Significance
We do not have a clear understanding of the impact of past climatic changes on evolution. This question has been investigated for a few lineages in the fossil record, but a global vision is still lacking. Here, we present a phylogenetic comparative framework for examining the effects of past climate changes on morphological evolution with data from almost all existing birds and mammals. We show that global temperatures fluctuations through the Cenozoic impacted body size evolution. The evolution of body size was faster during periods of global cooling in most of the groups, challenging the hypothesis that evolution is faster under warm climates. These results have important implications for our understanding of how ongoing climate changes may affect future evolution.
Keywords: evolutionary rates, macroevolution, climate, endotherms, phylogenetics
Abstract
How ecological and morphological diversity accumulates over geological time is much debated. Adaptive radiation theory has been successful in testing the effects of biotic interactions on the rapid divergence of phenotypes within a clade, but this theory ignores abiotic effects. The role of abiotic drivers on the tempo of phenotypic evolution has been tested only in a few lineages or small clades from the fossil record. Here, we develop a phylogenetic comparative framework for testing if and how clade-wide rates of phenotypic evolution vary with abiotic drivers. We apply this approach to comprehensive bird and mammal phylogenies, body size data for 9,465 extant species, and global average temperature trends over the Cenozoic. Across birds and mammals, we find that the rate of body size evolution is primarily driven by past climate. Unexpectedly, evolutionary rates are inferred to be higher during periods of cold rather than warm climates in most groups, suggesting that temperature influences evolutionary rates by modifying selective pressures rather than through its effect on energy availability and metabolism. The effect of climate on the rate of body size evolution seems to be a general feature of endotherm evolution, regardless of wide differences in species’ ecology and evolutionary history. These results suggest that climatic changes played a major role in shaping species’ evolution in the past and could also play a major role in shaping their evolution in the future.
More than 60 y ago, George Gaylord Simpson postulated that much of biological diversity on Earth originated during adaptive radiations—the diversification of ecological traits in a rapidly speciating group of organisms (1, 2). Adaptive radiation theory posits that interspecific competition is the main force driving divergence, thus placing biotic interactions at the center of phenotypic evolution. Accordingly, recent developments in the study of trait evolution have focused on biotic models: for example, accounting for diversity dependence (3, 4) or trait-driven competitive effects (5). By comparison and despite the alternative widespread view that environmental factors play a major role in evolution (6–9), abiotic models have received far less attention, considered only for few ancestor–descendant lineages and small clades in the fossil record (10–12). In particular, the lack of robust comparative phylogenetic methods for analyzing the effect of environmental changes on trait evolution from extant data has hindered our understanding of the relative role of biotic and abiotic factors in shaping phenotypic diversity.
Here, we develop a general maximum likelihood comparative phylogenetic framework for estimating the effect of measured environmental variables on the tempo of phenotypic evolution. We then focus on the effect of climatic variations as measured by average global temperature through the Cenozoic (13, 14). Temperature is thought to influence biological processes at all levels of organization through its effects on metabolic rates, body size, and productivity (8, 15). However, how it influences phenotypic rates is not well-understood. We test the performance of our framework using intensive simulations. Finally, we illustrate this framework by using it and comparison with classical models of phenotypic evolution in combination with body size and phylogenetic data for 6,110 extant bird and 3,355 extant mammal species to evaluate whether and how Cenozoic temperature fluctuations influenced rates of body size evolution.
Results and Discussion
We extended the Brownian motion (BM) process (16–19) with time-varying evolutionary rate to account for the possibility that one or several environmental variables influence this rate and developed the maximum likelihood inference tool that allows fitting this model to comparative data (Materials and Methods). We applied this general model to evaluate the effect of temperature T on the rate of phenotypic evolution using two simple models relating phenotypic rates to temperature T either linearly [linear climatic dependence (the Clim-lin model)] or exponentially [exponential climatic dependence (the Clim-exp model)]. In these two models, a single parameter measures the strength and direction of temperature dependence. When applied to simulated data (SI Appendix), our phylogenetic comparative framework was able to recover input parameter values (SI Appendix, Figs. S1–S4). As expected, the power to detect the climatic models when they were the generating models increased with the strength of temperature dependence and tree size (SI Appendix, Figs. S5–S8). Importantly, the climatic models were typically not selected when they were not the generating models (the false discovery rate never exceeded ) (SI Appendix, Figs. S9–S15), meaning that our model comparison framework provides a conservative test for the effect of temperature on rates of phenotypic evolution.
We applied our climatic models to rates of body size evolution in birds and mammals (Materials and Methods). We used the two most up to date species-level phylogenies for mammals (20, 21), but these phylogenies are less reliable than the bird phylogeny, in particular with respect to their branch lengths. We thus focus on the bird results, with the mammal results presented in SI Appendix. We found similar trends for the two groups. Our climatic model with exponential dependency of evolutionary rates to temperature (Clim-exp) was better supported than all other models for most groups (Fig. 1 and SI Appendix, Figs. S16–S18). Anecdotally, groups restricted to regions that have been relatively climatically stable in the last several million years, such as the tropics (the neotropical bird families Thamnophilidae and Ramphastidae and the Primates) and Oceania (Meliphagidae, Diprotodontia, and Dasyuromorphia), supported other models than the climatic ones.
Fig. 1.
The climatic model outperforms all others (results for birds) (equivalent results for mammals are shown in SI Appendix, Figs. S17 and S18). (A) The height of each colored bar represents the relative support for each model (mean Akaike weight over 1,000 trees from the posterior distribution). (B) The height of each bar represents the proportion of trees from the posterior distribution for which the Clim-exp model is ranked first to last. OU is equivalent to ACexp. ACDClin, linear increase or decrease; DCexp, exponential decrease; DDexp, exponential diversity dependence; DDlin, linear diversity dependence; EB, early burst.
Estimated values were negative, indicating a consistent trend for a slowdown in rates of body size evolution during periods of climate warming (Fig. 2 and SI Appendix, Figs. S16–S18). The only few groups that showed a tendency toward positive values (Procellariiformes, Thamnophilidae, Meliphagidae, Ramphastidae, and the Primates) were groups for which climatic models were poorly supported. The inferred negative exponential association between rates of body size evolution and temperature implies that these rates increased during the cold climatic periods of the Cenozoic, such as the Oligocene and late Miocene (Fig. 2B and SI Appendix, Fig. S19).
Fig. 2.
(A) Rates of body size evolution are negatively associated with temperature in most bird orders (equivalent results for mammals are shown in SI Appendix, Figs. S17 and S18). Boxplots represent, for each bird order, the median, the first and third quartiles, and extreme values of estimated values for 1,000 trees from the posterior distribution; measures the strength and direction of the temperature dependency of evolutionary rates. The different clades are represented on the complete bird phylogeny (9,993 species); species that were not included in the analyses are represented in black. (B) Rate through time curves for each bird order obtained using median estimates of over the posterior distribution of trees (equivalent results for mammals are shown in SI Appendix, Fig. S19). Body size evolution consistently accelerates during the Oligocene cold period and from the mid-Miocene to the recent past. Plio., Pliocene; P., Pleistocene.
The support for the Clim-exp model with negative held across posterior distributions of trees, the two distinct phylogenies that we used for mammals, and major bird and mammalian families, suggesting that these results were robust to phylogenetic uncertainty and taxonomic scale (Figs. 1 and 2 and SI Appendix, Figs. S16–S18). In addition, we tested whether the well-known tendency for increasing body size over evolutionary time [Cope’s or Depéret’s rule (22, 23)] could artificially favor the support of our climatic model (Materials and Methods) and found that it was not the case (SI Appendix, Fig. S20).
Previous studies reporting a tendency for increasing rates of body size evolution through time have attributed this increase to episodic and short-term bursts of evolution (24, 25). Simulating data with randomly distributed episodic bursts (Materials and Methods), we found that it is unlikely that rate shifts confined to few branches are mistakenly interpreted as climatic processes (SI Appendix, Fig. S21). There is a possibility that processes unrelated to climate generating an increase in evolutionary rates through time—for example, higher extinction rates in slow-evolving species or phenotypic rates increasing with species richness in expanding clades—could support a negative association between rates and temperature by purely noncausal correlation because of the trend toward cooler climates during the Cenozoic. However, when fitting our climatic model using increasingly smoothed climatic curves to test whether and to which extent specificities of the temperature curve matter in explaining support for a temperature effect (Materials and Methods), we found that the support was significantly affected when features of the temperature curve were removed (Fig. 3 and SI Appendix, Figs. S22–S24). Anecdotally, the signal gradually started to be lost for a degree of smoothing corresponding to softening the remarkable cooling events associated with the onset of the Antarctic (33.9–25 and 16–12 Ma) and Northern hemisphere (6 Ma to present day) ice sheets (13, 14). Given that these climatic events also coincide with known diversification events (26), climate could influence rates of body size evolution indirectly through its effect on taxic diversification.
Fig. 3.
The climatic model is less supported when removing details of the temperature curve. (A) Climatic curves obtained with various degrees of smoothing (df). The horizontal bars indicate the qualitative representation of ice volume in each hemisphere (13) [dashed bars represent periods of minimal ice coverage (), and full bars represent periods of maximum ice coverage ()]. (B) In dark gray, the proportion of trees from the posterior distribution for which the fit with the smoothed climatic curve remains as good as with the original curve ) for the most speciose order of birds (Passeriformes) is shown. SI Appendix, Figs. S22 and S23 show similar results for the other bird orders and mammals, and SI Appendix, Fig. S24 shows results at the family level. Plio., Pliocene; P., Pleistocene.
Focusing on the bird analyses for which we had empirical estimates of error on body size measurements, we used simulations to test that the support for the Clim-exp model was not driven by such measurement error (ME) (Materials and Methods) and found that it was unlikely to be the case (SI Appendix, Figs. S25 and S26). We further evaluated the effect of ME on rate trajectories using a “model-free” approach, where rates are estimated on time bins (Materials and Methods and SI Appendix). MEs tend to increases variance at the tips and as such, artificially increase rates of phenotypic evolution in the recent past (last 2.5 Ma) (SI Appendix, Fig. S27). The effect of ME extends to the Miocene, although it is less pronounced than in the Plio-Pleistocene, and creates a spurious support for a positive rather than negative association between evolutionary rates and temperature (Fig. 4). ME cannot explain the high rates during the cold period of the Oligocene (33.9–25 Ma) followed by the low rates during the warm period (25–16 Ma) spanning the early to mid-Miocene observed in many groups (Fig. 4 and SI Appendix, Figs. S27 and S28).
Fig. 4.
ME cannot explain rate differences between the cold Oligocene period (33.9–25 Ma) and the following warm period (25–16 Ma) spanning most of the early to mid-Miocene (SI Appendix, Figs. S27 and S28). Rate differences ( mean over 1,000 trees from the posterior distribution; error bars represent the confidence intervals on the mean rate differences) estimated on (A) empirical data, (B) data simulated under the Brownian process with ME, and (C) data simulated under the OU process with ME. MEs bias evolutionary rate estimates toward increasing values from the Oligocene to the following early to mid-Miocene period (red), whereas around one-half of the empirical datasets show decreasing values (blue). Some of the trends found in this analysis differ from those obtained with the climatic model (e.g., for the Procellariformes and Anseriformes); these apparent contradictions are discussed at length in SI Appendix. a, Anseriformes; b, Gruiformes; c, Piciformes; d, Galliformes; e, Pelecaniformes; f, Charadriiformes; g, Strigiformes; h, Passeriformes; i, Columbiformes; j, Apodiformes; k, Accipitriformes; l, Coraciiformes; m, Cuculiformes; n, Caprimulgiformes; o, Psittaciformes; p, Procellariiformes.
Whether climate played a dominant role in driving evolutionary rates over the whole Cenozoic or mainly during the extensive climatic fluctuations of the Oligocene and Miocene (and potentially, Plio-Pleistocene) is not clear. Our results do not exclude the possibility that biotic factors played an important role in clades’ early history: the signal of early biotic factors on current phenotypes could have been overwritten by the strong recent climatic effect (27); biotic factors could also have resulted in the extinction of the clades in which they were too strong by constraining phenotypic innovation (28). Testing these hypotheses will require analyzing extinct (fossil) data along with phenotypes of extant taxa (29), and our framework—not limited to ultrametric trees—can be used to do so.
Our result that phenotypic diversity accumulates faster during periods of cold rather than warm climates can seem counterintuitive in light of the widely accepted ideas that rates of molecular evolution are higher at higher temperatures (30, 31), that stronger biotic interactions in warm and stable environments spur phenotypic evolution (8, 32), and that warmer climates provide the energetic foundation for higher divergence (8). However, both the association between molecular and morphological rates and the stronger role of biotic interactions in warm climates are debated (33–35); in addition, energetic effects should mainly apply to ectotherms (30). There is a possibility that our analyses, conducted on ectotherms, would show a correlation with climate opposite to the one that we observe on endotherms.
Fast evolutionary rates under cold climates are consistent with the macroecological observation that rates of phenotypic evolution are higher at high latitudes (36, 37). This latitudinal gradient has been attributed to stronger geographical climatic heterogeneity in temperate rather than tropical regions driving stronger climatic niche divergent selection and ultimately, faster phenotypic divergence (36, 38). This latter hypothesis is particularly relevant in the case of body sizes, which evolve directly through physiological adaptation to climatic differences, following Bergman’s rule [organisms evolve larger sizes under cold temperatures (22)]. The same mechanisms could operate at the macroevolutionary scale, with periods of cold climates corresponding to periods when temperate biomes and thus, also geographical climatic heterogeneity were more widespread. Other than geographical climatic heterogeneity, temporal fluctuations are thought to be more intense at high latitudes and in periods of climate cooling (13), and they could also foster rapid evolution by rapidly changing the direction of selection. We do not exclude the possibility that it is not cold average temperature per se but rather, that it is its correlation with high geographical and/or temporal climatic heterogeneity that spurs phenotypic divergence (37, 38).
It has been proposed that the disparity in body sizes that we observe today across species within clades accumulated early in clades history (2, 27) or that this disparity results from rare and randomly localized bursts of evolution spread throughout the tree and corresponding to the exploration of new adaptive zones (24, 39). Here, we find that the pace of body size evolution responds to an external climatic forcing that operates on entire clades and across groups as diverse as birds and mammals. Directly interpreting these results in the context of the current climatic changes should be done with caution given that contemporary changes are orders of magnitude faster than historical ones. However, our study highlights global temperature as a manifest driver of evolutionary rates, suggesting that human-driven climate changes will have (or already have had) a major effect on evolution.
Materials and Methods
A General Model of Phenotypic Evolution Accounting for Environmental Variations.
To test the effect of past measured environmental variables on rates of phenotypic evolution, we extend the BM process (16–19) with time-varying evolutionary rate :
[1] |
where is a white noise with mean = and variance of . We allow to be influenced by one or k environmental variables , which themselves vary through time:
[2] |
The likelihood corresponding to this model is the classical multivariate normal distribution (18, 40), with the variance–covariance matrix given by
[3] |
where represents the time between the root and the most recent common ancestor of species i and j (e.g., ref. 41 has related models). To speed up the computation of the likelihood, we used a stretching–pruning approach, which consists of transforming (stretching) the branches of the tree according to the expected variance–covariance (42) before computing the likelihood recursively using a fast dynamic algorithm based on independent contrasts (pruning) (40, 43, 44). The integrals 3 were computed numerically using the Gauss–Kronrod quadrature formula (45) implemented in the “integrate” function from the stats R base package (46). Finally, maximum likelihood optimization was performed using the quasi-Newton method (47) (L-BFGS-B) implemented in the “optim” function in R. These implementations are available in the RPANDA package (48) publicly available from the CRAN repository (function ). They can be used on both ultrametric and nonultrametric trees, therefore allowing the possibility to analyze combined fossil and extant data.
We applied this general model to test if and how rates of phenotypic evolution are related to changes in temperature T. We scaled the temperature curve between zero and one; in what follows, T stands for scaled temperature. We considered two simple models relating phenotypic rates to temperature T either linearly [ (the Clim-lin model)] or exponentially [ (the Clim-exp model)], where is the hypothetical clade-specific phenotypic rate at an average global-scale temperature of C and reflects the strength and direction of the dependency to temperature. In these models, rates of phenotypic evolution are increasing with increasing temperature when is positive, are decreasing otherwise, and reduce to a constant rate BM when . For computational convenience, the Clim-lin model was parameterized as , such that with a scaled temperature curve, is made up between and , increasing with temperature when and decreasing with temperature when (49). We thoroughly tested the ability of our approach to recover input parameters using extensive simulations (SI Appendix).
Model Comparison.
We compared the fit of the climatic models with six competitive models of trait evolution. We fitted the classical BM and an Ornstein–Uhlenbeck (OU) process, which both assume a constant diffusion (50, 51). On ultrametric trees and assuming that the root state is at the optimal trait value, the likelihood of the OU model is identical to a time-dependent model with increasing exponentially with time [known as the accelerating rate (AC) model (52); we name it the exponential increase (ACexp) model here for clarity]. We, therefore, refer to this process as the OU/ACexp process. We also consider a time-dependent model with decreasing exponentially with time [the early burst model (41, 53); we name it the exponential decrease here for clarity] and a time-dependent model with varying linearly with time either positively or negatively (4, 41) (coined linear increase or decrease). Finally, we consider the two models that have been used so far to model diversity-dependent effects, with constrained to decay with the number of lineages (3, 4) either exponentially (exponential diversity dependence) or linearly (linear diversity dependence). The relative statistical support for the various models was assessed using the Akaike weights (54). We thoroughly assessed the statistical properties of our model comparison framework using intensive simulations (SI Appendix). In particular, we tested our ability to recover the climatic model when it was the generating model and also, that it was not spuriously detected when it was not the generating model.
Body Size Data.
We extracted body mass estimates (in grams) for 9,993 bird species from the EltonTraits 1.0 database (55) and 3,574 mammal species from the PanTHERIA 1.0 database (56). We discarded estimates for 261 bird species that were based on genus or family mean values and that could have biased our evolutionary rate estimates. Body mass estimates were log-transformed before analysis.
Phylogenetic Trees.
Bird phylogenies were taken from the recently updated (v2.iii) (57) posterior distribution by Jetz et al. (58), from which we discarded species that did not have molecular information. Mammal phylogenies were taken from two sources. The first consisted of 1,000 trees sampled from the pseudoposterior distribution by Kuhn et al. (20), which was obtained by randomly resolving polytomies from the widely used supermatrix tree by Bininda-Emonds et al. (59). Because these random polytomy resolutions could inflate evolutionary rate estimates and bias our results (60–62), we also conducted all of our analyses on 1,000 trees from the posterior sample (v.1.002) of a recently published phylogeny of 4,160 extant mammal species by Faurby and Svenning (21) largely based on sequence alignments and ages by Meredith et al. (63). However, Faurby and Svenning (21) focused on resolving topological conflicts rather than branch length, and the authors themselves caution against interpreting branch lengths in their phylogeny. Thus, although the two phylogenies supported consistent results, we reported results for only the birds in the text.
We aligned the phylogenetic and body size data; to test the robustness of our results to taxonomic scale, we conducted analyses at both the order and family levels. We dismissed phylogenies with less than 50 species, because results from simulations showed that a minimum of 50 species was necessary to be able to statistically distinguish our climatic models from other models (SI Appendix). For birds, this alignment resulted in the analysis of 16 orders and 36 families, representing a total of 6,110 species. For mammals, this alignment resulted in the analysis of 12 orders and 15 families, representing a total of 3,355 species [11 orders and 12 families representing a total of 2,664 species for the trees by Faurby and Svenning (21)].
Temperature Data.
We used the temperature curve by Cramer et al. (14). Similar to the more widely used Zachos curve (13), the curve by Cramer et al. (14) is derived from benthic foraminiferal (bf) isotopic ratio. However, contrary to the Zachos curve, the curve by Cramer et al. (14) accounts for fluctuations in sea water (sw) through time, which is important for periods of large-scale glaciations when differences in can go up to in Vienna Standard Mean Ocean Water (VSMOW) (64). In addition, the curve by Cramer et al. (14) provides temperature estimates for the last 108 My, thus spanning the full time range over which extant bird and mammal orders originated. Although this curve is derived from the marine record, it correlates well with the more fragmented continental record (65). Rather than local or seasonal fluctuations, these curves reflect planetary-scale climatic trends that are expected to have led to temporally coordinated changes in several clades (7, 9, 66).
Simulating Cope’s Rule.
We simulated Cope’s or Depéret’s rule (23)—the general tendency for increasing body sizes through time—to check whether this trend could artificially favor the support of our climatic model. We simulated evolution toward larger size as taxa chasing an increasing size optimum (67) using a generalization of the OU model (also called Hull–White model) (4):
[4] |
We simulated an adaptive optima changing either linearly through time according to or linearly as a function of temperature according to Bergman’s rule (15, 22). Our simulations were run on the phylogenies corresponding to each order with two sets of parameter values. We chose values corresponding to a phylogenetic half-life [time for the OU process to reach one-half the time to stationarity (50)], representing and of the tree height; was chosen to be times the observed trait variance [as expected under the stationary condition (50)], and was fixed to 0.02 (0.02 in the case of the optima tracking temperature). Simulations were performed recursively using a forward algorithm from the root to the tips using our own code.
Assessing the Effect of Episodic Bursts of Phenotypic Evolution.
It has been proposed that phenotypic evolution in most vertebrate groups proceeds by rare but substantial bursts along isolated branches (24, 39) [from a 2- to a 52-fold increase, with median value around five in the mammalian supertree (figure 1B in ref. 24)] and that such bursts might drive the support of homogeneous models estimated over entire clades (24). We believe this to be unlikely, because the pattern of interspecific covariances for a process of punctuated evolution with large normally distributed changes is expected to be almost nondifferentiable from that of a BM process (18). We nevertheless tested the possibility that localized shifts in trait evolution artificially favor support for our climatic models using simulations. For each order-level phylogeny, we performed 1,000 simulations of Brownian evolution with localized shifts in . Each simulation consisted of randomly selecting edges in the tree where shifts occur (the number of shifts was a proportion ranging from 1 to of the number of species in each order). The amplitude of each shift was drawn from a truncated log-normal distribution with mean = 1.5, variance = 0.5, and lower and upper bounds = 2 and 52, respectively; these parameters reproduce the range of rate increases previously observed on mammals, with a median value around five (24). The simulations were performed by stretching the randomly selected branches according to the selected rate increases before simulating a homogeneous Brownian process with using the recursive function “rTraitCont” from the R package ape (68). We then fitted eight competitive models to each simulated dataset and compared their relative fits.
Testing Whether Specificities of the Temperature Curve Matter.
To test whether the fit of the climatic model could be explained by the overall cooling trend over the Cenozoic rather than specificities of the temperature curve, we assessed the impact of increasingly smoothing the temperature curve on the support of the Clim-exp model. We used cubic splines with a decreasing effective number of dfs to smooth the curve (69). For each degree of smoothing, we computed the proportion of trees from the posterior distribution of 1,000 trees for which the fit with the smoothed climatic curve remains as good as with the original curve ) (SI Appendix, Figs. S22–S24). The AIC threshold of four represents a useful approximation for the confidence set on the reference (unsmoothed) model (54).
Assessing the Robustness to ME.
We used simulations to test if ME in the body size data could artificially drive the observed climatic signal. We first derived empirical distributions of ME for each bird order using data from ref. 70 (SI Appendix). Next, for each order, we simulated tip data under BM and OU on 1,000 trees from the posterior distribution, and on each of these tip data, we added ME drawn from the empirical distribution (SI Appendix). Finally, we conducted our model fitting procedure on the resulting simulated data.
To refine our understanding of what type of climatic signal ME would spuriously create or in contrast, blur, we conducted time bin analyses. For each order, we sliced trees from the posterior distribution into 2.5-Ma time bins using the “make.era.map” function in phytools (71). We then jointly estimated maximum likelihood rates for each time bin using the “mvBM” function in mvMORPH (44). We performed these analyses on the empirical body size data and data simulated under BM and OU and with ME as described above. Finally, we reported estimated differences in rates (both empirical and simulated) corresponding to a cold period spanning most of the Oligocene (33.9–25 Ma) and a warm period spanning from the late Oligocene to the mid-Miocene (25–16 Ma). Average rates on these periods were obtained by computing the mean rates across the corresponding time bins (the periods were approximated to span 35–25 and 25–15 Ma, respectively, to match the time bins). This approach is useful to visually inspect temporal trends and focus on specific time periods; however, the uncertainty around estimates in each time bin is high and hampers the statistical assessment of general climatic effects in contrast to our proposed framework.
Supplementary Material
Acknowledgments
We thank Olivier Billaud, Jonathan P. Drury, Eric Lewitus, Odile Maliet, Marc Manceau, Olivier Missa, Graham Slater, and Marius Somveille for helpful comments on the manuscript. This research was supported by European Research Council Grant ERC 616419-PANDA and Agence Nationale de la Recherche Grant ANR ECOEVOBIO (to H.M.).
Footnotes
The authors declare no conflict of interest.
This article is a PNAS Direct Submission. L.J.H. is a Guest Editor invited by the Editorial Board.
This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1606868114/-/DCSupplemental.
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