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. 2014 Apr 8;197(2):769–780. doi: 10.1534/genetics.114.164822

Effects of Overlapping Generations on Linkage Disequilibrium Estimates of Effective Population Size

Robin S Waples *,1, Tiago Antao , Gordon Luikart
PMCID: PMC4063931  PMID: 24717176

Abstract

Use of single-sample genetic methods to estimate effective population size has skyrocketed in recent years. Although the underlying models assume discrete generations, they are widely applied to age-structured species. We simulated genetic data for 21 iteroparous animal and plant species to evaluate two untested hypotheses regarding performance of the single-sample method based on linkage disequilibrium (LD): (1) estimates based on single-cohort samples reflect the effective number of breeders in one reproductive cycle (Nb), and (2) mixed-age samples reflect the effective size per generation (Ne). We calculated true Ne and Nb, using the model species’ vital rates, and verified these with individual-based simulations. We show that single-cohort samples should be equally influenced by Nb and Ne and confirm this with simulated results: N^b was a linear (r2 = 0.98) function of the harmonic mean of Ne and Nb. We provide a quantitative bias correction for raw N^b based on the ratio Nb/Ne, which can be estimated from two or three simple life history traits. Bias-adjusted estimates were within 5% of true Nb for all 21 study species and proved robust when challenged with new data. Mixed-age adult samples produced downwardly biased estimates in all species, which we attribute to a two-locus Wahlund effect (mixture LD) caused by combining parents from different cohorts in a single sample. Results from this study will facilitate interpretation of rapidly accumulating genetic estimates in terms of both Ne (which influences long-term evolutionary processes) and Nb (which is more important for understanding eco-evolutionary dynamics and mating systems).

Keywords: age structure, life history, iteroparity, ldne, computer simulations, AgeNe, effective number of breeders


THE recent explosion of population genetic information for nonmodel species has been driven by the confluence of several developments: nonlethal methods for sampling DNA in natural populations, rapid increases in availability of a large number of molecular markers, increases in computational power, and more sophisticated data analysis software (Beaumont and Rannala 2004; Excoffier and Heckel 2006; Allendorf et al. 2010). One result of this information explosion has been a surge in the use of genetic methods to estimate effective population size (Wang 2005; Leberg 2005; Luikart et al. 2010), fueled largely by a 10-fold increase over the last 3–5 years in estimates based on single-sample methods [as opposed to the two-sample temporal method] (Palstra and Fraser 2012). Effective population size is the evolutionary analog of census size (N). Whereas N governs ecological processes such as competition, predation, and population growth rate, evolutionary processes (including the rates of genetic drift and loss of genetic variability and the effectiveness of selection and gene flow) depend primarily on the effective size of the population, which is generally lower than the census size because of disparities among individuals in their genetic contribution to the next generation (Frankham 1995).

Although most genetic methods for estimating effective size use models that assume discrete generations, they are widely applied to iteroparous species with overlapping generations. For such species, two related quantities are of interest: effective size per generation (Ne) and the effective number of breeders in one reproductive cycle (Nb). Ne is more important in shaping long-term evolutionary processes, and almost all population genetic theory is based on the concept of Ne per generation (Crow and Kimura 1970; Charlesworth 2009). However, many eco-evolutionary processes in age-structured species (such as sexual selection) play out in a theater defined by seasonal bouts of reproduction, for which Nb is a more relevant parameter than Ne (see Waples and Antao 2014). Furthermore, Nb is easier to estimate and monitor for long-lived species, because it requires data only for one breeding season rather than the species’ entire life span (Schwartz et al. 2007). A few of the many recent articles that use genetic methods to estimate Nb in natural populations include Côté et al. (2013), Duong et al. (2013), and Whiteley et al. (2014). The relationship between Nb and Ne for semelparous, age-structured species (e.g., Pacific salmon and monocarpic plants) was worked out by Nunney (2002), Vitalis et al. (2004), and Waples (2002, 2006), but those analyses did not consider effects of iteroparity.

As a result of these developments, researchers faced with the task of trying to interpret the rapidly accumulating body of estimates of effective size in iteroparous species have faced two major difficulties: (1) How does one know whether a particular genetic estimate is more applicable to Ne or to Nb—or is not a reasonable proxy for either one? (2) What is the relationship between Ne and Nb in iteroparous species? A recent study (Waples et al. 2013) that calculated both Ne and Nb from published demographic data for 63 species of animals and plants provides new insights into the second question. The ratio Nb/Ne varied a surprising sixfold across species and, unexpectedly, Nb per season was larger than Ne per generation in over half the species. However, up to two-thirds of the variance in Nb/Ne was explained by just two life history traits (age at maturity and adult life span). Factors that produce high Nb/Ne ratios include early maturity combined with a long life span, constant fecundity with age, and Poisson variance in reproductive success of same-age, same-sex (SASS) individuals; factors that produce low Nb/Ne ratios include delayed maturity combined with a short adult life span, large variations in fecundity with age, and overdispersed variance of SASS individuals (Waples et al. 2013). These results suggest that, for the first time, it should be possible to translate estimates of Nb in iterporarous species into estimates of Ne per generation, as long as one can estimate some basic life history traits for the target species. That study, however, was based entirely on the species’ vital rates and did not consider population genetics data.

Here we tackle the first major information gap identified above: What biases associated with age structure are involved in estimating Ne or Nb from genetic data for iteroparous species, and how do the patterns of bias depend on the life history of the target species and the experimental design? Robinson and Moyer (2013) made a start at addressing these issues by simulating age-structured data for three species and applying the single-sample genetic estimator based on linkage disequilibrium (LD) (Hill 1981; Waples and Do 2008). We considerably expand this approach, using simulated data for 21 iteroparous species, selected for taxonomic and life history diversity from the larger set examined by Waples et al. (2013). We used the simulated data to evaluate two published but untested hypotheses regarding performance of the LD method: (1) estimates based on samples from a single cohort primarily reflect Nb (Waples 2005), and (2) mixed-age samples drawn from a number of cohorts equal to a generation length (e.g., 3 cohorts for a sparrow or ∼10 for a grizzly bear) provide a reasonable estimate of Ne (Waples and Do 2010).

We show that the pattern of bias in estimates of effective size (N^e or N^b) from the LD method is determined primarily by the actual ratio Nb/Ne for the target species. Because the Nb/Ne ratio can be predicted from simple life history traits (Waples et al. 2013), this provides a generally applicable, quantitative means of adjusting LD estimates of effective size to produce largely unbiased estimates of Nb or Ne in iteroparous species. We also quantify the effects of variation in some important life history features (intermittent breeding by females, constraints on litter size, overdispersed variance in reproductive success, and skewed primary sex ratio) that are not accounted for in most models but are important for many real species.

Methods

Model species

Notation and definitions are provided in Table 1. Our analyses focused on 21 of the 63 species analyzed by Waples et al. (2013), including three plants, three invertebrates, two amphibians, two reptiles, three fish, three birds, and six mammals; see Supporting Information, Table S1. For some analyses we also evaluated a synthetic “species” based on generic vital rates (age-specific survival and fecundity) used in figure 1A of Waples et al. (2011). The vital rates for each model species (which are provided in Appendix S2 in Waples et al. 2013) were used in two major ways: (1) to calculate Ne and Nb using a hybrid Felsenstein–Hill method [AgeNe (Waples et al. 2011)], and (2) to parameterize simulations of age-structured genetic data. We then estimated effective size from the simulated genetic data, using the LD method, and assessed bias by comparing the estimates with the true Ne and Nb. These processes are described in more detail below.

Table 1. Definitions and notation used in this study.

Ne Effective population size per generation
Nb Effective number of breeders in one time period
N^b,N^e An estimate of Nb or Ne based on genetic data
N^b(Adj) An estimate of Nb adjusted to account for bias due to age structure
NT Total number of individuals age 1 and older alive at any given time
NA Total number of adults (individuals with age ≥α) alive at any given time
N1 Total number of offspring produced per time period that survive to age 1
x Age (units can be days, weeks, months, or years)
sx Probability of surviving from age x to age x + 1
lx Cumulative probability of surviving to age x (lx=i=1xsi1, with s0 = l1 = 1)
bx Mean number of offspring in one time period produced by a parent of age x
ω Maximum age
α Age at maturity (first age with bx > 0)a
AL Adult life span = ωα + 1
Gen Generation length (mean age of parents of a newborn cohort)
CVf Coefficient of variation of bx for adult life span (using only ages with bx > 0)b
HMean Harmonic mean
SASS Individuals of the same age and sex
a

This follows the definition used by Waples et al. (2013), who adopted a simple rule to deal with a large number of diverse data sets. When sufficient data are available, a more precise estimate would be age at which 50% are mature or weighted age at first maturity.

b

When bx varied between sexes, CVf was computed over data for both sexes, after standardizing bx to values that produce a population of constant size.

Analysis of vital rates

AgeNe uses a discrete-time, age-structured, and deterministic model. Individuals of age x produce an average of bx offspring and then survive to age x + 1 with probability sx. Both bx and sx can differ between males and females. We track only individuals that survive to their first birthday, so fecundities are scaled to result in a stable population that produces a fixed number (N1) of individuals per cohort that survive to age 1. Given a specified value for N1 and a life table of vital rates, AgeNe calculates the total population size (NT), the adult population size (NA), and numbers in each age class (Nx), as well as Ne and Nb. NT, NA, Ne, and Nb all scale linearly with N1, but ratios of these key variables are independent of N1.

AgeNe uses a species’ vital rates to calculate mean (k¯) and variance (Vk) of lifetime reproductive success for the N1 individuals in a cohort. The modeled populations are constant in size, so E(k¯) = 2, in which case the generational effective size for the population is given by

Ne4N1GenVk+2 (1)

(Hill 1972, equation 16), where Gen = generation length = mean age of parents of a newborn cohort. From the vital rates, AgeNe also calculates the mean and variance (k¯ and Vk) in the number of offspring produced in one reproductive cycle by all NA adults in the population. These data are then used to calculate inbreeding Nb for each cycle as (Crow and Denniston 1988; Caballero 1994)

Nb=k¯NA2k¯1+Vk/k¯. (2)

The following assumptions of AgeNe follow those of Felsenstein (1971) and Hill (1972): (1) all reproduction occurs at intervals of exactly one time unit (on an individual’s birthday), (2) survival and fecundity are independent of events in previous time periods, and (3) there is no upper bound to the number of offspring an individual can produce in one breeding cycle. In addition, we adopted the following assumptions for what we refer to as the standard model: each newborn had an equal probability of being male or female, and SASS individuals had Poisson variance in reproductive success (so Vk = k¯).

We also considered the following variations of the standard model, using subsets of the model species: skewed primary sex ratio, overdispersed variance in reproductive success of SASS individuals, intermittent breeding by females, and small litter/clutch size. The first two variations were evaluated using AgeNe; for intermittent breeding and small litter size, we used results developed by Waples and Antao (2014).

Computer simulations

We used the forward-time, individual-based program simuPOP (Peng and Kimmel 2005; Peng and Amos 2008) to simulate realistic, age-structured genetic data for each of the study species. Each simulation tracked both demographic and genetic processes for 100 time periods, with each period representing one reproductive cycle (measured in days, months, or years, depending on the species; Table S1). Demographics were governed by the same vital rates used in the AgeNe analyses described above.

In time period 0, the age of each of the NT individuals was drawn randomly from the stable age distribution. Because survival and reproduction were random and independent, total population size, and the number of each sex in each age class, varied randomly around the mean values expected in a stable population. Furthermore, although the primary sex ratio varied randomly around 0.5, the adult sex ratio could differ from this due to sex-specific survival rates and ages at maturity. Each newborn individual “picked” its two parents by drawing one male and one female randomly from the pool of potential parents, with the probability of choosing a parent of age x proportional to bx for that sex. Thus, all potential parents of the same sex and age had an equal opportunity to be the parent of each newborn, but that was not necessarily true for individuals of different ages or sex. After a burn-in period of 50 cycles (more than enough to allow approximate demographic and genetic equilibrium; Figure S1), we tracked demographic and genetic parameters for another 50 cycles before starting another replicate. Twenty replicates were run for each scenario, which provided 20 × 50 = 1000 time periods for sampling. Multiple temporal samples within each simulation are not entirely independent, but (as shown in Results) overall replication was more than sufficient to produce robust measures of central tendency.

Analysis of simulated data

Beginning in time period 51, we tracked lifetime production of offspring by each of the N1 newborns in a single cohort, and from these data we calculated lifetime k¯, Vk, and Ne from Equation 1. We also calculated seasonal k¯, Vk, and Nb for each reproductive cycle. Arithmetic means of these means and variances, and harmonic means of Ne and Nb, were calculated across replicates and compared with values predicted by analysis of the vital rates, using AgeNe. Negative and infinite estimates of effective size were converted to 106 (see Waples and Do 2010 for a discussion of how to interpret negative estimates of effective size).

For the genetic analyses, because we are interested in evaluating potential biases related to age structure rather than precision, we used large samples (S = 100 individuals) and a large number (100) of “microsatellite-like” markers, each having 10 possible allelic states. Allele frequencies for each locus in each replicate were separately initialized using a Dirichlet distribution with equal prior for each allele. The simulations covered only relatively few generations, so mutation was ignored. Multilocus genotypes in offspring were generated randomly, assuming simple Mendelian inheritance from the two randomly chosen parents. During the period of sampling, heterozygosities were generally in the range 0.7–0.85, comparable to what is found for microsatellite data in many natural populations. For model validation, we conducted longer runs (50 cycles burn-in + 550 cycles = 600 cycles total) for selected species to track the loss of heterozygosity over time and compare that with the rate expected given the values calculated by AgeNe for Ne and generation length.

Following Waples and Yokota (2007), in each of the 1000 replicate time periods we used three sampling strategies for the genetic data: (a) only newborns (i.e., a single cohort), (b) only adults, and (c) all individuals in the population. We also considered samples from two or three consecutive cohorts. In each case, individuals were sampled randomly without replacement from these targeted groups; for the population and adult samples, this meant that samples were skewed toward younger individuals. For each sample, we used the genetic data to estimate effective size, using the LD method implemented in LDNe (Waples and Do 2008). The LD method is based on the following relationship for unlinked loci, as assumed here (Hill 1981),

E(r2)1(3Ne),soN^b=1(3r2), (3)

where r2′ is the squared correlation of alleles at different loci and is an index of the amount of disequilibrium due to drift, after accounting for effects of sampling. We screened out alleles at frequencies <0.05 because Waples and Do (2010) found this minimized bias for samples sizes of ≥50.

Performance of bias adjustments was evaluated by calculating the percent root mean-squared bias (RMSB), which is analogous to the root mean-squared error except that our analysis focuses on bias and does not include a term for precision. We calculated the percent RMSB as 100[(1N^b/Nb)2]/21, where the summation is across all 21 model species, or the equivalent for Ne.

Results

Model validation

We first verified that demographic data generated by simuPOP were consistent with analytical expectations from AgeNe based on each species’ vital rates. As expected for dynamically stable populations, lifetime k¯ from the simulations was almost exactly 2.0 in every species. Similarly, mean lifetime Vk, Ne per generation, and Nb per cycle calculated from the demographic data were within 1% of the expected (AgeNe) values for most species and within 4% for all species (Table 2). Simulated Nb was slightly higher than expected in a few species, a result that can be attributed to small numbers of individuals in older age classes. For example, Nb/E(Nb) for bison, bottlenose dolphin, and grizzly bear was 1.015–1.024 for small (100–200) values of N1, but this slight disparity largely disappeared for N1 = 1000 [Nb/E(Nb) = 1.001–1.004; Table 2].

Table 2. Demographic data for the modeled species.

Per generation Per cycle
Species N1 Gen Vk E(Vk) Vk/E(Vk) Ne E(Ne) Ne/E(Ne) Nb E(Nb) Nb/E(Nb) N^b/E(Nb)
Mole crab 1000 12.8 187.72 190.41 0.986 270.4 266.1 1.016 133.7 131 1.021 1.137
Mosquito 50 22.5 3.75 3.83 0.979 781.9 771.2 1.014 214.3 206 1.040 1.136
Sea urchin 500 1.5 3.92 3.92 1.000 517.2 517.8 0.999 655.5 656 0.999 0.864
Primrose 500 8.4 42.34 41.96 1.009 380.1 382.8 0.993 456.9 457 1.000 0.862
Sagebrush 200 7.8 17.54 17.35 1.011 318.7 322.8 0.987 514.3 518 0.993 0.739
Seaweed 500 8.3 27.37 27.35 1.001 565.9 566.9 0.998 714.4 715 0.999 0.838
Cascade frog 1000 3.3 25.45 25.36 1.003 484.3 485.4 0.998 243.4 244 0.998 1.078
Wood frog 2000 2.1 28.26 28.10 1.006 556.4 559.4 0.995 332.9 335 0.994 1.057
Great tit 500 1.9 4.31 4.30 1.002 590.5 591.9 0.998 856.0 854 1.002 0.801
Sage grouse 200 3.9 5.23 5.25 0.996 426.8 425.3 1.004 733.1 720 1.018 0.739
Sparrow 1000 3.0 30.48 30.41 1.002 369.5 370.0 0.999 363.3 365 0.995 0.934
Atlantic cod 2000 12.9 443.60 443.90 0.999 231.4 230.8 1.003 161.1 161 1.001 1.043
Brown trout 5000 8.0 494.77 491.97 1.006 320.8 321.8 0.997 154.2 155 0.995 1.116
Sardine 1000 5.9 28.94 28.94 1.000 756.8 757.7 0.999 800.4 801 0.999 0.903
Bison 200 7.4 12.40 12.44 0.997 408.9 409.0 1.000 401.0 395 1.015 0.947
Bison 1000 7.4 12.46 12.44 1.002 2039.8 2043.1 0.998 1985.0 1978 1.004 0.947
Bighorn sheep 200 5.7 6.80 6.80 1.000 520.4 521.5 0.998 641.5 640 1.002 0.858
Bottlenose dolphin 100 14.7 8.91 9.04 0.986 538.8 533.2 1.011 526.5 514 1.024 0.944
Bottlenose dolphin 1000 14.7 9.03 9.04 0.999 5334.5 5331.6 1.001 5163.0 5158 1.001 0.944
Elephant seal 500 7.9 31.38 30.99 1.013 471.0 477.2 0.987 211.3 211 1.001 1.156
Grizzly bear 100 10.5 8.88 8.92 0.996 386.0 385.2 1.002 455.2 444 1.025 0.854
Grizzly bear 1000 10.5 8.90 8.92 0.998 3861.2 3852.0 1.002 4473.5 4461 1.003 0.854
Red deer 100 8.4 2.57 2.58 0.995 734.8 732.2 1.004 625.4 607 1.030 1.008
Green snake 400 2.5 6.93 6.93 1.000 447.4 447.5 1.000 607.9 608 1.000 0.827
Synthetic 250 2.6 4.07 4.08 0.997 430.6 429.6 1.002 503.3 501 1.005 0.886

Observed values from simulations are compared to expected values from AgeNe based on age-specific survival and fecundity for each model species. See Table S1 for the model species’ life history information and Table 1 for notation. Not shown are empirical values for k¯ (mean lifetime number of offspring), which were all within 0.25% of the expected value of 2.0. The last column shows how raw (unadjusted) genetic estimates from single cohorts compare to true Nb.

For 10 species we also verified that modeled populations lost heterozygosity at the rate expected based on the nominal Ne value obtained from AgeNe. Results (Figure 1) show that, despite the random demographic variability generated in the simulations, actual rates of genetic drift in the modeled populations agreed closely with theoretical expectations. These results supported the use of effective sizes calculated by AgeNe to represent the true Ne and Nb for each scenario. We then assessed bias in the genetically based estimates by comparing these AgeNe values with LDNe estimates for each sample of genotypes simulated with simuPOP.

Figure 1.

Figure 1

Comparison of observed Ne (based on rate of loss of heterozygosity in simulated populations) and the expected value (calculated from AgeNe based on published vital rates). Results are shown for nine modeled species, in addition to the synthetic life table used in Waples et al. (2011).

Genetic estimates of Nb

Samples from single cohorts:

Waples (2005) suggested that when the LD method is used based on such samples, the estimate primarily reflects Nb in the parents that produced the cohort. However, those results were for a model involving semelparity with variable age at maturity, as occurs in Pacific salmon and some other species, and its applicability to iteroparous species remains untested. We can refine the expectation for N^b for iteroparous species as follows. Assuming selective neutrality, the amount of LD in a closed population with discrete generations is the sum of two quantities: (1) residual or “background” LD from previous generations that has not broken down by recombination between loci and (2) new LD generated by reproduction of a finite number of individuals (Hill and Robertson 1968). If the population is stable in size, overall LD reaches an equilibrium value characteristic of Ne and the recombination rates of the loci involved (Sved 1971). At that point, creation of new LD each generation must exactly compensate for the LD lost through recombination. When loci are unlinked, half of the existing LD decays each generation, so (from Equation 3) the expected amount of residual LD left after recombination is E(r2′) ≈ 1/(6Ne). At equilibrium, therefore, the same amount must be newly generated by mating of Ne effective individuals each generation.

If population size changes, the residual disequilibria and the newly generated disequilibria reflect different effective sizes, and an estimate of Ne based on r2′ can be biased upward or downward for a few generations (Waples 2005). Something like this occurs within age-structured populations. LD generated by breeders in a single time period is a function of Nb, while residual LD in the population as a whole is a function of Ne. In general, therefore, we expect that in the progeny of parents that reproduce in a single time period, the total amount of drift LD can be approximated by

E(r2)1(6Ne)+1(6Nb)=1/Ne+1/Nb6. (4)

If Ne = Nb, this simplifies to Hill’s relationship E(r2′) ≈ 1/(3Ne). More generally, if we note that the harmonic mean of Ne and Nb is HMean(Ne, Nb) = 2/(1/Ne + 1/Nb), then (1/Ne + 1/Nb) = 2/HMean(Ne, Nb), and making this substitution in Equation 4 produces

E(r2)(16)×2HMean(Ne,Nb)=13×HMean(Ne,Nb). (5)

That is, when Ne and Nb differ, the amount of LD in a sample from a single cohort should be a function of the harmonic mean of Ne and Nb. It follows that if Ne is larger than Nb, the amount of residual LD will be smaller than would typically occur in a population with Ne = Nb, and N^b should be upwardly biased. The reverse should occur when Ne < Nb, while there should be little bias for species for which Ne and Nb are about the same magnitude (e.g., sparrow, sardine, and bison; Table S1).

The 21 species modeled here exhibit the full range of values for the ratio of Nb to Ne considered in the larger study by Waples et al. (2013) (from Nb/Ne = 0.267 in the mosquito to Nb/Ne = 1.694 in the sage grouse; Table S1). When analyzing samples from a single cohort, the ratio of estimated Nb (N^b) to true Nb in these species clustered around 1.0 (Table S1). However, for 10 species N^b was >10% lower than true Nb, and for 4 species the estimate was >10% too high. The species with the strongest downward bias were the sage grouse and the sagebrush (both with N^b/Nb = 0.74), while the strongest upward bias (N^b/Nb = 1.14) occurred in the mole crab and the elephant seal.

The relationship between N^b and HMean(Ne, Nb) was almost perfectly linear (r = 0.992), with slope that did not differ significantly from 1 (b = 1.015 ± 0.029) (Figure 2A). Consistently, however, N^b was slightly lower (median = 7% lower) than HMean(Ne, Nb). We believe this reflects a factor not accounted for in Equation 5 above: in each cycle the newborn cohort is produced by matings among parents of a variety of ages, who themselves were progeny of different groups of parents with slightly different allele frequencies. This produces a type of mixture LD [a two-locus Wahlund effect (Nei and Li 1973; Sinnock 1975)] in the parents every cycle, and (for unlinked loci) half of this is passed on to their offspring.

Figure 2.

Figure 2

Bias associated with genetic estimates of Nb when using samples from a single cohort. (A) Relationship between N^b and the harmonic mean of true Ne and Nb for 21 model species and one synthetic life table. Dotted line is the expectation based on Equation 3 in the text; solid line is regression for empirical data. (B) Pattern of bias in N^b as a function of the ratio Nb/Ne. Solid circles are results for model species from this study; open triangles are from Robinson and Moyer (2013) for comparable analyses (single-cohort samples of 100 individuals; N^b calculated from LDNe, using Pcrit = 0.05 criterion for screening out rare alleles). The regression line is plotted using only data from this study.

Although the relationship in Figure 2A is striking, it does not provide a practical method for accounting for effects of both true Ne and true Nb on N^b. Fortunately, this can be accomplished with a simple rearrangement of the variables. Combining Equations 3 and 4 produces the following when considering use of single-cohort samples to estimate Nb:

E(N^b)1(3r2)=6/31/Ne+1/Nb=2(Ne+Nb)/(Ne×Nb). (6)

We wish to find an expression for the relative bias in N^b (measured by N^b/Nb = the ratio of estimated and true Nb) as a function of the ratio Nb/Ne, because we know the latter can be estimated from life history data independent of the absolute magnitude of Ne or Nb (Waples et al. 2013). Dividing each side of Equation 6 by Nb gives

E(N^b)Nb2/Nb(Ne+Nb)/(Ne×Nb)=21+Nb/Ne. (7)

Equation 7 predicts a curvilinear relationship between the index of bias (N^b/Nb) and the ratio of seasonal and generational effective size (Nb/Ne). However, this is not a good fit to the empirical data for the model species, even when Equation 7 is adjusted to account for the Wahlund effect (Figure S2). Instead, the relationship between N^b/Nb and Nb/Ne was almost perfectly linear in the model species (r2 = 0.984; Figure 2B). As expected from Equation 5, N^b consistently overestimates Nb in species for which true Ne is larger than true Nb, consistently underestimates Nb in species for which Ne < Nb, and is relatively unbiased in species for which Nb and Ne are approximately equal. Actually, the “no bias in N^b” point occurs with Nb slightly larger than Ne (Figure 2B), which reflects the fact that N^b in Figure 2A is slightly lower than HMean(Ne, Nb), due presumably to the mixture LD from age structure mentioned above.

A bias adjustment for N^b:

A simple adjustment to raw N^b can remove most of the bias. Rearrangement of the regression in Figure 2B leads to the following:

N^b(Adj)=N^b1.260.323×(Nb/Ne). (8)

Figure 3 shows that after applying this correction, adjusted N^b(Adj) was within 5% of the true value for all 21 study species.

Figure 3.

Figure 3

Effects of adjusting bias in raw N^b for each model species, based on information for two life history traits (AL and α), three life history traits (AL, α, and CVf), or the true ratio Nb/Ne. Samples were taken from single cohorts.

Unless they have detailed demographic information for their target species, researchers will not know the true ratio Nb/Ne, but this can be predicted from just two or three simple life history traits (Waples et al. 2013). Using the ratio of two traits [adult life span (AL) and age at maturity (α)], this relationship holds: Nb/Ne = 0.485 + 0.758 log × (AL/α); adjusted r2 = 0.67. With the addition of CVf (an index of variation in fecundity with age), the relationship becomes Nb/Ne = 0.833 + 0.637 log × (AL) – 0.793 × log(α) – 0.423 × CVf; adjusted r2 = 0.84. Inserting these results into Equation 8 produces the bias adjustments shown in Table 3, based on life history traits of the study species. Figure 3 also shows how the pattern of bias in the 21 species is reduced by adjusting N^b based on two or three life history traits.

Table 3. Formulas to adjust genetic estimates of effective size to correct biases due to age structure.
Method Formula
To estimate Nb
 Using true Nb/Ne N^b(Adj)=rawN^b1.260.323×(Nb/Ne)
 Using two traits N^b(Adj2)=rawN^b1.1030.245×log(AL/α)
 Using three traits N^b(Adj3)=rawN^b0.9910.206×log(AL)+0.256×log(α)+0.137CVf
To estimate Ne
 Using true Nb/Ne N^e(Adj)=N^b(Adj)Nb/Ne
 Using two traits N^e(Adj2)=N^b(Adj2)0.485+0.758×log(AL/α)
 Using three traits N^e(Adj3)=N^b(Adj3)0.833+0.637×log(AL)0.793×log(α)0.423×CVf

Raw N^b is the unadjusted estimate obtained using the LD method from a sample from a single cohort. AL, adult life span; α, age at maturity; CVf, an index of variation in age-specific fecundity (see Table 1 for definitions and notation). Different adjustments are provided, depending on whether the goal is to estimate Nb or Ne and on the type of information available for the species of interest (data for two or three life history traits or an estimate of true Nb/Ne). Adjustments based on Nb/Ne use results from AgeNe and the regression shown in Figure 2B; adjustments based on two or three life history traits use the relationships described in Waples et al. (2013).

We illustrate these adjustments using data for the great tit, Parus major. From Table S1 we see that α = 1, AL = 8, AL/α = 8, CVf = 0.249, and true Nb/Ne = 1.443. For the simulated data and sampling from a single cohort, N^b = 684, 20% lower than the true value of 854. If all one knew was that the ratio AL/α was ∼8, the two-variable formula in Table 3 could be used to adjust the raw estimate: N^b(Adj2) = 684/[1.103 – 0.245 × log(8)] = 684/0.882 = 776. This would cut the bias by about half. If one also could estimate the variation in age-specific fecundity, a (generally) more accurate adjustment could be made using the three-variable formula from Table 3: N^b(Adj3) = 684/[0.991 − 0.206 × log(8) + 0.256 × log(1) + 0.137 × 0.249]= 684/0.839 = 815, which is closer but still ∼5% too low. Finally, if one knew the true Nb/Ne ratio, the optimal adjustment would be N^b(Adj) = 684/[1.26 – 0.323 × 1.443] = 684/0.794 = 862, which is just under 1% too large.

Figure 4 shows how adjustments to N^b in Table 3 reduced the percent RMSB in the 21 model species. The raw (naive) estimate of Nb has a typical bias of ±14%, and this can be reduced sevenfold (to 2%) if one knows the Nb/Ne ratio. If Nb/Ne is estimated from two life history traits, the RMSB can be reduced by more than half (to 6.3%) compared to the naive N^b, and with information for three traits the RMSB can be nearly halved again (to 3.3%).

Figure 4.

Figure 4

Percent root mean-squared bias in N^b and N^e and how it changes when raw estimates are adjusted per formulas in Table 3, using true Nb/Ne or information for two or three life history traits. Results apply to samples from single cohorts and are averaged across the 21 model species.

Samples from multiple consecutive cohorts:

Often it is easier to sample mixed-age individuals than it is to collect individuals from a single cohort. Furthermore, even when sampling individual cohorts is feasible, sample sizes can be so small that it is necessary to combine individuals from several cohorts (e.g., Skrbinšek et al. 2012). To examine these scenarios, for 16 of the modeled species we evaluated how the pattern of bias in N^b changes when samples are taken randomly and in equal proportions from either two or three consecutive cohorts.

Again, the general pattern of bias depends on the ratio Nb/Ne (Figure 5; see also Figure S4, Figure S5, Figure S6, Figure S7, Figure S8, and Figure S9). When Nb << Ne (as in the elephant seal), N^b from a single cohort is higher than true Nb and increases when the sample combines two or three cohorts; when Nb >> Ne (as in the great tit), N^b from a single cohort underestimates true Nb and the downward bias increases when the sample combines two or three cohorts; when NbNe (as in the bison), there is little bias for any of these sampling schemes. Results for all species are plotted in Figure S3A, which includes the regression line from Figure 2B based on single-cohort samples; Figure S3A shows that multiple-cohort samples follow the same general pattern, but with stronger overall bias. The ratio Nb/Ne is a good quantitative predictor of bias in N^b for samples from two or three cohorts; the relationship is strong for Nb/Ne > 0.6, but higher variability for species with low Nb/Ne ratios reduces the overall fit (r2 = 0.79 and 0.77 for samples from two or three cohorts, respectively).

Figure 5.

Figure 5

Effects of different sampling strategies (sampling from one to three consecutive cohorts or randomly from all adults or the population as a whole) on genetic estimates of effective size, using the LD method. Results are shown for three model species with low (elephant seal), medium (bison), and high (great tit) Nb/Ne ratios. The empirical estimates (solid circles and solid lines) are compared to true Ne (dashed-dotted line) and true Nb (dotted line). See Figure S4, Figure S5, Figure S6, Figure S7, Figure S8, and Figure S9 for similar results for all model species.

Genetic estimates of Ne

Samples from single cohorts:

In the case of single-cohort samples, we saw above that it is possible to make quantitative adjustments for bias in N^b, provided one knows the ratio Nb/Ne or can estimate it from life history traits. If so, then it is also possible to obtain an estimate of Ne via a simple two-step process, using the equations in the bottom half of Table 3: (1) calculate the bias-adjusted N^b based on known or estimated Nb/Ne, and (2) divide adjusted N^b by Nb/Ne or by the estimators of Nb/Ne developed by Waples et al. (2013) based on two or three life history traits. If the raw N^b is used naively as an estimate of Ne, the RMSB is twice as large as for an estimate of Nb (Figure 4). If Nb/Ne can be estimated from two life history traits, this bias can be cut in half, and if true Nb/Ne is known, N^e and N^b both have the same low bias (2%).

Population samples:

Another potential strategy to estimate Ne is to sample only mature adults or from the population as a whole; for many species this will be the only feasible option. Waples and Do (2010) speculated that if such samples included enough cohorts to approximately represent a generation, the resulting estimate from the LD method might be close to Ne per generation. We tested this conjecture in two ways. First, we drew samples randomly from all adults; these samples included a number of cohorts equal to the AL for each species. If the conjecture were correct, we would expect that estimates based on these adult samples should converge on true Ne as AL approaches the generation length (Gen) (Table S1 lists AL, Gen, and other life history information for each model species). In every species, estimates based on random samples of adults were lower than true Ne (Figure 5, Figure 6, Figure S4, Figure S5, Figure S6, Figure S7, Figure S8, and Figure S9). However, the least amount of downward bias in N^e occurred in the cod (Figure 6), which is the species for which the number of cohorts in an adult sample is closest to the generation length (AL/Gen = 14/12.9 = 1.09 generations of cohorts; N^e = 91% of true Ne). AL/Gen is also relatively close to 1 for the species with the second-smallest bias (elephant seal; N^e/Ne= 0.86, AL/Gen = 1.46). As AL/Gen increased across species, estimates of Ne based on adult samples generally declined.

Figure 6.

Figure 6

Pattern of bias in estimates of Ne based on random samples of all adults. The number of cohorts represented in a sample of adults is the adult life span (AL). Values on the x-axis (note the log scaling) therefore indicate how many generations of cohorts are included in a sample of adults. The four species for which AL is closest to Gen, as well as some outliers, are indicated.

These results are generally consistent with predictions of the above hypothesis. On the other hand, the results showed considerable variability, and for two other species with 1 < AL/Gen < 1.5 (wood frog and Cascade frog), N^e based on adult sampling was 25–30% lower than true Ne. The only species for which adult samples represented less than one generation of cohorts was the mosquito, for which N^e based on just over one-half of a generation of cohorts showed the strongest downward bias (N^e less than half of true Ne; Figure 6).

A second test of the hypothesis is possible for the four species for which Gen ≤ 3, in which case we can compare estimates based on combined samples from two or three cohorts with true Ne. For the great tit (Gen = 1.9) and wood frog (Gen = 2.1), estimates based on two cohorts were 82% and 101% of true Ne, respectively, and for the Cascade frog (Gen = 3.3) the estimate based on three cohorts was 102% of true Ne. Generation length for the green snake is 2.5, and estimates based on samples from two or three cohorts were 98% and 82% of true Ne, respectively.

Life history variations

By relaxing some of the assumptions of the standard model for AgeNe, we evaluated whether variant life histories change Nb and Ne in ways that would cause a deviation in the pattern of bias depicted in Figure 2B. Analytical methods were used to develop expectations for true Nb and Ne, and we compared these results with demographic estimates of effective size from the age-structured simulations. Results of these analyses are summarized in Table S2, which shows generally excellent agreement between expected (analytical) and observed (simulated) effective sizes. Analytical expectations for effects of intermittent breeding and small litter size on Ne per generation are not available, so we used simulated demographic values for these scenarios to represent true Ne.

Consequences of these life history variations for Nb and Ne can be summarized as follows. Skewed primary sex ratio reduces both Nb and Ne in a predictable way, but the proportional reductions are identical so this does not affect the ratio Nb/Ne (Waples et al. 2013). Overdispersed variance of SASS individuals generally reduces Nb more than Ne and hence reduces the Nb/Ne ratio, but the magnitude of this effect varies considerably across species (Waples et al. 2013). Nb is increased sharply if females can produce only one offspring per litter or clutch; conversely, Nb is reduced if some females are excluded from breeding each season, and the effect is more pronounced for high-fecundity species with type III survival (mosquito and loggerhead turtle) than it is for low-fecundity species with type I survival (bison, dolphin, and grizzly bear) (Waples and Antao 2014). Neither skip breeding nor small litter size had much effect on Ne per generation in these scenarios (Waples and Antao 2014).

Next, we calculated N^b based on single-cohort genetic samples and plotted the pattern of bias as a function of the updated Nb/Ne ratios (Figure 7). It is apparent from these results that bias in N^b for simulated populations with variant life history features is very similar to the pattern found for scenarios that used the standard model. All of the intermittent-breeding and litter-size scenarios produced results that fall closely on the regression line developed for the standard model. A slight (<5%) additional upward bias in N^b was found for some species (sardine and bison) modeled with overdispersed variance in reproductive success.

Figure 7.

Figure 7

Pattern of bias in estimates of Nb for single-cohort samples from simulated populations under life history variations that deviate from the standard model. Solid triangles, maximum litter size is 1 (L1) or females are forced to skip up to four breeding cycles after reproducing; solid circles, skewed (70% male) primary sex ratio; stars, overdispersed variance among same-age, same-sex individuals. For example, “sardine 8M4F” denotes results for simulations using the sardine life table with Vk for males of each age being eight times the mean and Vk for females of each age being four times the mean. The solid line is the regression of N^b/Nb with Nb/Ne under the standard model (from Figure 2B). Data for life history variants for the model species are taken from Table S2.

Discussion

Many natural populations have overlapping generations, whereas most population genetics theory assumes discrete generations and ignores age structure. This disconnect introduces a number of potential biases that have received limited quantitative evaluation. Here, we use verbal arguments and numerical methods to conduct the first comprehensive evaluation of how genetic estimates of effective size based on the single-sample LD method are related to true Nb and true Ne and how this relationship is affected by the species’ life history and the experimental design.

Estimating Nb

We showed using an extension of standard population genetics theory that single-cohort samples for iteroparous species using the LD method should be equally affected by Nb and Ne (Equation 5). Empirical results for simulated age-structured populations confirmed this, although we found that the estimates were consistently slightly lower than HMean(Ne, Nb) (Figure 2A). We attribute this latter result to a type of two-locus Wahlund effect that creates mixture LD when parents of different ages (and with slightly different allele frequencies) mate.

The strongly linear relationship (r2 > 0.98) shown in Figure 2B makes it possible to develop a simple linear adjustment to raw N^b to produce an adjusted estimate that is nearly unbiased, provided the true ratio Nb/Ne is known (RMSB = 2%; Table 3, Figure 3, and Figure 4). If this ratio is not known but can be estimated from two or three simple life history traits (Waples et al. 2013), modified adjustments to N^b are possible (Table 3). The effect of these adjustments in reducing bias can be substantial (Figure 3 and Figure 4).

We used two cross-validation methods to evaluate robustness of the relationship shown in Figure 2B. First, we compared our results to those reported by Robinson and Moyer (2013), who used AgeNe to calculate true Ne and Nb for three age-structured species (mussel, sturgeon, and white-crowned sparrow) and three additional variants of the sparrow fecundity schedule; they then used SPIP (Anderson and Dunham 2005) to simulate age-structured genetic data for these species and used LDNe to estimate effective size. Results for the six Robinson and Moyer “species” are plotted as open triangles in Figure 2B. It is evident that the key relationship derived for our 21 model species also holds for these independently derived estimates of Nb. Second, for a subset of our model species we considered life history variations that can change both Nb and Ne (and hence the Nb/Ne ratio) in ways not accounted for in most standard models. These evaluations created 19 new datapoints not used in deriving the regression between N^b/Nb and Nb/Ne, and these new results clearly reflect the same underlying pattern of bias in N^b (Figure 7). Therefore, we believe the adjustments to raw N^b proposed in Table 3 should be widely applicable to populations in nature. Our simulation results also indicate that mixed samples from two or three cohorts can provide reasonably reliable adjusted estimates of Nb, although the pattern of bias is not quite as predictable as it is for single-cohort samples, particularly for species with Nb/Ne < ∼0.6 (Figure S2 and Table 3).

Estimating Ne

Our empirical results provide some qualified support for the hypothesis (Waples and Do 2010) that a sample that includes as many cohorts as there are in a generation should produce an estimate approximately equal to Ne. For four short-lived species with Gen ≤ 3, estimates based on combined samples from two or three cohorts produced estimates that averaged 93% of true Ne. All estimates based on random samples of adults were smaller than true Ne (Figure 6, Figure S4, Figure S5, Figure S6, Figure S7, Figure S8, and Figure S9), but there was a tendency for the bias to be less when the number of cohorts included in the adult sample corresponded more closely to the generation length (Figure 6).

Fortunately, a more robust approach is possible. Although single-cohort samples have traditionally been thought of as providing information primarily about Nb [based on a model involving semelparous, age-structured species (Waples 2005)], Equation 5 and Figure 2 indicate that both Nb and Ne strongly influence effective size estimates in iteroparous species. This means that samples from single cohorts can also be used to estimate Ne directly, using the bias-adjusted N^b and an estimate of Nb/Ne, as shown in Table 3. The raw estimate from a single-cohort sample is not a reliable indicator of true Ne (RMSB ≈ 28%; Figure 4), but the bias can be cut in half if Nb/Ne can be estimated from two key life history traits, and if enough information about vital rates is available to accurately calculate Nb/Ne, then Ne can be estimated with as much accuracy as Nb (Figure 4). If samples can be obtained from individual cohorts, therefore, this appears to provide the most reliable means for estimating Ne using the LD method.

Caveats

The 21 model species used here to develop the bias adjustments span the full range of true Nb/Ne ratios (0.267–1.694) reported by Waples et al. (2013) in their 63-species study. Nevertheless, care should be taken in extrapolating outside this range. The relationship between N^b/Nb and Nb/Ne becomes more variable for Nb/Ne < 0.5 (Figure 2B); all estimates are upwardly biased, but it is difficult to predict the exact amount of bias. Nevertheless, even accounting for these uncertainties, residual bias after applying the proposed corrections should be no larger than ∼5–10%, which is relatively small considering the other sources of uncertainty typically associated with estimating effective size in natural populations (Wang 2005; Luikart et al. 2010; Palstra and Fraser 2012). It should be noted that because we wanted to focus on effects of age structure, in computing the bias adjustments for N^b (Table 3) we screened out alleles with frequencies <0.05 for the LDNe estimates, as Waples and Do (2010) found that this minimized bias due to rare alleles. Using a more lenient criterion (e.g., 0.02 or 0.01) increases precision but at the cost of some upward bias in the estimates that is not modeled here.

So far our discussion has focused on samples drawn from one or a few cohorts or randomly from all adults. We also present results for random samples from the entire population (Figure 6, Figure S4, Figure S5, Figure S6, Figure S7, Figure S8, and Figure S9), which for some species might be the easiest to obtain. Estimates based on these samples generally produce results that are qualitatively similar to those for adult samples; however, interpretation of whole-population samples is complicated because they can be strongly affected by assumptions about juvenile survival rates, which are poorly known for many species. Mortality before age at maturity does not affect any of the ratios Nb/Ne, Nb/NA, and Ne/NA, but it has a large effect on the proportional representation of different age classes in a sample drawn randomly from the population as a whole. Caution should therefore be used in interpreting results for such samples when estimating effective size in iteroparous species.

Some life history variations can affect Nb more strongly than Ne, which means that it is important to account for these factors in estimating the Nb/Ne ratio. This is particularly true for species with highly overdispersed variance in reproductive success of SASS individuals (Waples et al. 2013), species for which intermittent breeding of females is common, and species for which females can produce only a single offspring per reproductive cycle (Waples and Antao 2014). AgeNe can explicitly account for any user-specified magnitude of overdispersion in Vk, and the analytical methods described by Waples and Antao (2014) can account for effects of intermittent breeding and litter-size constraints. Once these adjustments to the Nb/Ne ratio are made, the pattern of bias follows that developed for standard model scenarios (Figure 7). One life history variant we did not consider is when individuals consistently (across multiple breeding cycles) have higher or lower reproductive success than others in their cohort. Persistent differences like this can reduce Ne (Lee et al. 2011) and perhaps increase the Nb/Ne ratio in ways not accounted for here.

Because of the complexity of the issues involved in evaluating effective size in iteroparous species, our evaluations have focused entirely on bias. Precision also can be a limiting factor for genetic estimates of effective size and is important to consider in any practical application. Fortunately, a number of previous studies have evaluated precision of the LD method under realistic experimental designs with known Ne (England et al. 2010; Tallmon et al. 2010; Waples and Do 2010; Antao et al. 2011; Robinson and Moyer 2013; Holleley et al. 2014), and these should be consulted for general guidelines. Figure S10 depicts the range of variation among replicate N^b estimates among the model species under standard model conditions.

Relationship to previous work

In an evaluation of bias that can result if the standard temporal method (Nei and Tajima 1981) is applied to iteroparous species with overlapping generations, Waples and Yokota (2007) used three model species—one each with type I, type II, and type III survivorship. Subsequently, it has become clear that other life history traits, especially age at maturity and adult life span, have a greater influence on Ne and Nb than does juvenile survivorship (Waples et al. 2013). Accordingly, in this article we used a much larger and taxonomically diverse array of model species.

Wang et al. (2010) proposed a single-sample method based on parentage assignments to estimate Ne and other genetic parameters in species with overlapping generations. This approach uses a modification of Wang’s (2009) sibship method, as implemented in the computer program Colony (Wang 2004); it appears to have considerable potential but requires the user to know the age and sex of each individual in the sample and perhaps as a consequence has not been widely used or evaluated.

Robinson and Moyer (2013) concluded that single-cohort samples generally provide an adequate estimate of Nb; they did not propose a quantitative bias adjustment, but Figure 2B shows that their results fit nicely into the relationship we found between N^b/Nb and Nb/Ne. Robinson and Moyer (2013) also found that random samples of adults produced estimates that were no more than 15% downwardly biased compared to true Ne; in contrast, we found downward bias >15% in 14 of the 16 species we evaluated and ≥30% in 5 species (Figure 6). We believe this difference can be explained by the much wider range of life histories considered in this study: Nb/Ne = (0.267–1.69) in our model species vs. (0.4–0.99) in the species Robinson and Moyer considered and the number of generations of cohorts included in an adult sample = (0.53–4.2) in the present study vs. (1.06–1.72) in Robinson and Moyer’s study.

Conclusions

Genetic estimates of effective size of age-structured populations using the LD method are strongly affected by both Ne per generation and Nb per season or reproductive cycle. This complicates interpretation but also provides a means for correcting bias. Samples from single cohorts are the most amenable to quantitative bias adjustment. If the ratio Nb/Ne is known or can be estimated from two or three simple life history traits, Nb can be estimated with little (≤5–10%) bias. Single-cohort samples also can be used to estimate Ne, albeit with slightly more potential bias. Random samples of adults consistently underestimated true Ne, but the downward bias tended to be less when the number of cohorts in the sample more closely approximated the generation length. Results from this study will facilitate interpretation of rapidly accumulating genetic estimates in terms of both Ne (which influences long-term evolutionary processes) and Nb (which is more important for understanding eco-evolutionary dynamics and mating systems).

Acknowledgments

We thank David Tallmon, Dave Gregovich, and Andres Perez-Figueroa for helping to initiate this project; Joe Felsenstein, Bill Hill, and John Sved for useful discussions; and two anonymous reviewers for useful comments. This work originated within the Genetic Monitoring Working Group, jointly supported by the National Evolutionary Synthesis Center (Durham, NC) and the National Center for Ecological Analysis and Synthesis (Santa Barbara, CA). G.L. was supported in part by funding from US National Science Foundation grants DEB-1258203 and DEB-1067613 and Montana Fish, Wildlife, and Parks; and T.A. was supported by a Sir Henry Wellcome Postdoctoral Fellowship.

Footnotes

Communicating editor: M. W. Hahn

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