The hardware and bandwidth for this mirror is donated by METANET, the Webhosting and Full Service-Cloud Provider.
If you wish to report a bug, or if you are interested in having us mirror your free-software or open-source project, please feel free to contact us at mirror[@]metanet.ch.
The goal of kindisperse is to simulate and estimate close-kin dispersal kernels.
Dispersal is a key evolutionary process that connects organisms in space and time. Assessing the dispersal of organisms within an area is an important component of estimating risks from invasive species, planning pest management operations, and evaluating conservation strategies for threatened species.
Leveraging decreases in sequencing costs, out new method instead estimates dispersal from the spatial distribution of close-kin. This method requires that close kin dyads be identified and scored for two variables: (i) the geographical distance between the two individuals in the dyad, and (ii) their estimated order of kinship (1st order e.g. full-sib; 2nd order e.g. half-sib; 3rd order e.g. first cousin).
Close-kin-based dispersal can provide an estimate of the intergenerational (or parent-offspring) dispersal kernel - a key factor that connects biological events across the lifespan of an organism with broader demographic and population-genetic processes such as isolation by distance. A dispersal kernel is the probability density function describing the distributions of the locations of dispersed individuals relative to the source point. Intergenerational dispersal kernels themselves can be framed in terms of any number of breeding and dispersal processes, defined by both reference life-stage and number of generations, and leave their mark in the spatial distribution of various categories of close kin, which can be treated as samplings from a set of underlying kernels. Actual kernels vary, but are typically described in terms of sigma, the second moment of the kernel, also known as its scale parameter. More complex kernels can also incorporate a parameter for shape or kurtosis (kappa), representing the fourth moment of the kernel.
In the case of an insect like the mosquito, the most basic intergenerational kernel, the lifespan or parent-offspring kernel, reflects all dispersal and breeding processes connecting e.g. the immature (egg, larval, pupal) location of a parent to the immature location of its offspring. However, this kernel can be combined with additional breeding, dispersal and sampling events to produce other, composite dispersal or distribution kernels that contain information about intergenerational dispersal. For example, the distribution of two immature full-sibling mosquitoes reflects not a full lifespan of dispersal, but two ‘draws’ from the component kernel associated with the mother’s ovipositing behaviour. Were we to sample the same full-sibling females as ovipositing adults, this would instead represent two draws from a composite ‘lifespan and additional oviposition’ kernel. Avuncular larvae, should they exist, would represent draws from related but distinct intergenerational dispersal kernels - an oviposition kernel, and a composite ‘oviposition and lifespan’ kernel. The avuncular distribution kernel would thus reflect a further compositing of these dispersal events.
There is a rich literature examining the kernels of basic dispersal events, and analysing them in terms of various kernel functions, whether Gaussian, exponential, or others with differing properties and shapes, often reflecting the tendency of dispersal events to be disproportionately clustered around the source and/or be dispersed at great distances from the source (i.e. for the kernel to be fat-tailed). Most of this literature explores dispersal in terms of probability of a dispersed sample being at a certain radius from the dispersed source. In the case of close-kin recaptures of e.g. first cousins, we are instead presented with dispersal events that must be approached in two dimensions with respect to both radius of dispersal and additionally angle of dispersal. A successful estimator of intergenerational dispersal using close-kin recaptures must find strategies to decompose the extraneous spatial and breeding components affecting the kernels, and ultimately re-express dispersal in terms of an axial sigma - that aspect of dispersal which operates within one dimension across a two-dimensional space. This is the sigma component relied upon by Wright (1946) for isolation by distance , and which is reflected in estimations of neighbourhood area.
The method we have developed relies upon the fact that different kinship categories reflect different but related underlying intergenerational dispersal composites, and uses the relationships between these kinship distribution kernels to extract information about the core parent-offspring dispersal kernel that produced the derivative kernels. For example, the immature distribution kernel of full siblings differs from the immature distribution of first cousins by a single lifespan: using an additive variance framework, the first cousin variance that is not accounted for by subtracting the full sibling variance constitutes an estimate of the parent-offspring distribution, from which an intergenerational kernel estimate can be derived. This is because both immature full-sibling and immature first cousins are ‘phased’ with respect to the organisms’ life cycle - that is, they are separated by an integer multiple of parent-offspring dispersal events. It is this phasing that enables the extraction of a ‘pure’ effective dispersal estimate, via the additive property of variance. Other examples of phased relationships include half sibling immatures to half cousin immatures (one cycle), full sibling immatures to second cousin immatures (two cycles), or even (for mosquitoes) full sibling immatures to second cousin ovipositing adults (three cycles).
Further details can be found in Jasper et al. (2019), “A genomic approach to inferring kinship reveals limited intergenerational dispersal in the yellow fever mosquito.”
This package supplements these papers by supplying methods for (a) importing and exporting information about distances and kinship relationships for dyads of individuals, (b) estimating the axial distribution (axial sigma for dispersal or position distributions) from empirical distributions of kin-dyads, and (c) estimating the intergenerational (parent-offspring) dispersal distribution (axial sigma) that underlies the distributions of multiple phased kin categories. This package also implements several simulation tools for further exploring and testing the properties of intergenerational dispersal kernels, as well as to assist in designing experiment layouts and sampling schemes. Finally, for ease of use, the package supplies an integrated shiny app which also implements the vast majority of package functionality in a user-friendly interface.
You can install the released version of kindisperse from CRAN with:
install.packages("kindisperse")
And the development version from GitHub with:
# install.packages("devtools")
::install_github("moshejasper/kindisperse") devtools
Once installed, load the package as follows:
library(kindisperse)
#> kindisperse 0.10.2
The kindisperse app bundles most of the tools supplied in this package for ease of use.
To run the app, enter the function run_kindisperse()
and in a moment the app will appear in a separate window. To close, exit this window, or alternatively hit the ‘stop’ button or equivalent in RStudio.
To calculate axial values, etc. of objects within the app, they first must be passed to the app from the computer or the R package environment. One option is to save objects to the computer via either .csv or .kindata formats, then load them using the in-app interface.
Alternatively, objects you have loaded or created in the R package environment can be passed to the app by first mounting them to the special appdata
environment which can be accessed from within the app via the Load
tab. Mounted objects must be of class KinPairData
or KinPairSimulation
. To mount an object, use the mount_appdata(obj, "nm")
function (unmount with unmount_appdata("nm")
). The appdata
environment can be viewed with display_appdata()
and cleared with reset_appdata()
. Objects mounted to appdata from within the app can also be retrieved with retrieve_appdata()
or retrieveall_appdata()
.
<- simulate_kindist_composite(nsims = 100, ovisigma = 25, kinship = "FS")
fullsibs reset_appdata()
mount_appdata(fullsibs, "fullsibs")
display_appdata()
#> <environment: kindisperse_appdata>
#> parent: <environment: namespace:kindisperse>
#> bindings:
#> * fullsibs: <KnPrSmlt>
<- retrieve_appdata("fullsibs")
fullsibs2 reset_appdata()
The app also uses a temporary environment for in-app data handling and storage. Following a session, objects stored in this space can be bulk-accessed via the function retrieve_tempdata()
, and reset via the function reset_tempdata()
.
Package functions and typical usage are introduced below
KINDISPERSE is is built to run three types of simulation. The first is a graphical simulation showing the dispersal of close kin over several generations. The second and third are both simulations of close kin dyads, one using a simple PO kernel, the other a composite one. The package also includes one subsampling function to assist in using these simulations for field study design.
This is designed primarily for introducing, exploring, and easily visualising dispersal concepts. It is packaged in two parallel functions: the simulation function (simgraph_data()
) and the visualisation function(simgraph_graph()
). A standard example of their use is shown below, in this case, modeling families including first cousins with a kernel sigma of 25m, and site dimensions of 250x250m. The first graph shows the dispersal events leading to first cousins within five of these families.
## run graphical simulation
<- simgraph_data(nsims = 1000, posigma = 25, dims = 250)
graphdata simgraph_graph(graphdata, nsim = 5, kinship = "1C")
However, the options of both can be tweaked to show other data types, e.g. a pinwheel graph focused on 1,000 first cousin dyads.
<- simgraph_data(nsims = 1000, posigma = 25, dims = 250)
graphdata simgraph_graph(graphdata, nsims = 1000, pinwheel = T, kinship = "1C")
or a histogram of first cousin dyads:
<- simgraph_data(nsims = 1000, posigma = 25, dims = 250)
graphdata simgraph_graph(graphdata, nsims = 1000, histogram = T, kinship = "1C")
The simgraph functions are also implemented in the ‘Tutorial’ tab of the kindisperse app.
These are designed for simulating and testing the impacts of various dispersal and sampling parameters on a dataset, and for testing and validating the estimation functions. They return an object of class KinPairSimulation
, which supplies a tibble (dataframe) of simulation results, as well as metadata capturing the simulation parameters.
Three kernel types are supported for the next two simulations at present: Gaussian
, Laplace
, and vgamma
(variance-gamma). These are passed to the functions with the method
parameter. If using vgamma, also supply its shape parameter with the argument shape
. Small values of shape
correspond to an increasingly leptokurtic kernel - i.e. a strong central clustering with an increased number of very widely spaced individuals (long tails).
The simple simulation, simulate_kindist_simple()
, simulates intergenerational dispersal for each kin category based on a simple parent-offspring dispersal sigma, with no attempt to distinguish between the various breeding and dispersal events across a lifespan. For this reason, it cannot distinguish between full and half siblings (for example), as immature full and half siblings have been separated by less than a lifespan’s worth of dispersal; it would render them as at distance 0 from their parent (if they were in the adult oviposition stage, however, they would be rendered as at one lifespans’ dispersal from parents).
Example usage is shown below:
simulate_kindist_simple(nsims = 5, sigma = 100, method = "Gaussian", kinship = "PO", lifestage = "immature")
#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: simple
#> kerneltype: Gaussian
#> kinship: PO
#> simdims: 100 100
#> posigma: 100
#> lifestage: immature
#>
#> tab
#> # A tibble: 5 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 1a 1b PO 140. 68.0 31.1 88.8 169.
#> 2 2a 2b PO 296. 38.3 48.7 -249. -23.2
#> 3 3a 3b PO 118. 38.9 15.2 127. 93.5
#> 4 4a 4b PO 59.1 82.6 69.9 140. 56.5
#> 5 5a 5b PO 198. 58.9 60.0 186. -91.2
#> -----------------------------------
The composite simulation, simulate_kindist_composite()
, defines four smaller dispersal movements which make up the lifestage dispersal kernel. It distinguishes between full and half siblings, cousins, etc. and handles immature kin dyads that are separated by less than a lifespan of dispersal (e.g. immature FS). The four phases are ‘initial’ (handling any dispersal between hatching and breeding), ‘breeding’ (movement of the male across the breeding aspect of the cycle), ‘gravid’ (movement of the female after breeding but before deposition of young), and ‘oviposition’ (movement made while ovipositing/ bearing young). The addition of the variances of these four kernels together consitutes the lifespan dispersal kernel; the relationships between different categories inform the phase. For example, full-siblings, whether sampled at oviposition or immature states, differ in hatch position based on the ovipositing movements of the mother (including e.g. skip oviposition in the case of some mosquitoes). These categories (and any others containing a full-sib relationship buried in the pedigree) are thus of the ‘full-sibling’ or ‘FS’ phase. Half siblings, in mosquitoes (which this package is modelled on) are expected to be due to having the same father and separate mothers: the last contribution of the father’s dispersal is at the breeding stage, so the ‘HS’ phase are differentiated by the breeding, gravid, and oviposition phases, but share in common the initial phase. The parent-offspring ‘PO’ phase, on the other hand, share all (or none) of the component dispersal distributions.
An example composite simulation is demostrated below:
simulate_kindist_composite(nsims = 5, initsigma = 50, breedsigma = 30, gravsigma = 50, ovisigma = 10, method = "Laplace", kinship = "H1C", lifestage = "ovipositional")
#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: composite
#> kerneltype: Laplace
#> kinship: H1C
#> simdims: 100 100
#> initsigma 50
#> breedsigma 30
#> gravsigma 50
#> ovisigma 10
#> lifestage: ovipositional
#>
#> tab
#> # A tibble: 5 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 1a 1b H1C 375. -240. -3.72 113. -128.
#> 2 2a 2b H1C 276. -107. -170. 12.9 78.6
#> 3 3a 3b H1C 111. 79.7 45.4 173. 107.
#> 4 4a 4b H1C 242. 173. 224. -56.9 149.
#> 5 5a 5b H1C 95.7 139. -48.3 111. -140.
#> -----------------------------------
Finally, a custom simulation function, simulate_kindist_custom()
enables the simulation of dispersal in organisms with breeding cycles different to the original mosquito species this package was modeled for. These simulations take a model object (of class DispersalModel
, generated with the function dispersal_model()
) which contains detailed information about breeding phases, the full sibling (FS) and half sibling (HS) branch point, the sampling point, and further optional parameters defining the accessible breeding cycle more carefully. We illustrate this functions’s use in the context of implementing kindisperse in a new species subsequently, but an initial example is given here. First, we generate a custom dispersal model:
<- dispersal_model(juvenile = 50, breeding = 40, gestation = 30, .FS = "juvenile", .HS = "breeding", .sampling_stage = "gestation")
dmodel
dmodel#> KINDISPERSE INTERGENERATIONAL DISPERSAL MODEL
#> ---------------------------------------------
#> stage: juvenile breeding gestation
#> dispersal: 50 40 30
#>
#> FS branch: juvenile
#> HS branch: breeding
#> sampling stage: gestation
#> cycle: 0 0
#> ---------------------------------------------
Next, we use this model to simulate dispersal in our organism:
simulate_kindist_custom(nsims = 5, model = dmodel, kinship = "PO")
#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: custom
#> kerneltype: Gaussian
#> kinship: PO
#> simdims: 100 100
#> juvenile 50
#> breeding 40
#> gestation 30
#> cycle: 0 0
#> lifestage: gestation
#>
#> tab
#> # A tibble: 5 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 1a 1b PO 57.1 26.6 14.6 31.0 71.6
#> 2 2a 2b PO 90.9 19.6 65.0 -69.7 48.2
#> 3 3a 3b PO 80.0 22.1 77.6 -17.0 7.89
#> 4 4a 4b PO 84.4 16.6 64.4 -57.8 104.
#> 5 5a 5b PO 31.7 63.4 0.874 71.2 31.6
#> -----------------------------------
This is done via another function, sample_kindist()
, and enables the examination of how field sampling conditions could bias the estimation of axial sigma. It works with the KinPairSimulation
or KinPairData
classes and filters based on the study area size, number of kin expected to be found, and trap spacing. It is demonstrated below.
<- simulate_kindist_composite(nsims = 100000, kinship = "H2C")
compsim
sample_kindist(compsim, upper = 1000, lower = 200, spacing = 50, n = 25)
#> Removing distances farther than 1000
#> Removing distances closer than 200
#> Setting trap spacing to 50
#> Down-sampling to 25 kin pairs
#> 25 kin pairs remaining.
#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: composite
#> kerneltype: Gaussian
#> kinship: H2C
#> simdims: 100 100
#> initsigma 100
#> breedsigma 50
#> gravsigma 50
#> ovisigma 25
#> lifestage: immature
#>
#> FILTERED
#> --------
#> upper: 1000
#> lower: 200
#> spacing: 50
#> samplenum: 25
#>
#> tab
#> # A tibble: 25 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 73035a 73035b H2C 325 50.9 -90.9 111. 214.
#> 2 31590a 31590b H2C 525 135. 41.6 -389. -6.31
#> 3 86019a 86019b H2C 425 461. 428. 307. 58.0
#> 4 76172a 76172b H2C 475 114. -366. 74.0 86.4
#> 5 79130a 79130b H2C 225 365. -29.1 134. -100.
#> 6 68255a 68255b H2C 225 112. -1.27 174. 239.
#> 7 4467a 4467b H2C 375 157. 95.1 271. 440.
#> 8 98263a 98263b H2C 675 34.2 87.1 -354. -440.
#> 9 99625a 99625b H2C 375 -168. 8.57 215. -41.7
#> 10 32078a 32078b H2C 575 -4.69 478. 172. -67.0
#> # ... with 15 more rows
#> -----------------------------------
Files can be loaded and saved to and from three separate formats: .csv and .tsv (via functions csv_to_kinpair()
, tsv_to_kinpair()
, or to save, kinpair_to_csv()
and kinpair_to_tsv()
, as well as the package-specific .kindata format which wraps an rds file storing package objects (via functions read_kindata()
and write_kindata()
). These files read to or save from an object of class KinPairData
(including simulation objects of class KinPairSimulation
).
.csv or equivalent files used should have a single column with the header ‘distance’ that contains the geographical distances between kin dyads, and preferably another column labelled ‘kinship’ which carries the kinship category in a form recognized by this package (see documentation for further details). Example below:
<- simulate_kindist_simple(nsims = 25, kinship = "FS", lifestage = "immature")
kinobject #kinpair_to_csv(kinobject, "FS_kin.csv") # saves file
#csv_to_kinpair("FS_kin.csv") # reloads it
Within the package, there are several ways to convert measures of kin dispersal distances into the KinPairData
format required for calculations of axial distance: vector_to_kinpair()
which takes a vector of kinpair distances, and df_to_kinpair()
which takes a data.frame
or tibble
with a similar layout to the .csv
files mentioned earlier (column of geographical distances labelled ‘distance’ and optional columns of kin categories (‘kinship’) and lifestages (’lifestage)). Inverse function is kinpair_to_tibble()
. See relevant documentation. Example below:
<- c(25, 23, 43, 26, 14, 38)
kinvect
vector_to_kinpair(kinvect, kinship = "H1C", lifestage = "immature")
#> KINDISPERSE RECORD OF KIN PAIRS
#> -------------------------------
#> kinship: H1C
#> lifestage: immature
#> cycle: 0
#>
#> tab
#> # A tibble: 6 x 4
#> id1 id2 kinship distance
#> <chr> <chr> <chr> <dbl>
#> 1 1a 1b H1C 25
#> 2 2a 2b H1C 23
#> 3 3a 3b H1C 43
#> 4 4a 4b H1C 26
#> 5 5a 5b H1C 14
#> 6 6a 6b H1C 38
#> -------------------------------
Once converted, in most cases these KinPairData
objects can be sampled in the same way as the simulations above with the function sample_kindata()
.
The package contains a series of functions to estimate and manipulate axial sigma values (axial distributions) of simulated and empirical close-kin distributions, as well as to leverage several such distributions of related categories to supply a bootstrapped estimate of the intergenerational dispersal kernel axial sigma.
Axial sigma is most simply estimated with the function axials(x, composite = 1)
. This function estimates the axial value of a simple kernel assuming that all distances measured represent one dispersal event governed by the kernel (e.g. the distance between a parent and their offspring at the equivalent lifestage, such as both as eggs). For slightly more complex situations, such as full siblings, where the distances between them result from two or more draws from the same underlying distribution (ovipositing parent to offspring #1, ovipositing parent to offspring #2), the value of composite
can be adjusted to reflect the number of such symmetrical component events (for this specific case, you can also use axials_norm()
). (e.g. the great-grandparent to great-grandchild category, ‘GGG’ is a combination of three draws from the PO distribution, and thus would take composite = 3
):
<- simulate_kindist_simple(nsims = 1000, sigma = 75, kinship = "PO")
paroff axials(paroff)
#> [1] 76.35671
<- simulate_kindist_composite(nsims = 10000, ovisigma = 25, kinship = "FS")
fullsibs axials(fullsibs, composite = 2)
#> [1] 25.09441
Various auxillary functions exist to further manipulate axial distances within an additive variance framework, enabling the stepwise combination or averaging or decomposition of axial sigma values representing different distributions. These include axials_decompose()
(divides into component parts as in the composite option above), axials_add()
(adds two distributions together, e.g. FS + FS + PO + PO = 1C), axials_combine()
(mixes two distributions together equally, e.g. 1C and H1C becomes the distribution of an even mix of both), and axials_subtract()
subtracts a smaller distribution from a greater distribution to find the residual distribution (e.g. GG - PO = PO; FS(immature) - FS(ovipositional) = PO). For confidence intervals, there are also the permuting functions axpermute()
and axpermute_subtract()
.
axials_subtract(24, 19)
#> [1] 14.66288
Building on the above functions, the final estimation function axials_standard()
and its permuted implementation axpermute_standard()
take information about dispersal information across several phased categories and use it to make an estimate of the core, parent-offspring dispersal kernel (defined by axial sigma). Using this equation requires knowing representative spatial distributions of at least two phased kinship classes that are separated by at least one complete lifespan. In some cases, this phased requirement can be met by compositing two known distributions to approximate the distribution of a mixed category (e.g. mixing FS and HS categories to create a composited category that can be compared to an undistinguishe mixture of 1C and H1C individuals).
The function works by subtracting out the phased component of the distributions (e.g. the additional oviposition present in FS and 1C) leaving the residual lifespan components, then decomposing these down to a single span. When bootstrapped as in the axpermute_standard()
function, these equations output the 95% confidence intervals of the resulting PO sigma estimate, as well as the estimate of median sigma. This estimate is the same sigma that interacts with Wright’s neighbourhood size (the radius of NS is equal to 2x the axial sigma estimate).
Let’s try out some simulated values see the function in action. First, we’ll set up our individual axial sigmas for the component distributions.
# set up initial sigma values
= 50
init = 25
brd = 75
grv = 10
ovs
# calculate theoretical PO value
<- sqrt(init^2 + brd^2 + grv^2 + ovs^2)
po_sigma
po_sigma#> [1] 94.07444
Here we have set up a baseline of the theoretical value of the intergenerational kernel (axial) sigma for comparison below.
First, a simple example (full sibs and first cousins) - note that the larger value must be inputted first, i.e. as avect
in the equation. Because they are simulated objects, categories don’t need to be supplied.
# set up sims
<- simulate_kindist_composite(nsims = 75, initsigma = init, breedsigma = brd, gravsigma = grv, ovisigma = ovs, kinship = "FS")
fullsibs
<- simulate_kindist_composite(nsims = 75, initsigma = init, breedsigma = brd, gravsigma = grv, ovisigma = ovs, kinship = "1C")
fullcous
# calculate PO axial sigma C.I.
axpermute_standard(fullcous, fullsibs)
#> 2.5% mean 97.5%
#> 84.48496 97.77777 109.82592
As we can see, the C.I. neatly brackets the actual axial value, though with fairly large wings due to the small sample size. Now we set up a more complex case, involving a mixture of full and half cousins and a compensating compositing of full and half siblings (this will involve some data-wrangling):
# Set up new distributions
<- simulate_kindist_composite(nsims = 75, initsigma = init, breedsigma = brd, gravsigma = grv, ovisigma = ovs, kinship = "HS")
halfsibs
<- simulate_kindist_composite(nsims = 75, initsigma = init, breedsigma = brd, gravsigma = grv, ovisigma = ovs, kinship = "H1C")
halfcous
# combine cousin distributions and recompose as object. Chaning kinship
# to standard value for unknown as I will be combining the distributions.
<- dplyr::mutate(kinpair_to_tibble(fullcous), kinship = "UN")
fc <- dplyr::mutate(kinpair_to_tibble(halfcous), kinship = "UN")
hc <- tibble::add_row(fc, hc)
cc <- df_to_kinpair(cc)
cousins
cousins#> KINDISPERSE RECORD OF KIN PAIRS
#> -------------------------------
#> kinship: UN
#> lifestage: immature
#> cycle: 0
#>
#> tab
#> # A tibble: 150 x 9
#> id1 id2 kinship distance x1 y1 x2 y2 lifestage
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl> <chr>
#> 1 1a 1b UN 337. 106. 98.6 -229. 134. immature
#> 2 2a 2b UN 266. 138. -149. 40.3 98.7 immature
#> 3 3a 3b UN 76.8 -87.2 212. -40.8 151. immature
#> 4 4a 4b UN 331. -148. 208. 33.3 -68.3 immature
#> 5 5a 5b UN 46.0 -11.2 -10.6 7.86 31.2 immature
#> 6 6a 6b UN 110. 109. 143. 16.8 81.8 immature
#> 7 7a 7b UN 133. -18.6 94.7 -57.4 -32.1 immature
#> 8 8a 8b UN 58.3 49.9 -16.9 -8.25 -20.4 immature
#> 9 9a 9b UN 169. 150. 25.2 51.7 163. immature
#> 10 10a 10b UN 141. 89.9 193. -45.4 152. immature
#> # ... with 140 more rows
#> -------------------------------
Note this is now a KinPairData
object rather than a KinPairSimulation
. The conversion to tibble and back has stripped the simulation class data. Now to run the estimation function, supplying missing category data:
# amix allows supply of additional (mixed) kin category H1C to acat 1C;
# bcomp allows supply of distribution to composite with bvect (this is done to match
# the cousin mixture in phase)
axpermute_standard(avect = cousins, acat = "1C", amix = TRUE, amixcat = "H1C", bvect = fullsibs, bcomp = TRUE, bcompvect = halfsibs)
#> 2.5% mean 97.5%
#> 88.27622 100.37872 111.97746
This estimate is a lot more convoluted, and not as ‘spot on’- but the theoretical value of 94 is well within the confidence intervals.
Using custom dispersal simulations and parameters, we are well placed to explore what is typically involved in adapting this method and package to a species with a different life history and breeding structure to that of Ae. aegypti and other related species. The example chosen here is a species of Antechinus - a small marsupial native to Australia. Note that this example is for illustrative purposes only.
Breeding and dispersal can be highly diverse processes between organisms - simply copying and pasting a method from one species to another without careful consideration of their differences and unique contexts is unwise. What relevant information can we find about species of Antechinus?
For Antechinus, mating takes place across a single week each year, and is promiscuous. Males only mate once, and die shortly after mating. Females live up to two years, producing two litters in that time. Each litter will likely contain offspring from multiple males (Cockburn, Scott, and Scotts 1985). In the same paper, Cockburn et al. recognize seven life history stages:
No. | Stage | Duration |
---|---|---|
1 | Pouch young | 5-7 weeks |
2 | Nest young | 8-10 weeks |
3 | Juveniles | rest of year 1 |
4 | Reproductives | 2 weeks |
5 | Mothers | 4-5 weeks gestation, then ongoing |
6 | 2nd year reproductives | 2 weeks |
7 | 2nd year mothers | 4-5 weeks gestation, then ongoing |
Pouch young exhibit obligatory attachment to the mother’s teat. Nest young still feed on the teat, but are left in the nest (typically a hole in a tree) when the mother forages for food, until weaning. Juveniles describe the post-weaning, physiologically independent animals before synchronised reproduction occurs. This interval covers most of the first year. Reproductives (male and female) describe the animals within the very short mating window each year (males mate with multiple females, and vice versa). Mothers covers pregnancy, lactation (overlapping with nest and pouch young) and post-lactation (overlapping with the juvenile phase).
Natal dispersal (occuring after weaning) is strongly male-biased (Cockburn, Scott, and Scotts 1985), with males dispersing from the nest and often from the maternal home range, while females dispersal is more localised. In that time, males can disperse over hundreds of metres - in some species (e.g. Antechnius stuartii), more than a kilometre (Banks and Lindenmayer 2014). Female dispersal is not frequently beyond 50 metres (Fisher 2005).
Our key research questions will drive which aspects of the above life history we want to focus on further. For this exercise, we want to be able to estimate parent-offspring dispersal so that we can gain an estimate of the neighbourhood area. Importantly, we need this estimate to get around the sex-biased disersal in this species.
Let’s define a life cycle. Pouch and nest young are still completely dependent on the mother, so will show no independent dispersal. We start our description of a single intergenerational breeding cycle with the juvenile stage, followed by breeding. We will break down the ‘mother’ lifestage into ‘gestation’ and ‘pouch.’
So, our basic breeding cycle will be something like: juvenile –> breeding –> gestation –> pouch.
What kinship categories do we expect to see in Antechinus populations? Let’s break this down by order:
Within this category we have the PO
and FS
classes. Full sibs share the same mother, and the fathers only mate during one breeding cycle, so we can expect all full sibs to be part of the same cohort, and FS phased disperal to begin in the juvenile phase, as offspring leave the nest.
The HS
kinship class can be generated by a male mating with multiple females, or a female mating with multiple males. Both of these have different dispersal modes (the former is shaped by breeding dispersal, the latter in a similar manner to the FS
class). For our initial simulation, we will only treat the former kind of HS
dispersal. Note that as females bear young over two generations, a third class of HS
is possible, between an adult female mother and the pouch young of her (now 2nd yr) mother - cases like this are readily distinguishable by other life history traits, e.g. age.
The GG
kinship class (between 2nd yr mother and her grandchildren)
The AV
kinship class (between an adult female and the offspring of her full sibling - a partially sex-biased category)
Important categories here include 1C
and HAV
. (GAV
is also possible, but clearly distinguishable by life history).
1C
- first cousins. Part of same generational cohort and the FS
dispersal phase.
HAV
- half avuncular. Most will be intergenerational (females of previous generation to males and females of present generation). However, because females breed across two cycles, this category can occur within the same generational cohort (see below).
1C
individuals will be part of the same generational cohort and result from parent-offspring dispersal events, making them a prime target (along with the FS category) for developing an intergenerational dispersal estimate.
Armed with the above categories, we are well placed to put together a rudimentary model of Antechinus. We will assign dispersal parameters to approximately reflect what we consider important in the above. As we are focusing on intergenerational dispersal in general, for now, we will ignore sex-biased aspects of dispersal (though we will take them into account when planning sampling).
<- dispersal_model(juvenile = 100, breeding = 50, gestation = 25, pouch = 25, .FS = "juvenile", .HS = "breeding", .sampling_stage = "juvenile")
antechinus_model
antechinus_model#> KINDISPERSE INTERGENERATIONAL DISPERSAL MODEL
#> ---------------------------------------------
#> stage: breeding gestation pouch juvenile
#> dispersal: 50 25 25 100
#>
#> FS branch: juvenile
#> HS branch: breeding
#> sampling stage: juvenile
#> cycle: 0 0
#> ---------------------------------------------
Note that at this stage we have initially set sampling stage to juvenile
i.e. sampling free-living individuals before their first breeding season. We will return to this later.
We begin with a simple PO
simulation.
library(magrittr)
<- simulate_kindist_custom(nsims = 10000, model = antechinus_model, kinship = "PO")
ant_po
ant_po#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: custom
#> kerneltype: Gaussian
#> kinship: PO
#> simdims: 100 100
#> breeding 50
#> gestation 25
#> pouch 25
#> juvenile 100
#> cycle: 0 0
#> lifestage: juvenile
#>
#> tab
#> # A tibble: 10,000 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 1a 1b PO 141. 35.4 43.7 -106. 50.0
#> 2 2a 2b PO 119. 44.1 77.0 -75.3 72.1
#> 3 3a 3b PO 128. 24.6 88.5 -97.5 51.7
#> 4 4a 4b PO 118. 96.2 48.1 205. 93.8
#> 5 5a 5b PO 7.11 43.8 25.4 46.4 32.0
#> 6 6a 6b PO 150. 88.3 44.9 172. -79.8
#> 7 7a 7b PO 166. 5.95 28.8 44.7 -132.
#> 8 8a 8b PO 100. 74.6 58.6 125. 145.
#> 9 9a 9b PO 174. 36.5 81.4 128. -67.3
#> 10 10a 10b PO 62.0 70.8 6.36 120. -31.8
#> # ... with 9,990 more rows
#> -----------------------------------
Now we’ll use the axials()
function to characterise our ‘default’ dispersal for the model:
axials(ant_po)
: 117.4923741
The value is around 117 the ‘expected’ value of PO we should get back from more complex estimation processes.
For a basic PO estimation, we are going to combine the FS and 1C categories:
<- simulate_kindist_custom(nsims = 10000, model = antechinus_model, kinship = "FS")
ant_fs <- simulate_kindist_custom(nsims = 10000, model = antechinus_model, kinship = "1C")
ant_1c
axials_standard(ant_1c, ant_fs) # larger dispersal category goes first.
#> [1] 115.7949
The FS/1C strategy has been validated theoretically - but an important issue remains: the HAV
category. While all males only breed during one breeding season, in some Antechinus species, many females breed for a second season. This means that the situation will arise where a mother bears offspring in one breeding season, and both the mother and her offspring bear young in the subsequent breeding season. As the second batch of young she bears are related to her previous litter as half-siblings, they are related to the that litter’s offspring under the half-avuncular HAV
kinship category. As HAV
is of the same order of kinship (3rd) as 1C
, and (via this pathway) will be of the same lifestage, yet both pass through differing dispersal routes, without further information it would be impossible to use this class. Similar issues would hold for the H1C
(half-cousin) and 1C1
(first cousin once removed) categories at the fourth order of kinship.
If we were simply sampling juvenile Antechinus as in our initial setup, there would be no way to correct for this ambiguity in the data. We need to include richer pedigree information to distinguish between the various classes. Instead of sampling at the juvenile stage, let’s switch the focus to females with pouch young, and instead of genotyping one individual, plan to genotype all pouch young of a female:
<- dispersal_model(juvenile = 100, breeding = 50, gestation = 25, pouch = 25, .FS = "juvenile", .HS = "breeding",
antechinus_model .sampling_stage = "pouch", .breeding_stage = "breeding", .visible_stage = "juvenile")
antechinus_model#> KINDISPERSE INTERGENERATIONAL DISPERSAL MODEL
#> ---------------------------------------------
#> stage: juvenile breeding gestation pouch
#> dispersal: 100 50 25 25
#>
#> FS branch: juvenile
#> HS branch: breeding
#> sampling stage: pouch
#> cycle: 0 0
#> ---------------------------------------------
Note that we have made several other previously implied model parameters explicit this time also (the default values are preserved here, but the concepts are important). Firstly, the breeding_stage
parameter defines which stage in the breeding cycle breeding actually occurs at. This is by default anchored to the HS
branch, but in situations where we might with to model HS
dispersal that begins later (e.g. where offspring have multiple fathers but the same mother) - we might shift the HS
branch to the juvenile stage, but preserve our information on breeding with this parameter. Second, the visible_stage
parameter defines at what point in the life cycle an individual is considered ‘available by default for sampling’ in preference to its parent. This is by default anchored to the FS
branch, and approximates birth, hatching, etc. in many species - but in many species (e.g. marsupials) an animal will be born, but still attached to the parent from the perspective of dispersal. In such situations, the visible_stage
parameter describes which individual will be sampled by default at an overlapping lifestage. As in our model, visible_stage
is anchored to the FS-branch juvenile stage, the default sampled pouch individuals will be the mothers rather than the offspring. In a simulation, the pouch offspring can be accessed by setting the breeding cycle parameter to -1
.
By sampling at this stage, we unlock four different kinds of generational comparisons, all synced to the same life point: (1) intra-pouch relationships (i.e. between different pouch young carried by the same mother), (2) inter-pouch relationships (kinships between young carried by different females), (3) kinship between adult females, and (4) kinships between pouch young and adult females other than their mother.
All of these categories can be combined with the genotypic data to resolve pedigree information and enable more thorough calculations of breeding dispersal, via the following resolution:
Yes! We can check other pedigree relationships to distinguish between the 1C and HAV categories. Firstly, we compare the parents. If they are FS, their offspring are 1C and in isolation constitute an estimate of female intergenerational dispersal as in (f) above. But an even more useful test is to reciprocally cross-check the kinship between pouch young and the mother of their putative cousins. If the two mothers were not full siblings, we expect this pairing to produce an unrelated kin category in the case of 1C offspring. However, in the HAV case, one of the mothers must also be the grandmother of the other pouch young! This would produce the 2nd order (GG) relationship between the pouch young and their grandmother. Thus, pedigree information helps us to distinguish between HAV and 1C pouch young. Once 1C pouch young have been identified (via all approaches) they will constitute an estimate of the elusive intergenerational category PO (sex-independent). Similarly, the HAV offspring where the GG individual is not the parent of the other mother can be used to derive an estimate of male intergenerational dispersal!
For this reason, our key kinship category targets are:
Pedigree relationships we also need to test include:
We run the initial simulations here: (setting the dispersal model to vgamma to allow longer-tailed dispersal)
<- simulate_kindist_custom(nsims = 100000, model = antechinus_model, kinship = "1C", cycle = -1, method = "vgamma")
ant_1c_juv
ant_1c_juv#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: custom
#> kerneltype: vgamma
#> kernelshape: 0.5
#> kinship: 1C
#> simdims: 100 100
#> juvenile 100
#> breeding 50
#> gestation 25
#> pouch 25
#> cycle: -1 -1
#> lifestage: pouch
#>
#> tab
#> # A tibble: 100,000 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 1a 1b 1C 310. 92.1 267. 46.7 -39.3
#> 2 2a 2b 1C 171. 51.3 34.8 -101. 112.
#> 3 3a 3b 1C 274. 155. 357. 73.8 94.6
#> 4 4a 4b 1C 50.0 -31.0 -0.819 -66.1 34.7
#> 5 5a 5b 1C 14.8 52.0 123. 48.0 109.
#> 6 6a 6b 1C 200. 134. 157. 117. -41.5
#> 7 7a 7b 1C 32.5 -110. 201. -114. 233.
#> 8 8a 8b 1C 336. 371. 50.8 103. 252.
#> 9 9a 9b 1C 28.3 11.4 170. 35.8 156.
#> 10 10a 10b 1C 210. -5.84 -121. 147. 23.9
#> # ... with 99,990 more rows
#> -----------------------------------
<- simulate_kindist_custom(nsims = 100000, model = antechinus_model, kinship = "FS", cycle = -1, method = "vgamma")
ant_fs_juv
ant_fs_juv#> KINDISPERSE SIMULATION of KIN PAIRS
#> -----------------------------------
#> simtype: custom
#> kerneltype: vgamma
#> kernelshape: 0.5
#> kinship: FS
#> simdims: 100 100
#> juvenile 100
#> breeding 50
#> gestation 25
#> pouch 25
#> cycle: -1 -1
#> lifestage: pouch
#>
#> tab
#> # A tibble: 100,000 x 8
#> id1 id2 kinship distance x1 y1 x2 y2
#> <chr> <chr> <chr> <dbl> <dbl> <dbl> <dbl> <dbl>
#> 1 1a 1b FS 0 98.7 67.0 98.7 67.0
#> 2 2a 2b FS 0 31.7 42.9 31.7 42.9
#> 3 3a 3b FS 0 39.7 85.1 39.7 85.1
#> 4 4a 4b FS 0 68.6 88.7 68.6 88.7
#> 5 5a 5b FS 0 20.8 7.84 20.8 7.84
#> 6 6a 6b FS 0 37.3 34.8 37.3 34.8
#> 7 7a 7b FS 0 53.0 89.6 53.0 89.6
#> 8 8a 8b FS 0 9.92 16.5 9.92 16.5
#> 9 9a 9b FS 0 38.7 54.5 38.7 54.5
#> 10 10a 10b FS 0 36.7 49.4 36.7 49.4
#> # ... with 99,990 more rows
#> -----------------------------------
Inspecting the results, we see that the 1C category is well-dispersed, while the FS category is entirely zero (FS offspring in the pouch are not dispersed at all).
Finally, we run a simple PO estimation with these simulations (we override a key check on the breeding cycle that would otherwise be triggered by FS being used before their breeding cycle start point, as they have not dispersed at all, so will not confound the estimate)
axpermute_standard(ant_1c_juv, ant_fs_juv, nsamp = 100, override = TRUE)
#> 2.5% mean 97.5%
#> 102.2679 117.4515 134.7855
This is excellent so far. Mean dispersal is still around 117, so assuming sampling is adequate, this approach will lead us to intergenerational dispersal.
Now, before we go any further, we need to estimate how large a study site we will need to gain an adequate understanding of dispersal, and avoid missing rarer long-tailed dispersal events. We know that our FS pouch young haven’t dispersed, so we won’t need to worry about them. But what about the 1C category? At this point in an actual study, the existing model should be refined as much as possible to provide ‘realistic’ estimates of dispersal at each stage (erring on the side of larger estimates if uncertain).
Let’s check an initial sampling site of 100m by 100m:
%>% sample_kindist(dims = 100, n = 1000) %>% axpermute_standard(ant_fs_juv, nsamp = 100, override = TRUE)
ant_1c_juv #> Setting central sampling area to 100 by 100
#> Down-sampling to 1000 kin pairs
#> 1000 kin pairs remaining.
#> 2.5% mean 97.5%
#> 24.86166 27.12850 29.53726
A 100x100 metre sampling area is woefully inadequate (estimating the kernel to only ~ 27m, well short of the 117 we need)! We try again, this time in a 1km x 1km site:
%>% sample_kindist(dims = 1000, n = 1000) %>% axpermute_standard(ant_fs_juv, nsamp = 100, override = TRUE)
ant_1c_juv #> Setting central sampling area to 1000 by 1000
#> Down-sampling to 1000 kin pairs
#> 1000 kin pairs remaining.
#> 2.5% mean 97.5%
#> 87.71667 99.79123 111.75111
We are doing better here: with an average of ~100m. But we’re still 15% short, and barely including the correct value in our C.I.s What about 2km x 2km?
%>% sample_kindist(dims = 2000, n = 1000) %>% axpermute_standard(ant_fs_juv, nsamp = 100, override = TRUE)
ant_1c_juv #> Setting central sampling area to 2000 by 2000
#> Down-sampling to 1000 kin pairs
#> 1000 kin pairs remaining.
#> 2.5% mean 97.5%
#> 98.98307 115.75127 133.27780
This estimate is acceptable, with a mean only a few metres short, and the true value well within C.I.s. Accordingly, we make the decision to sample within a grid of at least 2km by 2 km.
Now we are as prepared as possible to perform sampling, genotype individuals, etc.
Follow the instructions given in 4.2 and 4.3 to load sample data into the program and supply estimates. The axials_standard
and axials_permute
functions contain the parameters acycle
and bcycle
, which enable the calibration of the estimation process to pouch young (remember to use the override
parameter in this context). Or you could simply avoid phase information, set the FS category to zero (as they are non-dispersed), and perform a 1C-FS subtraction as is (which will effectively just decompose the 1C into two PO increments - works in this case as at the pouch phase we have synced FS dispersal to PO dispersal (as all FS offspring coincide with maternal parent)).
Once you have generated in-field estimates of dispersal, it is always good practice to substitute these estimate back into the original simulation and rerun the sampling analysis in 4.4.7 again. If the new estimate is significantly underestimated by the simulation after subsampling to the dimensions of your study site, it is likely that the study site is too small, and is biasing estimates of dispersal - one approach from here would be to progressively increase the dispersal distance until the new subsampled estimate matches the one generated by the study (this will be a more likely figure for dispersal in the species, and should inform future studies).
These binaries (installable software) and packages are in development.
They may not be fully stable and should be used with caution. We make no claims about them.