid:4)5
b1(cid:4)(cid:4)(cid:4)5
1
b1(cid:4)(cid:4)(cid:4)5
2
C1(cid:4)(cid:4)(cid:4)5
l
z × 102
Δ1…5
σ1…4
z
Prior
U½0.1; 0.9(cid:3)
U½0.5; 5.0(cid:3)
U½0.87; 1.07(cid:3)
U½0.03; 0.07(cid:3)
U½0.55; 0.91(cid:3)
U½6.0; 64.4(cid:3)
U½−5.0; 5.0(cid:3)
U½−5.0; 5.0(cid:3)
U½−5.0; 5.0(cid:3)
U½−5.0; 5.0(cid:3)
U½0.0; 2.0(cid:3)
U½0.8; 3.0(cid:3)
U½0.67; 3.0(cid:3)
U½−4.2; 4.2(cid:3)
δð1.21Þ, δð1.15Þ, δð1.88Þ, δð1.97Þ, δð1.78Þ,
δð2.48Þ
N ½−0.9; 0.7(cid:3), N ½−3.5; 1.1(cid:3), N ½−0.5; 0.6(cid:3),
N ½−0.7; 0.6(cid:3), N ½0.2; 0.7(cid:3), N ½0.2; 0.8(cid:3)
N ½0.98; 0.062(cid:3), N ½1.31; 0.093(cid:3),
N ½0.87; 0.054(cid:3), N ½0.92; 0.05(cid:3),
N ½1.08; 0.067(cid:3), N ½0.845; 0.073(cid:3)
U½0.8; 3.0(cid:3)
U½0.67; 2.52(cid:3)
U½−3.5; 3.5(cid:3)
δð1.31Þ, δð−0.52Þ, δð0.34Þ, δð2.25Þ, δð1.97Þ
N ½0.6; 0.4(cid:3), N ½0.1; 0.3(cid:3), N ½0.4; 0.3(cid:3),
N ½−0.2; 0.5(cid:3), N ½−0.7; 1.0(cid:3)
δð1Þ, δð1Þ, δð1Þ, δð1Þ, N ½1.23; 0.054(cid:3)
METACALIBRATION
m1…4 × 103
Δ1…4
z × 10−2
N ½−6.0; 9.1(cid:3), N ½−20.0; 7.8(cid:3), N ½−24.0; 7.6(cid:3),
N ½−37.0; 7.6(cid:3)
N ½0.0; 1.8(cid:3), N ½0.0; 1.5(cid:3), N ½0.0; 1.1(cid:3),
N ½0.0; 1.7(cid:3)
connection (or, nonlinear galaxy bias). We take the
approach of only fitting the correlation functions on angular
scales we can reliably model. In Paper I we determined the
corresponding angular scale cuts by requiring the cosmo-
logical constraints to not be significantly biased when
prescriptions for unmodeled effects are introduced. In
Figs. 2 and 19 the scale cuts are marked by the gray bands.
where the sums run over all of the N elements in the data
and model vectors. The posterior on the model parameters
is then given by:
Pð ⃗mð ⃗pÞj⃗dÞ ∝ Lð⃗dj ⃗mð ⃗pÞÞPpriorð ⃗pÞ;
ð12Þ
where Ppriorð ⃗pÞ is a prior on the model parameters. Our
choice of priors is summarized in Table I.
The covariance matrix used here consists of an analytical
lognormal covariance combined with empirical noise
estimation from simulations. The covariance has been
extensively validated in Paper I. In Appendix A Fig. 11
we show that the diagonal elements of our final analytic
covariance are in excellent agreement with a covariance
estimated from data using jackknife resampling.
Our modeling and inference framework is built within
the COSMOSIS package [40] and is designed to be consistent
with those developed as part of [16]. We generate parameter
samples using the nested sampler POLYCHORD [41].
III. DATA
A. CMB lensing maps
There are two major advances in the galaxy and CMB
data used here relative to the DES Y1 and SPT analysis
presented in [9,10]. First, for the CMB map in the SPT
footprint, we used the method developed in [42] and
described in Paper I to remove contamination from the
tSZ effect by combining data from SPT and Planck. Such
contamination was one of the limiting factors in our Y1
analysis. Second, the DES Y3 data cover a significantly
larger area on the sky than the DES Y1 data. Consequently,
the DES Y3 footprint extends beyond the SPT footprint,
necessitating the use of the Planck-only lensing map [14]
over part of the DES Y3 patch. As discussed in Paper I,
the different noise properties and filtering of the two
lensing maps necessitates separate treatment throughout.
The “SPT þ Planck” lensing map, which overlaps with
the DES footprint at < −40 degrees in declination,
is
filtered by l
max ¼ 5000 and a Gaussian smooth-
ing of θ
FWHM ¼ 6 arcmin. This map is produced using
the combination of 150 GHz data from the 2500 deg2
SPT-SZ survey [e.g., 13], Planck 143 GHz data, and the
min ¼ 8, l
4See e.g., [39] for tests of the validity of this assumption in the
context of cosmic shear, which would also apply here.
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C. CHANG et al.
PHYS. REV. D 107, 023530 (2023)
tSZ-cleaned CMB Planck temperature map generated using
the Spectral Matching Independent Component Analysis
the SMICA-noSZ map). The
(SMICA) algorithm (i.e.
“Planck” lensing map, which overlaps with the DES
footprint at > −39.5 degrees in declination, is filtered by
max ¼ 3800 and a Gaussian smoothing of
min ¼ 8, l
l
θ
FWHM ¼ 8 arcmin is applied. This map is reconstructed
using the Planck SMICA-noSZ temperature map alone.
We leave a small 0.5 deg gap between the two lensing maps
to reduced the correlation between structures on the
boundaries. The resulting effective overlapping areas with
DES are 1764 deg2 and 2156 deg2 respectively for the
SPT þ Planck and Planck patches respectively.
B. The DES Y3 data products
is mostly in the southern hemisphere,
DES [43] is a photometric survey in five broadband
filters (grizY), with a footprint of nearly 5000 deg2 of sky
that
imaging
hundreds of millions of galaxies. It employs the 570-
megapixel Dark Energy Camera [DECam, 1] on the Cerro
Tololo Inter-American Observatory (CTIO) 4 m Blanco
telescope in Chile. We use data from the first three years
(Y3) of DES observations. The foundation of the various
DES Y3 data products is the Y3 Gold catalog described
in [44], which achieves S=N ∼ 10 for extended objects up
to i ∼ 23.0 over an unmasked area of 4143 deg2. In this
work we use three galaxy samples: two lens samples for
the galaxy density-CMB lensing correlation, hδgκ
CMBi,
and one source sample for the galaxy shear-CMB lensing
correlation, hγ
CMBi. We briefly describe each sample
below. These samples are the same as those used in [16]
and we direct the readers to a more detailed description of
the samples therein.
κ
t
1. Lens samples: MAGLIM and REDMAGIC
We will show results from two lens galaxy samples
named MAGLIM and REDMAGIC. Following [16], the first
four bins of the MAGLIM sample will constitute our fiducial
sample, though we show results from the other bins and
samples to help understand potential systematic effects in
the DES galaxy selection.
The MAGLIM sample consists of 10.7 million galaxies
selected with a magnitude cut that evolves linearly with the
photometric redshift estimate: i < 4zphot þ 18. zphot is deter-
mined using the Directional Neighborhood Fitting algorithm
[DNF, 45]. [46] optimized the magnitude cut to balance the
statistical power of the sample size and the accuracy of
the photometric redshifts for cosmological constraints from
galaxy clustering and galaxy-galaxy lensing. MAGLIM is
divided into six tomographic bins. The top panel of Fig. 1
shows the per-bin redshift distributions, which have been
validated using cross-correlations with spectroscopic gal-
axies in [38]. Weights are derived to account for survey
systematics, as described in [47].
FIG. 1. Redshift distribution for the tomographic bins for the
galaxy samples used in this work: the MAGLIM lens sample (top),
the REDMAGIC lens sample (middle) and the METACAL source
sample (bottom). The fiducial lens sample only uses the first four
bins of the MAGLIM sample, or the solid lines. We perform tests
with the nonfiducial samples (dashed lines)
for diagnostic
purposes.
The REDMAGIC sample consists of 2.6 million luminous
red galaxies (LRGs) with small photometric redshift
errors [48]. REDMAGIC is constructed using a red sequence
template calibrated via the REDMAPPER algorithm [49,50].
The lens galaxies are divided into five tomographic bins.
The redshift distributions are shown in the middle panel
of Fig. 1. These distributions are estimated using draws
from the redshift probability distribution functions of the
individual REDMAGIC galaxies. As with MAGLIM, [38]
validates the redshift distributions, and [47] derives sys-
tematics weights.
We note that in [16] the two high-redshift bins were
excluded in MAGLIM due to poor fits in the 3 × 2 pt
analysis, while the REDMAGIC sample was excluded due
to an internal tension between galaxy-galaxy lensing and
galaxy clustering. With the addition of CMB lensing cross-
correlations, one of the aims of this work will be to shed
light on potential systematic effects in the lens samples. We
briefly discuss this issue in Sec. VI D but there will be a
more in-depth discussion in Paper III when we combine
with the 3 × 2 pt probes.
2. Source sample: METACALIBRATION
For the source sample, we use the DES Y3 shear catalog
presented in [51], which contains over 100 million galaxies.
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The galaxy shapes are estimated using the METACALIBRATION
algorithm [52,53]. The shear catalog has been thoroughly
tested in [51,54]. In [54], the authors used realistic image
simulations to constrain the multiplicative bias of the shear
estimate to be at most 2%–3%, primarily attributed to a shear-
dependent detection bias coupled with object blending
effects. The residual shear calibration biases are folded into
the modeling pipeline and are listed in Table I.
The source galaxies are divided into four tomographic
bins based on the SOMPZ algorithm described in [55],
utilizing deep field data described in [56] and image
simulations described in [57]. The bottom panel of
Fig. 1 shows the redshift distributions, which have been
validated in [58,17].
IV. CORRELATION FUNCTION ESTIMATORS
Our estimator for the galaxy-CMB lensing correlation
[Eq. (5)] is
hδgκ
CMBðθαÞi ¼ hδgκ
CMBðθαÞi0 − hδRκ
CMBðθαÞi;
ð13Þ
where
hδgκ
CMBðθαÞi0 ¼
1
δgκCMB
θα
N
XNg
XNpix
i¼1
j¼1
ηδg
i
ηκCMB
j
κ
CMB;jΘαðj
ˆθi − ˆθjjÞ
ð14Þ
and
Our estimator for the galaxy shear-CMB lensing corre-
lation [Eq. (6)] is
PNgal
i¼1
hγ
κ
CMBðθαÞi ¼
t
PNpix
j¼1 ηe
κ
P
ηκCMB
i
j
sðθαÞ
CMB;jeij
t
ηκCMB
ηe
i
j
Θαðj
ˆθi − ˆθjjÞ
;
ð16Þ
where eij
is the component of the corrected ellipticity
t
oriented orthogonally to the line connecting pixel j and the
CMB value in the pixel is κj
source galaxy. The κ
CMB and ηe
i
and ηκCMB
are the weights associated with the source galaxy
j
and the κ
CMB pixel, respectively. The weights for the source
galaxies are derived in Gatti et al. [51] and combines the
signal-to-noise and size of each galaxy. sðθαÞ is the
METACALIBRATION response. We find that sðθÞ is approx-
imately constant over the angular scales of interest, but
different for each redshift bin. We carry out these mea-
surements using the TREECORR package5 [59] in the angular
range 2.50 < θ < 250.00. Note that Eq. (16) does not
require subtracting a random component as in Eq. (13)
since unlike a density field, the mask geometry cannot
generate an artificial signal in a shear field.
κ
CMBi and hγ
CMBi correla-
tion functions are shown in Fig. 2. The hδgκ
CMBi mea-
surements using the REDMAGIC sample are shown in
Appendix C. The signal-to-noise (S/N) of the different
measurements are listed in Table II. Here, signal-to-noise is
calculated via
The measured MAGLIM hδgκ
t
v
u
u
t
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
XN
C−1
ij dj
dT
i
ij
;
ð17Þ
hδRκ
CMBðθαÞi ¼
1
NRκCMB
θα
XNrand
XNpix
i¼1
j¼1
ηδR
i
ηκCMB
j
κ
CMB;jΘαðj
ˆθi − ˆθjjÞ;
S=N ≡
ð15Þ
where the sum in i is over all galaxies and the sum in j is
δgκCMB
over all pixels in the CMB convergence map; N
θα
) is the number of galaxy-κ
δRκCMB
(N
CMB pixel (random-
θα
CMB pixel) pairs that fall within the angular bin θα; ηδg,
κ
ηδR and ηκCMB are the weights associated with the galaxies,
the randoms and the κ
CMB pixels. The weights for the
galaxies/randoms are derived in Rodríguez-Monroy [47]
using a combination of maps of survey properties
(e.g., seeing, depth, airmass) to correct for any spurious
signals in the large-scale structure, while the κ
CMB weights
account for differences in the noise levels of pixels in the
κ
CMB map. The random catalog is used to sample the
selection function of the lens galaxies, and has a number
density much higher than the galaxies. ˆθi (ˆθj) is the
angular position of galaxy i (pixel j), and Θα is an
ˆθi − ˆθjj falls in the angular
indicator function that is 1 if j
bin θα and 0 otherwise.
t
κ
where d is the data vector of interest and C is the covariance
matrix. The final signal-to-noise of the fiducial hδgκ
CMBi þ
hγ
CMBi data vector after the linear bias scale cuts is 23.9,
about two times larger than in the Y1 study [11]—the main
improvement, in addition to the increased sky area, comes
from extending our analysis to smaller scales, enabled by
the tSZ-cleaned CMB lensing map. The tSZ signal
is
correlated with large-scale structure, and can propagate into
a bias in the estimated κ
CMB if not mitigated. In the DES Y1
analysis presented in [11], tSZ cleaning was not imple-
mented at the κ
CMB map level, necessitating removal of
small-scale CMB lensing correlation measurements from
the model fits. This problem was particularly severe for
hγ
CMBi. Comparing results for the SPT þ Planck and
Planck patches in Table II, the SPT þ Planck area domi-
nates the signal-to-noise before scale cuts in all the probes,
even with a smaller sky area. This is due to the lower noise
level of the SPT maps. However, since the higher signal-to-
κ
t
5https://github.com/rmjarvis/TreeCorr.
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C. CHANG et al.
PHYS. REV. D 107, 023530 (2023)
FIG. 2. Measurement of the MAGLIM galaxy density-CMB lensing correlation (top) and galaxy shear-CMB lensing correlation
(bottom). For each set of measurements, the upper row shows measurement with the SPT þ Planck CMB lensing map and the lower
row shows measurement with the Planck CMB lensing map. The shapes and amplitudes are different due to the difference in the L
cut and smoothing of the CMB lensing map. The light (dark) shaded regions in the hδgκ
CMBi panels indicate the data points removed
when assuming linear (nonlinear) galaxy bias, while the shaded regions in the hγ
CMBi panels show the data points removed in all
cases (only two bins require scale cuts). The dashed dark gray line shows the best-fit fiducial model for the fiducial lens sample,
while the χ2 per degree of freedom (ν) evaluated at the best-fit model with scale cuts for linear galaxy bias model is shown in the
upper left corner of each panel.
κ
t
t
κ
CMBi, even though hδgκ
noise necessitates a more stringent scale cut, the resulting
signal-to-noise after scale cuts is only slightly higher for
the SPT þ Planck patch. Finally, comparing hδgκ
CMBi and
hγ
CMBi starts with ∼75% more
signal-to-noise before scale cuts compared to hγ
CMBi, the
scale cuts remove significantly more signal in hδgκ
CMBi
compared to hγ
CMBi. This is due to limits in our ability to
model nonlinear galaxy bias on small scales—indeed we
see that the signal-to-noise in hδgκ
CMBi increases by 13%
when switching from linear to nonlinear galaxy bias model.
Overall, these signal-to-noise levels are consistent with the
forecasts in Paper I.
κ
κ
t
t
V. BLINDING AND UNBLINDING
Following [16], we adopt a strict, multilevel blinding
procedure in our analysis designed to minimize the impact
of experimenter bias. The first level of blinding occurs at
the shear catalog level, where all shears are multiplied by a
023530-10
secret factor [51]. The second level of blinding occurs at the
two-point function level, where we follow the procedure
outlined in [60] and shift the data vectors by an unknown
amount while maintaining the degeneracy between the
different parts of the data vector under the same cosmology.
The main analyses in this paper were conducted after the
unblinding of the shear catalog, so the most relevant
blinding step is the data vector blinding. Below we outline
the list of tests that were used to determine whether our
measurement is sufficiently robust to unblind:
(i) Pass all tests described in Appendix B, which indicate
no outstanding systematic contamination in the data
vectors. These tests include: (1) check for spurious
correlation of our signal with survey property maps,
(2) check the cross-shear component of hγ
CMBi,
(3) check the impact of weights used for the lens
galaxies, (4) check the effect of the point-source mask
in the CMB lensing map on our measurements, and
(5) check that cross-correlating an external large-scale
κ
t
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PHYS. REV. D 107, 023530 (2023)
TABLE II. Signal-to-noise for
the
hδgκCMBi þ hγtκCMBi data vector when different scale cuts are
applied. Rows involving the two high-redshift MAGLIM bins and
the REDMAGIC sample are shown in gray to indicate that they are
not part of the fiducial analysis.
the different parts of
Scale cuts
None Linear bias Nonlinear bias
SPT þ Planck
hδgκCMBi MAGLIM
hδgκCMBi MAGLIM 6 bin
hδgκCMBi REDMAGIC
hγ
CMBi MAGLIM
κ
t
26.8
30.2
23.7
15.0
17.9
20.5
17.0
10.4
CMBi MAGLIM
CMBi MAGLIM 6 bin
CMBi REDMAGIC
Planck
hδgκ
hδgκ
hδgκ
hγtκCMBi MAGLIM
Combined
hδgκCMBi MAGLIM
32.2
hγtκCMBi MAGLIM
18.2
hδgκCMBi þ hγtκCMBi MAGLIM 34.8
14.5
17.4
14.2
13.4
13.1
15.9
12.5
10.4
19.6
16.9
23.9
17.3
20.0
15.7
13.4
13.8
16.8
12.8
10.4
22.2
16.9
25.7
structure tracer (the cosmic infrared background in
this case) with different versions of our CMB lensing
maps yields consistent results.
(ii) With unblinded chains, use the posterior predictive
distribution (PPD) method developed in [61] to
evaluate the consistency between the two subsets
of the data vectors that use different CMB lensing
maps (i.e. the SPT þ Planck patch and the Planck
patch). The p-value should be larger than 0.01.
(iii) With unblinded chains, verify that the goodness-of-
fit of the data with respect to the fiducial model has a
p-value larger than 0.01 according to the same PPD
framework.
CMBi þ hγ
Except for the first step, all the above are applied to the
hδgκ
CMBi data vectors with the fiducial analysis
choices (ΛCDM cosmology and linear galaxy bias scale
cuts), for the first four bins of the MAGLIM lens sample.
κ
t
VI. PARAMETER CONSTRAINTS FROM
CROSS-CORRELATIONS OF DES
WITH CMB LENSING
CMBi þ hγ
Following the steps outlined in the previous section,
we found (1) no evidence for significant systematic biases
in our measurements, as shown in Appendix B, (2) we
obtain a p-value greater than 0.01 when comparing the
hδgκ
CMBi constraints from the Planck region to
constraints from the SPT þ Planck region, and (3) the
goodness-of-fit test of the fiducial hδgκ
CMBi
unblinded chain has a p-value greater than 0.01. In the
following, we will quote the precise p-values obtained from
these tests using the updated covariance matrix.
CMBi þ hγ
κ
κ
t
t
With all the unblinding tests passed, we froze all analysis
choices and unblinded our cosmological constraints. We
then updated the covariance matrix to match the best-fit
parameters from the cosmological analysis.6 The results
we present below use the updated covariance matrix.
The main constraints on cosmological parameters are
summarized in Table III.
A. Cosmological constraints from cross-correlations
In Fig. 3 we show constraints from hδgκ
CMBi
using the first 4 bins of the MAGLIM sample. For compari-
son, we also show constraints from hγ
CMBi-only, cosmic
shear (from [62,63]), and 3 × 2 pt (from [16]).
κ
t
We find that our analysis of hδgκ
CMBi þ hγ
CMBi þ hγ
CMBi gives
κ
κ
t
t
the following constraints:
m ¼ 0.272þ0.032
Ω
−0.052 ;
σ8 ¼ 0.781þ0.073
−0.073 ;
S8 ¼ 0.736þ0.032
−0.028 :
κ
t
m constraints. While hδgκ
As can be seen from Fig. 3 and expected from Paper I,
the constraints are dominated by hγ
CMBi
slightly improving the Ω
CMBi by
itself does not tightly constrain cosmology because of the
degeneracy with galaxy bias, the shape information in
hδgκ
CMBi provides additional information on Ωm when
combined with hγ
CMBi, with hδgκ
κ
CMBi.
t
t
t
κ
κ
CMBi þ hγ
Figure 3 also shows constraints from DES-only probes,
including cosmic shear and 3 × 2 pt. We find that the
constraints on S8 from hδgκ
CMBi are compa-
rable to those from cosmic shear and 3 × 2 pt, and in
reasonable agreement. The uncertainties of the hδgκ
CMBi þ
hγ
CMBi constraints on S8 are roughly 30% (70%) larger
than that of cosmic shear (3 × 2 pt). We will perform a
complete assessment of consistency between these probes
in Paper III. We can also see that the degeneracy direction
of the hδgκ
CMBi constraints are slightly differ-
ent from 3 × 2 pt, which will help in breaking degeneracies
when combined.
CMBi þ hγ
κ
t
We consider constraints from the SPT þ Planck and
Planck patches separately in Fig. 4. As discussed earlier in
Sec. V, the consistency of these two patches was part of the
unblinding criteria, thus these two constraints are consistent
6This procedure is the same as in [16]. Since we cannot know
the cosmological and nuisance parameters exactly before running
the full inference, a set of fiducial parameters were used to
generate the first-pass of the covariance that was used for all
blinded chains. After unblinding, we update the parameters to
values closer to the best-fit parameters from the data. After
confirming that the 5 × 2 pt best-fit constraints Paper III are
consistent with the 3 × 2 pt best-fit constraints, we chose to use
the 3 × 2 pt best-fit parameters for evaluating the covariance
matrix, as this makes our modeling choices more consistent with
that of [16].
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PHYS. REV. D 107, 023530 (2023)
TABLE III. ΛCDM constraints on Ω
CMBi þ hγ
CMBi and different lens samples. We show the constraints
using both linear and nonlinear galaxy bias. The last column shows the p-value corresponding to the goodness of fit for the chain. The
parts shown in gray indicate that they are not part of the fiducial samples.
m, σ8 and S8 using hδgκ
κ
t
Dataset
hγtκCMBi MAGLIM
hδgκCMBi þ hγtκCMBi MAGLIM 4 bin linear galaxy bias
hδgκCMBi þ hγtκCMBi MAGLIM 4 bin nonlinear galaxy bias
hδgκCMBi þ hγtκCMBi MAGLIM 6 bin linear galaxy bias
hδgκCMBi þ hγtκCMBi MAGLIM 6 bin nonlinear galaxy bias
hδgκCMBi þ hγtκCMBi REDMAGIC linear galaxy bias
hδgκ
CMBi REDMAGIC nonlinear galaxy bias
CMBi þ hγ
κ
t
under the PPD metric. We find a p-value of 0.37 (0.33)
when comparing the Planck (SPT þ Planck) results to
constraints from SPT þ Planck (Planck). We also observe
that the constraints are somewhat tighter in the SPT þ
Planck patch in S8, consistent with the slightly larger
signal-to-noise (see Table II). We note however, that the
signal-to-noise before scale cuts of the SPT þ Planck
patch is significantly larger than the Planck patch due to
the lower noise and smaller beam size of the SPT lensing
map (for hδgκ
CMBi: 26.8 vs. 17.9; for hγ
CMBi: 15.0 vs.
10.4), though most of the signal-to-noise is on the small
scales which we had to remove due to uncertainties in the
theoretical modeling. This highlights the importance of
improving the small-scale modeling in future work.
κ
t
FIG. 3. Constraints on cosmological parameters Ω
from hδgκ
κ
show the corresponding constraints from hγ
shear and 3 × 2 pt for comparison.
m, σ8, and S8
CMBi using the MAGLIM sample. We also
CMBi-only, cosmic
t
CMBi þ hγ
κ
t
σ8
0.790þ0.080
−0.092
0.781þ0.073
−0.073
0.820þ0.079
−0.067
0.755þ0.071
−0.071
0.769þ0.071
−0.071
0.793þ0.072
−0.083
0.794þ0.069
−0.069
Ωm
0.270þ0.043
−0.061
0.272þ0.032
−0.052
0.245þ0.026
−0.044
0.288þ0.037
−0.053
0.273þ0.034
−0.047
0.266þ0.036
−0.050
0.253þ0.030
−0.046
S8
0.740þ0.034
−0.029
0.736þ0.032
−0.028
0.734þ0.035
−0.028
0.732þ0.032
−0.029
0.727þ0.035
−0.028
0.738þ0.034
−0.030
0.723þ0.033
−0.030
PPD p-value
0.72
0.50
0.51
0.45
0.45
0.39
0.41
B. Lensing ratio and IA modeling
As discussed in Sec. II, we have included the lensing
ratio likelihood in all our constraints. As was investigated
in detail in [17], the inclusion of the lensing ratio informa-
tion mainly constrains the IA parameters and source galaxy
redshift biases. The TATT IA model adopted here is a
general and flexible model that allows for a large range of
possible IA contributions. As such, it is expected that
including the lensing ratio could have a fairly large impact
for data vectors that are not already constraining the IA
parameters well. We now examine the effect of the lensing
ratio on our fiducial hδgκ
CMBi constraints by
first removing the lensing ratio prior in our fiducial result,
and then doing the same comparison with a different,
CMBi þ hγ
κ
t
m, σ8, and S8
FIG. 4. Constraints on cosmological parameters Ω
using the hδgκ
κ
CMBi probes. We also show the con-
t
straints only using the SPT þ Planck area and only using the
Planck area.
CMBi þ hγ
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t
κ
CMBi þ hγ
other probes in the plot. We note that this degeneracy
is likely sourced by the lensing ratio likelihood,
which on its own is degenerate in the η1 − η2 plane.
This is consistent with what we have seen in the
simulations in Paper I. The fact that it appears more
prominent in hδgκ
CMBi than in the other
probes is partly related to the fact that a1 and a2 are
constrained to be further away from zero in the case
of hδgκ
CMBi, allowing η1 and η2 (the
redshift evolution of the terms associated with a1
and a2) to be constrained better. Another relevant
factor is that hδgκ
CMBi probes slightly
larger redshift ranges than cosmic shear and 3 × 2 pt
due to the CMB lensing kernal, which allows for a
longer redshift lever arm to constrain η1 and η2,
resulting in qualitatively different behaviors in the
η1 − η2 parameter space.
CMBi þ hγ
CMBi þ hγ
κ
κ
t
t
C. Nonlinear galaxy bias
As discussed in Sec. II, we test a nonlinear galaxy bias
model
in addition to our baseline linear galaxy bias
analysis. With a nonlinear galaxy bias model we are able
to use somewhat smaller scales and utilize more signal in
the data (see Table II). In Fig. 7 we show the cosmological
constraints of our fiducial hδgκ
CMBi data vector
with the nonlinear galaxy bias model. We find that the
constraints between the two different galaxy bias models
are consistent. There is a small improvement in the Ω
m
direction, which is not surprising given that nonlinear bias
impacts hδgκ
CMBi improves the Ω
CMBi, and hδgκ
m con-
straints relative to hγ
κ
CMBi alone. The overall improvement
t
is nevertheless not very significant, as hγ
CMBi is domi-
nating the constraints.
CMBi þ hγ
κ
κ
t
t
D. Comparison with alternative lens choices
t
κ
CMBi þ hγ
We have defined our fiducial lens sample to be the first
four bins of the MAGLIM sample. This choice is informed by
the 3 × 2 pt analysis in [16], where alternative lens samples
were also tested but were deemed to be potentially
contaminated by systematic effects and therefore not used
in the final cosmology analysis. Here, we examine the
hδgκ
CMBi constraints using the two alternative
choices for lenses: (1) including the two high-redshift bins
in MAGLIM to form a 6-bin MAGLIM sample, and (2) the
REDMAGIC lens sample. As we have emphasized through-
out
the paper, since the galaxy-CMB lensing cross-
correlation is in principle less sensitive to some of the
systematic effects,
these tests could potentially shed
light on the issues seen in [16]. We only examine the
hδgκ
CMBi constraints here, but will carry out
a more extensive investigation in combination with the
3 × 2 pt probes in Paper III.
CMBi þ hγ
κ
t
In Fig. 8 we show constraints from hδgκ
CMBi
lens samples: 4-bin MAGLIM
CMBi þ hγ
κ
t
using the three different
FIG. 5. Constraints on cosmological parameters Ωm, σ8, and S8
using the hδgκCMBi þ hγtκCMBi probes with and without includ-
ing the lensing ratio (SR) likelihood, and when assuming the
NLA IA model instead of our fiducial IA model TATT.
more restrictive IA model, the NLA model (see Sec. II).
These results are shown in Fig. 5.
We make several observations from Fig. 5. First, the
lensing ratio significantly tightens the constraints in the S8
direction (roughly a factor of 2), as expected from Paper I.
Second, without the lensing ratio, different IA models
result in different S8 constraints, with TATT resulting in
∼40% larger uncertainties than NLA. This is expected
given that TATT is a more general model with three more
free parameters to marginalize over compared to NLA.
That being said, the constraints are still fully consistent
when using the different IA models. Third, when lensing
ratio is included,
there is very little difference in the
constraints between the two different IA models. This
suggests that the IA constraints coming from the lensing
ratio are sufficient to make the final constraints insensitive
to the particular IA model of choice.
Finally, it is interesting to look at the constraints on the
IA parameters for our fiducial hδgκ
CMBi analy-
sis with and without the lensing ratio. We show this in
Fig. 6, and compare them with constraints from cosmic
shear [62,63] and 3 × 2 pt [16]. We find two noticeable
degeneracies in these parameters:
CMBi þ hγ
κ
t
(i) The lensing ratio restricts the a1 − a2 parameter
space to a narrow band. This is seen in the cosmic
shear and 3 × 2 pt results, as well as the hδgκ
CMBi þ
hγ
CMBi results, although hδgκ
CMBi pre-
fers somewhat higher a2 values.
CMBi þ hγ
κ
κ
(ii) There is a noticeable η1 − η2 degeneracy that shows
CMBi þ hγ
CMBi and not in the
up uniquely in hδgκ
κ
t
t
t
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PHYS. REV. D 107, 023530 (2023)
FIG. 6. Constraints on S8 and the IA parameters from our fiducial hδgκ
include the hδgκ
CMBi þ hγ
CMBi constraints without the lensing ratio (SR) likelihood for comparison.
CMBi þ hγ
t
κ
CMBi results, cosmic shear and 3 × 2 pt. We also
κ
t
t
κ
(fiducial), 6-bin MAGLIM and REDMAGIC. The best-fit
parameters as well as the goodness-of-fit are listed in
Table III. Broadly, all three constraints appear to be very
consistent with each other. This is not surprising given that
the constraining power is dominated by hγ
CMBi as we
discussed earlier. In [16] it was shown that for the 3 × 2 pt
analysis, both the 6-bin MAGLIM and the REDMAGIC
samples give goodness-of-fits that fail our criteria, while
for hδgκ
CMBi all three samples give acceptable
goodness-of-fits values as seen in Table III. This could
imply that the systematic effects that contaminated the
other correlation functions in 3 × 2 pt are not affecting
the hδgκ
CMBi results strongly. Compared to the
fiducial constraints, the constraining power of the 6-bin
MAGLIM sample is slightly higher in the Ω
m direction due to
the added signal-to-noise from the high-redshift bins, while
CMBi þ hγ
CMBi þ hγ
κ
κ
t
t
m and S8.
the constraining power of the REDMAGIC sample is slightly
lower in both Ω
The DES Y3 3 × 2 pt analyses found that the poor fits
for the alternative lens samples can be explained by
inconsistent galaxy bias between galaxy-galaxy lensing
hδgγ
ti and galaxy clustering hδgδgi. That is, when allowing
the galaxy bias to be different in galaxy-galaxy lensing and
galaxy clustering,
improves signifi-
the goodness-of-fit
cantly. Operationally, this is achieved in [16] by adding
a free parameter, Xlens, defined such that
Xi
lens ¼ bi
hδgγti=bi
hδgδgi;
ð18Þ
hδgγti (bi
where bi
hδgγ
hδgδgi) is the linear galaxy bias parameter for
ti (hδgδgi) in lens galaxy redshift bin i. Xlens is expected
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FIG. 7. Fiducial hδgκ
logical parameters Ω
galaxy bias models.
CMBi þ hγ
CMBi constraints on cosmo-
m, σ8, and S8 using linear and nonlinear
κ
t
in general
the constraints from hδgκ
Our CMB lensing cross-correlation analysis provides an
interesting way to explore this systematic effect.
In
essence, with fixed cosmology, we can fit for galaxy bias
using hδgκ
CMBi and compare with the galaxy bias derived
from hδgγti and hδgδgi. Our results are shown in Fig. 9. We
find that
CMBi on
galaxy bias are weaker than both galaxy-galaxy lensing
and galaxy clustering, this is expected due to the lower
signal-to-noise. As such, the hδgκ
CMBi-inferred galaxy bias
values are largely consistent with both galaxy-galaxy
lensing and galaxy clustering. There are a few bins,
though, where hδgκ
CMBi does show a preference for the
galaxy bias values to agree more with one of the two
probes. Noticeably, for the last two MAGLIM bins, hδgκ
CMBi
prefers a galaxy bias value that is closer to that inferred by
galaxy clustering. On the other hand, for the highest two
REDMAGIC bins, hδgκ
CMBi prefers galaxy bias values that
are closer to galaxy-galaxy lensing. These findings are
investigations on Xlens
consistent with the various
described in [34,64] and suggest potential issues in the
measurements or modeling of galaxy-galaxy lensing in the
two high-redshift MAGLIM bins and galaxy clustering in
the REDMAGIC sample.7 However, we caution that these
results can be cosmology-dependent, and change slightly if
a different cosmology is assumed.
t
t
κ
E. Implications for S8 tension
In Fig. 10, we compare our constraints on S8 from
hγ
κ
CMBi to those from recent measurements of cosmic
shear from galaxy surveys (light blue circles) as well as
other recent hγ
CMBi constraints (dark blue squares). We
κ
show only the constraint
CMBi (rather
than
t
hδgκ
κ
to compare only
CMBi) since we want
measurements of gravitational
lensing. These lensing
measurements are not sensitive to the details of galaxy
bias, unlike hδgκ
CMBi. We see that the constraints on S8
obtained from hγ
κ
CMBi in this work (gray band) are for the
t
first time comparable to the state-of-the-art cosmic shear
measurements.
CMBi þ hγ
from hγ
t
FIG. 8. Fiducial constraints on cosmological parameters Ω
m,
σ8, and S8 using the hδgκ
CMBi þ hγ
CMBi probes compared with
using the REDMAGIC lens sample instead of the MAGLIM lens
sample.
κ
t
Figure 10 also shows the inferred value of S8 from
the primary CMB (black triangles), as measured by
Planck [21], ACT DR4 [65], combining ACT DR4 and
the Wilkinson Microwave Anisotropy Probe [WMAP, 65],
and SPT-3G [66]. As discussed in several previous works
[e.g., 62,63,67] and can be seen in the figure, there is a
∼2.7σ tension8 between the S8 value inferred from cosmic
to equal 1 in the case of no significant systematic effects.
≠ 1 for the two high-redshift
In [16] it was found that Xlens
bins in the MAGLIM sample and for all bins in the REDMAGIC
though there was not enough information to
sample,
determine whether the systematic effect was in hδgγ
ti
or hδgδgi.
7In particular, [34] tested an alternative REDMAGIC sample
and suggested potential remedies to the systematic effect in
REDMAGIC that will be explored in future work.
8Here we are quoting the 1D parameter difference in S8, or
8 − S2
, where the superscript 1 and 2 refer
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
8Þ þ σ2ðS2
σ2ðS1
8Þ
ðS1
to the two datasets we are comparing.
8Þ=
p
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C. CHANG et al.
PHYS. REV. D 107, 023530 (2023)
FIG. 9. With fixed cosmological parameters, the inferred galaxy bias from hδgκ
the MAGLIM sample (top) and the REDMAGIC sample (bottom).
CMBi, galaxy-galaxy lensing and galaxy clustering, for
FIG. 10. Comparison of late-time measurements of S8 from lensing-only data (cosmic shear hγγi and galaxy shear-CMB lensing cross-
correlation hγ
CMBi) to the inferred value of S8 from the primary CMB.
κ
t
shear and the Planck primary CMB constraint—cosmic
shear results prefer a lower S8 value. This is intriguing
given that it could indicate an inconsistency in the ΛCDM
model. We also see that
the other CMB datasets are
currently much less constraining, but show some variation,
with the lowest S8 value from SPT-3G fairly consistent with
all the cosmic shear results.
With this work, we can now meaningfully add hγ
CMBi
into this comparison, and as we see in Fig. 10, the hγ
CMBi
constraints on S8 are also largely below that coming from
the primary CMB. This is potentially exciting, since the
hγ
CMBi measurements come from a cross-correlation
between two very different surveys, and are therefore
κ
κ
κ
t
t
t
expected to be highly robust to systematic errors. Our
results therefore lend support to the existence of the S8
tension. In Paper III we will perform a more rigorous and
complete analysis of the consistency of our constraints here
with other datasets.
VII. SUMMARY
We have presented measurements of
two cross-
correlations between galaxy surveys and CMB lensing:
the galaxy position-CMB lensing correlation (hδgκ
CMBi),
and the galaxy shear-CMB lensing correlation (hγ
κ
CMBi).
t
These measurements are sensitive to the statistics of
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PHYS. REV. D 107, 023530 (2023)
large-scale structure, and are additionally expected to be
very robust
to many observational systematics. Our
measurements make use of the latest data from the first
three years of observations of DES, and a new CMB
lensing map constructed explicitly for cross-correlations
using SPT and Planck data. In particular, our fiducial
results are from four tomographic bins of the MAGLIM lens
galaxy sample. The signal-to-noise of the full data vector
without angular scale cuts is ∼30; the part of the data
vector used for cosmological inference has a signal-to-
noise of ∼20. The main reduction of the signal-to-noise
comes from uncertainty in the modeling of nonlinear
galaxy bias, which necessitates removal of the small-angle
hδgκ
CMBi correlation measurements. Compared to the
DES Y1 analysis, the signal-to-noise increased by a factor
of ∼2 and we are no longer limited by contamination of
tSZ in the CMB lensing map.
−0.044 ; S8 ¼ 0.734þ0.035
The joint analysis of these two cross-correlations results
−0.052 ; S8 ¼ 0.736þ0.032
m ¼ 0.272þ0.032
in the constraints Ω
−0.028
m ¼ 0.245þ0.026
(Ω
−0.028 ) when assuming lin-
ear (nonlinear) galaxy bias in our modeling. For S8, these
constraints are more than a factor of 2 tighter than our DES
Y1 results, ∼30% looser than constraints from DES Y3
cosmic shear and ∼70% looser than constraints from DES
Y3 3 × 2 pt. We highlight here several interesting findings
from this work:
t
t
t
κ
κ
κ
(i) We find that hγ
κ
CMBi þ hγ
CMBi þ hγ
CMBi dominates the constraints in
the hδgκ
CMBi combination, confirming
t
our findings from the simulated analysis in Paper I.
(ii) We find that the lensing ratio has a large impact on
the hδgκ
CMBi constraints, improving the
S8 constraints by ∼40%. In addition, the hδgκ
CMBi þ
hγ
CMBi data vector constrains the η1 − η2 degen-
eracy direction, something not seen in the DES Y3
3 × 2 pt data vectors.
(iii) We investigate the use of
two alternative lens
samples for the analysis: the 6-bin MAGLIM sample
and the REDMAGIC sample. In contrast to the fiducial
DES Y3 3 × 2 pt analysis, we find that
the
hδgκ
CMBi analysis using the two alter-
native lens samples pass our unblinding criteria and
show no signs of systematic contamination.
(iv) With fixed cosmology, we use the hδgκ
CMBi þ hγ
κ
t
t
κ
CMBi þ
hγ
CMBi data vector to constrain the galaxy bias
values using the 6-bin MAGLIM sample and the
REDMAGIC sample. For
the two high-redshift
MAGLIM bins, we find bias values that agree more
with galaxy clustering. On the other hand, for the
REDMAGIC sample, we find bias values more con-
sistent with galaxy-galaxy lensing. These provide
additional information for understanding the sys-
tematic effect seen in [16] from these two alternative
lens samples.
κ
(v) Comparing with previous cosmic shear and hγ
CMBi
constraints, we find that
in line with previous
findings, our hγ
CMBi constraint on S8 is lower
than the primary CMB constraint from Planck. In
addition, for the first time, hγ
CMBi has achieved
comparable precision to state-of-the-art cosmic
shear constraints.
κ
κ
t
t
t
The constraints derived in this paper from hδgκ
CMBi þ
hγ
κ
CMBi can now be compared and combined with the
t
DES Y3 3 × 2 pt probes [16], which we will do in Paper
III. We will present therein our final combined results along
with tests for consistency with external datasets. It
is
however intriguing that with the galaxy-CMB lensing
cross-correlation probes alone, our datasets provide very
competitive constraints on the late-time large-scale struc-
ture compared to galaxy-only probes. Due to the relative
insensitivity to certain systematic effects, this additional
constraint is especially important for cross-checking and
significantly improving the robustness of the galaxy-only
results. Another unique aspect of this work compared to
other cross-correlation analyses is that we have carried out
our work in an analysis framework that is fully coherent
with the galaxy-only probes, making it easy to compare and
combine.
Looking forward to the final datasets from DES, SPT,
and ACT, as well as datasets from the Vera C. Rubin
Observatory’s Legacy Survey of Space and Time9 (LSST),
the ESA’s Euclid mission,10 the Roman Space Telescope,11
(SO), and CMB Stage-413
the Simons Observatory12
(CMB-S4), our results show that
there are significant
opportunities for combining the galaxy and CMB lensing
datasets to both improve the constraints on cosmological
parameters and to make the constraints themselves more
robust to systematic effects.
ACKNOWLEDGMENTS
C. C. and Y. O. are supported by DOE grant No. DE-
SC0021949. The South Pole Telescope program is sup-
ported by the National Science Foundation (NSF) through
the grant No. OPP-1852617. Partial support is also pro-
vided by the Kavli Institute of Cosmological Physics at the
University of Chicago. Argonne National Laboratory’s
work was supported by the U.S. Department of Energy,
Office of Science, Office of High Energy Physics, under
contract No. DE-AC02- 06CH11357. Work at Fermi
National Accelerator Laboratory, a DOE-OS, HEP User
9https://www.lsst.org.
10https://www.euclid-ec.org.
11https://roman.gsfc.nasa.gov.
12https://simonsobservatory.org/.
13https://cmb-s4.org/.
023530-17
C. CHANG et al.
PHYS. REV. D 107, 023530 (2023)
support
the National Center
the University of
Facility managed by the Fermi Research Alliance, LLC,
was supported under Contract No. DE-AC02- 07CH11359.
The Melbourne authors acknowledge support from the
Australian Research Council’s Discovery Projects scheme
(No. DP200101068). The McGill authors acknowledge
funding from the Natural Sciences and Engineering
Research Council of Canada, Canadian Institute for
Advanced research, and the Fonds de recherche du
Qu´ebec Nature et technologies. The CU Boulder group
acknowledges support from NSF Grant No. AST-0956135.
The Munich group acknowledges the support by the
ORIGINS Cluster (funded by the Deutsche Forschungsge-
meinschaft (DFG, German Research Foundation) under
Germany’s Excellence Strategy—EXC-2094–390783311),
the MaxPlanck-Gesellschaft Faculty Fellowship Program,
and the Ludwig-Maximilians-Universität München. J. V.
acknowledges
from the Sloan Foundation.
Funding for the DES Projects has been provided by the
U.S. Department of Energy,
the U.S. National Science
the Ministry of Science and Education of
Foundation,
Spain, the Science and Technology Facilities Council of
the United Kingdom, the Higher Education Funding Council
for England,
for Supercomputing
Illinois at Urbana-
Applications at
Champaign, the Kavli Institute of Cosmological Physics
at the University of Chicago, the Center for Cosmology
and Astro-Particle Physics at the Ohio State University, the
Mitchell Institute for Fundamental Physics and Astronomy
at Texas A&M University, Financiadora de Estudos e
Projetos, Fundação Carlos Chagas Filho de Amparo `a
Pesquisa do Estado do Rio de Janeiro, Conselho Nacional
de Desenvolvimento Científico e Tecnológico and the
Minist´erio da Ciência, Tecnologia
the
Deutsche Forschungsgemeinschaft and the Collaborating
Institutions in the Dark Energy Survey. The Collaborating
Institutions are Argonne National Laboratory, the University
of California at Santa Cruz, the University of Cambridge,
Centro de Investigaciones Energ´eticas, Medioambientales y
Tecnológicas-Madrid, the University of Chicago, University
College London, the DES-Brazil Consortium, the University
of Edinburgh, the Eidgenössische Technische Hochschule
(ETH) Zürich, Fermi National Accelerator Laboratory, the
University of Illinois at Urbana-Champaign, the Institut de
Ci`encies de l’Espai (IEEC/CSIC), the Institut de Física
d’Altes Energies, Lawrence Berkeley National Laboratory,
the Ludwig-Maximilians Universität München and the
associated Excellence Cluster Universe, the University of
Michigan, NFS’s NOIRLab, the University of Nottingham,
The Ohio State University, the University of Pennsylvania,
the University of Portsmouth, SLAC National Accelerator
Laboratory, Stanford University, the University of Sussex,
Inovação,
e
system is
Texas A&M University, and the OzDES Membership
Consortium. Based in part on observations at Cerro
Tololo Inter-American Observatory at NSF’s NOIRLab
(NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is
managed by the Association of Universities for Research
in Astronomy (AURA) under a cooperative agreement
with the National Science Foundation. The DES data
management
supported by the National
Science Foundation under Grants No. AST-1138766 and
No. AST-1536171. The DES participants from Spanish
institutions are partially supported by MICINN under
grants No. ESP2017-89838, No. PGC2018-094773,
No. PGC2018-102021, No. SEV-2016-0588, No. SEV-
2016-0597, and No. MDM-2015-0509, some of which
include ERDF funds from the European Union. I. F. A. E.
is partially funded by the CERCA program of
the
Generalitat de Catalunya. Research leading to these results
has received funding from the European Research Council
under the European Union’s Seventh Framework Program
(No. FP7/2007-2013) including ERC grant agreements
No. 240672, No. 291329, and No. 306478. We acknowl-
edge support from the Brazilian Instituto Nacional de
Ciência e Tecnologia (INCT) do e-Universo (CNPq grant
No. 465376/2014-2). This manuscript has been authored
by Fermi Research Alliance, LLC under Contract No. DE-
AC02-07CH11359 with the U.S. Department of Energy,
Office of Science, Office of High Energy Physics.
APPENDIX A: JACKKNIFE COVARIANCE
MATRIX
We have performed extensive validation tests on our
methodology of modeling in the covariance matrix in
Paper I. The ultimate check, however, is to compare the
covariance matrix with a data-driven jackknife covariance
matrix. The jackknife covariance incorporates naturally
the noise in the data as well as any non-cosmological
spatial variation in the data that might be important. This
comparison was done after unblinding and the update of
the covariance described in footnote 6, and is only used as
a confirmation—that is, we cannot change any analysis
choices based on this check.
into 80 patches)
In Fig. 11 we show the diagonal elements of the
covariance matrix (calculated using the
jackknife
delete-one block jackknife method by dividing the foot-
print
lens sample,
compared with our fiducial covariance matrix. We find
excellent agreement between them on all scales, both
hδgκ
κ
CMBi and hγ
CMBi, and on both the SPT þ Planck
t
and Planck patch.
the fiducial
for
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FIG. 11. Comparison between the diagonal elements of the jackknife covariance and our fiducial covariance matrix (analytical
covariance with noise-noise correction applied).
APPENDIX B: DIAGNOSTIC TESTS
We perform a number of diagnostic tests to make sure
that our measurements are not significantly contaminated
by potential systematic effects. As we have discussed in
Sec. I, cross-survey correlations like those presented here
to possible
are expected to be inherently more robust
systematic effects. In addition, extensive tests have been
done on both the galaxy and CMB data products in
[13,47,51,62,63,68]. We perform a series of diagnostic
tests specific to the cross-correlation probes.
1. Cross-correlation with survey property maps
If a given contaminant associated with some survey
property simultaneously affects the galaxy and the CMB
fields that we are cross-correlating, the cross-correlation
signal will contain a spurious component
is not
cosmological. A possible example is dust, which could
simultaneously contaminate
the CMB lensing map
(through thermal emission in CMB bands) and the galaxy
density field (through extinction). In addition to dust,
we consider several other possible survey properties.
This test is designed to detect such effects. We calculate
the correlation statistic, Xf
S, between the observables of
interest and various survey property maps:
that
Xf
SðθÞ ¼
hκ
CMB
SðθÞihfSðθÞi
hSSðθÞi
;
ðB1Þ
CMBi and Xf
where S is the survey property map of interest, and f is
either δg or γ
t. This expression captures correlation of the
systematic with both κ
CMB and f, and is normalized to have
the same units as hfκ
the
CMBi. Henceforth, we omit
θ-dependence in the notation for simplicity, but note that
all the factors in Eq. (B1) are functions of θ. Unless the
systematic map is correlated with both f and κ
CMB, it will
not bias hfκ
S will be consistent with zero. Note
that Xf
S should also be compared with the statistical
uncertainty of hfκ
CMBi, as a certain systematic could be
significantly detected but have little impact on the final
results if it is much smaller than the statistical uncertainty.
CMBi, we consider two S fields: stellar density
and extinction. For hγ
CMBi, we look in addition at two
fields associated with PSF modeling errors. The quantities
q and w measure the point-spread function (PSF) modeling
residuals as introduced in [51], q ¼ e(cid:2)
is the
difference of the true ellipticity of the PSF as measured
by stars and that
inferred by the PSF model, and
− TmodelÞ=T(cid:2), where T is a measure of size
w ¼ e(cid:2)ðT(cid:2)
of the PSF, is the impact on the PSF model ellipticity when
For hδgκ
− emodel
κ
t
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FIG. 12. The measured systematic contamination of hδgκCMBi for the MAGLIM lens sample, as assessed by Eq. (B1), for the SPT þ
Planck field (top) and the Planck field (bottom) and for different redshift bins. For reference, the gray band shows 10% of the statistical
uncertainties for the corresponding data vectors. In all cases, the measured bias is significantly below the statistical uncertainties on the
hδgκCMBi measurements.
FIG. 13. Same as Fig. 12 but for the REDMAGIC lens sample.
− Tmodel. As both q and w are
the PSF size is wrong by T(cid:2)
spin-2 quantities like the ellipticity, we first decompose
them into E and B modes using the same method used
for generating weak lensing convergence maps in [69].
We then use the E-mode maps as the S maps to perform
the cross-correlation test. The rationale here is that if there
is a nontrivial E-mode component, it could signify con-
tamination in the shear signal and will correlate with the
shear field.
Figures 12–14 show the result of our measured Xf
S for
the different parts of the data vector. For comparison, we
also plot the statistical uncertainty on the data vector;
given that the statistical uncertainties are much larger
than the measured biases in all cases, we scale the
statistical uncertainties by 0.1 (hδgκ
CMBi) and 0.01
CMBi). The χ2 values per degree of freedom for
(hγ
κ
t
the Xf
S measurements with respect to the null model are
shown in Tables IV–VI together with the probability-to-
exceed (PTE) values. The χ2 as well as the error bars on
the plots are derived from jackknife resampling where we
use 65 equal-area jackknife patches for the SPT þ Planck
footprint and 85 patches for the Planck area. To obtain a
more reliable jackknife covariance, we measure Xf
S using
10 angular bins instead of the 20 bins used for the data
vectors. In general, most of the systematic effects are very
consistent with zero.
For hδgκ
CMBi, we find that the absolute level of the
potential systematic effects as quantified by Xf
S is 1-2
orders of magnitudes smaller than the statistical errors.
There appears to be more cross-correlation for the SPT þ
Planck area, especially with extinction. All of the PTE
values of these cross-correlations are above our threshold
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FIG. 14. The measured systematic contamination of hγtκCMBi, as assessed by Eq. (B1), for the SPT þ Planck field (top) and the
Planck field (bottom) and for different redshift bins. The gray band shows 1% of the statistical uncertainties for the corresponding data
vectors.
t
κ
for concern of 0.01, so we deem these results acceptable.
CMBi, we find that the absolute levels of the Xf
For hγ
S
measurements is much lower (> 2 orders of magnitude)—
this is expected as it is much less obvious how the survey
property maps will leave an imprint on the shear field.
Interestingly, we also find that overall the error bars are
larger in the SPT þ Planck patch compared to the Planck
patch. This can be due to the survey property maps
containing higher
fluctuation in the SPT þ
Planck area as part of the footprint is close to the galactic
plane or the Large Magellanic Cloud (LMC).
spatial
2. Cross-shear component
t
×
κ
κ
κ
During the measurement of hγ
CMBi, we additionally
measure its cross-shear counterpart hγ
CMBi. We replace
et in Eq. (16) with e×, the corrected ellipticity oriented 45°
to the line connecting map pixel and the source galaxy. The
correlation hγ
CMBi should be consistent with zero. Any
×
significant detection of hγ
CMBi could signal systematic
effects in the hγ
κ
×
CMBi measurements.
Our results are shown in Fig. 15 with the χ2 per degree of
freedom and PTE values listed in Table VI. We find no
significant detection of hγ
κ
CMBi in all parts of the data
vector.
κ
×
t
TABLE IV. The χ2 per degree of freedom for the systematics
diagnostics quantity [Eq. (B1)] for the MAGLIM hδgκ
CMBi mea-
surements. The different columns represent the different survey
properties S, whereas the different rows are for the tomographic
bins in both the SPT þ Planck patch and the Planck patch. The
corresponding PTE values are listed in the parentheses.
3. hδgκCMBi measurements with and without weights
As discussed in [47], weights are applied to the lens
galaxies in order to remove correlations with various survey
properties. When performing the hδgκ
CMBi measurement in
SPT þ Planck
Planck
S
Bin
1
2
3
4
5
6
1
2
3
4
5
6
Stellar density
Extinction
TABLE V. Same as Table IV but for the REDMAGIC lens sample.
χ2=d:o:f: (PTE)
0.42 (0.85)
0.10 (0.99)
0.21 (0.98)
0.13 (0.99)
0.22 (0.98)
0.36 (0.93)
0.02 (0.99)
0.12 (0.99)
0.15 (0.99)
0.08 (0.99)
0.06 (0.99)
0.05 (0.99)
0.90 (0.49)
0.65 (0.71)
0.64 (0.72)
1.12 (0.34)
1.34 (0.21)
1.66 (0.10)
0.40 (0.87)
0.26 (0.96)
0.28 (0.96)
0.33 (0.93)
0.21 (0.98)
0.18 (0.98)
SPT þ Planck
Planck
S
Bin
1
2
3
4
5
1
2
3
4
5
Stellar density
Extinction
χ2=d:o:f: (PTE)
0.09 (0.99)
0.50 (0.83)
0.42 (0.88)
0.28 (0.96)
0.73 (0.64)
0.09 (0.99)
0.09 (0.99)
0.05 (0.99)
0.04 (0.99)
0.04 (0.99)
0.20 (0.97)
0.56 (0.78)
0.38 (0.91)
0.76 (0.62)
1.13 (0.33)
0.38 (0.89)
0.16 (0.99)
0.19 (0.98)
0.16 (0.99)
0.16 (0.99)
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TABLE VI. The χ2 per degree of freedom for the systematics diagnostics quantity [Eq. (B1)] for the hγ
CMBi measurements. The
different columns represent the different survey properties S, whereas the different rows are for the tomographic bins in both
the SPT þ Planck patch and the Planck patch. The corresponding PTE values are listed in the parentheses. The last column lists the
corresponding numbers for the cross-shear measurement described in Sec. B 2.
κ
t
SPT þ Planck
Planck
S
Bin
1
2
3
4
1
2
3
4
Stellar density
Extinction
PSF model error q
χ2=d:o:f: (PTE)
PSF model error w
γ×
0.12 (0.99)
0.17 (0.99)
0.32 (0.94)
0.20 (0.97)
0.09 (0.99)
0.09 (0.99)
0.12 (0.99)
0.16 (0.99)
0.12 (0.99)
0.38 (0.95)
0.39 (0.90)
0.41 (0.86)
0.06 (0.99)
0.04 (0.99)
0.07 (0.99)
0.18 (0.99)
0.34 (0.96)
0.20 (0.99)
0.40 (0.89)
0.19 (0.97)
0.11 (0.99)
0.25 (0.98)
0.19 (0.99)
0.27 (0.98)
0.15 (0.99)
0.18 (0.99)
0.30 (0.95)
0.15 (0.98)
0.08 (0.99)
0.17 (0.99)
0.14 (0.99)
0.18 (0.99)
1.11 (0.34)
1.18 (0.29)
0.60 (0.75)
1.91 (0.07)
1.15 (0.31)
1.28 (0.23)
1.16 (0.31)
1.12 (0.33)
the effect of
Eq. (14), these weights are applied (i.e. the ηδg). In a cross-
these weights will be non-
correlation,
negligible if the systematic effect that is being corrected
by the weights also correlates with the CMB lensing map.
We note that this test is not always a null-test, as we
consider it more correct to use the weights. Rather, it
shows qualitatively the level of the correction from these
weights—naively, the smaller the correction to start with,
the less likely the residual contamination will be.
In Fig. 16 we show the difference between the hδgκ
CMBi
measurements with and without using the lens weights,
for the two lens samples. To understand the significance of
these results, we calculate the Δχ2 between the data vectors
with and without weights for the fiducial MAGLIM sample,
using the analytic covariance for the data vector and find a
Δχ2 of 1.23 after scale cuts. Propagating this into cosmo-
logical constraints by running two chains using hδgκ
CMBi
with and without weights (fixing galaxy bias) gives a
negligible 0.02σ shift in the Ω
− S8 plane. It is also worth
m
pointing out that we see that the weights most significantly
affect the two high-redshift bins in the MAGLIM sample,
this is likely due to the fact that the high-redshift bins
are fainter and more affected by the spatially varying
observing conditions.
4. Biases from source masking
In constructing the CMB lensing maps for this analysis,
we apply a special procedure at the locations of bright point
sources to reduce their impact on the output lensing maps.
As described in more detail in Paper I, the CMB lensing
estimator that we use involves two CMB maps, or “legs.”
One of these is high-resolution map (i.e. the SPT þ Planck
temperature map), and the other
is a low-resolution
tSZ-cleaned map (i.e. the Planck SMICAnosz temperature
map). To reduce the impact of point sources, we inpaint
the point sources with fluxes 6.4 < F < 200 mJy using the
method described in [70]. The total
inpainted area is
roughly 3.6% of the map. The corresponding location in
the tSZ-cleaned map are left untouched. We expect this
procedure to result in a reasonable estimate of κ
CMB at the
FIG. 15. Cross-correlation between than cross-component of shear with CMB lensing for the SPT þ Planck field (top) and the Planck
field (bottom) and for different redshift bins. The gray band shows the statistical uncertainties for hγ
κ
CMBi.
t
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FIG. 18. Cross-correlation between CIB and the Planck
lensing map in the North patch (solid gray), the Planck lensing
map in the South patch (open red), and the SPT þ Planck
lensing map (black).
FIG. 16. The difference in the hδgκCMBi cross-correlation
between the two lens galaxy samples MAGLIM and REDMAGIC
with CMB lensing when using weights and without weights, over
the statistical uncertainty of the measurement σ.
locations of the point sources, given that only one leg is
inpainted, and the area being inpainted is small (such that
Gaussian constrained inpainting predicts the pixels values
of the inpainted region well) although it is possible that the
noise properties of these regions differ somewhat from the
map as a whole.
To test whether the inpainting procedure results in any
bias, we also measure the cross-correlation with the lensing
map after masking (i.e. completely removing) all the point
sources down to 6.4 mJy. We show in Fig. 17 the difference
in the data vectors using the alternative mask and the
fiducial one. We find that there is no coherent difference in
the correlation measurements across the range of angular
scales considered. There is, however, some scatter about
our nominal measurements. The level of this scatter is
small, roughly 0.25 and 0.50σ across the full range of
angular scales for hδgκ
CMBi and hγ
CMBi respectively.14
Given that such scatter is expected to have negligible
impact on our results, and since some scatter between
the data points is expected simply due to the different
selection of pixels in the masked and unmasked CMB
lensing maps, we do not find this to be a cause for worry.
Our baseline results will use the unmasked version of the
CMB lensing map.
κ
t
5. Variations in the CMB lensing map
Our fiducial analysis uses the SPT þ Planck map in
the Dec < −40° region and the Planck lensing map in the
region Dec > −39.5°. We left a 0.5° gap between the two
maps to avoid correlation between the large-scale structure
on the boundary. Here we like to verify that the cross-
correlation of our CMB lensing maps with another large-
scale structure tracer is consistent between the two patches
and the two CMB lensing data sets. We choose to use the
cosmic infrared background (CIB) map from [71]15 as this
large-scale structure tracer. We carry out the following two
14This scatter results from the slightly higher-noise region
caused by the half-leg lensing reconstruction, with the point
sources left in the non-inpainted map effectively behaving as
noise.
15Here we use the nH ¼ 2.5e20 cm−1 maps as defined in [71].
FIG. 17. Difference in the data vectors using the alternative
mask and the fiducial one. This test is only done for the SPT þ
Planck patch, as it is specific to the SPT lensing reconstruction.
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FIG. 19. Same as Fig. 2 but for the REDMAGIC sample.
tests: (1) we compare the cross-correlations between the
CIB map and the Planck lensing map split into two sub-
regions (the “North” region with DEC > −39.5° and the
“South” region with DEC < −40°), and verify that they are
consistent; (2) we compare in the South patch the cross-
correlations between the CIB map with either the Planck
CMB lensing map or our SPT þ Planck lensing map, and
verify that they are consistent.
The resulting correlation measurements are shown in
Fig. 18—the high signal-to-noise is expected due to the
significant overlap in the kernels of the two tracers. We
make two comparisons:
(1) CIB × Planck North vs. CIB × Planck South: We
find a two-sample χ2=ν of 24.28=20 with a PTE of
0.23. This demonstrates that the two patches are
consistent with each other.
(2) SPT þ Planck vs. Planck South: We compute the
two-sample χ2, and find χ2=ν ¼ 23.9=20., with a
PTE of 0.25. This demonstrates that the two mea-
surements are consistent with each other.
We note that there are two caveats associated with these
that, at
cross-correlation measurements. The first
is
there may be residuals. Second,
545 GHz, galactic emission is non-negligible, and while
the CIB maps from [71] are intended to be free of galactic
dust,
CMB
correlation is most sensitive to redshifts higher than those
probed by DES galaxies, thus we are extrapolating the
results above to lower redshift.
the CIB-κ
APPENDIX C: REDMAGIC RESULTS
In this appendix we show the results for the second lens
sample—the REDMAGIC sample. The data vector is shown
in Fig. 19 with signal-to-noise values listed in Table II. We
find that (1) no significant systematic effects were found
as described in Appendix B, (2) we get a p-value greater
than 0.01 when comparing the hδgκ
CMBi con-
straints from Planck to constraints from SPT þ Planck,
and (3) the goodness-of-fit of the fiducial hδgκ
CMBi þ
hγ
CMBi unblinded chain corresponds to a p-value greater
than 0.01. These results allowed us to unblind our results,
and the final constraints are listed in Table III and the
fiducial constraints are shown in Fig. 8.
CMBi þ hγ
κ
κ
t
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10.1371_journal.pcbi.1007117.pdf
|
Data Availability Statement: All relevant data are
within the manuscript and its Supporting
Information files.
|
All relevant data are within the manuscript and its Supporting Information files.
|
RESEARCH ARTICLE
Development of a physiologically-based
pharmacokinetic pediatric brain model for
prediction of cerebrospinal fluid drug
concentrations and the influence of
meningitis
Laurens F. M. VerscheijdenID
M. RusselID
1*
1, Jan B. Koenderink1, Saskia N. de WildtID
1,2, Frans G.
1 Department of Pharmacology and Toxicology, Radboud University Medical Center, Radboud Institute for
Molecular Life Sciences, Nijmegen, The Netherlands, 2 Intensive Care and Department of Pediatric Surgery,
Erasmus MC-Sophia Children’s Hospital, Rotterdam, The Netherlands
* [email protected]
Abstract
Different pediatric physiologically-based pharmacokinetic (PBPK) models have been
described incorporating developmental changes that influence plasma drug concentrations.
Drug disposition into cerebrospinal fluid (CSF) is also subject to age-related variation and
can be further influenced by brain diseases affecting blood-brain barrier integrity, like menin-
gitis. Here, we developed a generic pediatric brain PBPK model to predict CSF concentra-
tions of drugs that undergo passive transfer, including age-appropriate parameters. The
model was validated for the analgesics paracetamol, ibuprofen, flurbiprofen and naproxen,
and for a pediatric meningitis population by empirical optimization of the blood-brain barrier
penetration of the antibiotic meropenem. Plasma and CSF drug concentrations derived
from the literature were used to perform visual predictive checks and to calculate ratios
between simulated and observed area under the concentration curves (AUCs) in order to
evaluate model performance. Model-simulated concentrations were comparable to
observed data over a broad age range (3 months–15 years postnatal age) for all drugs
investigated. The ratios between observed and simulated AUCs (AUCo/AUCp) were within
2-fold difference both in plasma (range 0.92–1.09) and in CSF (range 0.64–1.23) indicating
acceptable model performance. The model was also able to describe disease-mediated
changes in neonates and young children (<3m postnatal age) related to meningitis and sep-
sis (range AUCo/AUCp plasma: 1.64–1.66, range AUCo/AUCp CSF: 1.43–1.73). Our
model provides a new computational tool to predict CSF drug concentrations in children with
and without meningitis and can be used as a template model for other compounds that pas-
sively enter the CNS.
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OPEN ACCESS
Citation: Verscheijden LFM, Koenderink JB, de
Wildt SN, Russel FGM (2019) Development of a
physiologically-based pharmacokinetic pediatric
brain model for prediction of cerebrospinal fluid
drug concentrations and the influence of
meningitis. PLoS Comput Biol 15(6): e1007117.
https://doi.org/10.1371/journal.pcbi.1007117
Editor: James Gallo, University at Buffalo - The
State University of New York, UNITED STATES
Received: February 1, 2019
Accepted: May 21, 2019
Published: June 13, 2019
Copyright: © 2019 Verscheijden et al. This is an
open access article distributed under the terms of
the Creative Commons Attribution License, which
permits unrestricted use, distribution, and
reproduction in any medium, provided the original
author and source are credited.
Data Availability Statement: All relevant data are
within the manuscript and its Supporting
Information files.
Funding: The authors received no specific funding
for this work.
Competing interests: The authors have declared
that no competing interests exist.
PLOS Computational Biology | https://doi.org/10.1371/journal.pcbi.1007117 June 13, 2019
1 / 19
Development of a pediatric brain PBPK model
Author summary
Developmental processes in children affect pharmacokinetics and should ideally be taken
into account when establishing drug dosing regimens. One way to incorporate develop-
mental differences is by making use of physiologically-based pharmacokinetic (PBPK)
models in which kinetic equations are used to describe drug disposition processes and
developmental biology. With these equations the absorption of drugs into the model, the
flow of drugs between different compartments (representing major organs/tissues), and
excretion from the model are predicted. PBPK models can also be used to describe drug
concentrations in different target tissues, which often correlate better with the clinical
effects. Here, we developed a generic pediatric PBPK model of drug disposition in the
cerebrospinal fluid (CSF), that was able to describe clinically measured drug concentra-
tions of several drugs in neonates and children. The model could be useful in predicting
CSF concentrations of other drugs in pediatric populations where clinical data is often
sparse or absent and by this means guide first-in-child dose recommendations.
Introduction
Growth and development significantly impact handling of drugs in children across the pediat-
ric age range. Simple linear bodyweight-based extrapolations from adult to pediatric doses
have resulted in toxicity or therapy failure [1]. Taking developmental changes of the processes
involved in drug disposition into account in dosing guidelines will lead to improved therapeu-
tic efficacy and safe exposure in children of different ages [2].
Physiologically-based pharmacokinetic (PBPK) modeling is an important tool to simulate
drug exposure and design dosing guidelines. PBPK models are compartmental kinetic models
in which physiological and drug-specific parameters are as much as possible separated [3].
Physiological parameters describe biological values and processes, and if sufficient data
describing developmental biology is available, they can be used to predict plasma drug concen-
trations in pediatric populations. By this means, PBPK models can guide first-in-child dosing
regimens for drugs of which pediatric clinical drug concentrations are scarcely available,
resulting in more focused, data-rich clinical trials. There are multiple examples of the success-
ful application of pediatric PBPK models in the drug development process [4].
PBPK models also allow predictions of drug concentrations in target tissues, which often
correlate better with the clinical effect. This is especially the case for organs like the brain that
are characterized by permeability-limited disposition of various drugs, leading to a significant
lag time between their peak plasma and tissue concentrations [5–7]. For drugs acting in the
brain, differences in blood and cerebrospinal fluid (CSF) dynamics, blood-brain barrier (BBB)
and blood-CSF barrier (BCSFB) permeability, brain and CSF compartment volumes, as well as
disease-mediated changes could influence the amount of drug entering the different parts of
the central nervous system and should be included to facilitate robust predictions.
Recently, brain PBPK models for adult populations were developed to allow predictions of
drug concentrations in brain parenchyma and CSF. For example, Gaohua et al. developed an
adult brain PBPK model consisting of 4 compartments, which was validated using measured
paracetamol CSF concentrations [8]. Yamamoto et al. used a different approach by first build-
ing a rat model that incorporated multiple brain and CSF compartments [9, 10]. Physiological
parameters were in turn adjusted in order to develop a human version [11]. Finally, they
extended this adult model into a morphine pediatric brain PBPK model. This model allowed
simulations of morphine extracellular fluid concentrations after traumatic brain injury in six
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Development of a pediatric brain PBPK model
children older than 2 years of age [12]. To become more widely accepted, pediatric brain
PBPK models should be validated with observed data of different drugs and more individuals
across the pediatric age range to increase confidence in the physiological parameters included.
In addition to the validation of a brain PBPK model for a relatively healthy pediatric popu-
lation, including pathophysiological changes associated with conditions known to affect brain
drug concentrations is important to demonstrate model performance in diseased children.
Meningitis is a severe condition that leads to impaired BBB and enhanced penetration of
drugs into brain and CSF, particularly in newborns and young children [13, 14].
The aim of our study was to describe drug CSF concentrations and describe the effects of
meningitis in children by developing and validating a generic pediatric brain PBPK model
based on different drugs that enter the brain by passive transfer. Our model provides a new
computational tool to predict CSF concentrations in children of drugs that undergo passive
transfer and it could serve as a good template for further extension to carrier-mediated trans-
port and disposition in different regions of the central nervous system.
Results
The full code of the pediatric PBPK model for paracetamol is available in Rstudio format (S1
File). Summary tables of physiological and drug-related parameters are reported in S1 Table
and S2 Table, respectively, and can be used to adapt the model to the adult situation and for
other drugs. The healthy pediatric brain model was built for paracetamol and subsequently val-
idated using the nonsteroidal anti-inflammatory drugs (NSAIDs) ibuprofen, flurbiprofen and
naproxen. BBB permeability of the antibiotic meropenem was optimized in an adult popula-
tion suffering from meningitis and subsequently simulations were performed for a pediatric
population with meningitis and sepsis (methods).
Building a healthy adult brain PBPK model using paracetamol
First, the adult brain PBPK model was built and validated using published paracetamol data
[7, 15]. Model simulations of plasma and CSF concentrations largely overlaid the observed
data and the ratios of the respective AUCs were within twofold difference (Fig 1, Table 1).
Building a healthy pediatric brain PBPK model using paracetamol
After inclusion of the age-related data, simulations of paracetamol concentrations were per-
formed for children aged between 3 months and 13 years. The pediatric model simulations
also largely overlaid with observed data (Fig 1). Ratios of simulated over observed plasma and
CSF AUCs were also within twofold difference (Table 1). An equivalent dose of approximately
15 mg/kg resulted in a CSF AUC0-6h that was 34% higher in children between 3 months and
13 years of age compared to adults. Because CSF production rate is possibly influenced by co-
medication, a sensitivity analysis was performed to investigate the effect of CSF production
rate on paracetamol concentration-time profiles [16]. Twofold differences in CSF production
had a significant impact on the paracetamol CSF profiles (Fig 2A and 2B), while leaving the
shape of the plasma concentration-time curves virtually unaffected (difference in AUC, Cmax
and Tmax <1% from original concentration-time profile).
Validation of the pediatric brain PBPK model using ibuprofen,
flurbiprofen and naproxen
To validate the physiological parameters included in the paracetamol model for children aged
between 3 months and 15 years, simulations were performed with another set of drugs that
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Development of a pediatric brain PBPK model
Fig 1. Simulations of paracetamol concentration-time profiles. Plasma and CSF concentration-time profiles of paracetamol after a single intravenous
dose of 1000 mg in adults (A, B) and (15 mg/kg) (C,D) in children. Solid black lines indicate simulation of median profiles, the grey area represents 90% CI
and dotted lines indicate the minimum and maximum simulation. Dots indicate measured data derived from clinical studies together with the reported S.
E.M (adult) or individual observations (pediatric). Log-transformed results are depicted in the right upper corners.
https://doi.org/10.1371/journal.pcbi.1007117.g001
were not used to build the pediatric model, i.e. ibuprofen, flurbiprofen and naproxen. The
model predicted clinically observed data reasonably well, except for flurbiprofen for which
plasma volume of distribution seemed to be overestimated. For this drug a Kp scalar of 0.33
Table 1. Ratio observed/predicted AUC for plasma and CSF drug concentrations.
Drug
Paracetamol
Paracetamol
Ibuprofen (oral)
Ibuprofen (IV)
Flurbiprofen
Naproxen
Meropenem
Meropenem
Meropenem
Population
Plasma
Adult
Paediatric
Paediatric
Paediatric
Paediatric
Paediatric
Adult
Pediatric(sepsis)
Pediatric(meningitis)
1.01
1.09
0.94
0.92
0.99
1.07
1.07
1.66
1.64
https://doi.org/10.1371/journal.pcbi.1007117.t001
CSF
1.18
1.23
1.05
0.64
0.76
0.99
1.23
1.73
1.41
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Development of a pediatric brain PBPK model
Fig 2. The effect of CSF production rate on paracetamol CSF concentration-time profiles. The red lines indicate the simulations using the default CSF
production rate. The black lines indicate a twofold increase or reduction in CSF production rate, respectively. The grey lines indicate a fivefold increase or
reduction in CSF production rate, respectively.
https://doi.org/10.1371/journal.pcbi.1007117.g002
(i.e. Kp of every compartment multiplied by 0.33) was introduced to adjust volume of distribu-
tion such that simulations of plasma concentrations better correlated with observations (Fig
3). The difference between observed and simulated AUCs for both plasma and CSF were
within 2-fold (Table 1).
Meropenem permeability in the adult brain meningitis PBPK model
Drug-related parameters of meropenem were included in the adult model. No individual
doses were reported in the study of Lu et al., which was used for validation [17]. Therefore, an
intravenous dose of 1500 mg/8h was chosen for our virtual population, which was in the range
of the doses used by Lu et al. (1000 mg/8h, 1000 mg/6h, 2000 mg/8h). Simulations of plasma
concentration-time profiles matched well with observed data points. After optimizing perme-
ability in this model, a BBB permeability surface area product of 0.003 L/h (PS 0.0015 L/h for
BCSFB) together with a CV of 150% was found (Fig 4, Table 1).
Meropenem permeability in the pediatric brain meningitis PBPK model
The BBB/BCSFB permeability values estimated in the adult model were also used in the pediat-
ric model for children aged between 1 day and 3 months, after correction for brain weight.
This resulted in a <2 fold overlay between pediatric plasma and CSF concentrations both for
patients with meningitis and sepsis (Fig 5, Table 1).
Discussion
The pediatric brain PBPK model described here could predict CSF concentrations of the anal-
gesics paracetamol, ibuprofen and naproxen, and the antibiotic meropenem over a wide age
range. The CSF AUCs were simulated within 2-fold error of clinically observed values without
the need of changing system parameters of the compartments describing the healthy brain.
This shows that parameterization of these compartments was sufficiently robust to allow for
simulations of other drugs as well, and that the model could be useful in deriving mechanisti-
cally-informed dosing regimens for children.
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Development of a pediatric brain PBPK model
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Development of a pediatric brain PBPK model
Fig 3. Simulations of pediatric concentration-time profiles for ibuprofen, flurbiprofen and naproxen. Simulations of oral ibuprofen (10 mg/kg in
suspected sepsis patients) (A,B), IV ibuprofen (10 mg/kg in surgery patients) (C,D), IV flurbiprofen (0.9 mg/kg in surgery patients) (E,F), and oral
naproxen (10 mg/kg in surgery patients) (G,H) concentration-time profiles. Solid black lines indicate simulation of median profiles, the grey area
represents 90% CI and dotted lines indicate the minimum and maximum simulation. Dots indicate measured data derived from clinical studies. Log-
transformed concentration-time data are depicted in the right upper corners (0 values were discarded).
https://doi.org/10.1371/journal.pcbi.1007117.g003
Pharmacokinetic simulations were validated in relatively healthy children between 3
months and 15 years of age, which resulted in accurate AUC estimates (Table 1). In addition,
an attempt was made to perform simulations in children younger than 3 months, including
premature neonates, suffering from meningitis/sepsis. Although also in this case the simulated
AUCs were within 2-fold of observations, a trend towards an overestimation of plasma and
CSF levels could be observed (Table 1). It remains to be elucidated whether this is the result of
an influence of age and/or disease, or of the pharmacokinetic simulations in the validation
study, which were limited by the availability of only peak and through concentrations.
PBPK models are inherently complex, due to the many different drug-specific and (physio-
logical) system-specific parameters. Their robustness and reliability remain a challenge and
there is a clear need to validate model performance with sound experimental data. In this
study, most of the physiological processes could be incorporated in an age-appropriate man-
ner, however, due to absence of data, the relative flows between brain compartments expressed
as percentage of CSF production rate, were assumed to be the same as in adults.
Our pediatric brain model is structurally similar to that described by Gaohua et al. for an
adult population [8]. Recently, another pediatric brain PBPK model was developed to simulate
concentrations of morphine in brain extracellular fluid of traumatic brain injury patients, but
it was only validated with experimental data derived from six children [12]. Although this
model provides proof of principle for prediction of brain drug concentrations in children, the
pathophysiological changes associated with severe traumatic brain injury may have impacted
morphine disposition and hence extrapolation to other patient populations. Other models are
based on animal studies and, although they have been validated more extensively, translation
to the human situation remains difficult [18, 19].
Depending on the pathophysiological data available, the pediatric model described in this
study can be extended with different disease conditions. We simulated drug concentrations in
Fig 4. Simulations of adult concentration-time profiles for intravenous meropenem in meningitis patients. Simulations of adult plasma and CSF
concentration-time profiles (i.v. 1500 mg/8h) (A,B). Solid black lines indicate simulated median profiles, the grey area represents 90% CI and dotted lines
indicate the minimum and maximum simulation. Dots indicate measured data derived from clinical studies. Log-transformed results are depicted in the
left upper corners.
https://doi.org/10.1371/journal.pcbi.1007117.g004
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Development of a pediatric brain PBPK model
Fig 5. Simulations of pediatric concentration-time profiles for intravenous meropenem. Simulations of plasma and CSF for patients suffering from
sepsis (i.v. 20 mg/kg/8h) (A,B), or meningitis (i.v. 40 mg/kg/8h) (C,D). Solid black lines indicate simulated median profiles, the grey area represents 90%
CI and dotted lines indicate the minimum and maximum simulation. Dots indicate measured data derived from clinical studies. Log-transformed results
are depicted in the left upper corners.
https://doi.org/10.1371/journal.pcbi.1007117.g005
a population of children with meningitis and sepsis. Blood-brain barrier permeability has been
described to initially increase during meningitis, although at later times it will return to normal
values due to antibiotic-mediated recovery of patients [13]. Since quantitative data on mem-
brane permeability of meropenem were not available from literature, the brain permeability
parameter was obtained for the adult population by empirical optimization. The value we
derived this way (0.003 L/h) is in the same order of magnitude as intercompartmental clear-
ances that have been described in population PK models for adults and children (0.0017 and
0.0007 L/h, respectively) [17, 20]. This estimated permeability was subsequently applied in
simulations with the pediatric model, which is also in accordance with studies in which a cor-
relation between TNFα and blood-brain barrier damage was found, but not between TNFα
and age [21].
Simulated and measured maximum concentrations and AUCcsf/AUCserum ratios were
higher in patients suffering from sepsis/meningitis compared to relatively healthy individuals.
The highest measured concentration in the healthy population was 1.6 mg/L and the AUCcsf/
AUCserum ratio was 0.047[22]. In our simulations the upper bound of the 90% confidence
interval was around 5mg/L and AUCcsf/AUCserum ratios ranged from 0.09–0.12, indicating
that inflammation increased BBB permeability. In the studies of Lu et al. and Germovsek et al.
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Development of a pediatric brain PBPK model
that we used for validation, samples were taken at different moments after the start of dosing
and patients likely differed in disease severity, which might explain the large variability in BBB
and BCSFB permeability observed [17, 20]. Time-dependent effects on permeability could,
however, not be estimated from the available data. In septic children (without meningitis) the
same estimate on meropenem blood-brain barrier permeability resulted in an acceptable over-
lay between simulations and observed values, which can possibly be explained by a sepsis-
induced increase in BBB permeability [23].
In the current model, drugs were included for which carrier-mediated transport does not
play a major role in BBB and BCSFB. A next step will be to incorporate membrane transporters
in the model for relevant drug substrates. Data on quantitative proteomics of transporter
abundance in adults could form the bases for in vitro-in vivo extrapolation (IVIVE) of trans-
porter-mediated transport in an adult brain PBPK model [24, 25]. However, for pediatric pop-
ulations absolute protein expression of BBB/BCSFB transporters has not yet been quantified.
Immunohistochemistry studies indicate that expression may not be fully matured in young
children as has been described for the ABC transporter P-glycoprotein [26, 27]. Only for very
few other transporters information on human ontogeny is available [27].
A limitation of the current study is that data used for validation were obtained in children
over a broad age range, which could not be further stratified. Children were suffering from a
clinical condition and/or receiving co-medication that could have influenced the pharmacoki-
netic profiles. Next, CSF drug concentrations were used to validate the simulations and
although this is a relevant compartment for antibitiotics during meningitis, the parenchymal
extracellular or intracellular fluid is probably more important for other drugs, like analgesics.
Future research should be aimed at refining the model by dividing the brain into an intracellu-
lar and extracellular space and by expanding the CSF compartments, to better describe the
continuum between cranial and spinal CSF. This requires more clinical data on drug disposi-
tion in brain tissue and age-appropriate physiological parameters.
It has become more widely accepted that drug research should have an increased focus on
pediatric populations to improve safety and reduce off-label dosing [28]. Simple body weight-
based scaling ignores developmental processes as illustrated by the simulations in this study
with normalized paracetamol doses that did not result in equivalent CSF concentration-time
profiles. Modeling and simulation have been recognized as a way to make optimal use of exist-
ing data, which could result in more focused clinical trials in children. Moreover, in PBPK
modeling, parameters can be partly or completely estimated from in vitro or in silico studies,
further reducing the need for in vivo studies [29]. The ultimate goal of pediatric PBPK model-
ing would be to build models without making use of clinical data and although this might be
difficult due to the uncertainty in underlying physiological processes, it could provide guid-
ance for dose selection in first-in-child drug studies. Thereafter, clinical data can be used to
improve model performance in a “learn and confirm” cycle [30]. Several published models
have shown that it is possible to use a bottom-up in vitro-in vivo extrapolation (IVIVE)
approach for the estimation of rates of plasma absorption and elimination, which was not yet
incorporated in the current model. Linking the brain pediatric PBPK model developed in this
study to the existing IVIVE-based models could eventually provide the possibility to mechanis-
tically predict brain concentrations, which would facilitate dosing based on higher quality data
as compared to simply scaling from adult dosing regimens.
In conclusion, a mechanistic pediatric PBPK model was developed incorporating 4 differ-
ent brain compartments, which was used to simulate the plasma and CSF pharmacokinetics of
different drugs. The model can be valuable to predict CSF concentrations in cases where clini-
cal data in this compartment is restricted.
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Development of a pediatric brain PBPK model
Materials and methods
Approach
A five-step approach was used to build and validate the PBPK brain model for a pediatric pop-
ulation (Fig 6). These steps are briefly summarized below.
Step 1. Building of an adult PBPK brain model (paracetamol)
The adult PBPK brain model developed by Gaohua et al. was used as a template and para-
cetamol as model compound because it is not a substrate for drug transporter proteins
expressed in the blood-brain barrier (BBB) or blood CSF barrier (BCSFB) [8].
Step 2. Building of a pediatric PBPK brain model (paracetamol)
Physiological parameters in the adult model were changed to age-appropriate pediatric
parameters. Paracetamol was used to allow simulations in relatively healthy children.
Step 3. Validation of the pediatric PBPK brain model (ibuprofen, flurbiprofen, naproxen)
Physiological parameters included in the model were validated further by simulation of
plasma and CSF levels of ibuprofen, flurbiprofen and naproxen in relatively healthy children.
These drugs were chosen because they are no known substrates for BBB drug transporters, and
pediatric CSF concentrations were available in the literature.
Step 4. Building of an adult meningitis PBPK brain model (meropenem)
To the best of our knowledge, no mechanistic data is currently available quantifying the
influence of meningitis on brain drug permeability. The impact of meningitis on the passage
of meropenem across the BBB and BCSFB was therefore estimated in the adult brain PBPK
model (described below step 1) using empirical optimization.
Step 5. Building of a pediatric meningitis PBPK brain model (meropenem)
Meropenem BBB passage estimated in the adult meningitis PBPK model was incorporated
in a pediatric model to allow simulations for children with meningitis (combining steps 2, 3
and 4). Because children suffering from sepsis (without meningitis) were also included in the
clinical study used for validation, simulations were also done for this population.
Fig 6. Workflow used for the building and validation of the pediatric brain PBPK model.
https://doi.org/10.1371/journal.pcbi.1007117.g006
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Development of a pediatric brain PBPK model
At each step, the model was validated using published plasma and CSF concentration data,
as described below.
Step 1 Adult PBPK brain model
Plasma model. A PBPK model was coded in R software Version 1.1.442 and consisted of
14 compartments representing major organs and tissues (Fig 7). Average physiological param-
eter values and inter-individual variability were derived from literature [31], or values and
equations reported in the Simcyp simulator (Version 17 Release 1) [32–35]. As these are based
on weight, height, body surface area, sex and/or age-related equations, correlation between
parameters was partly accounted for, because variability in the original parameters is propa-
gated to the estimated/predicted parameter (e.g. a high body weight will on average result in
higher organ volumes). Residual parameter variability was assumed to be log-normally distrib-
uted. Organ partitioning coefficients were based on previous publications taking into account
both logP and ionization of compounds [36–38]. Plasma elimination from the model was
included using in vivo-measured clearance values reported in literature. Clearance were not
extrapolated from in vitro experiments, because in this way less robust plasma concentration-
time profiles would be generated, which would impede proper assessment of predicted CSF
concentrations. Because total body clearance in the adult model was not attributed to specific
organs or patient characteristics, only uncorrelated variability in clearance was included. This
was described in the adult model as:
Pi ¼ Ppop � eZZ
ð1Þ
Fig 7. Schematic outline of the PBPK model including four brain compartments (modified from Gaohua et al.) [8]. Qsin and Qsout represent CSF
shuttle flow between cranial CSF and spinal CSF compartments. Qssink and Qcsink are the flows from CSF compartments to blood. Qbulk represents bulk
flow from brain mass to cranial CSF. PSB, PSC and PSE represent permeability surface area products between brain blood and brain mass, brain blood and
cranial CSF, and brain mass and cranial CSF, respectively. Subscripts lu, br, ad, bo, he, ki, mu, sk, li, re, gu, sp, ha denote lung, brain, adipose tissue, bone,
heart, kidney, muscle, skin, liver, rest tissue, gut, spleen and hepatic artery, respectively. CL is the total clearance from the model. IV is an intravenous dose
and oral is an oral dose route of administration.
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Development of a pediatric brain PBPK model
where Pi is the parameter for an individual, Ppop is the population average, Z is the standard
normal variable, and η is the variance.
Brain model. The brain part of the model was connected to the plasma PBPK model as
described before and subdivided into 4 compartments, consisting of brain blood, brain mass,
cranial CSF and spinal CSF (Fig 7) [8]. The time-based differential equations used to describe
concentration changes in these brain compartments were as follows:
Vbb �
dCbb
dt
¼ Qbrain � Cbla (cid:0) Cbb
ð
�
ð
Þ þ PSb � fubm � Cbm (cid:0)
�
fubb � Cbb
Þ
þ PSc
fuccsf � Cccsf (cid:0)
fubb � Cbb
þ Qssink � Cscsf þ Qcsink � Cccsf
ð2Þ
Vbm
dCbm
dt
Vccsf �
dCccsf
dt
ð
¼ PSb � fubb � Cbb (cid:0)
fubm � Cbm
�
Þ þ PSe � fuccsf � Cccsf (cid:0)
�
fubm � Cbm
(cid:0) Qbulk
� Cbm
�
¼ PSe � fubm � Cbm (cid:0)
fuccsf � Cccsf
ð3Þ
�
�
þ PSc � fubb � Cbb (cid:0)
�
fuccsf � Cccsf
þ Qbulk
� Cbm þ Qsout � Cscsf (cid:0) Qsin � Cccsf (cid:0) Qcsink � Cccsf
Vscsf �
dCscsf
dt
¼ Qsin � Cccsf (cid:0) Qsout � Cscsf (cid:0) Qssink � Cscsf
ð4Þ
ð5Þ
Where Vbb, Vbm, Vccsf, Vscsf, fubm, fubb, fuccsf, fuscsf, Cbb, Cbm, Cccsf and Cscsf represent volumes,
unbound fractions and concentrations in brain blood, brain mass, cranial CSF and spinal CSF,
respectively. Qbrain denotes brain blood flow and Cbla denotes concentration in arterial blood.
Qsin and Qsout represent CSF shuttle flow between cranial CSF and spinal CSF compartments.
Qssink and Qcsink are the flows from CSF compartments to blood. Qbulk represents bulk flow
from brain mass to cranial CSF. PSb, PSc and PSe represent permeability surface area products
between brain blood and brain mass, brain blood and cranial CSF, and brain mass and cranial
CSF, respectively.
The following assumptions were made: (1) The BBB is a barrier between brain mass and
brain blood, and the BCSFB between cranial CSF and brain blood. The barrier separating
brain mass and cranial CSF is of high permeability. No barrier exists between cranial CSF and
spinal CSF. (2) Compartments are of constant volume and well-stirred. (3) Permeability sur-
face area products of the BCSFB are two-fold smaller than corresponding BBB values, as was
previously described [8, 11, 39]. (4) As drug metabolism was included as a total-body clear-
ance, a specific contribution of brain metabolism is assumed absent and drug entering the
brain mass compartment is returned into brain blood to preserve mass balance. (5) Trans-
porter-mediated transfer across barriers is considered negligible for the studied drugs, as they
are no known substrates for drug transporters expressed in BBB or BCSFB. Therefore, barrier
penetration is considered to occur by passive diffusion and described by permeability surface
area products [24].
(6) CSF production rate was multiplied by 2 in populations receiving spinal ketamine anes-
thesia, based on a two-fold increase that was observed in cats [16]. (7) A brain tissue binding
parameter was derived from literature or estimated using the prediction option incorporated
in Simcyp [32–35].
BBB permeability was estimated for each drug separately from rat carotid artery perfusion
data or cell-based passive permeability assays, and in the latter case scaled to in vivo values by
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Development of a pediatric brain PBPK model
using the equation:
PSbbb ¼ in vitro permeability � BBB surface
ð6Þ
where in vitro permeability is expressed as dm/h, and BBB surface in dm2. A sensitivity analysis
was performed to investigate the effect of CSF production rate change on the drug concentra-
tion-time curve in the spinal CSF compartment.
Step 2 Pediatric PBPK brain model
Plasma model. To translate the adult model to a pediatric model estimates of height,
weight, body surface area, organ volumes, tissue blood flows, hematocrit and albumin concen-
trations were adjusted using previously reported equations from literature [31] or the pediatric
Simcyp simulator [32–34]. This resulted in an age-appropriate set of parameters for each simu-
lated patient. Child-specific tissue composition was also incorporated, which affects the predic-
tion of organ partitioning coefficients. Pediatric plasma clearances were not estimated by the
model, but derived from literature (S2 Table, partially also from the same studies used for vali-
dation of the brain PBPK model) and consisted of body weight-based relations. The age range
for the patients in these studies overlapped with that of the simulated patients almost
completely, to reduce unjustified extrapolation of clearance values across ages. For oral dosing
studies a rate constant (ka) and variability was derived from literature, and if this value was
unavailable an estimate was made by using the MechPeff model incorporated in Simcyp [32–
34]. Unexplained variability for clearance and absorption was incorporated using Eq 1 (previ-
ous section).
Brain model. The time-based differential equations and assumptions made in the adult
brain PBPK model were also applied to the pediatric model. In addition, physiological values
for brain parameters were derived from literature leading to the following considerations: (1)
Brain volume, brain blood flow, spinal CSF volume and CSF production rate were adjusted as
a function of age [31, 35, 40–43]. (2) Cranial CSF volume was not expected to further increase
after birth [35, 44]. (3) Relative CSF flows between compartments, expressed as percentage of
CSF production, were assumed to be similar to adult values. (4) Since BBB surface area per
gram of brain is similar for adults and children, total surface area was smaller in children
because of a lower brain mass compared to adults [31, 43, 45] (Table 2).
Step 3 Validation of pediatric brain PBPK model
To validate the physiological parameters included in the pediatric PBPK model, plasma and
CSF concentrations were simulated with different drugs not used to build the model, namely
ibuprofen, flurbiprofen, and naproxen using both adult and pediatric models. Only drug-spe-
cific parameters were adjusted to perform simulations for these drugs, of which brain penetra-
tion is like paracetamol known not to be affected by drug transporters.
Step 4 Incorporation of meningitis in the adult model
In case of meningitis, blood-brain barrier function is known to be impaired [47]. To have an
estimate on permeability of meropenem through the BBB the permeability surface area prod-
uct was empirically optimized in the adult meropenem model, both for the population average
and coefficient of variation. Effects of meningitis on plasma clearance was already incorpo-
rated in the plasma parameter derived from the study that was also used for validation of the
model [17]. In addition, effects of meningitis on free fraction and erythrocyte-plasma parti-
tioning coefficients were not incorporated, because differences in albumin concentrations and
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Table 2. Pediatric brain physiological parameters.
Equation
ageþ0:315
9þ6:92�age
1:04
Vbrain total ¼ 10 �
Vbrain blood = 0.05 � Vbrain
Vccsf = 0.143
Vscsf ¼ 1:94�body weightþ0:13
Limit Vscsf � 0:143
0:8 � 0:2
Vendothelial = Vbrain total
Vbrain mass = Vbrain total−Vendothelial−Vbrain
blood−Vccsf−Vscsf
� 0.005
1000
Equation
Qcsfproductionrate(3m−18y) = 0.024
Qcsfproductionrateð<3mÞ ¼ 4:007�logðageÞþ7:088
Qcsfproductionrate (CV%) = 10
Qbulk = 0.25�Qcsfproductionrate
1000
Qbulk (CV%) = 8
Qsin = Qssink+Qsout
Qsout = 0.9�Qssink
Qsout (CV%) = 100
Qcsink = 0.75 � Qcsfproductionrate+Qbulk−Qsin+Qsout
Qssink = 0.38�(0.75�Qcsfproductionrate+Qbulk)
Qssink (CV%) = 30
Qbrain ¼ Qcarout � 10þ2290�ð10(cid:0) 0:608�age(cid:0) 10(cid:0) 0:639�ageÞ
100
BBB ¼ BBBadult � Vbrain total child
Vbrain total adult
Development of a pediatric brain PBPK model
Volumes(L)a
Notes
Description
Brain volume
Brain blood volume
Cranial CSF volume
Spinal CSF volume
Endothelial cell volume
Brain mass volume
Spinal CSF volume capped at 20% of total CSF volume (same as in
adult)
Fluid flow rates(L/h)
Description
Notes
CSF production rate
If ketamine used in clinical study. Production rate multiplied by 2.
Bulk flow brain mass to
cranial CSF
Relative CSF flows (as part of Qcsfproductionrate) assumed to be the
same for adults and children.
Flow from cranial CSF to
spinal CSF
Flow from spinal CSF to
cranial CSF
Flow from cranial CSF to
brain blood
Flow from spinal CSF to
brain blood
Brain blood flow
Cardiac output � fractional tissue flow
BBB surface area (m2)
BBB surface area
Ref.
[31]
[8, 35]
[35, 44]
[35, 40]
[35]
[35]
Ref.
[8, 35, 41,
42]
[8, 35]
[8, 35]
[8, 35]
[8, 35]
[8, 35]
[8, 35]
[8, 35]
[8, 35]
[35]
[31, 43,
45]
a Tissue volumes were converted to liters. Adult organ densities reported in Abduljalil et al. [46] were used to convert equations predicting organ weight to organ
volumes if needed.
https://doi.org/10.1371/journal.pcbi.1007117.t002
hematocrit levels were assumed to be of minor importance due to low protein binding and low
cell penetration of meropenem [48–51].
Step 5 Incorporation of meningitis in the pediatric model
The value for blood-brain barrier permeability estimated in the adult model was also used in
the pediatric model after correction for the difference in blood-brain barrier surface area. The
effect of meningitis on plasma clearance was already incorporated in the clearance parameter
derived from the NeoMero study, in which only patients were included suffering from sepsis
or meningitis [20]. Effects of meningitis on free fraction and erythrocyte-plasma partitioning
coefficients were not incorporated, as also for the pediatric population this was assumed to be
of minor importance (see previous section).
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Development of a pediatric brain PBPK model
Table 3. Characteristics of studies included for validation.
Study
Drug
Number of
patients
Co-medication
Age(y)
Indication
CSF collection
Singla et al., 2012
[15]
Bannwarth et al.,
1992 [7]
Kumpulainen
et al., 2007 [52]
Va¨litalo et al.,
2012 [53]
Kumpulainen
et al., 2010 [54]
Kokki et al., 2007
[55]
Har-Even et al.,
2014 [56]
Lu et al., 2016
[17]
Germovsek et al.,
2018 [20]
Paracetamol
Propacetamol (similar
to 50% dose of
paracetamol)
[58]
Paracetamol
Naproxen
Flurbiprofen
Ibuprofen
Ibuprofen
Meropenem
7
43
32
53
27
36
28
82
Meropenem
167
https://doi.org/10.1371/journal.pcbi.1007117.t003
-
-
Midazolam, ketamine,
propofol, thiopental
Midazolam, ketamine,
propofol, thiopental
Midazolam, ketamine,
propofol, thiopental,
paracetamol, ketoprofen,
fentanyl
19–44
Healthy
Spinal catheter
31–73
Nerve-root
compression
pain
Diagnostic lumbar
puncture
0.25–13
Elective surgery
0.25–12
0.25–13
Surgery lower
part body
Surgery lower
part body
Lumbar puncture for
spinal anesthesia
Lumbar puncture for
spinal anesthesia
Lumbar puncture for
spinal anesthesia
Midazolam, ketamine
0.25–12
Surgery
-
0.42–15
Suspected sepsis
Lumbar puncture for
spinal anesthesia
Lumbar puncture for sepsis
assessment
-
not reported
-
not reported
17–77
Meningitis
Lumbar drainage
0.0027–
0.25
Sepsis/
Meningitis
Opportunistic lumbar
puncture for sepsis/
meningitis assessment
Percentage
male (%)
100
56
59
74
78
69
64
61
53
In vivo observations and model evaluation
Clinical studies describing concentration-time profiles of paracetamol in adults (step 1) and
paracetamol (step 2), ibuprofen, flurbiprofen and naproxen (step 3), in children, were used for
validation and extracted from original publications with WebPlotDigitizer version 4.1 [7, 15,
17, 20, 52–56]. As plasma and CSF samples were taken in the setting of clinical care, the major-
ity of data was derived from individuals having a clinical condition, however, except for
patients suffering from sepsis and/or meningitis, this was not expected to affect brain perme-
ability (Table 3). Studies included healthy adult volunteers (1 study [15]), adult nerve root
compression pain/arthritis patients (1 study [7]), pediatric surgery patients receiving spinal
anesthesia (4 studies [52–55]) and pediatric (suspected) sepsis patients (1 study [56]). For step
4 (adults) and step 5 (children) meropenem PK studies, all patients suffered from (suspected)
sepsis and/or meningitis (2 studies [17, 20]). In the study of Germovsek et al. concentrations
were described as ‘time after dose’ at steady state, which was expected to be reached after 24h
[57]. Because in this study meropenem CSF values for children suffering from sepsis (without
meningitis) were available, simulations were performed for this population as well.
Simulations were run for 1000 virtual individuals who were matched with the individuals
in the original studies for dosing regimen, age range, and percentage male/female. Simulations
of CSF concentration-time profiles were visualized for the spinal compartment as clinical mea-
surements were performed by lumbar puncture. Results were compared with observations
using visual predictive checks in which median, 5th percentile, 95th percentile, minimum, and
maximum values were overlaid with clinical observations derived from literature. Also, plasma
and CSF AUC0-last were calculated for median simulated data and for observed data using a
non-compartmental (linear trapezoidal) approach. A naïve pooling approach was used for the
population data because variability between subjects was expected to cancel out in the analysis.
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Development of a pediatric brain PBPK model
In case of two observations at the same time, the average was used. AUCs were compared
between simulated data and observed data according to:
fold error ¼
observed AUC
predicted AUC
ð7Þ
and model simulations were considered acceptable if the ratio was within two-fold difference
[59]. Only plasma peak and through levels were available for the pediatric population receiving
meropenem and few high CSF values largely influenced AUC. This means that requirements
for the use of the naïve pooling approach are not met [60]. In contrast, AUC was for this study
calculated below the simulated concentration time profile reported.
Supporting information
S1 File. Rstudio code.
(R)
S1 Table. Physiological parameters.
(PDF)
S2 Table. Drug-related parameters.
(PDF)
Author Contributions
Conceptualization: Laurens F. M. Verscheijden, Jan B. Koenderink, Saskia N. de Wildt, Frans
G. M. Russel.
Data curation: Laurens F. M. Verscheijden.
Formal analysis: Laurens F. M. Verscheijden.
Supervision: Jan B. Koenderink, Saskia N. de Wildt, Frans G. M. Russel.
Validation: Laurens F. M. Verscheijden.
Visualization: Laurens F. M. Verscheijden.
Writing – original draft: Laurens F. M. Verscheijden, Saskia N. de Wildt, Frans G. M. Russel.
Writing – review & editing: Jan B. Koenderink, Saskia N. de Wildt, Frans G. M. Russel.
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| null |
10.1088_1402-4896_ad16b7.pdf
|
Data availability statement
The data that support the findings of this study are available upon reasonable request from the authors.
|
Data availability statement The data that support the findings of this study are available upon reasonable request from the authors.
|
RECEIVED
15 July 2023
REVISED
11 December 2023
ACCEPTED FOR PUBLICATION
18 December 2023
PUBLISHED
29 December 2023
Phys. Scr. 99 (2024) 015246
https://doi.org/10.1088/1402-4896/ad16b7
PAPER
Global and multistable dynamics in calcium oscillations model
Rajes Kannan Subramanian1, Zeric Tabekoueng Njitacke2,∗
Karthikeyan Rajagopal4
1 Center for Artificial Intelligence, Chennai Institute of Technology, Chennai 600069, Tamil Nadu, India
2 Department of Electrical and Electronic Engineering, College of Technology (COT), University of Buea, PO Box 63, Buea, Cameroon
3 Department of Automation, Biomechanics and Mechatronics, Lodz University of Technology, ul. Stefanowskiego 1/15, 90-537 Lodz,
, Jan Awrejcewicz3
and
Poland
4 Centre for Nonlinear Systems, Chennai Institute of Technology, Chennai 600069, Tamil Nadu, India
∗ Author to whom any correspondence should be addressed.
E-mail: [email protected]
Keywords: calcium oscillation, two-parameter charts, coexistence of bifurcations, multistability
Abstract
In most animal and plant cells, the information’s processing is insured by calcium ions. This
contribution studies the global dynamics of a model of calcium oscillation. From the stability analysis,
it is found that the oscillations of that model are self-excited since they are generated from unstable
equilibria. Using two-parameter charts, the general behavior of the model is explored. From the
hysteresis analysis using bifurcation diagrams with their related Largest Lyapunov Exponent (LLE)
graphs, the coexisting oscillation modes are recorded. This phenomenon is characterized by the
simultaneous existence of periodic and chaotic oscillations in the considered model by just varying the
initial conditions. Using a set of parameters for which the model exhibits multistability, the basins of
attraction related to each coexisting solution are computed and enable the capture of any coexisting
pattern.
1. Introduction
)
-
Ca
(
IP
3
+Ca2
+Ca2
+Ca
2
[
released on cytosolic
] which constitutes most cell types [7–9]. In [10],
,
cross-coupling model (ICC) of [11], the study of the
+Ca2 concentration. From the built model, under the variation of the
+Ca2 oscillations was introduced. That model was derived from the study of the
Calcium oscillations have a key role in the function of cells since they act in them from fertilization to death. The
oscillation processes are found in a variety of cell types, such as neuron cells [1], astrocyte cells [2], T-lymphocyte
cells [3], oocyte cells [4]and hepatocyte cells [5, 6]. From experimental work, it has been shown that
oscillations are related to the variation in free cytosolic
an improved model of the
+
2
mechanism in inositol trisphosphate
calcium-induced calcium release (CICR) mechanism in [12] and the consideration of the bell-shaped
dependence of
agonist, complex phenomena such as period adding, period doubling, mixed mode states, and chaos were
found, and they match well with experimental results. Reference [13] introduced three different models of
calcium oscillations, all of which are derived from one- or two-pool models centered on ICR. The first model
was created by taking into account the suppression of the
release channel on a single intracellular store
when cytosolic
1,4,5-trisphosphate (IP3) that is activated by
periodic and chaotic behaviors. Another model of
conducted on hepatocytes. This new model considered the feedback inhibition of calcium and activated
phospholipase C on the initial agonist receptor complex, along with the receptor type-dependent self-enhanced
behavior of the activated aG subunit. From the simulation, the authors showed the model was able to exhibit
rich dynamical behavior ranging from simple periodic to chaotic dynamics. The fractional version of the model
proposed in [14] has been introduced in [5]. Exploiting the modified trapezoidal rule for fractional integrals, the
bifurcation analyses of the model were addressed. Using the numerical simulation, different types of bursting
] levels are high. In the second model, the authors incorporated the degradation of inositol
+Ca2 oscillations was proposed in [14], based on experiments
+Ca .2 Through numerical simulations, these models revealed
+Ca2
[
+Ca2
© 2023 IOP Publishing Ltd
Phys. Scr. 99 (2024) 015246
R K Subramanian et al
calcium oscillations in non-excitable cells have been highlighted in [15]. After that, it is also found in the work of
[16] that focused on the fractional investigation of the calcium oscillations based on the Atangana-Baleanu
operator. As can be seen in the quoted literature, many works have been done in the area of designing and
+Ca2 oscillations, taking into consideration several additional hypotheses [5, 10–15]. Using time
investigating
delay with additive Gaussian colored noised, intracellular calcium oscillation (ICO) was investigated [17]. From
the work of the authors, the found that time delay was able to induce saw-tooth calcium wave and transition in
intracellular calcium oscillation. In the intracellular calcium oscillation system, which is defined by the processes
of active and passive intracellular
coherence resonance were examined [18]. The authors discovered that (i) a specific time delay or correlation
time value caused stochastic or reverse synchronization; (ii) a phenomenon known as reverse resonance was
obtained in the function of reciprocal coefficient of variance versus time delay or versus strength of noises as
time delay increased; and (iii) both stochastic and reverse resonance were observed in the function of reciprocal
coefficient of variance versus correlation time with varying strength of noises. Also, under the effect of the time
delay, the phenomenon of oscillatory coherence in the intracellular calcium oscillation system was captured
in [19].
transport driven by colored sounds, the effects of time delay on the
+Ca2
Therefore, a plethora of dynamical behaviors such as period adding, period doubling, mixed mode states,
bursting, and chaos were recorded. Some of those behaviors have already been found in some other biological
and mechanical systems, such as pancreatic beta-cells [20], electromechanical transducers [21], modified
Rayleigh-Duffing oscillators [22], neuron models [23–26]. Since the aforementioned works are all related to
dynamical systems, one striking and widespread phenomenon found in those systems is the coexistence of
patterns (multistability). Multistability in a model is characterized by the presence of multiple stable states,
which can be achieved by modifying the initial conditions while keeping the parameters constant [27, 28].
Despite the large number of works already addressed on the calcium oscillation model [23–26], there is currently
no study that specifically focuses on analyzing the coexisting bifurcations with more than two oscillating states in
such model. Since multistability analysis is important in calcium oscillation models because it helps to identify
the different stable states that the system can exhibit. This is important because many biological systems are able
to exhibit multiple stable states, which can have different functional consequences. For example, in pancreatic
cells, calcium oscillations are involved in regulating insulin secretion. Multistability analysis has shown that
these cells can exhibit different stable states of calcium oscillations, which may correspond to different levels of
insulin secretion [29]. Understanding the multistability of calcium oscillation models can also help to identify
potential therapeutic targets for diseases that involve abnormal calcium signaling, such as epilepsy or cardiac
arrhythmias [30, 31].
Therefore, in order to contribute to the existing literature and uncover previously unknown behaviors of the
calcium oscillation model proposed in [14] based on experiments in hepatocytes, this study will reexamine the
model using adapted computation techniques.
The remainder of this study is organized as follows: section 2 provides a review of the mathematical model
for calcium oscillations and examines its stability near equilibria. Section 3 employs numerical simulation
techniques to explore the overall dynamics of the model, including one- and two-parameter charts and basins of
attraction. Finally, section 4 offers a conclusion that summarizes the findings and presents potential directions
for future research.
2. Model and its features
In the cells of plants and animals, calcium ions are the main element involved in information processing since
cytoplasmic free calcium ions enable the second messenger under the effect of a variety of stimuli. From the
experimental investigations of hepatocytes [32], the mathematical model of the calcium oscillation of
equation (1) has been introduced.
d
x
dt
d
u
dt
d
y
dt
d
v
dt
⎧
⎪
⎪
⎪
⎪
⎨
⎪
⎪
⎪
⎪
⎩
= +
k
1
k x
2
-
k
3
xu
+
k
4
x
-
k
5
xy
+
x
k
6
=
k x
7
-
k
8
u
+
u
k
9
k u
12
+
k x
13
-
k
14
y
+
y
k
15
-
k
16
y
+
y
k
17
=
k
10
v
= -
k
10
+
uyv
+
k
11
uyv
+
k
11
+
k
16
y
+
k
17
In equation (1), the first variable x represents the concentration of the aG ( which is one of three guanine
nucleotide-binding protein components, all of which are heterotrimeric membrane-associated G proteins)
v
y
( )
1
2
Phys. Scr. 99 (2024) 015246
R K Subramanian et al
Table 1. Equilibrium points for varying k10 and their stability.
Control parameter
Equilibrium points
Eigenvalues and their stability
=k
10
3.63
=k
10
5
-
)
(
7.814; 29.575; 0.775; 0.155
-
)
(
10.054; 53.709;
0.051
1.318;
-
)
(
19.124;
153.502; 32.724; 0.001
-
-
-
)
(
2.664
0.00;
0.056;
0.029;
-
-
-
(
)
2.613
0.005;
0.646;
0.352;
-
-
-
)
(
2.535
0.017;
2.155;
1.240;
-
-
-
-
)
(
7.814; 29.575; 0.775; 0.11
-
)
(
0.037
10.054; 3.709;
1.318;
-
)
(
153.502; 32.724; 0
19.124;
-
-
(
)
0.056; 0;
0.029;
2.662
-
-
-
-
(
)
2.593
0.646;
0.352;
-
-
-
-
)
(
2.488
2.155;
1.240;
-
0.005;
0.017;
2
l =
0.189
1,2
l = 96.749,
2
1
l = 6833.018,
1
l = 3.103,
1
l = 5.390,
1
l = 29.063,
1
unstable node
l =
0.191
1,2
l = 132.911,
1
l = 9410.44,
1
l = 3.104,
1
l = 5.390,
1
l = 29.066,
1
unstable node
2
2
l = -
3,4
1.184j
l = -15.589
l = -0.164
2
2
l = -1.172,
l = -0.718,
2
l = -1.237,
unstable
0.335
1.224
24.155
l = -
3,4
l =
3,4
l = -8.225,
l = -10.252,
3
l = -18.566,
3
3
12.283j
unstable
unstable
1.404j
7.902j
l = -962.771
4
l = -1035.832
4
l = -1276.513
4
unstable node
unstable node
1.186j
l = -
3,4
2
l = -15.429
l = -0.1642,
2
unstable
0.336
30.025
l = -
3,4
l =
3,4
l = -5.981,
l = -7.562,
4
3
l = -13.996,
l = -1276.211
11.752
j
unstable
+
j
1.405
7.902
j
unstable
l = -962.769
l = -1035.797
1.224
3
4
4
3
l = -1.171,
l = -0.718,
2
l = -1.237,
unstable node
unstable node
subunits. u stands for the concentration of active PLC (phospholipase C, which is a membrane-associated
enzyme family that cleaves phospholipids immediately before the phosphate group). The third variable y
represents the free calcium concentration in the cytosol. The fourth variable v is considered as the concentration
of calcium in the endoplasmic reticulum (ER). In addition, the constant k1 stands for the spontaneous activation
of the aG sub-unit, k a2 mimicking the accelerated development of the active aG after the binding if agonist to the
membrane receptor. In other word, k2 can stands for the concentration of the agonist. In general,
=k i
i (
description of those coefficient is found in [29].
) are constant values use to setup the calcium model under consideration more detailed
17
1
v
0.
= = = =
y
The equilibrium points of the considered model are obtained by solving the equation given as
u
x
computed and recorded in the second column of table 1 for the following values of the coefficient: =k
=k
=k
6
2
=k
=k
16
12
With the help of MAPLE, the equilibria on the calcium oscillation model have been
=k
3
=k
13
2.7738,
0.7,
0.64,
13.58,
=k
7
=k
17
2.08,
0.05.
=k
4
=k
14
=k
5
=k
15
1.18,
4.85,
0.19,
153,
4.88,
0.16,
1
=k
11
32.24,
29.09,
=k
9
=k
8
2.67,
0.09,
The Jacobian matrix around the any of the equilibrium of the considered calcium model is given by
equation (2).
J
=
a
k
7
-
¯
u
k
13
0
⎡
⎢
⎢
⎢
⎢
⎢
⎢
⎢
⎢
⎢
⎣
With = -
a
k
2
¯
x
+
¯
k y
14
+
k
15
-
2
-
¯
k x
3
+
k
4
¯
x
k
8
+
+
+
( ¯
u
k
9
¯ ¯
k yv
10
+
¯
k
v
11
¯ ¯
k yv
10
+
¯
k
v
11
-
¯
k u
8
+
k
2
)
9
k
12
4
¯
k u
3
+
k
k
16
+
k
17
+
( ¯
x
+
2
¯ ¯
k ux
3
+
)
k
4
¯
k y
16
+
k
17
-
¯
k x
5
+
k
6
¯
x
0
b
-
¯ ¯
k uv
10
+
¯
k
v
11
+
k
16
+
k
17
¯
y
-
( ¯
y
¯
k y
16
+
k
17
2
)
0
0
¯ ¯
k yu
10
+
¯
k
v
11
¯ ¯
k uy
10
+
¯
k
v
11
-
-
+
2
¯ ¯ ¯
k yuv
10
+
)
( ¯
k
v
11
¯ ¯ ¯
k uyv
10
+
)
( ¯
v
k
11
2
⎤
⎥
⎥
⎥
⎥
⎥
⎥
⎥
⎥
⎥
⎦
-
¯
k y
5
+
k
6
¯
x
+
( ¯
x
¯ ¯
k yx
5
+
k
6
2
)
,
b
=
¯ ¯
k uv
10
+
¯
k
v
11
-
k
14
+
k
15
¯
y
( ¯
y
Afterward, the eigenvalues with their related stability have been obtained and discussed in the third line of
( ¯
y
¯
y
)
)
2
table 1 by solving equation (2).
det
(
J
l-
I
)
=
0
With I representing a fourth order, identify matrix. From the computation, it is found that for each discrete
value of the control parameter, the calcium oscillation model has six equilibria. The determination of the
eigenvalues related to each of those equilibria revealed that the model displays self-excited oscillation from the
nature of the eigenvalues, which can be either unstable saddle-focus or unstable nodes. The properties of having
a large number of fixed points can be the origin of some coexisting states that may be found during the
investigation of the considered model.
3
( )
2
( )
3
Phys. Scr. 99 (2024) 015246
R K Subramanian et al
Figure 1. Two-dimensional charts showing the global behavior the calcium oscillation model under the variation of the paramter in
=k
=k
(
various planes. The plane k
The
16
8
data in red are associated with chaotic motion while those in blue are associated with periodic motion. Initial conditions are
(
0.01; 0.01; 0.01; 20
by decreasing the control parameters.
) in addition, the left diagrams are obtained by increasing the control parameter while the right one are obtained
) obtained for =k
) obtained for =k
(
the plane k
32.24,
32.24,
4.88,
4.85.
k,10
k,10
16
5
8
5
3. Numerical results
Since most of the previous works addressed on that calcium model were just some routes that gave birth to its
chaotic dynamics. Our goal in this work is the investigation of the global behavior dynamics of that calcium
oscillation model, using some two-dimensional charts that will exploit the sign of the Largest Lyapunov
Exponent (LLE). The largest Lyapunov exponent of our model have been computed using the formula of
equation (4)
l
max
=
lim
t¥
1
t
⎡
⎣
ln
(
2
d
¯
x
+
2
d
¯
u
+
2
d
¯
y
+
d
2
¯ )
v
⎤
⎦
( )
4
and computed from the variational equations obtained by perturbing the solutions of the considered calcium
d
d
+
oscillation model as follows:
v, with the help of the
u
u,
algorithm developed in [33].
2
2
+
d
d
¯ is the distance between neighboring trajectories;
¯
v
y
2
l
(
exp
asymptotically
Using some bifurcation diagrams that will be computed using a hysteresis approach based on the
+
d
x,
x
2
2
+
d
d
¯
¯
u
x
d
d
+
¯
¯
v
y
u
+
=
+
v
+
y
d
y, and
d
¯
u
d
¯
x
max
+
+
)
.
t
x
v
y
2
2
2
continuation method or diagrams using a fixed initial condition based parallel bifurcation branch approach, the
possible existence of the coexisting dynamics will be addressed. Almost all these characterization tools will be
integrated using the Runge–Kutta algorithm with a fixed time step of ´ -
10 3 with the format of the variable
extended precision mode.
1
3.1. Two-dimensional charts
The two-parameter charts from which the global behavior of the calcium oscillation model is examined are
captured by varying simultaneously in the backward and upward directions two control parameters of the
model. The two-parameter charts and the attraction basin, are obtained by numerically computing the LE
spectrum on a grid of
400 values of the chosen space parameters, in order to have diagrams with uniform
´400
4
Phys. Scr. 99 (2024) 015246
R K Subramanian et al
Figure 2. Bifurcation diagrams (a(i) and b(i)) showing the behavior of the calcium model under the variation of one parameters with
their corresponding Largest Lyapunov Exponents (a(ii) and b(ii)). There, the local maxima of the concentration of the aG subunits
) are recorded under the variation of the coefficient k .10 This particular diagram enables to see the rate of change of the
(
xmax
concentration of the aG subunits under the variation of the coefficient k10 The enlargement of figures 2(a(i) and (b(i)) and found in
figures 2(a(ii) and (b(ii)).
Figure 3. Coexisting patterns in the calcium model for the value of the parameter
initial states 5.25; 2.25; 0; 0
with coexisting phase portraits, while figure 3 (b) is associated with the related time series showing the temporal evolution of the
coexisting concentration of the aG subunits.
=k
10
) while the periodic one sis obtained using the initial states
The chaotic pattern is obtained using the
-
) Figure 3(a) is associated
3.63.
(
5.25;
8.25; 0; 0 .
(
shapes. The integration was realized in Turbo pascal with variables in extended precision mode and ran on an
octa-core workstation with an Intel core i7 processor. For each variation of the control parameter, the LLE of the
model is computed and used to differentiate the two main behaviors of the model. On the one hand, the model
exhibits chaotic behavior supported by a positive LLE, and on the other, periodic behavior supported by a null
LLE. More importantly, this upward and backward computational technique represents an effective way to track
windows in which the model can experience coexisting patterns. Upon analysis of the two-parameter charts
presented in figure 1, it is evident that the diagrams in the left panel are generated by simultaneously increasing
5
Phys. Scr. 99 (2024) 015246
R K Subramanian et al
Figure 4. Demarcation diagram showing the set of initial conditions related to each of the coexisting patterns of figure 3. The red
domain is associated with chaotic patterns, blue with periodic patterns and yellow with unbounded motion. Figure 4 (a) is obtained
( )
for
0
while figure 4(b) is obtained for
( )
0
( )
0
( )
0
=
=
=
=
u
0
0
x
v
y
.
both control parameters, whereas the diagrams in the right panel are derived by decreasing both control
parameters. Moreover, it can be observed that the predominant behaviors depicted on these charts are periodic,
as their occurrence area surpasses that of the chaotic behaviors.
y
v
0.
=
( )
0
( )
0
3.63
] and
] and
15, 0
=k
10
and computing the
( )) when
0
15, 15
u0 ,
Î -
[
Î -
[
] only chaotic and periodic patterns can captured while for
3.2. Coexisting oscillation modes
Coexisting behaviors occur when, for the same set of system parameters, the model is able to display two or more
completely different patterns by just changing the initial conditions. This phenomenon can be observed in the
calcium oscillation model, as shown in figures 2 (a(i) and b(i)), along with the corresponding LLE graph (a(ii)
and b(ii)). These figures. present two sets of data, with the blue set obtained by increasing the control parameter
K10 and the red set obtained by decreasing the control parameters. Figure 2 clearly demonstrates that the
diagrams in b (i, ii) are magnifications of those in a (i, ii). Depending on the sweeping direction, the calcium
oscillation model has two different routes to chaotic patterns, which are related to the hysteresis of the model. In
that region of coexisting bifurcation, taking a discrete value of the parameters
model starting from different initial conditions, as can be seen in the caption of figure 3, the model experiences
the coexistence of the chaotic (red) and the periodic (blue) patterns (see figure 3). To obtain probability that any
of the coexisting attractors can be found, the basins of attraction of figure 4 have been computed. Figure 4(a) in
=
( ( )
obtained in the plane x
As it can be seen on that demarcation diagram, for
Î
[
( )
( )
x 0
0, 15
u 0
Î -
( )
[
( )
u 0
x 0
same line as it can be seen in figure 4(b) when varying y 0( ) between -5, 30
each of the three coexisting behavior occupy a specific domain of initial condition where it can
( )
x
0
be found. Therefore, the high sensitivity of the calcium oscillation model to the variation of the initial condition
is demonstrated and validated by the previous investigation. In the work of the authors, such as Pankratova et al
[34], the author investigated the bistability of the calcium oscillation. That bistability involves the coexistence of
a steady state (point attractor) and an oscillatory mode. In contrast, our coexisting patterns found multistability
since more than two patterns coexist in the model depending on the choice of the initial conditions. In our
model, we have the coexistence of a steady state, two oscillatory modes (periodic and chaotic), and an
unbounded region, which are well supported using the basin of attraction of figure 4. To the best of the author’s
knowledge, there is no work related to the experimental observation of the multistability in the calcium
oscillation, but concerning some neural circuits [35] and some nonlinear oscillators such as Chua [36] or Jerk
[37], multistability has been revealed experimentally, and it has been found that the coexisting patterns were able
to move randomly from one to another without any modification of a parameter of the circuit only by switching
ON and OFF the power supply. In addition, the sudden changing of patterns was related to environmental
conditions such as noise temperatures or magnetic fields. Therefore, such multistability can also be studied
experimentally in the calcium oscillation based on environmental conditions since it has already been proved
numerically.
] only chaotic patterns and unbounded motion can be recorded. In the
] with
] and v 0( ) between -5, 20
15, 15
( )
0
=
=
u
0
[
[
6
Phys. Scr. 99 (2024) 015246
4. Conclusion
R K Subramanian et al
This contribution was devoted to the further analysis of the calcium oscillation model obtained from hepatocyte
cells. From the computation of the equilibrium points, it has been found that the model exhibits self-excited
dynamics. Based on the numerical simulations exploiting the fourth-order Runge–Kutta algorithm, the global
dynamics of the model under the variation of parameters have been revealed through two-parameter charts.
From the hysteresis analysis, it has been found that model-supported multistability, characterized by the
coexistence of up to three distinct dynamical states for the same set of parameters. So far, the result on the
multistable dynamics involving more than two coexisting oscillatory modes in such a model has not yet been
reported and represents an enriching contribution regarding the dynamics of such a model. Therefore, the effect
of fields on such models as well as their network investigations will represent the scope of our future work.
Acknowledgments
This work was supported by the Centre for Nonlinear Systems, Chennai Institute of Technology (CIT), India via
grant number CIT/CAI/2023/RP/012.
Jan Awrejcewicz has been supported by the Polish National Science Centre under the Grant OPUS
18No.2019/ 35/B/ST8/00980.
Data availability statement
The data that support the findings of this study are available upon reasonable request from the authors.
Declarations
Conflict of interest
The authors declare that they have no conflict of interest.
ORCID iDs
Zeric Tabekoueng Njitacke
Jan Awrejcewicz
https://orcid.org/0000-0003-0387-921X
https://orcid.org/0000-0001-7797-8929
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[9] Sun S et al 2007 Physical manipulation of calcium oscillations facilitates osteodifferentiation of human mesenchymal stem cells FASEB
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[10] Shen P and Larter R 1995 Chaos in intracellular Ca2+
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[15] Perc M and Marhl M 2003 Different types of bursting calcium oscillations in non-excitable cells Chaos, Solitons Fractals 18 759–73
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[20] Fallah H 2016 Symmetric fold/super-Hopf bursting, chaos and mixed-mode oscillations in Pernarowski model of pancreatic beta-cells
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8
| null |
10.1016_j.isci.2021.102204.pdf
|
Data and code availability
The data that support the findings of this study and sequences were submitted to the NCBI sequence read
archive (SRA) under BioProject ID: PRJNA633714. Code for analysis is available on github repository:
https://github.com/galud27.
|
Data and code availability The data that support the findings of this study and sequences were submitted to the NCBI sequence read archive (SRA) under BioProject ID: PRJNA633714. Code for analysis is available on github repository: https://github.com/galud27 .
|
UC San Diego
UC San Diego Previously Published Works
Title
Sensitivity of the mangrove-estuarine microbial community to aquaculture effluent
Permalink
https://escholarship.org/uc/item/3229890c
Journal
iScience, 24(3)
ISSN
2589-0042
Authors
Erazo, Natalia G
Bowman, Jeff S
Publication Date
2021-03-01
DOI
10.1016/j.isci.2021.102204
Copyright Information
This work is made available under the terms of a Creative Commons Attribution-
NonCommercial-NoDerivatives License, available at
https://creativecommons.org/licenses/by-nc-nd/4.0/
Peer reviewed
eScholarship.org
Powered by the California Digital Library
University of California
iScience
ll
OPEN ACCESS
Article
Sensitivity of the mangrove-estuarine microbial
community to aquaculture effluent
Natalia G. Erazo,
Jeff S. Bowman
[email protected]
HIGHLIGHTS
In near-intact mangrove
forests, we observed the
presence of nitrogen
fixers
Calothrix could play a role
in increasing nitrogen
inventories via nitrogen
fixation
Disturbed sites were
correlated with increased
nitrogen and reduction in
diversity
Disturbed sites were
dominated by nitrifiers,
denitrifies, and sulfur-
oxidizing bacteria
Erazo & Bowman, iScience 24,
102204
March 19, 2021 ª 2021 The
Authors.
https://doi.org/10.1016/
j.isci.2021.102204
iScience
ll
OPEN ACCESS
Article
Sensitivity of the mangrove-estuarine
microbial community
to aquaculture effluent
Natalia G. Erazo1,3,4,* and Jeff S. Bowman1,2,3
SUMMARY
Mangrove-dominated estuaries host a diverse microbial assemblage that facili-
tates nutrient and carbon conversions and could play a vital role in maintaining
ecosystem health. In this study, we used 16S rRNA gene analysis, metabolic infer-
ence, nutrient concentrations, and d13C and d15N isotopes to evaluate the impact
of land use change on near-shore biogeochemical cycles and microbial community
structures within mangrove-dominated estuaries. Samples in close proximity to
3(cid:1); lower in mi-
active shrimp aquaculture were high in NH4
crobial community and metabolic diversity; and dominated by putative nitrifiers,
denitrifies, and sulfur-oxidizing bacteria. Near intact mangrove forests we
observed the presence of potential nitrogen fixers of the genus Calothrix and or-
der Rhizobiales. We identified possible indicators of aquaculture effluents such as
Pseudomonas balearica, Ponitmonas salivibrio, family Chromatiaceae, and genus
Arcobacter. These results highlight the sensitivity of the estuarine-mangrove mi-
crobial community, and their ecosystem functions, to land use changes.
(cid:1), and PO4
+, NO3
(cid:1) NO2
INTRODUCTION
Mangrove forests are among the most productive ecosystems in the world, harbor significant biodiversity,
and provide numerous ecosystem services (Ewel et al., 1998). These forests aid in the exchange of carbon
and nutrients with the coastal marine environment (Robertson et al., 2011), with an estimated export of 10%
of the marine dissolved organic matter to adjacent ecosystems (Dittmar and Lara, 2001). These forests act
as carbon sinks by sequestering CO2, help stabilize coastlines, and support coastal fisheries by acting as
nursery grounds for a range of marine species (Kathiresan and Bingham, 2001). Despite their ecological
and economic importance they have suffered severe losses in the past years (Duke et al., 2007). Although
deforestation rates have declined (Friess et al., 2020), mangrove forests are still threatened by pollution,
overextraction, conversion to aquaculture, agriculture, and the overall degradation of the environment
(Lovelock et al., 2004; Reef et al., 2010; Friess et al., 2019).
A key driver of the reduction in mangrove forest area is the expansion of shrimp aquaculture. Within
Ecuador, the expansion of aquaculture exceeds the global trend with deforestation rates higher than
80% (Hamilton and Lovette, 2015). Here, shrimp aquaculture has grown to a $1.3 billion industry by 2012
and represents the second largest component of the Ecuadorian economy after fossil fuels (Hamilton and
Lovette, 2015). Shrimp aquaculture effluent is associated with the input of excess nutrients to adjacent
coastal ecosystems; consequently, it can lead to changes in microbial community structure, biogeochemical
cycles, and eutrophication (Maher et al., 2016; Rosentreter et al., 2018). Changes in nutrient fluxes can indi-
rectly alter the redox state of the water column and sediment. This can shift mangrove forests from acting as
sinks to sources of greenhouse gases such as CO2, nitrous oxide, and methane (Maher et al., 2016).
Microorganisms (here meaning single-celled members of the domains bacteria, archaea, and eukarya) are
a key component of the mangrove forest and are present in the sediment, the water column, and as biofilms
on mangrove roots (Vazquez et al., 2000; Holguin et al., 2001). These microbes interact with mangroves as
co-dependent ecosystem engineers and are responsible for many of the biogeochemical processes attrib-
uted to mangrove forests (Holguin et al., 2006; Reis et al., 2017; Shiau and Chiu, 2020). Mangrove forest
productivity, for example, is dependent on the microbial recycling mechanisms that keep nitrogen and
1Scripps Institution of
Oceanography, UC San
Diego, 8622 Kennel Way, La
Jolla, CA 92037, USA
2Center for Microbiome
Innovation, UC San Diego, La
Jolla, CA, USA
3Center for Marine
Biodiversity and
Conservation, UC San Diego,
La Jolla, CA, USA
4Lead contact
*Correspondence:
[email protected]
https://doi.org/10.1016/j.isci.
2021.102204
iScience 24, 102204, March 19, 2021 ª 2021 The Authors.
This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
1
ll
OPEN ACCESS
iScience
Article
Table 1. Environmental properties for high, intermediate, and low disturbed mangrove forests
Disturbance
Low
Phosphate
(mM)a
0.23 G 0.23
Nitrate+nitrite
(mM)a
0.46 G 0.54
Ammonia
(mM)a
0.39 G 0.36
Chlorophyll
(mg L-1)a
11.52 G 5.86
Intermediate
0.33 G 0.33
0.87 G 0.46
1.77 G 0.60
8.80 G 2.58
High
2.41 G 1.01
9.91 G 8.75
12.79 G 7.50
p Valuef
9.10 3 1011
8.2 3 10
(cid:1)12
2.20 3 10
(cid:1)16
30.75 G
23.52
1.70 3 10
(cid:1)6
d13C
(range)b
(cid:1)18.45,
(cid:1)27.76
(cid:1)18.49,
(cid:1)29.00
(cid:1)27.01,
(cid:1)32.08
–
d15N
(range)b
0.36,
11.08
0.54, 8.84
0.73, 5.86
–
Samples
(n)c, d, e
89
34
29
–
aMean value.
bLow and high values provided.
cLow disturbance (Cayapas-Mataje = 88, Muisne = 1).
dIntermediate disturbance (Cayapas-Mataje = 33, Muisne = 1).
eHigh disturbance (Muisne = 29).
fp Value (Kruskal-Wallis test).
other nutrients within the system (Alongi, 1994). Because of the dependence of ecosystem functions on mi-
crobes, microbes can be used as sensitive indicators of environmental change and stress.
The planktonic microbial community in mangrove forests has been understudied when compared with the
sediment community (Gomes et al., 2011; Imchen et al., 2017; Zhang et al., 2017; Gong et al., 2019). In this
study, we evaluated the impact of land use change (mangrove forest converted to aquaculture) on micro-
bial community structure and key biogeochemical parameters in the water column. We tested the hypoth-
esis that shrimp aquaculture facilities are correlated with increased nitrogen inputs, altered microbial struc-
ture, and alpha diversity. We identified specific microbial taxa that were differentially present between
more and less perturbed sites associated with different levels of nutrient enrichment due to land use
change. These taxa can be further developed as indicators of perturbation and mangrove forest health.
The observed changes in the microbial community structure of the more and less disturbed sites high-
lighted the sensitivity of the mangrove forest to aquaculture effluent, with implications for coastal biogeo-
chemical cycling and carbon and nitrogen subsidies to adjacent ecosystems.
RESULTS
Physicochemical properties
(cid:1)1 for phosphate, 9.91 G 8.75 mmol L
(cid:1)1 for nitrate + nitrite, 12.79 G 7.50 mmol L
The disturbed sites (Muisne) were associated with higher levels of ammonia, nitrate + nitrite, phosphate,
and chlorophyll a near aquaculture effluent sites (Figure 1). The mean concentrations were 2.41 G
(cid:1)1 for ammonia,
1.01 mmol L
(cid:1)1 for chlorophyll a (Table 1 and Figure 2). These biogeochemical parameters were
and 30.75 G 23.52 mg L
(cid:1)6, respectively) in
significantly lower (Kruskal-Wallis test, p = 9.1 3 10
(cid:1)1 for phosphate, 0.46 G
the low disturbance forest (Cayapas-Mataje) with values of 0.23 G 0.23 mmol L
(cid:1)1 chlorophyll
0.54 mmol L
a. Areas of intermediate disturbance were found around limited aquaculture facilities where the mean con-
(cid:1)1 for nitrate + nitrite, 1.77 G
centrations were 0.33 G 0.33 mmol L
0.60 mmol L
(cid:1)1 for nitrate + nitrite, 0.39 G 0.36 mmol L
(cid:1)1 for phosphate, 0.87 G 0.46 mmol L
(cid:1)1 for ammonia, and 8.80 G 2.58 mg L
(cid:1)1 for chlorophyll (Table 1, Figure 2).
(cid:1)1 ammonia, and 11.52 G 5.86 mg L
(cid:1)16, 1.7 3 10
(cid:1)12, 2.2 3 10
(cid:1)11, 8.2 3 10
C and N isotope values ranged from (cid:1)18.45 to (cid:1)27.76&d13C in the low disturbed sites, (cid:1)18.94 to
(cid:1)29.00&d13C in the intermediate disturbed sites, and (cid:1)27.01 to (cid:1)32.08&d13C in the high disturbed sites
(Table 1, Figure 2). The d15N values ranged from 0.36 to 11.08& in the low disturbed sites, 0.54 to 8.84& in
the intermediate disturbed sites, and 0.73 to 5.86& in the high disturbed sites (Table 1, Figure 2). The N*
(cid:1)1; for low and intermediate distur-
value for the high disturbed sites ranged from (cid:1)43.68 to (cid:1)4.44 mmol L
(cid:1)1 (Figure 2). We identified higher N:P ratios associated
bance sites it ranged from (cid:1)28.10 to 0.21 mmol L
with high disturbance and lower ratios with low disturbance sites, and we observed a negative correlation
(cid:1)8) and 16S rRNA gene copy number (Spearman’s
with genome size (Spearman’s rho = (cid:1)0.46, p = 9.3 3 10
(cid:1)6) (Figure 2). The taxa most associated with smaller predicted genomes were Can-
rho = (cid:1)0.5, p = 1.7 3 10
didatus Dependentiae (1.14 Mb), Candidatus Nasuia deltocephalinicola (1.12 Mb), and Candidatus Pelagi-
bacter sp. IMCC9063 (1.28 Mb). The taxa most associated with larger predicted genomes were genera
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Figure 1. Map of study site in coastal Ecuador
(A) Study site in Esmeraldas, Ecuador, South America.
(B) Location of the two ecological reserves: Cayapas-Mataje (CM) and Muisne (M).
(C and D) (C) Map of land use changes in CM and (D) map of land use changes in M; green shows mangrove forest cover,
pink shows shrimp aquaculture cover, and yellow circles show sampling locations. The base maps were generated from
data obtained in Hamilton (2020).
Calothrix (12.05 Mb), Oscillatoria acuminata (7.80 Mb), Moorea producens PAL-8-15-08-1 (9.71 Mb), San-
daracinus amylolyticus (10.33 Mb), and Singulisphaera acidiphila (9.76 Mb).
Alpha diversity
For the bacterial community, the inverse Simpson’s indicator of diversity was significantly lower in the highly
disturbed sites when compared with the intermediate and low sites with mean G SD values of 36.08 G 26.41,
(cid:1)9) (Figure 3). The mean diversity
30.05 G 17.56, and 56.73 G 19.82 respectively, (Kruskal-Wallis, p = 3.5 3 10
for the archaeal community was 5.00 G 1.34 for high, 6.38 G 2.29 for intermediate, and 6.85 G 2.87 for low distur-
bance sites, and low and intermediate disturbance sites had significant higher diversity than high disturbance
(cid:1)6) (Figure 3). Alpha diversity for the archaeal community was lower than for
sites (Kruskal-Wallis, p = 1.4 3 10
the bacterial community. Low disturbance sites had higher diversity than intermediate disturbance sites for
the bacterial community, but no difference was observed between low and intermediate sites for the archaeal
community (Figure 3). We also evaluated the predicted metabolic diversity for the bacterial community; the
mean metabolic diversity for low disturbance was 244.01 G 8.72 (mean G SD); for intermediate disturbance,
was 235.22 G 8.02; and for high disturbance, was 237.87 G 9.29. The low disturbance sites had higher metabolic
diversity (Kruskal-Wallis, p = 2.2 3 10
(cid:1)7) when compared with intermediate and high disturbance sites.
Differentiated abundance of bacterial and archaeal communities and metabolic pathways
Unique reads are represented at the strain (closest completed genome or [CCG]) or clade level (closest
estimated genome [CEG]) depending on the point of placement by paprica. The bacterial community
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Figure 2. Biogeochemical and bacterial signatures
(A–C) (A) Nitrogen (ammonia and nitrate + nitrite) and phosphate species concentrations, (B) mean of genome size versus N:P ratio, (C) mean of number of
16S copies versus N:P ratio and Spearman’s correlation.
(D and E) (D) N* value and (E) chlorophyll values of three levels of disturbance. Kruskal-Wallis test and p values with Dunn post-test. **p < 0.01, ***p < 0.001.
(F) d13C and d15N isotopic signatures.
composition was dominated by the class Actinobacteria: Rhodoluna lacicola (CEG), Actinobacteria bacte-
rium IMCC26256 (CCG), Acidimicrobium ferrooxidans DSM 10331 (CCG); family Pelagibacteraceae: Can-
didatus Pelagibacter sp. IMCC9063 (CCG), Candidatus Puniceispirillum marinum IMCC1322 (CCG), Candi-
family Flavobacteriaceae: Kordia sp. SMS9 (CCG),
datus Pelagibacter ubique HTCC1062 (CCG);
Owenweeksia hongkongensis DSM 17368 (CCG); cyanobacteria: Synechococcus sp. WH 7803 (CCG);
and family Rhodobacteraceae: Thalassococcus sp. S3 (CCG) and Sulfitobacter sp. AM1-D1(CCG). The
archaeal community was dominated by the most abundant class Thermoplasmata: Candidatus Methano-
massiliicoccus intestinalis Issoire-Mx1 (CCG), class Methanococci: Methanococcales (CEG), and phylum
Thaumarchaeota (Figure S1).
Our DESeq2 results identified 333 amplicon sequence variants or ASVs that were significantly different between
sites separated by level of disturbance. Here we focus on the top 60 most abundant differentially present ASVs
that were significantly differentially present across our entire dataset (Figure 4). Members of Chromatiaceae bac-
(cid:1)9), genus Delf-
terium 2141T.STBD.0c.01a (CCG) (p = 2.02 3 10
(cid:1)7), Steroidobacter denitri-
tia (CEG) (p = 1.03 3 10
(cid:1)8) were the most
ficans (CEG) (p = 6.17 3 10
significantly most abundant taxa in the high disturbed site than in the low disturbed site. Cyanobacteria such as
(cid:1)29), and
M. producens PAL-8-15-08-1 (CCG) (p = 2.45 3 10
(cid:1)13), and Pseudomonas balearica DSM 6083 (CCG) (p = 2.52 3 10
(cid:1)14), Arcobacter nitrofigilis DSM 7299 (CCG) (p = 1.31 3 10
(cid:1)7), order Nostococales (CEG) (p = 7.84 3 10
(cid:1)19), family Planctomycetes (CEG) (p = 1.62 3 10
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Figure 3. Alpha diversity
(A–C) (A) Bacterial community diversity, (B) archaeal diversity, and (C) metabolic diversity for the three levels of disturbance using InvSimpson metric. Kruskal-
Wallis test and p values with Dunn post-test; ***p < 0.001.
Cyanobium gracile PCC 6307 (CCG) (p = 2.41 3 10
low disturbance sites were characterized by a higher abundance of SAR11 (CEG) (p = 2.17 3 10
dobacteraceae (CEG) (p = 2.30 3 10
yloceanibacter (CEG) (p = 1.42 3 10
(p = 9.12 3 10
othrix sp. NIES-4071 (CCG) (p = 1.79 3 10
(cid:1)38) were also more abundant in the high disturbed sites. The
(cid:1)14), family Rho-
(cid:1)40), family Flavobacteriaceae (CEG) (p = 8.26 3 10
(cid:1)28), and genus Meth-
(cid:1)8). Oscillatoria species such as Oscillatoria nigroviridis PCC 7112 (CCG)
(cid:1)7) were more abundant in the low and intermediate disturbed sites as well as cyanobacteria Cal-
(cid:1)20) (Figure 4).
For domain archaea we identified a total of seven (CEG) taxa that were the most abundant and differentially
(cid:1)13) was associated with high disturbed samples. Candi-
present. Candidatus Korarchaeota (p = 1.09 3 10
(cid:1)68), genus Meth-
datus Mancarchaeum acidiphilum (p = 4.28 3 10
(cid:1)56) were more abundant
anomassiliicoccus (p = 5.08 3 10
in low disturbed sites (Figure 4).
(cid:1)28), and genus Methanococcales (p = 3.79 3 10
(cid:1)40), genus Nitrosopumilus (p = 2.92 3 10
A correspondence analysis (CA) of bacterial and archaeal community structures depicted the dissimilar
relationship of samples for bacteria and archaea in terms of level of disturbance associated with aquacul-
ture (Figure 5). For bacteria, the first axis explained 30.6%, and the second axis, 18.3%. The top contributing
taxa to the difference were Betaproteobacteria (cos2 = 0.86), Acidothermus cellulolyticus 11B (cos2 = 0.83),
and S. denitrificans (cos2 = 0.91) (Figure 5). For the archaeal community, the first dimension accounted for
19.9% and the second dimension accounted for 11.8% of variability. Among the top contributors to the two
dimensions were class Thermoplasmata (cos2 = 0.61), Candidatus Methanomassiliicoccus intestinalis
(cos2 = 0.73), and Candidatus Mancarchaeum acidiphilum (cos2 = 0.63) (Figure 5). The results of our ANO-
SIM test showed that the bacterial and archaeal communities were significantly different for low and high
disturbance mangrove forests (R = 0.52 and p value = 0.001, R = 0.45 and p value = 0.001). We also observed
clear association of location of samples with ammonia concentration in dimension 1 (Spearman’s rho =
(cid:1)9) for bacteria, and for archaea
0.56, p = 1.4 3 10
only dimension 2 showed a significant correlation (Spearman’s rho = 0.49, p = 7.2 3 10
(cid:1)10) and dimension 2 (Spearman’s rho = 0.54, p = 1.2 3 10
(cid:1)5) (Figure S2).
A canonical correspondence analysis (CCA) was further performed to examine the relationships between
metabolic pathways and environmental factors. This showed that the biogeochemical parameters associ-
ated with nitrogen species, phosphate, N:P, chlorophyll a, and d13C and d15N together accounted for 20%
of the variability in the metabolic pathways. Nitrogen, phosphorus, and chlorophyll were factors that influ-
enced the metabolic pathways in the high disturbance sites. The first dimension accounted for 26.1%, and
the second dimension accounted for 9.1% of the variability. Here, the top contributors’ predicted meta-
bolic pathways of dimethylsulfoniopropionate (DMSP) degradation III methylation (cos2 = 0.61) and glycine
betaine (GBT) degradation I (cos2 = 0.62) were associated with low and intermediate disturbance. Taxa
associated with DMSP degradation III methylation were Candidatus Puniceispirillum marinum IMCC1322
and Thalassococcus sp. S3, and for GBT degradation, taxa were Alphaproteobacterium HIMB59, cyano-
bacteria, and Pelagibacteraceae. Other metabolic pathways with high contributions were arsenate
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Figure 4. Microbial and archaeal signatures of disturbance
(A and B) (A) Differentially abundant bacterial taxa (top 60) in high, intermediate, and low disturbance result from DESeq2
analysis; (B) differentially abundant archaeal taxa result from DESeq2. Samples and taxa were clustered using Bray-Curtis
dissimilarity distance.
detoxification (cos2 = 0.75) and methylphosphonate degradation (cos2 = 0.83), both associated with high
disturbance sites (Figure 6). Taxa associated with these pathways were Erythrobacter atlanticus and Can-
didatus Puniceispirillum marinum IMCC1322 for arsenate detoxification and Starkeya novella DSM 506 (or-
der Rizobiales) and Oceanicola sp. 3 for methylphosphonate degradation.
Weighted gene correlation network analysis
(cid:1)17, pink: r = 0.86, p = 2 3 10
(cid:1)50) Moorea producens PAL-8-15-08-01 (CCG) (r = 0.89, p = 5.18 3 10
Weighted gene correlation network analysis (WGCNA) found clusters of highly correlated taxa across samples.
We related these clusters to ammonia and nitrate + nitrite to better understand the impact of aquaculture effluent
on microbial community structure. We identified eight major modules or subnetworks. Each module was as-
signed a particular color (Figure S3). The blue and pink modules were positively correlated with ammonia and
(cid:1)43). The yellow module was negatively
nitrate + nitrite (blue: r = 0.64, p = 6.00 3 10
(cid:1)6) (Figure S3). Taxa associated with the pink
correlated with ammonia, nitrate, and nitrite (r = (cid:1)0.42, p = 6.00 3 10
(cid:1)53), Actinobacteria bacterium
module (Figure S4) included Sulfurivermis fontis (CEG) (r = 0.90, p = 1.45 3 10
(cid:1)53), Candidatus Methylopumilus planktonicus (CEG) (r = 0.89, p =
IMCC26256 (CCG) (r = 0.90, p = 9.62 3 10
(cid:1)50), Phycisphaera mikurensis
1.98 3 10
(cid:1)30), and
NBRC 102666 (r = 0.85, p = 1.19 3 10
(cid:1)30). All these taxa were significantly correlated with
Steroidobacter denitrificans (CEG) (r = 0.79, p = 2.31 3 10
ammonia, and with nitrate + nitrite (Table 2). Taxa most strongly associated with the blue module consisted of
(cid:1)8), A. cellulolyticus 11B (CCG) (r = 0.69, p =
C. bacterium 2141T.STBD.0c.01a (CCG) (r = 0.49, p = 8.88 3 10
(cid:1)14), Pontimonas salivibrio (CEG) (r = 0.59, p =
3.37 3 10
(cid:1)20) (Table 2, Figure S4). The taxa
1.52 3 10
that were most negatively correlated with ammonia in the yellow module were: O. acuminata PCC 6304 (CCG)
(cid:1)8), Candidatus pelagi-
(cid:1)3, Synechococcus sp. WH 7803 (CCG) (r = (cid:1)0.49, p = 4.25 3 10
(r = (cid:1)0.34, p = 9.57 3 10
(cid:1)7), and Coraliomargarita akajimensis DSM 45221 (CCG) (r =
bacter sp. IMCC9063 (CCG) (r = (cid:1)0.37, p = 1.17 3 10
(cid:1)0.36, p = 7.51 3 10
(cid:1)20), S. denitrificans (CEG) (r = 0.61, p = 3.62 3 10
(cid:1)15), M. producens PAL-8-15-08-01 (CCG) (r = 0.69, p = 5.07 3 10
(cid:1)40), Cyanobium gracile PCC 6307 (CCG) (r = 0.78, p = 7.76 3 10
(cid:1)6) (Table 2, Figure S4).
We further explored taxa that correlated with salinity to better understand the impact of tide on the micro-
(cid:1)8)
bial community structure. The red module was positively correlated with salinity (r = 0.47, p = 7.00 3 10
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Figure 5. Bacterial and archaeal community structure
(A–E) Correspondence analysis (CA) ordination of (A) the bacterial community for samples that cluster in ordination space
have similar community compositions, whereas those that are dispersed are less similar. (B) Square cosine components
for samples; large value of cos2 shows a relatively large contribution to the total distance for bacterial community. (C) CA
ordination for archaeal community. (D) Square cosine components for samples for archaeal community. (E) Contribution
of top 10 taxa with highest cos2 values for archaeal community (see Figure S2).
(Figure S3). Taxa associated with the red module included Acidimicrobium ferrooxidans DSM 10331 (CCG)
(cid:1)9), Synechococcus sp.
(cid:1)10), Haliglobus japonicus (CEG) (r = 0.52, p = 2.66 3 10
(r = 0.53, p = 8.19 3 10
(cid:1)8), Candidatus Puniceispirillum marinum IMCC1322 (CCG)) (r =
CC9605 (CCG) (r = 0.50, p = 2.28 3 10
0.47, p = 4.56 3 10
(cid:1)7), and Prochlorococcus marinus str. MIT 9301 (r = 0.40, p = 1.98 3 10
(cid:1)4) (Table 3).
We analyzed the Hellinger-transformed enzyme level output from paprica to better understand the enzy-
matic potential of those CEG and CCG that were correlated with ammonia. We found 35 enzymes associ-
ated with the nitrogen cycle (Figure 6). The enzyme nitrogenase EC 1.18.6.1 had a mean value of 0.23 G
0.05 for the low disturbed sites, significantly higher than that in the intermediate (0.17 G 0.06) and high
(cid:1)10) (Figure S5). Nitrate reductase EC 1.7.99.4 had a mean value
(0.17 G 0.05) disturbance sites (p = 1.2 3 10
of 0.23 G 0.05 for low disturbance site, 0.45 G 0.14 for intermediate disturbance site, and 0.44 G 0.13 for
high disturbance site, and the nitrate reductase value was significantly higher in the high disturbance sites
(cid:1)14). The same was observed with nitrate reductase NADH EC 1.7.1.4 with a mean of 0.13 G
(p = 8.7 3 10
0.05 for low disturbed sites, 0.23 G 0.14 for intermediate disturbance, and 0.23 G 0.13 for highly disturbed
(cid:1)15) (Figures 6 andS5). The taxa that were associated with nitrogenase were Methylocella
sites (p = 2 3 10
silvestris BL2, genus Calothrix, and Synechococcus sp. CC9605. For nitrate reductase members of the Be-
taproteobacteria, Desulfococcus oleovorans Hxd3, and P. mikurensis NBRC 102666 were found to
contribute to enzyme abundance. The taxa that were associated with nitrate reductase NADH were
A. cellulolyticus 11B and members of the Rhodobacteraceae (Table 4).
DISCUSSION
Mangrove forests are experiencing a high degree of perturbation through nutrient enrichment, pollution,
and deforestation. Shrimp aquaculture effluent in particular is associated with the input of excess nutrients
to mangrove forests. In this study we found that shrimp aquaculture effluent is associated with changes in
microbial community structure with likely consequences for biogeochemical cycles and mangrove forest
health. Previous work suggests that for intensive shrimp farming, 2.22 km2 of mangrove forest is required
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Figure 6. Metabolic pathways and nitrogen cycle enzyme indicators for levels of disturbance
(A) CCA ordination for metabolic pathways showing top four pathways with cos2 ranging from 0.6–0.8. Large value of cos2
shows a relatively large contribution to the total distance for bacterial metabolic prediction.
(B) Heatmap of key nitrogen cycle enzymes (Bray-Curtis distance) for the bacterial community (see Figure S5).
to remove effluent from one pond of 0.01 km2, whereas 0.20 km2 is required for less-intensive farming from
one pond of 0.01 km2 (Robertson and Phillips, 1995). As of 2014 in the Muisne region there were 20.47 km2
of shrimp farms and 12.06 km2 of mangrove forests, indicative of an intensive farming system. Cayapas-
Mataje had 11.04 km2 of shrimp aquaculture farms and 302.05 km2 of mangrove forest, suggesting less
intensive farming (Figure 1) (Hamilton, 2020). As the areal extent of shrimp aquaculture increases so
does the volume of the effluent, elevating the flux of ammonia and nitrate to the surrounding ecosystem.
Based on our observations we found that microbial communities in mangrove forests are significantly
altered by this perturbation.
The bacterial communities in our mangrove systems were characterized by members of the Pelagibacter-
aceae, Flavobacteriaceae, Rhodobacteraceae, Actinobacteria, and cyanobacteria (Figure 4, Figure S1).
The archaeal community was dominated by members of the Thermoplasmata, Thaumarchaeota, and
Methanococcales (Figure 4, Figure S1). This was in accordance with other studies that have identified
Rhodobacteraceae, SAR86 clade, Actinobacteria, and Flavobacteriaceae, and Thaumarchaeota as the
most abundant taxonomic groups (Dhal et al., 2020). Rhodobacteraceae has been found to be dominant
in mangrove-dominated estuaries, and members of this family are associated with marine phytoplankton
blooms where they play a role in transformations of derived phytoplankton organic matter (Ghosh et al.,
2010; Simon et al., 2017). The presence of Actinobacteria has been documented previously in mangrove
ecosystems (Azman et al., 2015; Gong et al., 2019), and it has been suggested that they could play a role
in carbon cycling by decomposing the plant biomass including refractory lignins (Scott et al., 2010). Thau-
marchaeota are the most abundant archaea in the surface ocean (Santoro et al., 2015), and Thermoplas-
mata have been found in mangrove ecosystems (Zhang et al., 2019). Both these groups play an important
role in the nitrogen cycle by carrying out the oxidation of ammonia in nitrification (Santoro et al., 2015;
Zhang et al., 2019).
Both bacterial and archaeal communities were less diverse at our more disturbed sites. This pattern
extended to predicted metabolic diversity (Figure 3). We hypothesize that this reduction in diversity could
cause reductions in ecosystem functions. This has been observed in previous mangrove forest studies, for
example, where lower microbial diversity was associated with a reduction in microbial productivity in sites
with high levels of deforestation, sewage, and fishing activities (Carugati et al., 2018).
Our results showed differences in biogeochemical parameters between sites at varying levels of distur-
bance (Figure 2). In particular, nitrogen was a driver of the microbial community structure leading to segre-
gation into three clusters of disturbance in the CA analysis based on our ANOSIM test and significantly
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Table 2. Significant correlated taxa with ammonia and nitrate+nitrite result from WGCNA
Taxon
Thermogutta terrifontisf
Acidothermus cellulolyticus 11B
Oceanicola sp. D3
Moorea producens PAL-8-15-08-1
Moorea producens PAL-8-15-08-1
Actinobacteria bacterium IMCC26256
Steroidobacter denitrificans
Aureitalea sp. RR4-38
Pontimonas salivibrio
Pontimonas salivibrio
Acidothermus cellulolyticus 11Bf
Candidatus Xiphinematobacter sp. Idaho
grape
Synechococcus sp. CB0101
Candidatus Cyclonatronum proteinivorum
Candidatus Cyclonatronum proteinivorum
Halioglobus pacificus
Synechococcus sp. WH 8101
Rhodoluna lacicola
Actinobacteria bacterium IMCC26256
Thiohalobacter thiocyanaticus
Actinobacteria bacterium IMCC26256
Chromatiaceae bacterium 2141T.STBD.0c.01a
Wenzhouxiangella marina
Thiolapillus brandeum
Candidatus Puniceispirillum marinum
IMCC1322
Thermogutta terrifontis
Candidatus Pelagibacter sp. IMCC9063
Sulfurivermis fontisd
Actinobacteria bacterium IMCC26256
Candidatus Methylopumilus planktonicus
Moorea producens PAL-8-15-08-1
Owenweeksia hongkongensis DSM 17368
Phycisphaera mikurensis NBRC 102666e
Thermogutta terrifontis
Candidatus Planktophila vernalis
Actinobacteria bacterium IMCC26256
Candidatus Xiphinematobacter sp. Idaho
grape
Candidatus Pelagibacter sp. IMCC9063
Owenweeksia hongkongensis DSM 17368
Syntrophus aciditrophicus SB
Candidatus Pelagibacter sp. IMCC9063
Phycisphaera mikurensis NBRC 102666e
Map IDa Module color GS.Nitrogenb
0.87
0.94
0.97
0.82
0.82
0.88
0.91
0.92
0.98
0.98
0.94
0.88
0.98
0.87
0.87
565
0.98
0.98
0.88
0.92
0.88
0.95
0.98
0.94
0.97
0.87
0.91
0.86
0.88
0.96
0.82
0.89
0.8
0.87
0.95
0.88
0.88
0.91
0.89
0.84
0.92
0.8
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Blue
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
0.74
0.69
0.69
0.69
0.67
0.62
0.61
0.61
0.59
0.59
0.58
0.58
0.58
0.57
0.56
0.56
0.54
0.53
0.53
0.51
0.50
0.49
0.48
0.45
0.45
0.44
0.40
0.90
0.90
0.89
0.89
0.87
0.85
0.85
0.85
0.84
0.83
0.82
0.81
0.80
0.79
0.79
p.GS.Nitrogenc
6.35 3 10
3.37 3 10
(cid:1)25
(cid:1)20
4.17 3 10
5.07 3 10
2.62 3 10
8.57 3 10
3.62 3 10
5.70 3 10
5.75 3 10
1.52 3 10
1.29 3 10
(cid:1)20
(cid:1)20
(cid:1)18
(cid:1)15
(cid:1)14
(cid:1)14
(cid:1)13
(cid:1)15
(cid:1)12
1.80 3 10
(cid:1)12
3.36 3 10
9.00 3 10
2.06 3 10
2.19 3 10
3.96 3 10
(cid:1)12
(cid:1)12
(cid:1)11
(cid:1)11
(cid:1)10
1.58 3 10
1.60 3 10
(cid:1)9
(cid:1)9
1.94 3 10
9.01 3 10
(cid:1)12
(cid:1)12
8.88 3 10
1.48 3 10
2.19 3 10
3.59 3 10
(cid:1)8
(cid:1)7
(cid:1)6
(cid:1)6
4.27 3 10
1.29 3 10
(cid:1)6
(cid:1)4
1.45 3 10
9.62 3 10
(cid:1)53
(cid:1)53
1.98 3 10
5.18 3 10
4.75 3 10
1.19 3 10
2.24 3 10
9.07 3 10
1.34 3 10
(cid:1)50
(cid:1)50
(cid:1)46
(cid:1)40
(cid:1)40
(cid:1)40
(cid:1)39
7.44 3 10
(cid:1)37
1.31 3 10
(cid:1)34
3.97 3 10
3.58 3 10
1.73 3 10
1.89 3 10
(cid:1)33
(cid:1)32
(cid:1)31
(cid:1)30
(Continued on next page)
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Table 2. Continued
Taxon
Steroidobacter denitrificans
Cyanobium gracile PCC 6307
Cyanobium gracile PCC 6307
Halioglobus japonicus
Halomicronema hongdechloris C2206
Thermogutta terrifontis
Marinifilaceae bacterium SPP2
Steroidobacter denitrificans
Aureitalea sp. RR4-38
Halioglobus pacificus
Synechococcus sp. WH 7803
Candidatus Methylopumilus planktonicus
Flavobacteriaceae bacterium
Thiolapillus brandeum
Owenweeksia hongkongensis DSM 17368
Thermogutta terrifontis
Candidatus Pelagibacter sp. IMCC9063
Coraliomargarita akajimensis DSM 45221
Oscillatoria acuminata PCC 6304
Acidothermus cellulolyticus 11Bf
Map IDa Module color GS.Nitrogenb
0.91
0.98
0.98
0.91
0.9
0.87
0.85
0.91
0.92
0.94
0.99
0.96
0.91
0.94
0.89
0.87
0.92
0.89
0.81
0.94
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Pink
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
Yellow
0.79
0.78
0.72
0.56
0.53
0.53
0.47
0.40
(cid:1)0.57
(cid:1)0.50
(cid:1)0.49
(cid:1)0.47
(cid:1)0.45
(cid:1)0.42
(cid:1)0.39
(cid:1)0.38
(cid:1)0.37
(cid:1)0.36
(cid:1)0.34
(cid:1)0.34
p.GS.Nitrogenc
2.31 3 10
(cid:1)30
7.76 3 10
2.75 3 10
2.91 3 10
7.85 3 10
9.21 3 10
3.13 3 10
1.07 3 10
4.73 3 10
1.58 3 10
4.25 3 10
4.55 3 10
2.36 3 10
3.22 3 10
2.45 3 10
7.07 3 10
1.17 3 10
2.84 3 10
6.15 3 10
9.57 3 10
(cid:1)30
(cid:1)23
(cid:1)11
(cid:1)10
(cid:1)10
(cid:1)7
(cid:1)4
(cid:1)12
(cid:1)8
(cid:1)8
(cid:1)7
(cid:1)6
(cid:1)5
(cid:1)4
(cid:1)4
(cid:1)3
(cid:1)3
(cid:1)3
(cid:1)3
aMap ID phylogenetic classification. Value = 1 represents a perfect placement on the tree.
bGS = Pearson correlation to ammonia and nitrate + nitrite.
cp.GS = p-adjusted value (Bonferroni correction) for correlation to ammonia and nitrate+nitrite.
dRepresents presence of nitrogenase enzyme EC.1.18.61.
eRepresents presence of nitrate reductase enzyme EC.1.7.99.4.
fRepresents presence of nitrate reductase enzyme EC.1.7.1.4.
correlated with ammonia concentrations (Figure 5, Figure S2). We note that the variance explained by the
first and second dimensions in our ordination analyses is relatively low (30.6% and 19.9% for the bacterial
and archaeal communities, respectively). We attribute this to the complexity associated with the mangrove
ecosystem and the large number of physical, chemical, and biological factors that could impact changes in
the microbial community.
We found a strong connection between N:P ratio and genome size among planktonic bacteria across study
sites (Figure 2). Generally, smaller predicted genomes and lower 16S rRNA gene copy number was asso-
ciated with higher N:P ratios, whereas larger predicted genomes and higher 16S rRNA gene copy number
was associated with lower N:P ratios. The differences in genome sizes between communities associated
with different levels of disturbance suggest differing ecological strategies. Studies suggest that generalists
possess larger genomes in contrast to the smaller genomes in more specialized microbes (Sriswasdi et al.,
2017; Willis and Woodhouse, 2020). This falls from the generalist requirement for a larger gene repertoire
to boost activity in multiple environmental conditions and to cope with different stressors associated with a
broad physicochemical niche (such as low levels of nitrogen and tidal fluctuations in mangrove-dominated
estuaries). The low disturbance sites showed a higher metabolic diversity and larger genomes, which we
interpret as a more generalist microbial community. Taxa with larger genomes included Planctomycetes
such as Singulisphaera acidiphila. This taxon has been found in other wetland ecosystems (Kulichevskaya
et al., 2008; Dedysh and Ivanova, 2019), and it has been shown to play an important role in degradation of
plant-derived polymers such as pectin and xylan (Dedysh and Ivanova, 2019). The S. acidiphila genome en-
codes several dozen proteins that do not belong to any of the currently carbohydrate-active enzymes, but
the enzymes display a distant relationship to glycosyltransferases and carbohydrate esterases, suggesting
that this taxon has a diverse glycolytic and carbohydrate metabolic potential (Dedysh and Ivanova, 2019).
Other taxa included Sandaracinus amylolyticus. This taxon has been found in association with plant
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Table 3. Significant correlated taxa with salinity result from WGCNA
Taxon
Acidimicrobium ferrooxidans DSM 10331
Kordia sp. SMS9
Halioglobus japonicus
Synechococcus sp. CC9605
Synechococcus sp. RCC307
Candidatus Puniceispirillum marinum
IMCC1322
Salipiger profundus
Halioglobus pacificus
Roseovarius mucosus
Acidimicrobium ferrooxidans DSM 10331
Candidatus Pelagibacter ubique HTCC1062
Owenweeksia hongkongensis DSM 17368
Prochlorococcus marinus str. MIT 9301
Synechococcus sp. KORDI-100
Sulfurivermis fontis
Map IDa Module color
GS.Salinityb
0.94
0.91
0.93
1.00
1.00
0.98
0.82
0.95
0.96
0.82
1.00
0.89
1.00
1.00
0.87
Red
Red
Red
Red
Red
Red
Red
Red
Red
Red
Red
Red
Red
Red
Red
0.53
0.53
0.52
0.50
0.47
0.47
0.46
0.46
0.44
0.41
0.40
0.40
0.40
0.39
0.39
aMap ID phylogenetic classification. Value = 1 represents a perfect placement on the tree.
bGS = Pearson correlation to salinity.
cp.GS = p-adjusted value (Bonferroni correction) for correlation to salinity.
p.GS.Salinityc
8.19 3 10
1.49 3 10
(cid:1)10
(cid:1)9
2.66 3 10
2.28 3 10
4.36 3 10
4.56 3 10
8.37 3 10
1.02 3 10
7.04 3 10
9.08 3 10
1.10 3 10
1.64 3 10
(cid:1)9
(cid:1)8
(cid:1)7
(cid:1)7
(cid:1)7
(cid:1)6
(cid:1)6
(cid:1)5
(cid:1)4
(cid:1)4
1.98 3 10
2.07 3 10
3.93 3 10
(cid:1)4
(cid:1)4
(cid:1)4
residues (Mohr et al., 2012), in coral ecosystems (Rubio-Portillo et al., 2016), and it is known to survive in
poor nutrient conditions by developing desiccation-resistant spores (Mohr et al., 2012).
We also observed larger genomes in cyanobacteria including members of the genus Calothrix, genus Os-
cillatoria, and M. producens PAL-8-15-08-1. Cyanobacteria are known to have large genomes with low cod-
ing density and a high level of gene duplication; it has been proposed that the large non-protein-coding
sequences contribute to the genome expansion and metabolic flexibility observed in diazotrophs (nitrogen
fixers) that are associated with nitrogen-limited environments (Sargent et al., 2016). The high diversity of
cyanobacteria observed in mangrove ecosystems suggests that they play a key role in the ecosystem. Rele-
vant functions associated with cyanobacteria include nitrogen and carbon fixation and the production of
herbivory-defense molecules and plant growth-promoting substances (Alvarenga et al., 2015).
In the disturbed sites the parasite C. Dependentiae accounted for much of the decrease in genome size.
Studies have found that C. Dependentiae infects a wide range of protists, including heterotrophs and
phytoplankton (Deeg et al., 2019). Other studies have shown that C. Dependentiae is associated with
free-living ameba, suggesting that it could be an endosymbiont (Delafont et al., 2015). C. Dependentiae
has very limited metabolic capability, lacks complete biosynthetic pathways for various essential cellular
building blocks, and has protein motifs to facilitate eukaryotic host interactions (Yeoh et al., 2016; Deeg
et al., 2019). C. Nasuia deltocephalinicola was also identified as having a small genome. C. Nasuia delto-
cephalinicola is an obligate symbiont of plant phloem-feeding pest insects, and its main role is to provide
essential amino acids that the host can neither synthesize nor obtain in sufficient quantities from a plant diet
(Bennett and Moran, 2013).
The increase in the concentration of nitrogen species associated with aquaculture effluent could further
select for specialist microbes with reduced metabolic potential and lower diversity in nitrogen-processing
enzymes. Our nitrogen isotope values are consistent with this, showing reduced variability for the highly
disturbed sites (Table 1, Figure 2). Previous work in mangrove systems (Bernardino et al., 2018) associated
reduced isotopic variability with a loss of trophic diversity. Higher variability in stable carbon isotopes has
also been observed in salt marshes due to contribution dominated by allochthonous material derived from
the phytoplankton community (Boschker et al., 1999). The larger variation in the isotopic signal observed in
the low and intermediate disturbance sites suggests that these pristine systems contain a more diverse
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Table 4. Number of enzymes copies for nitrogenase and nitrate reductase enzymes and top 10 associated taxa
Taxon
Methylocella silvestris BL2
Genus Calothrix
Synechococcus sp. CC9605
Family Rhodobacteraceae
Oscillatoria nigroviridis PCC 7112
Acidothermus cellulolyticus 11B
Phycisphaera mikurensis NBRC 102666
Rhodopirellula baltica SH 1
Desulfococcus oleovorans Hxd3
Class Betaproteobacteria
Nitrogenase EC.1.18.6.1 Nitrate reductase EC.1.7.99.4 Nitrate reductase NADH EC.1.7.1.4
16,984
15,186
38,937
0
0
0
0
0
0
0
4,246
3,796
0
0
5,418
0
8,288
10,956
4,773
17,102
0
0
0
1,273
5,418
23,205
0
21,912
0
0
trophic food web as result of a wide range of metabolic and fixation pathways, and environmental condi-
tions in the mangrove-estuarine ecosystem (Boschker and Middelburg, 2002).
The low N:P ratios we observed in the low disturbance sites suggest that the system is N limited. Pristine
mangrove forests tend to be N limited, although nutrients are not uniformly distributed within the
mangrove ecosystem and they can switch from N to P limitation. It has been shown that mangrove trees
within fringe and tidally exposed zones tend to be N limited (Feller et al., 2003). One way mangrove trees
cope with N limitation is through associations with diazotrophs that play a crucial role in N cycling within the
mangrove forest (Holguin et al., 1992). Here we showed that the biological nitrogen fixation signal,
confirmed by the N* value (the linear combination of nitrate and phosphate that eliminates the effect of
nitrification; thus, the remaining variability can be explained by nitrogen fixation and denitrification)
(Gruber and Sarmiento, 1997) and nitrogenase EC.1.18.6.1 abundance, were higher at low disturbance sites
in contrast to high disturbance sites (Figures 2, 6, and S5). The microbial denitrification signal was further
confirmed by negative N* values in the highest disturbance sites (Figure 2) (Gruber and Sarmiento, 1997).
Because excess nitrate is being introduced into the system via aquaculture effluent, we expect denitrifica-
tion rates to be high. Conversely, the lowest disturbance sites have a slight positive N* consistent with our
identification of putative diazotrophs such as genus Calothrix, genus Oscillatoria, and taxa of the order Rhi-
zobiales such as M. silvestris (Essien et al., 2008; Liu et al., 2019).
GBT degradation I was one of the major pathways contributing to the differences observed between low
and high disturbed sites (Figures 6 and S3). GBT is an important source of nitrogen in oligotrophic systems,
acts as an organic osmolyte, and plays an important role in phytoplankton-bacteria interactions (Becker
et al., 2019; Jones et al., 2019; Zecher et al., 2020). The intertidal coastal mangrove ecosystem experiences
daily fluctuations in a range of environmental conditions, including water levels and salinity. Organisms
living in this dynamic environment cope with changing environmental conditions by synthesizing a range
of organic and inorganic osmolytes including GBT. The results from WGCNA showed that Pelagibactera-
ceae taxa correlated with salinity (Table 3) and primary contributors of the GBT degradation I pathway. This
suggests that osmolyte production is an important adaptation to salinity intrusions from oceanic waters
into the mangrove environment, and GBT could be an additional pool of organic N within this system.
Shrimp aquaculture impacts the water quality in adjacent mangrove forests by creating eutrophic condi-
tions that can lead to anoxia. Eutrophic conditions were evident through high levels of nutrients and chlo-
rophyll a (Figure 2, Table 1). Although we did not measure oxygen concentrations, we observed taxa indic-
ative of hypoxic or anoxic conditions. These included purple sulfur bacteria (PSB), such as family
Chromaticeae, and sulfur-oxidizing bacteria (SOB), such as genus Sulfurivermis (Figure 4, Table 2). PSB
use sulfide, elemental sulfur, and thiosulfate as electron donors in anoxygenic photosynthesis and have
been shown to play an important role in regime shifts from oxygenated to anoxic conditions (Diao et al.,
2018). PSB flourish in micro-aerobic conditions oxidizing sulfide into sulfate (Diao et al., 2018). As the oxy-
gen influx is reduced below a critical threshold, sulfate-reducing bacteria (SRB) and PSB can take over and
outcompete the SOB. This suggests a more anoxic regime in the high disturbance site, allowing for PSB
groups and SRB to become more abundant.
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Based on our WGCNA analysis we also found nitrate-reducing bacteria (NRB)—indicative of reduced ox-
ygen availability—that strongly correlated with the level of ammonia, nitrate, and nitrite. Putative NRB
taxa included P. mikurensis and S. denitrificans (Table 2). In addition, we also saw a microbial signature
associated with dissimilatory nitrate reduction to ammonium (DNRA) with the presence of genus Acido-
thermus, and anaerobic ammonium oxidation (annamox) with the presence of Planctomycetes (Thermo-
gutta terrifontis) (Table 2); the presence of the genes involved in these pathways (denitrification, annamox,
DNRA) were inferred by paprica, although further work is needed to confirm the presence and activity of
these enzymes. Overall, as nitrate and ammonia inputs increased with aquaculture effluent the relative
abundance of NRB increased.
We identified specific microbes that can be used as sensitive indicators of aquaculture impacts. These
included P. balearica (Figure 4), which has been associated with other contaminated wetland systems, sug-
gesting that this taxon could be a potential bio-indicator of a disturbed mangrove ecosystem (Salva` -Serra
et al., 2017). Similar studies have also identified aquaculture effluent as a source of pathogens to the coastal
ecosystem (Garren et al., 2009). In the disturbed site we saw the presence of members of the genus Arco-
bacter (Figure 4). These bacteria have been identified in coral systems exposed to aquaculture effluents,
and have been associated with feces (human, porcine, and bovine) and with sewage-contaminated waters
(Garren et al., 2009). PSB taxa such as family Chromaticeae have also been shown to be potential bio-in-
dicators for anthropogenic contamination associated with other agriculture effluent systems (Mohd-Nor
et al., 2018). P. salivibrio in the order Micrococcales was elevated at the disturbed sites. This taxon has
been isolated from high-salinity systems and aquaculture farms (Jang et al., 2013); high salinity levels
have been associated with shrimp aquaculture effluent due to high evaporation in the ponds (Barraza-
Guardado et al., 2013). Previous studies have shown that taxa in the Micrococcales order are part of the
core microbiome signal in shrimp ponds (Chen et al., 2017). Thus, P. salivibrio is a sensible indicator of
shrimp aquaculture effluent. Further work is needed to establish robust spatiotemporal baselines of micro-
bial indicators of aquaculture to effectively monitor biogeochemical changes and health of the mangrove
forests.
Aquaculture could impact the health of mangrove ecosystems involving the direct loss of mangrove forests,
effluent associated with high levels of nutrients, and the development of anoxic and sulfuric water condi-
tions (Robertson and Phillips, 1995). Aquaculture effluent released into mangrove forests may be seques-
tered and processed by bacteria. However, processing efficiency could change with increasing input. High
organic loadings, for example, may shift the balance from aerobic to anaerobic systems (Lønborg et al.,
2020). Anaerobic systems are less efficient in nutrient cycling. The signals of SOB, SRB, denitrifiers, and po-
tential pathogenic taxa associated with the perturbed site suggest that aquaculture effluent is playing a
role in shifting the microbial community to a more pathogenic and less nutrient efficient community that
could impact the health of the mangrove forest.
Conclusion
In this study, we showed the impacts of aquaculture effluent on the microbial community structure in
mangrove forests and identified microbial signals associated with NRB, PSB, and SRB taxa that could
have impacts in nutrient cycling. The high level of nutrients in the perturbed sites were associated with
changes in microbial community structure that could impact ecosystem functions. In the low disturbance
sites, we saw that the presence of Calothrix species and nitrogen fixers could be important in increasing
nitrogen inventories via nitrogen fixation. Denitrification reduces excess inorganic nitrogen concentration,
and in the highly disturbed sites we saw the presence of NRB-associated microbes. Nutrient cycling in
mangrove habitats is a balance between nutrient inputs, availability, and internal cycling, and the changes
in microbial community structure we see in disturbed sites could be indicators of biogeochemical changes.
The results of the study highlight the sensitivity of the mangrove-estuarine microbial community to aqua-
culture effluent, and the impacts of land use changes could be amplified by climate change such as chang-
ing precipitation patterns, heat, and rising sea level with severe consequences for the ecosystem.
Limitations of the study
Our analysis was based on comparison between sites of low, intermediate, and high disturbance in two
mangrove systems in coastal Ecuador. Although ammonia concentration is a good proxy for disturbance
from shrimp aquaculture effluent, quantification of land use changes, and the hydrological connections be-
tween aquaculture facilities and our sampling sites was beyond the scope of the current work. We
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considered salinity, macronutrient concentrations, and isotopes in our analysis, but anticipate that other
variables not considered here are contributing to differences in microbial community structure. These
include physical processes such as tides and hydrology. The complexity of these environments is evident
in our CCA and CA analyses, which capture a relatively small amount of variability in the first two dimensions
(see discussion section). Other limitations of note are typical of microbial community structure analyses.
These include primer bias and a dependence on relative rather than absolute abundance.
Resource availability
Lead contact
Further information and requests for resources should be directed to and will be fulfilled by the lead con-
tact, Natalia Erazo ([email protected]).
Materials availability
This study did not generate new unique reagents.
Data and code availability
The data that support the findings of this study and sequences were submitted to the NCBI sequence read
archive (SRA) under BioProject ID: PRJNA633714. Code for analysis is available on github repository:
https://github.com/galud27.
METHODS
All methods can be found in the accompanying Transparent methods supplemental file.
SUPPLEMENTAL INFORMATION
Supplemental information can be found online at https://doi.org/10.1016/j.isci.2021.102204.
ACKNOWLEDGMENTS
N.G.E. was supported by Organization of American States and SENESCYT fellowships. J.S.B. was sup-
ported by a grant from the Simons Foundation Early Career Investigator in Marine Microbiology program.
We would like to thank Jesse Wilson and Avishek Dutta for helpful discussion on methods and interpreta-
tion, Jesse Estacio for field work assistance, and Fernando Rivera for assistance with logistics and permits.
Samples were collected under the Ecuador environmental permit (MAE-UAFE-DPAE-2017-2009-E). We
would like to thank the platform (mindthegraph.com) used here to create the graphical abstract.
AUTHOR CONTRIBUTIONS
Conceptualization, N.G.E. and J.S.B.; Methodology, N.G.E. and J.S.B; Investigation, N.G.E. and J.S.B;
Writing – Original Draft, N.G.E.; Writing – Review & Editing, J.S.B.; Funding Acquisition and Supervision,
J.S.B.
DECLARATION OF INTERESTS
The authors declare no competing interests.
Received: July 30, 2020
Revised: September 25, 2020
Accepted: February 15, 2021
Published: March 19, 2021
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16
iScience 24, 102204, March 19, 2021
iScience, Volume 24
Supplemental information
Sensitivity of the mangrove-estuarine
microbial community
to aquaculture effluent
Natalia G. Erazo and Jeff S. Bowman
A
B
Disturbance
high
intermediate
low
1
0.8
0.6
0.4
0.2
0
Disturbance
Coraliomargarita akajimensis DSM 45221
Candidatus Carsonella ruddii
Candidatus Pelagibacter sp. IMCC9063
Thiolapillus brandeum
Synechococcus sp. WH 7803
Synechococcaceae
Candidatus Dependentiae
Candidatus Pelagibacter ubique HTCC1062
Acidimicrobium ferrooxidans DSM 10331
Pelagibacteraceae
Kordia sp. SMS9
Bacteria <prokaryotes>
Flavobacteriaceae bacterium
Candidatus Methylopumilus planktonicus
Synechococcus sp. CC9605
Geminocystis
Sulfurivermis fontis
Cyanobacteria
Cyanobacteria
Candidatus Vesicomyosocius okutanii HA
Chromatiaceae bacterium 2141T.STBD.0c.01a
Actinobacteria bacterium IMCC26256
Thalassococcus
Thalassococcus sp. S3
Celeribacter indicus
Flavobacteriaceae
Owenweeksia hongkongensis DSM 17368
Pelagibacteraceae
Sulfitobacter sp. AM1−D1
Owenweeksia hongkongensis DSM 17368
Rhodoluna lacicola
Pelagibacteraceae
Candidatus Pelagibacter sp. IMCC9063
Candidatus Methylopumilus planktonicus
Candidatus Puniceispirillum marinum IMCC1322
alpha proteobacterium HIMB59
Sulfurivermis fontis
Roseovarius mucosus
Halioglobus pacificus
Acidimicrobium ferrooxidans DSM 10331
Disturbance
high
intermediate
low
1
0.8
0.6
0.4
0.2
0
Disturbance
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:3)(cid:49)(cid:76)(cid:87)(cid:85)(cid:82)(cid:86)(cid:82)(cid:83)(cid:88)(cid:80)(cid:76)(cid:79)(cid:88)(cid:86)(cid:3)(cid:68)(cid:71)(cid:85)(cid:76)(cid:68)(cid:87)(cid:76)(cid:70)(cid:88)(cid:86)
(cid:55)(cid:75)(cid:68)(cid:88)(cid:80)(cid:68)(cid:85)(cid:70)(cid:75)(cid:68)(cid:72)(cid:82)(cid:87)(cid:68)
(cid:39)(cid:76)(cid:68)(cid:73)(cid:82)(cid:85)(cid:68)(cid:85)(cid:70)(cid:75)(cid:68)(cid:72)(cid:68)
(cid:55)(cid:75)(cid:68)(cid:88)(cid:80)(cid:68)(cid:85)(cid:70)(cid:75)(cid:68)(cid:72)(cid:82)(cid:87)(cid:68)
(cid:55)(cid:36)(cid:38)(cid:46)(cid:3)(cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:48)(cid:72)(cid:87)(cid:75)(cid:68)(cid:81)(cid:82)(cid:80)(cid:76)(cid:70)(cid:85)(cid:82)(cid:69)(cid:76)(cid:68)(cid:79)(cid:72)(cid:86)
(cid:55)(cid:36)(cid:38)(cid:46)(cid:3)(cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:55)(cid:36)(cid:38)(cid:46)(cid:3)(cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:55)(cid:36)(cid:38)(cid:46) (cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:55)(cid:36)(cid:38)(cid:46) (cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:55)(cid:36)(cid:38)(cid:46) (cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:55)(cid:75)(cid:68)(cid:88)(cid:80)(cid:68)(cid:85)(cid:70)(cid:75)(cid:68)(cid:72)(cid:82)(cid:87)(cid:68)
(cid:55)(cid:36)(cid:38)(cid:46) (cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:3)(cid:49)(cid:76)(cid:87)(cid:85)(cid:82)(cid:86)(cid:82)(cid:83)(cid:88)(cid:80)(cid:76)(cid:79)(cid:88)(cid:86)(cid:3)(cid:68)(cid:71)(cid:85)(cid:76)(cid:68)(cid:87)(cid:76)(cid:70)(cid:88)(cid:86)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:3)(cid:48)(cid:72)(cid:87)(cid:75)(cid:68)(cid:81)(cid:82)(cid:80)(cid:68)(cid:86)(cid:86)(cid:76)(cid:79)(cid:76)(cid:76)(cid:70)(cid:82)(cid:70)(cid:70)(cid:88)(cid:86)(cid:3)(cid:76)(cid:81)(cid:87)(cid:72)(cid:86)(cid:87)(cid:76)(cid:81)(cid:68)(cid:79)(cid:76)(cid:86)(cid:3)(cid:44)(cid:86)(cid:86)(cid:82)(cid:76)(cid:85)(cid:72)(cid:16)(cid:48)(cid:91)(cid:20)
(cid:55)(cid:36)(cid:38)(cid:46)(cid:3)(cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:3)(cid:49)(cid:76)(cid:87)(cid:85)(cid:82)(cid:86)(cid:82)(cid:83)(cid:88)(cid:80)(cid:76)(cid:79)(cid:88)(cid:86)(cid:3)(cid:68)(cid:71)(cid:85)(cid:76)(cid:68)(cid:87)(cid:76)(cid:70)(cid:88)(cid:86)
(cid:3)(cid:48)(cid:72)(cid:87)(cid:75)(cid:68)(cid:81)(cid:82)(cid:80)(cid:76)(cid:70)(cid:85)(cid:82)(cid:69)(cid:76)(cid:68)(cid:79)(cid:72)(cid:86)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:3)(cid:49)(cid:76)(cid:87)(cid:85)(cid:82)(cid:86)(cid:82)(cid:83)(cid:88)(cid:80)(cid:76)(cid:79)(cid:88)(cid:86)(cid:3)(cid:68)(cid:71)(cid:85)(cid:76)(cid:68)(cid:87)(cid:76)(cid:70)(cid:88)(cid:86)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:17)(cid:49)(cid:76)(cid:87)(cid:85)(cid:82)(cid:86)(cid:82)(cid:83)(cid:88)(cid:80)(cid:76)(cid:79)(cid:88)(cid:86)(cid:3)(cid:68)(cid:71)(cid:85)(cid:76)(cid:68)(cid:87)(cid:76)(cid:70)(cid:88)(cid:86)
(cid:55)(cid:36)(cid:38)(cid:46)(cid:3)(cid:74)(cid:85)(cid:82)(cid:88)(cid:83)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:17)(cid:48)(cid:72)(cid:87)(cid:75)(cid:68)(cid:81)(cid:82)(cid:80)(cid:68)(cid:86)(cid:86)(cid:76)(cid:79)(cid:76)(cid:76)(cid:70)(cid:82)(cid:70)(cid:70)(cid:88)(cid:86)(cid:17)(cid:76)(cid:81)(cid:87)(cid:72)(cid:86)(cid:87)(cid:76)(cid:81)(cid:68)(cid:79)(cid:76)(cid:86)(cid:17)(cid:44)(cid:86)(cid:86)(cid:82)(cid:76)(cid:85)(cid:72)(cid:17)(cid:48)(cid:91)(cid:20)(cid:17)(cid:20)(cid:3)
(cid:48)(cid:72)(cid:87)(cid:75)(cid:68)(cid:81)(cid:82)(cid:70)(cid:82)(cid:70)(cid:70)(cid:68)(cid:79)(cid:72)(cid:86)
(cid:38)(cid:68)(cid:81)(cid:71)(cid:76)(cid:71)(cid:68)(cid:87)(cid:88)(cid:86)(cid:17)(cid:48)(cid:72)(cid:87)(cid:75)(cid:68)(cid:81)(cid:82)(cid:80)(cid:68)(cid:86)(cid:86)(cid:76)(cid:79)(cid:76)(cid:76)(cid:70)(cid:82)(cid:70)(cid:70)(cid:88)(cid:86)(cid:17)(cid:76)(cid:81)(cid:87)(cid:72)(cid:86)(cid:87)(cid:76)(cid:81)(cid:68)(cid:79)(cid:76)(cid:86)(cid:17)(cid:44)(cid:86)(cid:86)(cid:82)(cid:76)(cid:85)(cid:72)(cid:17)(cid:48)(cid:91)1
Figure S1. Top abundant microbial community (bacteria and archaea). Heatmap for the most abundant bacteria (A) and archaea (B) taxa. Samples were clustered using Bray-Curtis
dissimilarity distance and normalized (Hellinger transformation) abundance. Related to Figure 4.
A
R = 0.56, p = 1.4e−10
B
1.5
R = 0.54, p = 1.2e−09
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R = 0.2, p = 0.075
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Figure S2. Microbial community structure and association to disturbance levels. CA dimension 1 and dimension 2 vs ammonia concentrations for bacteria (A, B) and for archaea (C, D) (Spearman
correlation). Related to Figure 5.
(cid:48)(cid:82)(cid:71)(cid:88)(cid:79)(cid:72)(cid:239)(cid:87)(cid:85)(cid:68)(cid:76)(cid:87)(cid:3)(cid:85)(cid:72)(cid:79)(cid:68)(cid:87)(cid:76)(cid:82)(cid:81)(cid:86)(cid:75)(cid:76)(cid:83)(cid:86)
green(cid:3)
(cid:239)(cid:19)(cid:17)(cid:23)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:19)(cid:26)(cid:12)
(cid:19)(cid:17)(cid:19)(cid:21)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:26)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:19)(cid:26)(cid:23)
(cid:11)(cid:19)(cid:17)(cid:23)(cid:12)
(cid:19)(cid:17)(cid:19)(cid:26)(cid:28)
(cid:11)(cid:19)(cid:17)(cid:22)(cid:12)
(cid:19)(cid:17)(cid:19)(cid:19)(cid:25)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:28)(cid:12)
(cid:19)(cid:17)(cid:22)(cid:25)
(cid:11)(cid:23)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:19)(cid:23)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:21)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:21)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:21)(cid:22)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:23)(cid:12)
(cid:19)(cid:17)(cid:22)(cid:27)
(cid:11)(cid:20)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:20)
turquoise(cid:3)
(cid:239)(cid:19)(cid:17)(cid:24)(cid:22)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:20)(cid:21)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:23)(cid:26)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:19)(cid:28)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:26)
(cid:11)(cid:23)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:25)
(cid:11)(cid:25)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:28)
(cid:11)(cid:26)(cid:72)(cid:239)(cid:19)(cid:26)(cid:12)
(cid:19)(cid:17)(cid:20)(cid:21)
(cid:11)(cid:19)(cid:17)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:23)(cid:23)
(cid:11)(cid:20)(cid:72)(cid:239)(cid:19)(cid:27)(cid:12)
(cid:19)(cid:17)(cid:19)(cid:25)(cid:24)
(cid:11)(cid:19)(cid:17)(cid:23)(cid:12)
(cid:19)(cid:17)(cid:24)(cid:21)
(cid:11)(cid:26)(cid:72)(cid:239)(cid:20)(cid:21)(cid:12)
(cid:19)(cid:17)(cid:22)(cid:25)
(cid:11)(cid:25)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
yellow(cid:3)
(cid:239)(cid:19)(cid:17)(cid:24)(cid:23)
(cid:11)(cid:20)(cid:72)(cid:239)(cid:20)(cid:21)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:24)(cid:20)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:20)(cid:20)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:24)
(cid:11)(cid:27)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:23)(cid:21)
(cid:11)(cid:27)(cid:72)(cid:239)(cid:19)(cid:27)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:23)(cid:21)
(cid:11)(cid:27)(cid:72)(cid:239)(cid:19)(cid:27)(cid:12)
(cid:19)(cid:17)(cid:21)(cid:20)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:27)(cid:12)
(cid:19)(cid:17)(cid:24)
(cid:11)(cid:23)(cid:72)(cid:239)(cid:20)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:19)(cid:22)(cid:21)
(cid:11)(cid:19)(cid:17)(cid:26)(cid:12)
(cid:19)(cid:17)(cid:22)(cid:22)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:19)(cid:24)(cid:12)
(cid:19)(cid:17)(cid:20)(cid:27)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:22)(cid:12)
k
r
o
w
t
e
n
b
u
s
/
e
l
u
d
o
M
blue(cid:3)
pink(cid:3)
(cid:19)(cid:17)(cid:25)(cid:23)
(cid:11)(cid:25)(cid:72)(cid:239)(cid:20)(cid:28)(cid:12)
(cid:19)(cid:17)(cid:26)(cid:20)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:21)(cid:23)(cid:12)
(cid:19)(cid:17)(cid:24)(cid:24)
(cid:11)(cid:23)(cid:72)(cid:239)(cid:20)(cid:22)(cid:12)
(cid:19)(cid:17)(cid:25)(cid:23)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:20)(cid:27)(cid:12)
(cid:19)(cid:17)(cid:25)(cid:23)
(cid:11)(cid:27)(cid:72)(cid:239)(cid:20)(cid:28)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:20)(cid:21)
(cid:11)(cid:19)(cid:17)(cid:20)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:25)(cid:21)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:20)(cid:26)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:20)(cid:23)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:27)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:23)(cid:28)
(cid:11)(cid:20)(cid:72)(cid:239)(cid:20)(cid:19)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:19)(cid:28)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:21)(cid:12)
(cid:19)(cid:17)(cid:27)(cid:27)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:23)(cid:28)(cid:12)
(cid:19)(cid:17)(cid:26)(cid:26)
(cid:11)(cid:24)(cid:72)(cid:239)(cid:22)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:28)(cid:23)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:25)(cid:28)(cid:12)
(cid:19)(cid:17)(cid:25)(cid:26)
(cid:11)(cid:26)(cid:72)(cid:239)(cid:21)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:27)(cid:25)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:23)(cid:24)(cid:12)
(cid:19)(cid:17)(cid:20)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:24)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:23)(cid:25)
(cid:11)(cid:23)(cid:72)(cid:239)(cid:19)(cid:28)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:20)(cid:26)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:23)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:25)(cid:25)
(cid:11)(cid:23)(cid:72)(cid:239)(cid:21)(cid:19)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:25)
(cid:11)(cid:24)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
brown(cid:3)
(cid:19)(cid:17)(cid:20)(cid:22)
(cid:11)(cid:19)(cid:17)(cid:20)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:21)(cid:20)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:28)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:20)(cid:27)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:22)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:21)(cid:26)
(cid:11)(cid:26)(cid:72)(cid:239)(cid:19)(cid:23)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:21)(cid:24)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:21)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:21)
(cid:11)(cid:26)(cid:72)(cid:239)(cid:19)(cid:24)(cid:12)
(cid:19)(cid:17)(cid:20)(cid:20)
(cid:11)(cid:19)(cid:17)(cid:21)(cid:12)
(cid:19)(cid:17)(cid:21)(cid:21)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:25)(cid:12)
(cid:19)(cid:17)(cid:20)(cid:27)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:22)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:25)(cid:28)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:21)(cid:21)(cid:12)
black(cid:3)
(cid:239)(cid:19)(cid:17)(cid:20)(cid:22)
(cid:11)(cid:19)(cid:17)(cid:20)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:26)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:21)
(cid:11)(cid:25)(cid:72)(cid:239)(cid:19)(cid:24)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:27)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:27)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:24)
(cid:11)(cid:27)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:19)(cid:17)(cid:21)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:21)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:24)(cid:23)
(cid:11)(cid:28)(cid:72)(cid:239)(cid:20)(cid:22)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:19)(cid:19)(cid:20)(cid:21)
(cid:11)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:24)
(cid:19)
(cid:239)(cid:19)(cid:17)(cid:24)
red
(cid:239)(cid:19)(cid:17)(cid:21)(cid:25)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:19)(cid:20)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:21)
(cid:11)(cid:26)(cid:72)(cid:239)(cid:19)(cid:24)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:21)
(cid:11)(cid:24)(cid:72)(cid:239)(cid:19)(cid:24)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:20)
(cid:11)(cid:20)(cid:72)(cid:239)(cid:19)(cid:23)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:23)
(cid:11)(cid:21)(cid:72)(cid:239)(cid:19)(cid:24)(cid:12)
(cid:239)(cid:19)(cid:17)(cid:22)(cid:25)
(cid:11)(cid:24)(cid:72)(cid:239)(cid:19)(cid:25)(cid:12)
(cid:19)(cid:17)(cid:21)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:20)(cid:12)
(cid:19)(cid:17)(cid:20)(cid:24)
(cid:11)(cid:19)(cid:17)(cid:19)(cid:25)(cid:12)
(cid:19)(cid:17)(cid:24)(cid:24)
(cid:11)(cid:22)(cid:72)(cid:239)(cid:20)(cid:22)(cid:12)
(cid:19)(cid:17)(cid:23)(cid:26)
(cid:11)(cid:28)(cid:72)(cid:239)(cid:20)(cid:19)(cid:12)
(cid:239)(cid:20)
Chl
Phosphate
Nitrate+Nitrite
Total Nitrogen
Ammonia
N:P
(cid:49)(cid:13)
15N 13C
Salinity
Figure S3. Microbial community and environmental variables. Weighted Gene Correlation Network Analysis (WGCNA) was used to identify subnetworks (or modules) of bacteria that correlated with environmental
variables. Pearson correlation coefficients for subnetworks that were significantly correlated with environmental variables are shown in the top number (ρ value) and the number in the parentheses is the p-value for
each relationship. Positive relationship is in red and negative relationship is in blue. Related to Table 2 & 3.
Module membership vs. Taxa significance cor=0.73,
p=5.6e−10
A
n
e
g
o
r
t
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r
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c
n
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.
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.
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.
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.
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0.6
0.8
Module Membership in blue module
C
Module membership vs. Taxa significance cor=0.53,
p=6.3e−05
n
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o
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t
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Module membership vs. Taxa significance cor=0.87,
p=4.9e−11
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0.6
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1.0
Module Membership in pink module
D
Module membership vs. Taxa significance cor=0.38,
p=0.013
5
.
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.
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.
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.
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.
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0.7
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0.9
Module Membership in yellow module
Module Membership in red module
Figure S4. WGCNA modules. Module membership of taxa in the blue (A), pink (B) and yellow (C) subnetworks (or modules) which strongly correlated with ammonia and nitrate + nitrite. Module membership of taxa in
red subnetwork (D) which strongly correlated with salinity. Related to Table 2 & 3.
A
B
Kruskal−Wallis, p = 1.2e−10
***
***
0.4
0.3
0.2
.
.
.
.
.
1
6
8
1
1
E
e
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0.1
low
intermediate
high
.
.
.
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4
9
9
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1
E
e
s
a
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c
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H
D
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a
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N
0.8
0.6
0.4
0.2
0.5
0.4
0.3
0.2
0.1
0.0
Kruskal−Wallis, p = 8.7e−14
***
***
low
intermediate
high
Kruskal−Wallis, p = 2e−15
***
***
low
intermediate
●
high
Figure S5. Metabolic pathways. (A) Contribution of top taxa from CCA ordination analysis and cos2 values. (B) Nitrogenase EC 1.18.6.1, Nitrate reductase EC 1.7.99.4 and Nitrite
reductase NADH EC 1.7.1.4 normalized (Hellinger transformation) abundance. Kruskal-Wallis test and p-values with Dunn post-test, ***denotes p-value<0.001. Related to Figure 6.
1
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Supplementary Information
Transparent Methods
Study sites, sample collection, and physiochemical parameter measurements
The study was conducted in two ecological reserves along the coast of Ecuador (Fig. 1). The
Cayapas-Mataje Ecological Reserve, located within Esmeraldas province along the Colombian
border (1° 17’ 02.14’’ N, 78° 54’ 22.29’’ W), encompasses 302.05 km2 of largely non-disturbed
mangrove forests. This reserve is located in the delta formed by the estuary of the Cayapas-
Santiago-Mataje rivers, and it is part of what used to be a continuous mangrove belt that ranged
from the central area of the Colombia Pacific coast to the south area of Esmeraldas in Ecuador.
Cayapas-Mataje is considered one of the most pristine mangrove ecosystems along the Pacific
coast of the Americas (Hamilton, 2020a). The dominant mangrove species is Rhizophora mangle,
representing 98% of all the mangrove area (Hamilton, 2020a). Traditional uses, such as artisanal
fishing and cockle picking are still practiced, and only 2% of mangrove forest area loss is attributed
to aquaculture (Hamilton, 2020b).
The Muisne Ecological Reserve, also located in the province of Esmeraldas (0° 36’ 41.81’’
N, −80° 1’ 14.36’’ W), is highly perturbed by aquaculture (Fig. 1). The site compromises the delta
of the Muisne River and numerous smaller rivers and contains a total of 12.06 km2 of mangrove
forests. The species composition is 71% Rhizophora mangle, 1% Avicennia germinans, and 28%
Languncularia racemose (Hamilton, 2020a). Muisne has been severely impacted by shrimp
aquaculture, accounting for 36% of mangrove loss. Only 1% of the remaining mangrove forest is
protected (Hamilton, 2020b).
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Water samples were taken from the surface (0.5 m depth) along a proximity gradient to the
mangrove trees. Samples were grouped by level of disturbance based on the concentration of
ammonia in the water column: Low = < 1 μM, Intermediate = 1 – 3 μM, High = > 3 μM. Similar
ammonia ranges have been identified in previous studies exposed to aquaculture effluent
(Robertson and Alongi, 1992); however, reported values in the literature can vary depending on
spatial parameters and aquaculture land expansion (Cifuentes et al., 1996; Barraza-Guardado et
al., 2013a, Samocha et al., 2004). Here we also take into account the area of shrimp aquaculture
in the two ecological sites. Muisne was identified as highly disturbed, and all the samples were
taken near shrimp aquaculture facilities (N = 29) with high levels of ammonia with the exception
of two samples near the mouth of the estuarine. The site has 20.47 km2 of shrimp farms and 12.06
km2 of mangrove forests for an approximate 2:1 ratio of aquaculture to mangrove forest (Hamilton,
2020b). Cayapas-Mataje has 11.04 km2 of shrimp aquaculture farms and 302.05 km2 of mangrove
forest for a 1:27 ratio of aquaculture to mangrove forest (Fig. 1) (Hamilton, 2020b). Thus, samples
that were collected along mangrove forests in Cayapas-Mataje (no presence of aquaculture) were
characterized as a low disturbance with lower levels of ammonia, and we included one sample
from Muisne with low level of ammonia (N = 89). Within Cayapas-Mataje, there’s a smaller
presence of shrimp aquaculture facilities and the samples that were collected near the shrimp
facilities were classified as intermediate disturbance with intermediate levels of ammonia in
addition to one sample from Muisne with intermediate ammonia (N = 34).
For DNA samples, approximately 400 ml of water was filtered through a sterile 47 mm 0.2
µm Supor filter (Pall) directly from 0.5 m depth using a peristaltic pump. The filter was
immediately stored on ice and transferred to long term storage at –80 °C within 8 hours.
Chlorophyll a concentration was measured with an Aquaflash handheld active fluorometer (Turner
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Designs) following the manufacturer’s instructions. Temperature, salinity, and turbidity were
measured using a YSI ProDss (Xylem).
For nutrient analysis, 50 ml of water was filtered through a combusted GF/F filter (Whatman),
frozen immediately after collection, and stored at –80 °C. Samples were sent to the UC Santa
Barbara Marine Institute and analyzed by flow injection analysis following standard protocols (
Lachat instrument methods: 31-107-04-1A, 31-107-06-5A, 31-115-01-3A). For CHN and isotope
analysis, 50 ml of water was filtered through a combusted GF/F filter, and filters were wrapped
into a tin envelope (Costech). Samples were analyzed by EA-IRMS at the Scripps Institute of
Oceanography Isotope Facility yielding percent carbon and nitrogen by mass, as well as δ13C and
δ15N following standard methods (Pestle, Crowley and Weirauch, 2014). The reference materials
used were NBS-19 and NBS-18, and IAEA N1 and the analytical precisions were +/- 0.3 to 0.5
for C and 0.7 to 1.0 for N. The standards used for δ13C and δ15N calculations were the Pee Dee
Belemnite and atmospheric N2, respectively.
DNA extraction and sequencing
DNA was extracted using the DNAeasy PowerWater DNA extraction kit (Qiagen). Extracted
DNA was quantified using the Qubit HS DNA quantification kit (Invitrogen) and then quality
checked by gel electrophoresis and PCR amplification of the 16S rRNA gene using primers 515F
and 806R (Walters et al., 2015) for bacteria and archaea. High quality extracted DNA was
submitted to the Argonne National Laboratory sequencing center for amplification and library
preparation with the same primer set, followed by 2 x 151 paired-end sequenced on the Illumina
Miseq platform. Sequences were submitted
to NCBI Bio project accession number:
PRJNA633714.
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Sequence analysis
Illumina Miseq reads were demultiplexed using the ‘iu-demultiplex’ command in Illumina
utils. Demultiplexed reads were quality controlled and denoised using the ‘FilterandTrim’ and
‘dada’ commands within the R package dada2 (Benjamin J Callahan et al., 2016), and assembled
with the ‘mergePairs’ command. The final merged reads had mean quality scores >30, and the
non-redundant fasta files of the generated unique reads produced by dada2 were used as an input
for
the paprica pipeline for microbial community structure and metabolic
inference
(https://github.com/bowmanjeffs/paprica). The paprica method for determining microbial
community structure differs from OTU clustering methods in that it relies on the placement of
reads on a phylogenetic tree created from the 16S rRNA gene reads from all completed bacterial
and archaeal genomes in Genbank (Bowman and Ducklow, 2015). Because the metabolic potential
of each phylogenetic edge on the reference tree is known, paprica generates a reasonable estimate
of genome sizes, gene content, and metabolic pathways for the organisms of origin of each read.
To estimate metabolic potential, a phylogenetic tree of the 16S rRNA genes from each completed
genome was generated. For each internal node on the reference tree we determined a “consensus
genome”, defined as all genomes shared by all members of the clade originating from the node,
and predict the metabolic pathways present in the consensus and complete genomes (Bowman and
Ducklow, 2015). Unique sequences (referred to as amplicon sequence variants or ASVs) and
estimated gene abundances were normalized according to predicted 16S rRNA gene copy number
prior to downstream analysis. The paprica community structure results are described in terms of
closest estimated genomes (CEGs; for phylogenetic placements to non-terminal edges) and closest
completed genomes (CCGs; for placements to terminal edges). CCGs are names according to their
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lowest consensus taxonomic ranking, while CEGs are named according to their closest relative on
the phylogenetic reference tree.
Diversity and statistics analysis
The alpha diversity index, inverse of Simpson, for ASVs was calculated using the phyloseq
package in R (McMurdie and Holmes, 2013) following methods described in Callahan (Ben J.
Callahan et al., 2016). Kruskal-Wallis tests were performed to test differences among groups in
the vegan package in R (Oksanen et al., 2019). For the biogeochemical parameters, we used the
Kruskal-Wallis test to test differences among groups, and the Spearman correlation to evaluate
relationships between N:P ratio, genome size, and 16S rRNA gene copy number. We determined
N* in disturbed and less disturbed sites; this is a measure of nitrogen vs. phosphorus availability
based on the Redfield ratio (N:P = 16:1) (Gruber and Sarmiento, 1997), and we calculated based
on nutrient concentrations using the following equation (Wilson, Abboud and Beman, 2017):
(1): 𝑁 ∗ = (𝑁𝑂!
" + 𝑁𝑂 $
" + 𝑁𝐻%
&) − 16 × 𝑃𝑂%
!"
We used correspondence analysis (CA) to quantify taxon contributions to the sample ordination.
This method allowed us to determine the degree of correspondence between sites and species, and
which taxa were associated with gradients of disturbance. We performed CA on Hellinger-
transformed data such that each value represents a contribution to the Pearson's χ2 (chi-squared)
statistic computed for the data (Legendre P., 1998). We also calculated a cos2 value that describes
the contribution of each taxa to the major axes of disturbance (Kuramae et al., 2012). Analysis of
similarity (ANOSIM) was used to assess significant differences with respect to level of
disturbance. This nonparametric permutation procedure uses the rank similarity matrix underlying
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an ordination plot to calculate an R test statistic, and it was calculated using the vegan package in
R (Oksanen et al., 2019). We examined association of levels of disturbance by a Spearman
correlation between ammonia concentrations and dimensions 1 and 2 of CA analysis. To examine
the impact of environmental variables associated to aquaculture outflow on the estimated
metabolic pathways we performed a canonical correspondence analysis (CCA) to the metabolic
output generated in paprica to restrict the sample ordination to nitrogen, phosphate, and isotopic
signals to better understand the impact of aquaculture outflow on microbial metabolic potential.
The cos2 value was used to determine the contribution of key metabolic pathways to the major
axis. The ordinations were performed in R using the factoMiner and CA package (Husson et al.,
123
2020).
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To identify unique reads differentially present between disturbed and non-disturbed sites
we used DESeq2 (Michael I Love, Huber and Anders, 2014), following the methods of Webb et
al. (2019).
DESeq2 performs differential abundance analysis based on the negative
binomial/Gamma-Poisson distribution. The default settings were used, which estimates size
factors with the median ratio method (Michael I. Love, Huber and Anders, 2014), followed by
estimation of dispersion. Next, a Wald test for generalized linear model coefficients was used to
test for significance of coefficients, considering size factors and dispersion. The p-values were
attained by the Wald test and corrected for multiple testing using the Benjamini and Hochberg
method (Michael I. Love, Huber and Anders, 2014). The most abundant bacterial and archaeal
taxa that were significantly differentially present were further examined to identify potential
microbial markers of shrimp aquaculture effluent. To determine the role of differentially abundant
microbes in nutrient cycling, we utilized the BioCyc database (Karp et al., 2019) in combination
with the paprica output to assess the potential for genes coding enzymes associated with nitrogen
fixation and denitrification. Enzymes included with our assessment included: nitrogenase; EC
1.18.6.1, EC 1,19.6.1, nitrate reductase; EC 17.99.4, EC 1.7.1.1, EC 1.7.1.2, EC 1.9.6.1, EC
1.7.2.2, and nitrite reductase; EC1.7.2.1, EC 1.7.2.2, EC 1.7.1.4.
To identify modules of highly correlated taxa we used Weighted Gene Correlation Network
Analysis (WGCNA) (Langfelder and Horvath, 2008), following the methods of Wilson et al.
(2018). A signed adjacency measure for each pair of features (unique reads) was calculated by
raising the absolute value of their Pearson correlation coefficient to the power of parameter p. The
value p = 8 was used for each global network to optimize the scale-free topology network fit. This
power allows the weighted correlation network to show a scale free topology where key nodes are
highly connected with others. The obtained adjacency matrix was then used to calculate the
topological overlap measure (TOM), which, for each pair of features, considers their weighted
pairwise correlation (direct relationships) and their weighted correlations with other features in the
network (indirect relationships). For identifying subnetworks or ‘modules’ a hierarchical
clustering was performed using a distance based on the TOM measure. This resulted in the
definition of several subnetworks, each represented by its first principal component. A subnetwork
is the association between the subnetworks and a given trait that is measured by the pairwise
relationships (correlations) between the taxa. To find correlations between subnetworks and
environmental factors, Pearson’s correlation coefficients were calculated between the considered
environmental factor and the respective principal components. P-values were adjusted using
Bonferroni method. All procedures were applied to Hellinger-transformed abundances.
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| null |
10.1371_journal.pone.0253387.pdf
|
Data Availability Statement: Raw genome
sequencing data for 23 strains are available from
the NCBI with BioProject PRJNA683613.
|
Raw genome sequencing data for 23 strains are available from the NCBI with BioProject PRJNA683613.
|
RESEARCH ARTICLE
Classification of cannabis strains in the
Canadian market with discriminant analysis of
principal components using genome-wide
single nucleotide polymorphisms
Dan Jin1,2, Philippe HenryID
3,4, Jacqueline Shan2, Jie ChenID
1,5*
a1111111111
a1111111111
a1111111111
a1111111111
a1111111111
OPEN ACCESS
Citation: Jin D, Henry P, Shan J, Chen J (2021)
Classification of cannabis strains in the Canadian
market with discriminant analysis of principal
components using genome-wide single nucleotide
polymorphisms. PLoS ONE 16(6): e0253387.
https://doi.org/10.1371/journal.pone.0253387
Editor: Tzen-Yuh Chiang, National Cheng Kung
University, TAIWAN
Received: November 10, 2020
Accepted: June 3, 2021
Published: June 28, 2021
Copyright: © 2021 Jin et al. This is an open access
article distributed under the terms of the Creative
Commons Attribution License, which permits
unrestricted use, distribution, and reproduction in
any medium, provided the original author and
source are credited.
Data Availability Statement: Raw genome
sequencing data for 23 strains are available from
the NCBI with BioProject PRJNA683613.
Funding: PBG BioPharma Inc. (https://
pbgbiopharma.com/) provided funding support in
the form of salaries for authors DJ and JS. PBG
BioPharma Inc. also provided financial support for
genome sequencing and travel expenses. JS is the
founder and CEO of PBG BioPharma Inc., and
reviewed the manuscript. Labs-Mart Inc. (http://
labs-mart.ca/) provided chemical standards and
1 Department of Biomedical Engineering, University of Alberta, Edmonton, Alberta, Canada, 2 PBG
BioPharma Inc., Leduc, Alberta, Canada, 3 Egret Bioscience Ltd., West Kelowna, British Columbia, Canada,
4 Lighthouse Genomics Inc., Salt Spring Island, British Columbia, Canada, 5 Department of Electrical and
Computer Engineering, University of Alberta, Edmonton, Alberta, Canada
* [email protected]
Abstract
The cannabis community typically uses the terms “Sativa” and “Indica” to characterize drug
strains with high tetrahydrocannabinol (THC) levels. Due to large scale, extensive, and
unrecorded hybridization in the past 40 years, this vernacular naming convention has
become unreliable and inadequate for identifying or selecting strains for clinical research
and medicinal production. Additionally, cannabidiol (CBD) dominant strains and balanced
strains (or intermediate strains, which have intermediate levels of THC and CBD), are not
included in the current classification studies despite the increasing research interest in the
therapeutic potential of CBD. This paper is the first in a series of studies proposing that a
new classification system be established based on genome-wide variation and supple-
mented by data on secondary metabolites and morphological characteristics. This study
performed a whole-genome sequencing of 23 cannabis strains marketed in Canada, aligned
sequences to a reference genome, and, after filtering for minor allele frequency of 10%,
identified 137,858 single nucleotide polymorphisms (SNPs). Discriminant analysis of princi-
pal components (DAPC) was applied to these SNPs and further identified 344 structural
SNPs, which classified individual strains into five chemotype-aligned groups: one CBD dom-
inant, one balanced, and three THC dominant clusters. These structural SNPs were all mul-
tiallelic and were predominantly tri-allelic (339/344). The largest portion of these SNPs
(37%) occurred on the same chromosome containing genes for CBD acid synthases
(CBDAS) and THC acid synthases (THCAS). The remainder (63%) were located on the
other nine chromosomes. These results showed that the genetic differences between mod-
ern cannabis strains were at a whole-genome level and not limited to THC or CBD produc-
tion. These SNPs contained enough genetic variation for classifying individual strains into
corresponding chemotypes. In an effort to elucidate the confused genetic backgrounds of
commercially available cannabis strains, this classification attempt investigated the utility of
DAPC for classifying modern cannabis strains and for identifying structural SNPs.
PLOS ONE | https://doi.org/10.1371/journal.pone.0253387 June 28, 2021
1 / 14
PLOS ONEinstrumentation support for chemical testing, but
did not have any additional role in study design,
data collection and analysis, decision to publish, or
preparation of the manuscript. Egret Bioscience
Ltd. (https://egret.bio) and Lighthouse Genomics
Inc. (https://lighthousegenomics.com/) provided
support in the form of salaries for author PH, but
did not have any additional role in the study design,
data collection and analysis, decision to publish, or
preparation of the manuscript. The specific roles of
these authors are articulated in the ‘author
contributions’ section.
Competing interests: The funder provided support
in the form of salaries for authors DJ, PH, and JS.
This does not alter our adherence to PLOS ONE
policies on sharing data and materials.
Genome-wide single nucleotide polymorphisms to classify cannabis strains
Introduction
Cannabis has a complex breeding history. Whether its botanical classification is monotypic
(sativa) or polytypic (sativa and indica) remains controversial [1]. Since the 1980s, breeding
for high psychoactive THC content has occurred very aggressively in North America [2].
Nearly all drug-type cannabis currently cultivated in the USA, Canada, and Europe are hybrid-
ized, resulting in thousands of strains [3]. Recent genetic studies focused on validating the ver-
nacular classification of “Sativa” and “Indica” [4–7]. However, this terminology is inadequate
for identifying or selecting strains for clinical research and medicinal production due to the
misuse of the botanical nomenclature, extensive cross-breeding, and unreliable labelling dur-
ing unrecorded hybridization [2]. One genetic study found that the reported ancestry percent-
age of “Sativa” vs. “Indica” for 81 drug stains is only moderately correlated with the calculated
genetic structure (r2 = 0.36) [5]. In addition, CBD dominant strains and balanced strains
(THC � CBD), which have gained increasing attention due to CBD’s use as a therapeutic [8–
12], have been omitted in recent classification studies.
Cannabis has a diploid genome (2n = 20) with nine autosomal chromosomes and one pair
of sex chromosomes [13]. The length of the haploid genome size is 818 Mbp for females and
843 Mbp for males [14]. An SNP is a variation of a single nucleotide at a specific position in
the genome, and it is useful for understanding the genetic basis of diversity among populations
[15]. SNPs are usually bi-allelic, with two alleles observed in the population [16]. Multiallelic
SNPs have more than one alternative allele for that locus. Tri-allelic SNPs, which have three
nucleotide substitution-based alleles at the same position, are relatively rare but are being con-
sidered of great relevance in epidemiological studies [17], in disaster victim identification
using mixed and/or degraded DNA samples [18], and in animals pedigree accuracy studies
[19]. Tri-allelic SNPs are reported to have a higher power of discrimination than bi-allelic
SNPs requiring fewer markers and lowering costs [18, 20]. However, tri-allelic SNPs have been
excluded in cannabis population structural analysis in the current literature [6, 21].
Cannabis classification studies that employ SNPs generally used partial genome informa-
tion with few or no overlap sequences between datasets [22]. Whole-genome sequencing is
used less often in the literature, but is preferable despite its higher cost because it enables com-
parison of genome datasets from different sources [22]. It also provides comprehensive genetic
information [22], as studies showed that differences between fiber- and drug-type cannabis are
at a genome-wide level and not necessarily limited to genes involved in THC production [5].
The recent release of the 10-chromosome map of the cannabis genome [23–27] may improve
the understanding of the genetic architecture, identify a superior set of SNPs associated with
interesting traits, and reduce future targeted genotyping costs by using fewer but more accu-
rate SNPs [28].
Several approaches are now available for the analysis of population genetic structure. One
of these approaches is the DAPC, which is a multivariate clustering method that combines the
merits of both principal component analysis (PCA) and discriminant analysis (DA) [7, 29–31].
PCA is a multivariate analysis that can be applied to large datasets to reduce dimensions, but
does not provide a group assessment, which is essential for investigating genetic structures of
biological populations [32]. DA achieves the best classification of individuals into pre-defined
groups by maximizing between-group variation and minimizing within-group variation, but
the number of variables (alleles) needs to be fewer than the number of observations (individu-
als), which is generally not the case for SNP data [29]. DAPC first uses PCA to transform raw
data (genome-wide identified SNPs) into principal components (PC), which are mutually
orthogonal linear combinations of the original variables. This ensures that variables submitted
to DA are perfectly uncorrelated and that there are fewer variables than number of individuals.
PLOS ONE | https://doi.org/10.1371/journal.pone.0253387 June 28, 2021
2 / 14
PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
Then, linear discriminant functions, which are synthetic variables of linear combinations of
these SNPs, are constructed to maximize inter-cluster differences and minimize intra-cluster
variation [29]. By combining the advantages of PCA and DA, DAPC can identify groups,
assign individuals to groups, visualize between-population differentiation, and identify indi-
vidual alleles that have contributed to population structuring.
The objectives of this study are to:
1. investigate whether modern cannabis strains can be classified and differentiated at the
whole-genome level, and
2. investigate the chromosomal location and putative functions of identified structural SNPs.
This study is a part of an integrated cannabis strain classification project utilizing genetic,
chemical, and morphological profiles, wherein plants were grown in a commercial greenhouse
under the same condition.
Materials and methods
DNA extraction and whole genome sequencing
This study included 23 commercially available cannabis strains, and the research was carried
out under a cannabis research license issued by Health Canada. Where possible, the reported
ancestry (“Sativa”, “Indica”, or “Sativa-dominant” and “Indica-dominant”) was obtained from
the licensed producer providing the strain or from an online strain database (https://www.
leafly.ca) (Table 1). Each strain was analyzed for chemical composition using methods estab-
lished in our previous study [33] and labelled as “THC dominant”, “balanced”, and “CBD
dominant”. DNA was extracted from 100 mg of fresh leaves for each strain using a Qiagen
DNeasy Plant Mini Kit (QIAGEN, Canada). DNA concentrations were determined using a
Qubit Fluorometer (Thermo Fisher Scientific, US). DNA integrity was tested by agarose gel
electrophoresis. Library construction and sequencing were performed by BGI (USA) using
DNBseq™ sequencing technology to a depth of 30x. DNBseq™ is a high-throughput sequencing
solution, where DNA is fragmented into 100–300 bp and made into DNA nanoballs (DNB™),
which are continuous DNA molecule with multiple head-to-tail copies of the same DNA frag-
ment by linear isothermal rolling-circle replication. They are loaded onto high-density
sequencing templates and sequenced by combinatorial probe-anchor synthesis (cPAS), where
fluorescently tagged nucleotides complete for addition to the growing chain. After the addition
of each nucleotide, high-resolution digital imaging is carried out where the DNB clusters are
excited by a light source and a characteristic fluorescent signal is emitted. Hundreds of and
thousands of clusters are sequenced in a massively parallel process. The emission wavelength,
along with the signal intensity, determines the base call and the number of the cycles deter-
mines the length of the read. Sequence reads were then aligned to the reference genome assem-
bly ASM23057v4 of a drug type strain Purple Kush (PK) in the NCBI BioProject database
under accession number PRJNA73819 [34] using Burrows-Wheeler Alignment (BWA) tool
[35]. New assignments of chromosomes numbers (1–10) were used as in ASM23057v5 [36].
The first step of SNP calling is marking duplications in BAM format files, and selected duplica-
tions are included in SNP calling by GATK (Genome Analysis Toolkit) (https://www.
broadinstitute.org/gatk/). Local realignment around inDels is performed to avoid the bias of
SNP calling, and the variation sites around inDel are identified as SNPs. A total of 235,334
SNPs was identified, including 225,046 bi-allelic and 10,288 multiallelic SNPs. After filtering
for SNPs with no missingness by locus and a minor allele frequency less than 10% using
PLOS ONE | https://doi.org/10.1371/journal.pone.0253387 June 28, 2021
3 / 14
PLOS ONETable 1. Strain information of 23 strains and preassigned clusters by DAPC.
Strain number
Strain name
Chemotypes
Clusters (W-SNPs)
Clusters (I-SNPs)
"Sativa" or "Indica"
Genome-wide single nucleotide polymorphisms to classify cannabis strains
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
Lemon Garlic OG
Royal Medic
Blue Hawaiian
Kandy Kush
Special
NN
Dance World
Treat
High
CB7
33˚
Banana Cake
Bananium
Burmese Blueberry
Divine Banana
Granddaddy Purple
Lemon Love
Lemon Sorbet
MeatHead
Nanitro
Platinum Jelly Punch
SBSK2 (Lemon Thai)
Super sherbet
1-Balanced
2-Balanced
3-CBD
4-CBD
5-CBD
6-CBD
7-Balanced
8-CBD
9-Balanced
10-CBD
11-THC
12-THC
13-THC
14-THC
15-THC
16-THC
17-THC
18-THC
19-THC
20-THC
21-THC
22-THC
23-THC
C1
C3
C3
C3
C3
C3
C3
C3
C3
C3
C1
C2
C3
C2
C2
C2
C1
C1
C2
C1
C1
C3
C1
C4
C2
C1
C1
C1
C1
C2
C1
C2
C1
C4
C5
C3
C5
C4
C5
C5
C4
C5
C4
C4
C3
C4
"Indica" dominant
"Sativa" dominant
"Sativa" dominant
"Sativa" dominant
Not provided
Not provided
"Sativa" dominant
Not provided
Not provided
Not provided
Not provided
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
"Indica" dominant
50/50 hybrid
"Indica" dominant
�The column of clusters W-SNPs was obtained using the whole set of 137,858 filtered SNPs. The column of clusters I-SNPs was obtained using 344 structural SNPs.
https://doi.org/10.1371/journal.pone.0253387.t001
VCFtools, 137,858 SNPs, including 128,810 bi-allelic and 9,048 multiallelic SNPs, remained
for analysis.
Analysis of population structure and identification of structural SNPs
The population structure in this work was analyzed by DAPC using the adegenet package [37]
in R software [38]. First, the find.clusters function ran successive K-means [39] for a range of k
values (where the number of clusters k = K), and identified the optimal number of clusters by
comparing the Bayesian Information Criterion (BIC) [40] of the corresponding models. After
groups were assigned, a cross-validation function (xvalDapc) was used to determine the opti-
mal number of PCs to avoid over-sacrificing information or over-fitting in the subsequent
DAPC. In cross-validation, the data were divided into a training set (90% of the data) and a
validation set (10% of the data) by default. DAPC was carried out on the training set and the
accuracy of predicting the membership of individuals in the validation set was used to identify
the number of PCs. The sampling and DAPC were repeated 30 times by default at each level of
PC retention. After assigning individuals to clusters, DA was carried out on the retained PCs
and contributions of the alleles to each discriminant function were stored. An SNPZIP analysis
(snpzip) in R was then used to provide objective delineation between structural and non-struc-
tural SNPs, as identified by DAPC, to determine which SNPs contribute significantly to the
between-population structure [41].
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First, the whole set of 137,858 SNPs were applied to DAPC to identify SNPs that contrib-
uted most to the identified clusters. DAPC was carried out again using the identified SNPs to
validate their differentiation efficiency by confirming the separation of the 23 strains into their
preassigned clusters. A short sequence (about 600 nt) around each one of these identified SNP
was searched using the BLAST software (https://blast.ncbi.nlm.nih.gov) against Cannabis
sativa Annotation Release 100 [42]. In addition to DAPC, other clustering methods, including
PCA, neighbor-joining (NJ) tree [43], and hierarchical dendrogram using Ward’s minimum
variance method [44], were also employed to assess the robustness of the final inferred clusters.
PCA and NJ tree were plotted using R. The hierarchical dendrogram was plotted using JMP
14.0.0.
Results and discussions
Discriminant analysis of principal components using 137,858 SNPs
As indicated by the elbow in the curve of BIC values as a function of k in Fig 1(a), the optimal
number of identified clusters was three, corresponding to the lowest BIC values. The number
of PCs retained for DAPC analysis was four, as calculated by cross-validation in Fig 1(b),
where it had 100% predictive success, and 0% associated root mean squared error (RMSE). In
this study, the number of PCs associated with the highest mean success was also associated
with the lowest MSE, which made it easier to choose the number of PCs to retain. For the sub-
sequent DAPC analysis, four PCs and two discriminant functions were retained. The DAPC
Fig 1. DAPC for 23 cannabis genotypes. (a) The x-axis is the number of clusters k and the y-axis is the corresponding value of
BIC. (b) The plot of DAPC cross-validation. The x-axis is the number of PCA axes retained for DAPC, and the y-axis is the
proportion of successful outcome prediction. Individual replicates appear as points, and the density of those points in different
regions of the plot is displayed in blue. (c) DAPC plot for 23 cannabis genotypes along two linear discriminants (LD 1 and LD 2).
https://doi.org/10.1371/journal.pone.0253387.g001
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PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
plot of 23 cannabis genotypes is shown in Fig 1(c). The grouping assignment for individual
strains by DAPC is listed in Table 1 (as W-SNPs). C1 is a THC dominant cluster and includes
six THC dominant strains (11, 17, 18, 20, 21, and 23-THC) and one balanced strain (1-bal-
anced). C2 is another THC dominant cluster and includes five THC dominant strains (12, 14,
15, 16, and 19-THC). C3 is a cluster dominated by CBD dominant and the balanced strains
which includes six CBD dominant strains (3, 4, 5, 6, 8, and 10-CBD), three balanced strains (2,
7, and 9-balanced), and two THC dominant strains (13 and 22-THC). While C2 is closer to C3
and is more distant to C1, C1and C3 are clearly separated along linear discriminant 1 (LD1).
While C1 and C3 are roughly at the same level with respect to linear discriminant 2 (LD2), C2
is separated from both. PCA was also carried out on the same set of SNPs and results are
shown in S1 Fig. Twenty-three cannabis strains are plotted along pair-wise PCs of the first 4
PCs, which account for 18.4%, 11.5%, 9.5%, and 8.7% of the total variance, respectively. Simi-
larly, the first PC suggests the existence of a relatively compact CBD & balanced clade on the
left side of the plot and a more dispersed THC dominant clade on the right side of the plot. Bal-
anced strains share a closer gene pool with CBD dominant strains, while the THC gene pool is
more dispersed. Because THC is psychoactive and its potency can be readily assessed through
consumption, selection for increasing THC content started early and widely for recreational
purposes by traditional breeding [45]. In contrast, CBD is non-psychoactive and must be ana-
lyzed in a laboratory for potency, and therefore breeding for high CBD concentrations began
later [45]. A complete genome assembly implied that CBD dominant varieties were generated
by integrating hemp-type CBD acid synthase gene clusters into a background of drug-type
cannabis to elevate CBDA production [24]. These balanced strains may have been created by
crossing purebred THC dominant types with CBD dominant types [46]. Therefore, there may
be a relatively limited selection of CBD dominant strains for breeding balanced strains.
Discriminant analysis of principal components using 344 structural SNPs
DAPC was repeated using identified 344 structural SNPs. The optimal number of identified
clusters was five, corresponding to the lowest BIC values (Fig 2(a)). Two PCs were retained for
the following DAPC analysis in Fig 2(b), where it had 98.9% predictive success and 0.04%
RMSE. For the subsequent DAPC analysis, two PCs and two discriminant functions were
retained. The grouping assignment for individual strains by DAPC is listed in Table 1 (as
I-SNPs). Within the five clusters (Fig 2(c)), C1 is a CBD dominant cluster that includes six
strains (3, 4, 5, 6, 8, and 10-CBD), C2 includes three balanced strains (2, 7, and 9-balanced),
and C3, C4, and C5 are THC dominant clusters that include two (13 and 22-THC), seven
(1-balanced, 11, 15, 18, 20, 21, 23-THC), and five (12, 14, 16, 17, and 19-THC) strains,
respectively.
These multiallelic SNPs were also subjected to PCA, NJ tree, and hierarchical clustering
analysis. In Fig 3, the 23 cannabis strains are plotted along PC1 and PC2, which account for
44.5% and 10.0% of the total variance, respectively. The proportions of explained variance are
higher compared to the previous PCA results (18.4% and 11.5%) obtained using the whole set
of SNPs. CBD dominant cluster C1 and balanced cluster C2 are on the left side of the scatter
plot (PC1<0) and the THC dominant clusters C3, C4, and C5 are on the right side of the scat-
ter plot (PC1>0). Notably, six CBD dominant strains are separated from three balanced
strains, while they were previously combined in the analysis using the whole set of SNPs. In
addition, two THC dominant strains 13-THC and 22-THC are separated from the CBD and
balanced cluster, and instead placed closer to other THC dominant strains. Strain 1-balanced
is closer to THC dominant strain regardless of whether the whole set of SNPs or 344 identified
SNPs were used.
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Fig 2. DAPC of 23 cannabis genotypes using 344 multiallelic structural SNPs. Clusters indicated as C1, C2, C3, C4, and C5 corresponds to the
I-SNPs in Table 1.
https://doi.org/10.1371/journal.pone.0253387.g002
The genetic structure from NJ-tree and hierarchical clustering using the 344 multiallelic are
displayed in Fig 4, mostly congruent with that of DAPC. In the NJ-tree, all six CBD dominant
strains are clustered together, with three balanced strains clustered closer on the same branch
(Fig 4(a)). Most THC dominant strains are also clustered adjacent to strains within their own
clusters. The dendrogram using hierarchical clustering by Ward’s method reveals two major
groups, where one group is comprised of CBD dominant & balanced strains, and the other of
THC dominant strains (Fig 4(b)). They are further separated into five subclusters, where CBD
dominant and balanced clusters are consistent with the DAPC grouping results, and several
THC dominant strains clustered differently. Two strains, 15-THC and 18-THC, were assigned
to C4 using DAPC but are assigned closer to C5 in the dendrogram. Two other strains,
14-THC and 16-THC, were assigned to C5 in DAPC but are assigned closer to C3 in the den-
drogram. The clustering results are congruent between DAPC and hierarchical clustering with
an assignment agreement rate of 83% (19/23).
Allele frequencies for 344 multiallelic SNPs in three chemotypes
DAPC identified 344 highly contributing SNPs (S1 Table). All the structural SNPs are multial-
lelic, among which 98.5% (339/344) are tri-allelic and the remainder 1.5% (5/344) are tetra-
allelic. The dendrogram of 23 strains using hierarchical clustering based on the allele counts in
the 344 structural SNPs (S2 Table) separated the strains into CBD dominant, balanced, and
THC dominant strains, mostly corresponding to the grouping results of DAPC (Fig 5). The
allele frequency was calculated by dividing the counts of that allele for all strains within the tar-
geted group by the sum of the counts for each allele for that SNP within the targeted group.
Allele frequencies of the structural SNPs were calculated for three major branches, each corre-
sponding one of three chemotypes. (S1 Table). If 1-balanced strain was assigned to the THC
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PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
Fig 3. Scatter plot of 23 cannabis strains on PC1 & PC2 using 344 structural SNPs. Clusters indicated as C1, C2, C3,
C4 and C5 correspond to I-SNPs in Table 1.
https://doi.org/10.1371/journal.pone.0253387.g003
dominant group as indicated by DAPC for allele frequency calculation, there are 87% (300/
344) SNPs in CBD dominant clusters, 46% (157/344) SNPs in balanced clusters, and 11% (39/
344) SNPs in THC dominant clusters that have one allele with allele frequencies > 80% (S1
Table). Among them, 140 SNPs shared same alleles with allele frequencies > 80% in CBD
dominant strains (140/300) and balanced strains (140/157), which further indicated that CBD
dominant strains and balanced strains closely share a gene pool. There are 38 SNPs that have
one allele present in CBD dominant strains with allele frequencies > 80% and are not detected
in THC dominant strains. There are 322 SNPs whose alleles that are present in THC dominant
strains but were not detected in CBD dominant strains.
If the 1-balanced strain is assigned to the balanced group for allele frequency calculation,
there are 87% (300/344) SNPs in CBD dominant clusters, 10% (36/344) SNPs in balanced clus-
ters, and 13% (44/344) SNPs in THC dominant clusters that have one allele with allele
frequencies > 80% (S2 Table). Among them, 32 SNPs shared same alleles with allele
frequencies > 80% in CBD dominant strains (32/300) and balanced strains (32/36). There are
38 SNPs that have one allele present in CBD dominant strains with allele frequencies > 80%
and are not detected in THC dominant strains. There are 321 SNPs whose alleles are present
in THC dominant strains but were not detected in CBD dominant strains. Assigning the 1-bal-
anced strain to the balanced group added more genetic diversity to the balanced group, and
the effect of adding or deleting this strain for the THC dominant group in terms of allele fre-
quency is small and can be neglected.
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PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
Fig 4. NJ-tree and hierarchical clustering using the 344 multiallelic SNPs (a) NJ-tree and (b) The dendrogram using hierarchical clustering by
Ward’s method for 23 cannabis genotypes. Clusters indicated as C1, C2, C3, C4, and C5 corresponds to I-SNPs in Table 1.
https://doi.org/10.1371/journal.pone.0253387.g004
Fig 5. Hierarchical clustering of 23 strains based on the allele counts for 344 structural SNPs identified by DAPC.
https://doi.org/10.1371/journal.pone.0253387.g005
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PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
Fig 6. Features of 344 multiallelic SNPs (a) Distribution of structural SNPs on chromosome 1–10 and unplaced
scaffolds. (b) BLAST results for structural SNPs against a fully annotated genome.
https://doi.org/10.1371/journal.pone.0253387.g006
BLAST analysis of 344 multiallelic SNPs
These 344 SNPs were spread across all 10 chromosomes (Fig 6(a)), indicating that commer-
cially available cannabis strains in North America are significantly differentiated at a genome-
wide level. The number of identified SNPs ranged from 7 to 127 on each genome, with 37% of
the genetic variation occurring (127 SNPs) on chromosome 6, where CBDAS and THCAS are
located [13]. The rest SNPs were spread over the remaining nine chromosomes. All ten chro-
mosomes have genes related to the biochemical pathways of secondary metabolites, including
cannabinoids, monoterpenes, and sesquiterpenes [13, 24, 47–51]. BLAST results showed that
90% (310/344) of these structural SNPs had no feature, 7% (24/344) are uncharacterized loci
with unknown functions, and 3% (10/344) are predicted for certain functions (Fig 6(b)).
Conclusions
Although the cannabis industry is rapidly advancing after the relaxation of legal restrictions in
North America, the increasing number of THC dominant strains, CBD dominant strains, and
balanced strains only adds confusion to the currently poorly understood genetic background
of the thousands of varieties already in existence. Although there were only 23 strains included
in this study, they covered the three typical chemotypes of cannabis strains currently available
in the market. Leveraging as much genetic variation as possible using whole-genome sequenc-
ing, we identified 344 multiallelic SNPs that were used to investigate the genetic structure of 23
cannabis genotypes using DAPC, PCA, NJ tree, and hierarchical clustering, which provided
consistent observations and groupings despite the differences in algorithms. The clustering
results revealed that these 23 strains could be separated into five clusters, with one cluster
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PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
containing six CBD dominant strains, another cluster containing three balanced strains, and
the remaining three clusters containing 13 THC dominant strains and one balanced strain.
CBD dominant strains and the balanced strains are closer genetically. This may be attributed
to how medical interest in breeding for non-psychoactive, CBD-elevated strains (CBD domi-
nant and balanced strains) has only recently been in vogue, resulting in an overlapping and
less diverse gene pool for CBD dominant and balanced strains compared to the longer breed-
ing history for THC strains. Some alleles are only present in CBD dominant strains or in THC
dominant strains. More alleles present in balanced strains are shared with CBD dominant
strains. One third of these structural SNPs are located on the chromosome containing THCAS
and CBDAS. The remaining SNPs are located on the other nine chromosomes. An area of
potential investigation is how the identified structural SNPs are associated with the production
of other cannabinoids, mono- and sesquiterpenes, flavonoids, other compounds, or morpho-
logical characteristics.
Since the late 20th century, genetic methodologies have been developed for separating
industrial hemp from drug-type cannabis for forensic purposes, thus differentiating CBD
dominant and THC dominant strains [52–56]. For the past 20 years, with the extensive hybrid-
ization of THC dominant strains, many classification studies have focused on separating
“Sativa” and “Indica” strains and many have suggested abolishing this vernacular [5–7]. The
genotyping results of this study indicate that modern, extensively hybridized strains can still be
separated using genome-wide information. As a powerful multivariate approach that investi-
gates population structures based solely on genetic information, DAPC separated strains into
clusters aligned with their chemotypes. Additionally, DAPC has the potential to sort the disor-
dered genetic background of thousands of THC dominant strains by identifying the number
of genetic clusters within THC dominant strains, describing clusters by interpreting group
memberships, and identifying the contributing SNPs that have the potential to be used as
genetic markers for strain classification and identification. This would require a concerted
effort from the cannabis industry by contributing whole genome sequence data to public data-
bases and by building a common taxonomy based on genomics. Optimally, the identified
genetic markers can be used as genomic fingerprints in combination with chemical finger-
prints and morphological characteristics for strain identification. These markers can be lever-
aged for strain selection in clinical trials and for manufacturing cannabis-based products and
medicines.
Supporting information
S1 Fig. PCA of 23 strains using whole set of SNPs.
(PDF)
S1 Table. 344 multiallelic SNPs identified by DAPC.
(XLSX)
S2 Table. Allele counts for 344 structural SNPs identified by DAPC.
(XLSX)
Acknowledgments
The authors are grateful to licensed grower Emerald Flower Farm who provided commercial
greenhouse to cultivate cannabis. The authors are also grateful to Dr. Limin Wu for assisting
DNA extraction, Dr. Jie Zeng for assisting BLAST analysis, and Shengxi Jin for proofreading
the manuscript.
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PLOS ONEGenome-wide single nucleotide polymorphisms to classify cannabis strains
Author Contributions
Conceptualization: Dan Jin.
Data curation: Dan Jin.
Formal analysis: Dan Jin, Philippe Henry.
Funding acquisition: Dan Jin, Jacqueline Shan.
Investigation: Dan Jin.
Methodology: Dan Jin, Philippe Henry.
Project administration: Dan Jin.
Resources: Dan Jin.
Software: Dan Jin, Philippe Henry.
Supervision: Jie Chen.
Validation: Dan Jin, Philippe Henry.
Visualization: Dan Jin, Philippe Henry.
Writing – original draft: Dan Jin.
Writing – review & editing: Philippe Henry, Jacqueline Shan, Jie Chen.
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