The R package openCR fits both non-spatial and spatial capture–recapture models to data from open animal populations, where there is turnover during sampling. The interface generally resembles that of secr (Efford 2022a) upon which openCR depends for some functions. This document explains the purpose and general features of openCR. Help pages should be consulted for more detail on particular functions. The vignette openCR-kernel.pdf explains the intricacies of movement kernels (see also Efford and Schofield 2022). Worked examples using published datasets are given in another vignette openCR-examples.pdf1. The spatial model was described by Efford and Schofield (2020).
This is still something of a work in progress, so be careful to check results ‘make sense’ and be aware of limitations.
openCR fits nonspatial open-population models of the Cormack-Jolly-Seber (CJS) and Jolly-Seber-Schwarz-Arnason (JSSA2 or ‘POPAN’) types. JSSA models are offered in both full and conditional likelihood forms, each with several parameterizations of recruitment, and incorporating Pollock’s robust design. Conditional-likelihood JSSA models are also called Pradel–Link–Barker (PLB) models. Pradel analyses are also provided.
Spatial versions of the CJS and JSSA model types are also provided3. The spatial models allow for ‘multi’, ‘proximity’ or ‘count’ detectors as defined in secr. Several functions are implemented for the decline in hazard of detection with distance. Movement between primary sessions may be modelled (cf Ergon and Gardner 2014; Glennie et al. 2019), but particular care is needed, especially with respect to kernel truncation.
Data are assumed to be from a robust design. Secondary sampling sessions are nested within primary sessions and all turnover (births, deaths, immigration or emigration) is between primary sessions (Pollock 1982). There may be a single secondary session per primary session (this limits identifiability of some parameters).
Models are specified using formula notation as in
secr. Possible predictors include both pre-defined
variables for learned responses, trend over time, etc., and
user-provided covariates. Models are fitted by numerically maximizing
the log likelihood. The likelihood is formed as a product over capture
histories (Pledger at al. 2010) rather than from summary statistics. The
fitted model is an object of class ‘openCR’ for which generic methods
are implemented (print
, predict
,
AIC
, plot
etc.).
Variation in a parameter between primary sessions is modelled as
e.g., model = phi ~ session
4. Within-session
variation in detection parameters may also be modelled (see field vole
example in openCR-examples.pdf).
A selection of parameterizations is offered for recruitment in JSSA models. Models can also be parameterized in terms of the time-specific population size (non-spatial models) or density (spatial models), avoiding the super-population parameter.
Super-population size (or density in the case of secr models) may be computed as a derived parameter from ‘CL’ models with the function derived(), which also computes time-specific population sizes and densities.
openCR has definite limitations that may or may not be addressed in future versions. Important differences between secr and openCR are noted here. Online help is not guaranteed: users should attempt to solve their own problems, or seek help from other users via phidot or secrgroup.
We start with a simple nonspatial example. Lebreton et al. (1992)
demonstrated Cormack-Jolly-Seber methods with a dataset on European
Dipper (Cinclus cinclus) collected by Marzolin (1988). The
object dipperCH
distributed with openCR
provides these data in the secr ‘capthist’ format. See
the Examples section of its help page ?dipperCH
for code to
input the data from other sources.
Dippers were captured annually over 1981–1987.
## R 1982 1983 1984 1985 1986 1987 NRecap
## 1981 22 11 2 0 0 0 0 9
## 1982 60 24 1 0 0 0 35
## 1983 78 34 2 0 0 42
## 1984 80 45 1 2 32
## 1985 88 51 0 37
## 1986 98 52 46
## 1987 93 93
We can fit a Cormack-Jolly-Seber model directly with
openCR.fit
and display the estimates:
## $p
## session estimate SE.estimate lcl ucl
## 1 1981 NA NA NA NA
## 2 1982 0.9021 0.02906 0.8286 0.9461
## 3 1983 0.9021 0.02906 0.8286 0.9461
## 4 1984 0.9021 0.02906 0.8286 0.9461
## 5 1985 0.9021 0.02906 0.8286 0.9461
## 6 1986 0.9021 0.02906 0.8286 0.9461
## 7 1987 0.9021 0.02906 0.8286 0.9461
##
## $phi
## session estimate SE.estimate lcl ucl
## 1 1981 0.6258 0.11165 0.3965 0.8098
## 2 1982 0.4542 0.06662 0.3295 0.5849
## 3 1983 0.4784 0.05845 0.3669 0.5921
## 4 1984 0.6244 0.05703 0.5079 0.7281
## 5 1985 0.6079 0.05483 0.4970 0.7088
## 6 1986 0.5833 0.05721 0.4688 0.6895
## 7 1987 NA NA NA NA
From this example you can see some of the virtues of openCR
See openCR-examples.pdf for more extensive analyses of this dataset.
There is a large literature on open-population capture–recapture modelling. Almost all modern models derive from the Cormack-Jolly-Seber (CJS) or Jolly-Seber (JS) models (Seber 1982), with refinements by Crosbie and Manly (1985), Schwarz and Arnason (1996), Pradel (1996) and others. The MARK software (White and Burnham 1999) implemented many of these developments and remains the standard. This section describes differences among models as they relate to openCR.
The split between the CJS and JS model lineages is fundamental. CJS models do not model the first capture of each animal; they condition on that capture and model subsequent recapture probabilities p and apparent survival ϕ. CJS estimates of apparent survival are robust and useful (Lebreton et al. 1992), but CJS models stop short of estimating abundance, recruitment or population trend.
JS models model the first capture of each animal, and lead either directly or indirectly to estimates of abundance and recruitment. The modern development of JS methods rests heavily on Schwarz and Arnason (1996), so openCR follows Pledger et al. (2010) in using the label ‘JSSA’. JSSA models were the basis of the POPAN software, which led to the POPAN data type in MARK. JSSA models are the main focus of openCR.
The JSSA model appears in several different forms whose unity is obscured by differing parameterizations of recruitment. The classic POPAN formulation uses entry probabilities: the members of a notional superpopulation enter the population with time-specific probability βj (PENT in MARK), an idea from Crosbie and Manly (1985). Other parameterizations are
Estimates of recruitment or implied recruitment from any one of these six parameterizations can be used to infer the others5. The choice of parameterization rests on which is more natural for the problem in hand (and allows the desired constraints to be applied) and on practicalities (some are more likely to give numerical problems than others).
Schwarz (2001) is illuminating (see also chapter on Jolly-Seber models by Schwarz and Arnason in the MARK book, Cooch and White 2019). Pradel (1996), Williams, Nichols and Conroy (2002: p.518 et seq.), Pledger et al. (2003, 2010) and Link and Barker (2005) also comment on and compare JS parameterizations. See also the MARK help page on ‘Recruitment Parameters in Jolly-Seber models’ (‘Recruitment Parameters’ in the help index).
For each JSSA recruitment parameterization there is a choice between models that include the total number of detected individuals (u⋅ or n in different notations), and models that condition on this number. Conditional-likelihood models do not directly estimate abundance; abundance is estimated as a derived parameter (Schwarz and Arnason 1996). Full-likelihood models include abundance as a parameter. The choice of formulation has virtually no effect on the parameter estimates6. The conditional likelihood form is somewhat faster and easier to fit (Schwarz and Arnason 1996), and it focuses on parameters that are estimated robustly (apparent survival, seniority, population growth rate).
The conditional models discussed by Pradel (1996), Link and Barker (2005), Schofield and Barker (2016) and others lack a distinguishing label to indicate their collective similarity. The label Pradel–Link–Barker PLB was suggested by Efford and Schofield (2020).
Historically the CJS and JS likelihoods have been expressed in terms
of ‘sufficient statistics’ that are time-specific counts of animals in
different categories, such as the number caught, the number marked etc.
This approach is used in the openCR function
JS.direct
and with the Pradel model type in
openCR.fit
. The likelihood may also be computed as a
product over terms, one for each observed capture history7. Modelling of
individual capture histories, is slower, but it is extremely flexible,
allowing direct inclusion of censoring, learned responses, individual
covariates, secondary sessions and other extensions. This is the
approach used in MARK and openCR.fit
.
Most published formulations of CJS and JSSA models admit only one secondary session per primary session. Data collected according to a robust design with multiple secondary sessions must be collapsed to a single sample per primary session. However, it is simple to adapt the capture-history models for multiple secondary occasions, and this makes better use of the data. MARK offers many specific robust design models. A robust design is assumed in openCR; data with a single secondary session per primary session are merely a special case.
Models may be spatially explicit or not. Nonspatial models ignore the spatial distribution of animals. Spatial models use the spatially explicit capture–recapture paradigm of Efford (2004), Borchers and Efford (2008) and Royle et al. (2014). Open population spatial models using MCMC were published by Gardner et al. (2010), Chandler and Clark (2014), Ergon and Gardner (2014), Whittington and Sawaya (2015) and others. Glennie et al. (2019) proposed a frequentist hidden Markov formulation. The spatial models in openCR are described by Efford and Schofield (2020) and provide very similar estimates to those of Glennie et al. (2019).
There are three major motivations for open spatial models
openCR fits spatial analogues of CJS and JSSA models by maximizing the likelihood. The abundance parameter is density D (animals per hectare) rather than population size N.
Recruitment in spatial models may be modelled using parameterizations to those described above for non-spatial models, replacing ‘number’ by ‘density’. The locations at which animals recruit are not modelled.
By definition, the interval between primary sessions is long enough for turnover due to births and deaths. It is also possible that resident animals shift their home ranges (i.e. disperse). Spatial models may either ignore such movement (Gardner et al. 2010, Chandler and Clark 2014, Whittington and Sawaya 2015) or attempt to model it (Ergon and Gardner 2014). There are good arguments for modelling movement:
Data should be provided to openCR.fit
as
secr ‘capthist’ objects. The occasions of a
single-session8 dataset are treated as open-population
temporal samples. For spatial analyses, the capthist object should use a
point detector type (‘multi’, ‘proximity’ or ‘count’).
openCR mostly uses the terminology of primary and secondary sessions (Pollock 1982) rather than ‘session’ and ‘occasions’ as in secr. Where ‘session’ appears without qualifier it refers to a primary session composed of one or more secondary sessions.
The optional intervals
attribute of the capthist object
defines the structure. If intervals are not specified then they default
to 1.0 and each occasion is treated as a primary session. If intervals
are specified then some may be zero; occasions separated by ‘zero’
intervals are treated as secondary sessions within the same primary
session, as in MARK.
Fig. 1. Structure of data for open-population
analysis in openCR. Primary sessions initially
correspond to the sessions (components) of a multi-session
secr capthist object; each primary session may have one
or more secondary sessions as numbered (top). For model fitting in
openCR.fit
the multi-session capthist is ‘joined’ to form a
single-session capthist with an ‘intervals’ attribute; non-zero
intervals indicate breaks between primary sessions (bottom). The
join
step is automatic when a multi-session capthist is
provided to openCR.fit
if stratified = FALSE
.
(See Appendix 1 for code to make this
figure).
To construct your own capthist objects –
secr::unRMarkInput
, orread.inp
.Examples of data input code also appear on the help pages for data
objects FebpossumCH
, fieldvoleCH
,
microtusCH
and dipperCH
.
A multi-session capthist object will be converted automatically to a
single-session object using function secr::join
unless
stratified = TRUE
(see below). An appropriate intervals
attribute is constructed, using the intervals attribute of the
multi-session object for the intervals between primary sessions (1.0 if
not specified), and setting other intervals to zero.
Table 1. Input formats for 2.2
Input | stratified |
Interpretation |
---|---|---|
single-session capthist | not used | secondary sessions split into primary sessions by ‘intervals’ |
multi-session capthist | FALSE | single stratum (each ‘session’ is one primary session) |
multi-session capthist | TRUE | multi-stratum (each ‘session’ is one stratum) |
From openCR 2.0 onwards any model may be stratified.
For stratified models (stratified = TRUE
in
openCR.fit
) each session of a multi-session capthist object
is interpreted as an independent stratum that contributes one component
of the log likelihood. Each stratum (session) has its own detectors and
capture data. This assumes that primary sessions within each stratum
have previously been joined manually in a nominally ‘single-session’
capthist. The function stratify
helps you construct
stratified capthist objects from collections of single-session
objects.
Fig. 2. Structure of data for stratified open-population analysis in openCR. Each stratum is a pre-joined (single-session) component of a multi-session capthist object. The internal structure and detector may differ between strata.
Stratified models may use ‘stratum’ as a factor-valued predictor. Groups of strata may be contrasted using stratum-level covariates as described later.
The various models available in openCR are named to encode the distinctions made in the ‘Brief survey’. Names are formed by concatenating four components:
Thus ‘JSSAsecrfCL’ is a spatial JSSA model parameterized in terms of
per capita recruitment f and
fitted by maximizing the conditional likelihood (a spatial version of
Link and Barker (2005), minus parameter covariation). Any movement model
is specified separately with the ‘movementmodel’ argument of
openCR.fit
.
Models of the form ‘JSSA…CL’ are variations on the Pradel–Link–Barker models. openCR 2.2 recognises labels of the form ‘PLB…’ as an alias for each of these models. Thus ‘PLBf’ is synonymous with ‘JSSAfCL’, and ‘PLBsecrl’ is synonymous with ‘JSSAsecrlCL’.
Parameters vary with the type of model, as listed below. Each of these primary parameters (‘real’ parameters in MARK) may also be modelled as a linear combination of predictors on a suitable link scale, allowing the inclusion of covariates and constraints. The coefficients of the parameter-specific linear combinations are called ‘beta’ parameters in MARK; the likelihood is maximized with respect to the concatenated list of beta parameters.
Table 2. Parameter definitions and default link functions (nonspatial models)
Parameter | Symbol | Link | Description |
---|---|---|---|
p | p | logit | capture probability (recapture probability for CJS) |
phi* | ϕ | logit | apparent survival |
b | b | mlogit | entry probability cf PENT in MARK |
f* | f | log | per capita recruitment rate |
gamma* | γ | logit | seniority (Pradel 1996) |
lambda* | λ | log | population growth rate (finite rate of increase) |
superN | N | log | superpopulation size |
BN | BN | log | number of entrants |
N | Nj | log | time-specific population size |
* parameters marked with an asterisk are scaled by the interval between primary sessions.
Table 3. Parameters of nonspatial openCR models
Type | Alias | p | phi | b | f | gamma | lambda | superN | BN | N |
---|---|---|---|---|---|---|---|---|---|---|
CJS | + | + | ||||||||
JSSAbCL | PLBb | + | + | + | ||||||
JSSAfCL | PLBf | + | + | + | ||||||
JSSAgCL | PLBg | + | + | + | ||||||
JSSAlCL | PLBl | + | + | + | ||||||
JSSAb | + | + | + | + | ||||||
JSSAf | + | + | + | + | ||||||
JSSAg | + | + | + | + | ||||||
JSSAl | + | + | + | + | ||||||
JSSAB | + | + | + | |||||||
JSSAN | + | + | + |
Models with type ending in CL are of the Pradel–Link–Barker type, with aliases as shown.
openCR mostly fits models by modelling capture
histories one-by-one. An alternative faster method is to evaluate the
likelihood expressed in terms of sufficient statistics. Sufficient
statistics vary among models, but they are typically counts such as
provided by the function JS.counts
. The ‘sufficient
statistics’ approach is not compatible with individual covariates. The
non-spatial model types ‘Pradel’ and ‘Pradelg’ are implemented in
openCR using sufficient statistics (Pradel 1996) and
therefore fall outside the main framework (Table 3). They correspond to
‘JSSAlCL’ and ‘JSSAgCL’ respectively, and estimate the same parameters
as those models. Estimates should coincide except when there are losses
on capture. ‘Pradel’ is parameterized in terms of population growth rate
(lambda) and ‘Pradelg’ is parameterized in terms of seniority
(gamma).
Additionally, the function JS.direct
computes classic
Jolly–Seber estimates using the sufficient statistics.
Table 4. Parameter definitions and default link functions (spatial models)
Parameter | Symbol | Link | Description |
---|---|---|---|
lambda0 | λ0 | log | detection function intercept |
sigma | σ | log | detection function scale (m) |
z | z | log | detection function shape parameter (HHR, HAN, HCG, HVP) |
phi* | ϕ | logit | apparent survival |
b | b | mlogit | entry probability (beta) |
f* | f | log | per capita recruitment rate |
gamma* | γ | logit | seniority (Pradel 1996) |
lambda* | λ | log | population growth rate (finite rate of increase) |
superD | D | log | superpopulation density |
BD | BD | log | entrants per hectare |
D | Dj | log | time-specific population density |
* parameters marked with an asterisk are scaled by the interval between primary sessions.
Table 5. Parameters of spatial openCR models
Type | Alias | lambda0 | sigma | z | phi | b | f | gamma | lambda | superD | BD | D |
---|---|---|---|---|---|---|---|---|---|---|---|---|
CJSsecr | + | + | + | + | ||||||||
JSSAsecrbCL | PLBsecrb | + | + | + | + | + | ||||||
JSSAsecrfCL | PLBsecrf | + | + | + | + | + | ||||||
JSSAsecrgCL | PLBsecrg | + | + | + | + | + | ||||||
JSSAsecrlCL | PLBsecrl | + | + | + | + | + | ||||||
JSSAsecrb | + | + | + | + | + | + | ||||||
JSSAsecrf | + | + | + | + | + | + | ||||||
JSSAsecrl | + | + | + | + | + | + | ||||||
JSSAsecrB | + | + | + | + | + | |||||||
JSSAsecrD | + | + | + | + | + | |||||||
secrCL | + | + | + | |||||||||
secrD | + | + | + | + |
Spatial models with type ending in CL have features in common with the Pradel–Link–Barker models, hence the aliases as shown.
Formulae define a linear model for each ‘real’ parameter (p, phi, sigma etc.) on the link scale (logit, log etc.). Alternative link functions not shown in Tables 2 and 4 are ‘loglog’ and ‘sin’, both as defined in MARK.
The default linear combination for each parameter is a constant, null model (~1, parameter constant over time, unaffected by individual differences etc.). To include other effects build formulae using either predefined (built-in) predictors listed here, or the names of covariates.
Table 6. Built-in predictors (‘sessions’ refers to primary sessions)
Predictor | Parameters | Description |
---|---|---|
stratum | all | Factor, one level per stratum (stratified = TRUE ) |
session | all except ‘superN’, ‘superD’ | Factor, one level per primary session |
t | all except ‘superN’, ‘superD’ | synonym of ‘session’ |
Session | all except ‘superN’, ‘superD’ | Continuous time |
b | p, phi, lambda0, sigma | learned response (persists across sessions) |
B | p, lambda0, sigma | transient (Markovian) response across sessions |
bk | p, phi, lambda0, sigma | detector-specific learned response (persists across sessions) |
bsession | p, lambda0, sigma | learned response within sessions |
Bsession | p, lambda0, sigma | transient (Markovian) response within sessions |
bksession | p, lambda0, sigma | detector-specific learned response within sessions |
Bksession | p, lambda0, sigma | detector-specific transient (Markovian) response within sessions |
h2 | all except abundance | 2-class finite mixture |
h3 | all except abundance | 3-class finite mixture |
age | all except abundance | age factor |
Age | all except abundance | linear effect on age |
Age2 | all except abundance | linear effect on age2 |
Differences among the various learned responses may be understood by examining their effect on the parameter index array (PIA). This table illustrates the PIA slice corresponding to an individual with the non-spatial detection history shown (4 primary sessions, each of 4 secondary sessions). The values ‘1’ and ‘2’ refer to different parameter combinations, most commonly to levels of lambda0.
Detection history : | 0100 0000 0000 0100 | |
---|---|---|
~bsession | 1122 1111 1111 1122 | persistent within primary session |
~Bsession | 1121 1111 1111 1121 | transient within primary session |
~b | 1122 2222 2222 2222 | persistent |
~B | 1122 2222 1111 1122 | transient across primary sessions |
IMPORTANT NOTE: Learned response predictors (‘b’, ‘bsession’ etc.) were re-defined in openCR 1.3.0. Models fitted with earlier versions should be re-fitted.
The rules for covariates largely follow secr (secr-overview.pdf). Covariates may be at the level of stratum, primary session, secondary session (detection parameters only), individual (CL models only), or detector (spatial models only). Further complexity may be modelled by providing custom design data cutting across these categories (see below).
Individual and detector covariates are named columns in the ‘covariates’ attributes of the respective capthist and traps object. Covariate names should differ from the built-in predictors (Table 6).
Stratum covariates are provided to openCR.fit
in the
argument ‘stratumcov’. That should be a dataframe with one row per
stratum; the name of any column may be used in a model formula.
Primary session covariates are provided to openCR.fit
in
the argument ‘sessioncov’, rather than associated with a data object. If
‘sessioncov’ is a vector (length equal to number of primary sessions)
rather than a dataframe then it may be referenced as ‘scov’ in model
formulae. For stratified data, ‘sessioncov’ may be a list with one
component per stratum (the lazy option of providing a single vector or
dataframe works only if all strata have the same sessions).
Covariates for detection parameters in secondary sessions are provided in the ‘timecov’ argument. If ‘timecov’ is a vector (length equal to total number of secondary sessions) rather than a dataframe then it may be referenced as ‘tcov’ in model formulae. For stratified data, ‘timecov’ may be a list with one component per stratum (the lazy option of providing a single vector or dataframe works only if all strata have the same primary and secondary sessions).
The types ‘secrD’ and ‘secrCL’ cause openCR.fit
to treat
the data as if from a closed population (no mortality, no recruitment,
no movement); the intervals attribute is ignored.
msk <- make.mask(traps(captdata), buffer = 100, type = 'trapbuffer')
fit_secr <- secr.fit(captdata, detectfn = 'HHN', mask = msk, trace = FALSE)
fit_openCR <- openCR.fit(captdata, detectfn = 'HHN', mask = msk, type = 'secrD')
# massage the predict.openCR results to the same format as predict.secr
pred_openCR <- plyr::rbind.fill(predict(fit_openCR))
pred_openCR <- pred_openCR[c(2,1,3), !(names(pred_openCR) %in% c('stratum','session'))]
rownames(pred_openCR) <- fit_secr$realnames
# compare estimates
predict(fit_secr)[,-1]
## estimate SE.estimate lcl ucl
## D 5.485 0.64703 4.356 6.9059
## lambda0 0.307 0.03413 0.247 0.3815
## sigma 28.764 1.30055 26.326 31.4283
## estimate SE.estimate lcl ucl
## D 5.485 0.64480 4.356 6.9059
## lambda0 0.307 0.03403 0.247 0.3815
## sigma 28.764 1.29988 26.326 31.4283
## secr.elapsed openCR.elapsed
## 1.655 1.322
The maximised log likelihoods differ because openCR
does not include the multinomial constant. secr has
function logmultinom
that lets us add it back:
# compare maximised log likelihoods
c(secr.logLik = logLik(fit_secr), openCR.logLik = logLik(fit_openCR) + logmultinom(captdata))
## secr.logLik openCR.logLik
## -758.9 -758.9
Two- and three-class finite mixtures (h2, h3) allow for individual heterogeneity in detection and turnover parameters (Pledger et al. 2003, 2010). Using one of these predictors in a formula causes a further real parameter ‘pmix’ to be added. pmix is the proportion in latent mixture class 2 for h2, and the proportions in classes 2 and 3 for h3 (the proportion in class 1 is obtained by subtracting from 1). The implementation in openCR assumes that class membership applies across all parameters. The posterior probabilities of class membership for all detected individuals are returned as the ‘posterior’ component of the fitted model.
Finite mixture likelihoods are prone to multimodality. Misleading estimates result when the numerical maximization settles on a local maximum (see also [secr-finitemixtures.pdf].
If age is modelled as a factor then it is useful to group older
animals in a maximum age class (‘maximumage’). ‘minimumage’,
‘maximumage’ and ‘initialage’ are optional components of the ‘details’
argument of openCR.fit
. ‘initialage’ can name an individual
covariate to avoid the assumption that all animals are the minimum age
at first detection.
Specify the details argument ‘agebreaks’ to group numeric ages into
age classes. Breaks are used with the cut
function to
generate a factor from the numeric ages; the cut
argument
‘right’ is set to FALSE to include the lower limit in each age class.
Extreme ages are shrunk to the interval [‘minimumage’, ‘maximumage’]
before grouping, so these arguments must be compatible with ‘agebreaks’
(e.g., ‘maximumage’ >= lower bound of oldest group). Check the
grouping by applying it to the matrix of numeric ages in your data. For
example,
agebrk <- c(0, 2, Inf)
# construct matrix of numeric ages (animal x secondary session)
age <- age.matrix(join(ovenCH), maximumage = 2, unborn = NA)
# tabulate the grouped ages
aclass <- cut(age, breaks = agebrk, right = FALSE)
table(age, aclass)
## aclass
## age [0,2) [2,Inf)
## 0 680 0
## 1 620 0
## 2 0 1000
The notation [0,2) indicates ages in the interval 0 ≤ age < 2. The numbers in older groups include animals never seen again and possibly dead.
This example illustrates how to use grouped ages in a model. The data are an undocumented non-spatial selection from the same brushtail possum study as OVpossumCH (trapping in February, June and September, 1980–1988, known-age females only; interval in years). The individual covariate ‘age’ records the age of each possum at first capture, in years.
# retrieve capthist object
datadir <- system.file('extdata', package = 'openCR')
CH <- readRDS(paste0(datadir,'/poss8088F.RDS'))
# model with grouped ages; any maximumage>=6 OK
fit <- openCR.fit(CH, model = list(phi ~ age), details = list(
agebreaks = c(0,2,4,6,Inf), initialage = 'age', maximumage = 6))
# show results for first session only, as no time effect fitted
# levels of age grouping factor are stored in 'design' object
newdat <- data.frame(age = fit$design$agelevels)
predict(fit, newdata = newdat)$phi
## session age estimate SE.estimate lcl ucl
## 1 Feb1980 [0,2) 0.5622 0.06095 0.4415 0.6760
## 2 Feb1980 [2,4) 0.9152 0.03530 0.8157 0.9634
## 3 Feb1980 [4,6) 0.8775 0.04529 0.7583 0.9424
## 4 Feb1980 [6,Inf) 0.8220 0.02079 0.7776 0.8592
If ‘agebreaks’ is omitted then the default uses bins of width 1 time unit from ‘minimumage’ up to, but not including, ‘maximumage’, with an extra bin for ‘maximumage’ and above (7 bins [0,1),…,[6,Inf) in this example).
The older ‘agecov’ mechanism is limited to sampling sessions separated by one time unit and is deprecated from 2.2.6.
For a quadratic relationship with age, specify an additive model with both Age and Age2 terms (e.g., model = phi ~ Age + Age2).
We have seen the role of the intervals attribute in defining primary and secondary sessions. Between-session intervals need to be specified only if they vary, or if you would like rates (phi, gamma, lambda, f) to be reported in time units other than the (implicitly constant) sampling interval. Scaling from the standardised parameter θj to the interval-specific value θj′ uses θj′ = θjTj where θj is one of ϕj or λj, and Tj is the duration of interval j.
Scaling γ follows the same pattern except that the relevant duration for γj is Tj − 1. Scaling per capita recruitment fj is more tricky. We use fj′ = (ϕj + fj)Tj − ϕjTj.
Occasionally there is a need for covariates that do not relate
specifically to individuals, sessions or detectors, and are not included
as canned predictors. For this you must construct your own dataframe of
design data and pass it as the ‘dframe’ argument of
openCR.fit
. Design data are used as input to the
model.matrix
function (the ‘data’ argument);
model.matrix
generates the design matrix for each real
parameter. Design data are usually constructed internally in
openCR.fit
from named covariates and other predictors that
appear in model formulae; if ‘dframe’ is provided then the internally
constructed design data are added as extra columns, overwriting any
custom columns of the same name. The same design dataframe is used for
all parameters.
Constructing ‘dframe’ is fiddly. The dataframe should have one row
for each combination of unique capture history, secondary session,
detector and latent class (mixture). For nonspatial models without
finite mixtures this collapses to one row for each capture history and
secondary session. The order of rows follows that of the elements in an
array with dimensions (n,
S, K, X) for n unique capture histories, S secondary sessions, K detectors and X latent classes9. The
secr function insertdim
can help to expand
data into the correct row order.
A warning: by default openCR.fit
replaces the input
capthist with a more compact version using only unique capture histories
(the number of each is kept in the individual covariate ‘freq’; see the
function squeeze
). Design data are in terms of the
‘squeezed’ capture histories.
In this example we define a function to construct custom design data for a learned response.
makedf.b <- function (ch, spatial = FALSE, nmix = 1, naive = FALSE) {
R <- 1 # assume single stratum
ch <- squeeze(ch)
# Construct matrix of logical values TRUE iff caught before
detected <- apply(abs(ch),1:2,sum)>0
detected <- t(apply(detected, 1, cumsum)>0)
if (naive)
b <- rep(FALSE, prod(dim(ch)[1:2]))
else
b <- t(apply(detected, 1, function(x) {x[which.max(x)] <- FALSE; x}))
# For a simple non-spatial case: data.frame(customb = as.vector(b))
# More generally:
n <- nrow(ch)
S <- ncol(ch)
K <- if (spatial) dim(ch)[3] else 1
data.frame(customb = insertdim(b, c(2,3,1), c(R,n,S,K,nmix)))
}
Now compare the result with the canned predictor ‘b’ for a persistent learned response.
ovenj <- join(ovenCH)
fitb <- openCR.fit(ovenj, model = p ~ b)
fitbc <- openCR.fit(ovenj, model = p ~ customb, dframe = makedf.b(ovenj))
AIC(fitb, fitbc)
## model npar rank logLik AIC AICc dAIC AICwt
## fitb p~b phi~1 3 2 -254.6 515.2 515.6 0 0.5
## fitbc p~customb phi~1 3 2 -254.6 515.2 515.6 0 0.5
Our custom model gives exactly the same result as the canned
predictor ‘b’ when type = ‘CJS’ because the precise secondary session of
first capture is irrelevant for CJS models (recaptures are modelled only
for subsequent primary sessions unless
details$CJSp1 == TRUE
).
Discrepancies can arise with non-CJS models because these account for animals never detected. The corresponding likelihood component uses a distinct design matrix for a ‘naive’ animal. To customize non-CJS models a separate dframe should be provided that applies to naive animals:
fitb2 <- openCR.fit(ovenj, model = p ~ b, type = 'JSSAfCL', start = fitb)
fitbc2 <- openCR.fit(ovenj, model = p ~ customb, type = 'JSSAfCL',
dframe = makedf.b(ovenj), dframe0 = makedf.b(ovenj, naive = TRUE))
AIC(fitb2, fitbc2)
## model npar rank logLik AIC AICc dAIC AICwt
## fitb2 p~b phi~1 f~1 4 4 -660.9 1330 1330 0 0.5
## fitbc2 p~customb phi~1 f~1 4 4 -660.9 1330 1330 0 0.5
An ad hoc adjustment for transience may be programmed as follows (cf Pradel et al. 1997).
makedf.resident <- function (ch, spatial = FALSE, nmix = 1) {
nstrata <- 1 # assume single stratum
ch <- squeeze(ch)
n <- nrow(ch)
S <- ncol(ch)
K <- if (spatial) dim(ch)[3] else 1
primary <- primarysessions(intervals(ch))
detected <- apply(abs(ch),1:2,sum)>0
nprimary <- apply(detected, 1, function(x) length(unique(primary[x])))
data.frame(resident = insertdim(nprimary>1, 1, c(nstrata, n, S, K, nmix)))
}
A simpler approach is to code an individual covariate that scores whether an individual was detected in more than one primary session.
addresidentcov <- function (ch) {
primary <- primarysessions(intervals(ch))
detected <- apply(abs(ch), 1:2, sum)>0
nprimary <- apply(detected, 1, function(x) length(unique(primary[x])))
covariates(ch) <- data.frame(residentcov = nprimary>1)
ch
}
Results are identical:
ovenj <- join(ovenCH)
ovenj <- addresidentcov(ovenj)
fitnull <- openCR.fit(ovenj, model = phi ~ 1)
fitcov <- openCR.fit(ovenj, model = phi ~ residentcov)
fitdf <- openCR.fit(ovenj, model = phi ~ resident, dframe = makedf.resident(ovenj))
fits <- openCRlist(fitnull, fitcov, fitdf)
AIC(fits)
## model npar rank logLik AIC AICc dAIC AICwt
## fitcov p~1 phi~residentcov 3 2 -225.8 457.6 458.0 0.00 1
## fitnull p~1 phi~1 2 2 -254.6 513.2 513.4 55.56 0
## fitdf p~1 phi~resident 3 2 -254.6 515.2 515.6 57.56 0
pred <- predict(fits, newdata = data.frame(resident = TRUE, residentcov = TRUE))
do.call(rbind, lapply(pred, '[[', 'phi'))
## session resident residentcov estimate SE.estimate lcl ucl
## fitnull 2005 TRUE TRUE 0.4630 0.05473 0.3590 0.5703
## fitcov 2005 TRUE TRUE 0.7387 0.08767 0.5372 0.8732
## fitdf 2005 TRUE TRUE 0.4630 0.05473 0.3590 0.5703
Hines et al. (2003) suggested extending the definition of residence to include animals captured at least d days apart within a primary session; either of the approaches here may be modified accordingly. Here is the code for two individual covariates:
addresidentcov2 <- function (ch, d = 1) {
primary <- primarysessions(intervals(ch))
secondary <- secondarysessions(intervals(ch))
detected <- apply(abs(ch), 1:2, sum)>0
nprimary <- apply(detected, 1, function(x) length(unique(primary[x])))
dsecondary <- apply(detected, 1, function(x)
max(by(secondary[x], primary[x], function(y) diff(range(y)))))
covariates(ch) <- data.frame(residentcov1 = nprimary>1,
residentcov2 = nprimary>1 | dsecondary>=d)
ch
}
Factor predictors take a number of discrete values (levels). These are usually represented by columns of 0’s and 1’s in the design matrix, where the number of columns (and coefficients) relates to the number of levels. The default in R is to use ‘treatment contrasts’; one coefficient describes a reference class (level) and other coefficients represent the effect size (difference from the reference class on the link scale). By default the first level is used as the reference: for time effects (t, session) the first primary session is the reference level10.
This may lead to trouble if the parameter is not identifiable in the
reference class. One workaround is to specify a session covariate with
differently ordered levels. Another is to switch to dummy variable
coding in which each coefficient represents the magnitude of one real
parameter on the link scale (useful in itself). Dummy variable coding is
achieved by removing the intercept from the formula (-1), assuming the
default contrast function for factor coding
(contr.treatment
; check with
options()$contrasts
). The following model fits yield the
same estimates of ‘real’ parameters and the same log-likelihood, but
with different ‘beta’ parameters:
## beta SE.beta lcl ucl
## p -1.54953 0.2459 -2.0315 -1.0675
## p.t3 0.32963 0.3280 -0.3133 0.9725
## p.t4 -1.42728 0.5259 -2.4581 -0.3965
## p.t5 -0.14375 0.4489 -1.0236 0.7361
## phi -0.03141 0.2399 -0.5016 0.4388
## beta SE.beta lcl ucl
## p.t2 -1.54955 0.2459 -2.0316 -1.0675
## p.t3 -1.21990 0.2188 -1.6487 -0.7911
## p.t4 -2.97677 0.4663 -3.8907 -2.0628
## p.t5 -1.69325 0.3783 -2.4347 -0.9518
## phi -0.03142 0.2399 -0.5016 0.4387
Dummy variable coding has proved useful for avoiding some
maximization problems. From openCR 2.1.0, dummy
variable coding can be selected with the ‘details’ argument
‘dummyvariablecoding’. This updates the model to remove the intercept,
and assigns the default starting value across all levels of a factor
(rather than zero for non-reference levels). The following fit is
therefore equivalent to the preceding fitd
.
## beta SE.beta lcl ucl
## p.t2 -1.54955 0.2459 -2.0316 -1.0675
## p.t3 -1.21990 0.2188 -1.6487 -0.7911
## p.t4 -2.97677 0.4663 -3.8907 -2.0628
## p.t5 -1.69325 0.3783 -2.4347 -0.9518
## phi -0.03142 0.2399 -0.5016 0.4387
Suppose you wish to estimate the average of a parameter across levels
of a factor such as time (session). Cooch and White (2019 Section 6.15)
advocate modifying the design matrix so that one beta parameter
(coefficient) relates directly to the mean. This is achieved very simply
in openCR.fit
11 by setting the contrast function for the
factor to contr.sum
in the details
argument12. With
the resulting factor coding the first coefficient corresponds to the
mean. Applying this to estimate the average time-specific survival rate
for the dippers assuming constant recapture probability:
fit <- openCR.fit(dipperCH, model = phi~t, details = list(contrasts = list(t = contr.sum)))
invlogit(coef(fit)['phi',c('beta','lcl','ucl')])
## beta lcl ucl
## phi 0.5633 0.505 0.6199
The mean is backtransformed from the link scale. This results in some bias owing to the nonlinearity of link functions other than the identity function. Cooch and White take the position that the bias is often ignorable.
Potential movement of home ranges between primary sessions (=
dispersal) is a critical part of open-population models (Efford and
Schofield 2022). The argument movementmodel
of
openCR.fit
allows the possibilities in Table 7. Two of
these do not model movement at all. The default ‘static’ is a null model
in which each animal retains the same home range. The ‘IND’ option
models the locations of an animal independently in each primary session;
information is sacrificed and the implied movement depends on the size
of the habitat mask.
The remaining options (‘BVN’, ‘BVE’, ‘BVC’, ‘BVT’, etc.) fit a dispersal kernel (Nathan et al. 2012) to represent movement between primary sessions. This usually requires at least one more parameter to represent the spatial scale of dispersal.
Table 7. Models for movement between primary sessions.
Movement model | Parameters | Description (aliases in parentheses) |
---|---|---|
static |
0 | Centres constant across primary sessions |
BVN |
1 | Bivariate normal (‘normal’, Gaussian) |
BVE |
1 | Bivariate Laplace kernel (‘exponential’) |
BVC |
1 | Bivariate Cauchy kernel |
BVT |
2 | Bivariate t (‘t2D’, 2Dt) |
RDE |
1 | Exponential distance moved |
RDG |
2 | Gamma distance moved |
RDL |
2 | Lognormal distance moved |
UNI |
0 | Uniform within arbitrary radius |
IND |
0 | Centres unconstrained within habitat mask |
(user function) | 0,1,2 | User-supplied function (ncores = 1 only) |
Note: ‘BVN’, ‘BVE’ and ‘BVT’ kernels were previously designated ‘normal’, ‘exponential’ and ‘t2D’ respectively, and these names are still recognised.
Note: The online vignette openCR-kernel.pdf covers movement kernels in detail. This section is retained for historical reasons and will be removed in future.
All movement kernels in openCR are radially symmetrical. Relative probability of movement is specified in terms of radial distance r from the point of origin (Table 8). Four of the built-in kernels (BVN, BVE, BVC, BVT) are defined directly as bivariate probability density functions g(r). Three others (denoted RDE, RDG, RDL) are defined indirectly by the univariate distribution of distance moved f(r) where a point on the kernel has polar coordinates (r, θ) assuming direction θ uniform on (0, 2π) (Cousens et al. 2008, Ergon and Gardner 2014).
The extent of the kernel is controlled by the argument ‘kernelradius’ that gives the radius in terms of mask cells. Cell-specific probabilities are normalised so that they sum to 1.0 across the kernel. Dispersal probability effectively falls to zero at the boundary of the kernel, so the kernel radius is a critical part of the model. The uniform ‘UNI’ kernel has no parameters but depends critically on the user-specified kernel radius.
Table 8. Kernel probability density functions. ‘move.a’ and ‘move.b’ are the names used in openCR for scale and shape parameters, as indicated in the table. Based in part on Nathan et al. (2012, Table 15.1) and Clark et al. (1999) with adjustment for parameterisation in openCR. g(r) = f(r)/(2πr).
Kernel | move.a |
move.b |
f(r) | Mean r* |
---|---|---|---|---|
BVN | α | — | $\frac{r}{ \alpha^2} e^{ \frac{-r^2}{2\alpha^2} }$ | $\alpha \sqrt{\frac{ \pi}{2}}$ |
BVE | α | — | $\frac{r}{\alpha^2} e^{ \frac{-r}{\alpha}}$ | 2α |
BVT | α | β | $\frac{2 \beta r}{\alpha^2} \left( 1 + \frac{r^2}{\alpha^2} \right)^{-(\beta+1)}$ | $\alpha \frac{\sqrt \pi}{2} \frac{\Gamma \left( \beta-0.5 \right)}{\Gamma (\beta)}$ |
RDE | α | — | $\frac{1}{\alpha} e^{\frac{-r}{\alpha}}$ | α |
RDG | α | β | $\frac{1}{\Gamma(\beta)\alpha^\beta} r^{\beta-1} e^{ \frac{-r}{\alpha} }$ | αβ |
RDL | exp μ | 1/(eσ2 − 1) | $\frac{1}{r \sigma \sqrt{2 \pi}} e^{ \frac{-(\ln(r)-\mu)^2}{2\sigma^2} }$ | $e^{\mu + \frac{\sigma^2}{2}}$ |
UNI |
— | — | ||
(user) | a | b |
* Continuous, untruncated, kernel. Expected values for the
discretized and truncated kernel will be less (see
summary.kernel
).
The ‘BVT’ kernel is the same as ‘2Dt’ of Clark et al. (1999) and
Nathan et al. (2012). The parameter α (move.a
) corresponds
to a in Nathan et al. (2012)
and $\sqrt u$ in Clark et al. (1999);
the parameter β
(move.b
) corresponds to b − 1 in Nathan et al. (2012) and
p in Clark et al. (1999).
Defining move.b
as β ≡ b − 1 is handy because
the default link for move.b
(log) then ensures b > 1. The degrees of freedom of
the corresponding t-distribution are given by ν = 2β.
The `BVT’ kernel approaches bivariate normal as β → ∞ and Cauchy as β → 0 (e.g., Clark et al. 1999). Clark et al. (1999 p. 1485) found it hard to fit this kernel to seed dispersal data. The mean is undefined for β ≤ 0.5.
openCR 2.2 introduces zero-inflated versions of kernels otherwise defined with one parameter or none. Zero-inflated kernels use the suffix ‘zi’, hence ‘BVNzi’, ‘BVEzi’, ‘RDEzi’, ‘UNIzi’. The kernel-free independent movement model ‘IND’ also has a zero-inflated form ‘INDzi’ that is not strictly independent or uncorrelated. Each of these models has an additional zero-inflation parameter (move.b or move.a depending on whether the base kernel does or does not already have a parameter). Zero-inflated kernels often fit well, but it is common for the fitted scale parameter ‘move.a’ of BVNzi, BVEzi and RDEzi models to become large and essentially unidentifiable as the kernel for r > 0 flattens.
A kernel function may be specified by the user and passed in the
argument movementmodel
. The function should have argument
r, and optionally a, or a and b (the last two correspond to
openCR parameters move.a
and
move.b
) It should return a vector of values one for each
element of r, although
length(r) = 1 when the likelihood is evaluated in C++
(details$R = FALSE
, the default). The code should give a
valid result when r = 0 that
will be used for the origin cell. With the default link (‘log’ for both
move.a
and move.b
) there is no risk of a ≤ 0 or b ≤ 0.
A big problem with standard kernels as defined in openCR <2.0.0 is that the number of cells increases with the square of the radius. Processing time is roughly proportional to the number of cells, and kernels with many cells fit slowly. openCR 2.0.0 introduces novel ‘sparse’ kernels that include only those grid cells that lie on 4 axes (N-S, E-W, NW-SE, NE-SW) (Efford 2022b). The number of cells then increases only linearly with radius. Cell-wise movement probabilities are adjusted so that the distribution of dispersal distances is almost unchanged (essentially multiplying by 2πr at radius r, and adjusting cells on the oblique axes by $\sqrt 2$).
Sparse kernels are obtained by setting
sparsekernel = TRUE
when fitting a model with
openCR.fit()
. Here is an example.
par(mar = c(3,1,4,5))
k <- make.kernel(movementmodel = 'BVN', kernelradius = 10, spacing = 10, move.a = 40,
sparse = TRUE, clip = TRUE)
plot(k)
symbols(0,0, add = TRUE, circles = 100, inches = FALSE)
Note that the maximum on each axis is no longer at the centre. In fact, the central cell is assigned zero weight because r = 0 (this is undesirable and may be corrected in future). Each oblique arm in the example has only 7 cells; these cells have higher weighting to avoid orientation bias.
Somewhat surprisingly, sparse kernels appear to work about the same as full kernels, only faster.
When a kernel is applied to cells near the edge of a habitat mask some projected movements will lie outside the mask. This creates a problem for the model. Kernel cell values are probabilities summing to one; the cell probabilities of a truncated kernel will no longer be true probabilities and results are prone to bias.
openCR.fit
offers two approaches to resolve this
problem:
If the mask is rectangular, the truncated cells (and their
probabilities) may be ‘wrapped’ to the opposing edge of the mask. This
works fine if the kernel is not too large. Wrapping does not impose a
computational burden. A rectangular mask is generated by
make.mask
with the default
type = 'traprect'
.
For any mask, the cell probabilities of a truncated kernel may be scaled (normalized) so that they sum to 1.0. This requires substantial additional computation.
The edge method is chosen by setting the argument ‘edgemethod’ in
openCR.fit
; the options are ‘truncate’ (default in 1.5.0
and later), ‘wrap’, and ‘none’. Wrapping is fast, but it will cause an
error if the mask is not rectangular. If a rectangular mask does not
make sense (e.g., because the habitat is patchy) then you must use
edgemethod = 'truncate'
for unbiased estimates.
Prior to 1.5.0 there was no adjustment (movement truncated without
normalization, equivalent to edgemethod = 'none'
in later
versions) and estimates from movement models could be biased because the
probability of a null (all-zero) history was estimated incorrectly.
A kernel may be constructed with make.kernel
and
visualised with the plot
method. Use the
summary
method to obtain a terse description.
par (mar = c(3,3,4,6), cex = 0.9)
k <- make.kernel (movementmodel = 'BVN', spacing = 10, move.a = 40, clip = TRUE)
plot(k, contour = TRUE)
## Kernel radius (cells) : 10
## Spacing (side of cell) : 10 (m)
## Number of cells : 349
## Movement model : BVN
## Parameter(s) : move.a = 40
## Proportion truncated : 0.03189
## Movement as truncated at edge of kernel
## Empirical mean distance : 47.91 (m)
## Expected distance : 47.19 (m)
## 50th percentile (median) : 45.61 (m)
## 90th percentile : 79.39 (m)
## Movement, untruncated kernel
## Expected distance : 50.13 (m)
## 50th percentile (median) : 47.1 (m)
## 90th percentile : 85.84 (m)
Use the secr function spotHeight(k)
to
display cell values on the plot.
The independent option ‘IND’ (previously ‘uncorrelated’) is not recommended. It discards information on the continuity of home ranges between primary sessions, and estimates may vary with the (often arbitrary) extent of the habitat mask.
Kernel-based movement models require extreme care. Definitive advice cannot yet be given on the safe use of these models. Long-distance movements will usually be poorly sampled and poorly modelled.
User-defined functions cannot be used with multithreaded C++, so
they will be slow to fit; always set ncores = 1
.
When one of the kernel models is used (movementmodel
not
‘static’, ‘IND’ or ‘INDzi’) the movement model may be modified by
weighting settlement according one or more local (mask) covariates. The
weights are given by a new parameter ‘settle’. By default the logarithm
of ‘settle’ is a linear combination of mask covariates with no
intercept. ‘settle’ may also vary by
The settlement model is invoked by setting
details = list(settlemodel = TRUE)
.
This code compares a model with uniform settlement to one in which settlement varies with the ‘y’ coordinate of the mask. The data are the ovenbird mistnetting data compressed to a single occasion per year.
ovenCHb <- reduce(ovenCHp, by = 'all', outputdetector = 'count')
msk <- make.mask(traps(ovenCHp[[1]]), buffer = 500, spacing = 40, type = 'trapbuffer')
# uniform settlement
fit0 <- openCR.fit(ovenCHb, type = 'PLBsecrf', mask = msk, binomN = 1,
movementmodel = 'BVN', details = list(settlemodel = FALSE))
# logarithmic N-S gradient in settlement
fit1 <- openCR.fit(ovenCHb, type = 'PLBsecrf', mask = msk, binomN = 1,
movementmodel = 'BVN', details = list(settlemodel = TRUE), model = settle~y)
In this example there is no evidence for a N-S gradient in settlement. The intercept is removed automatically when the link function is the default (‘log’), as shown in the resulting formula for ‘settle’.
## model npar rank logLik AIC dAIC AICwt
## fit0 lambda0~1 phi~1 f~1 sigma~1 move.a~1 5 5 -953.3 1917 0.000 0.5838
## fit1 lambda0~1 phi~1 f~1 sigma~1 move.a~1 settle~y - 1 6 6 -952.7 1917 0.677 0.4162
## beta SE.beta lcl ucl
## lambda0 -3.4907 0.13367 -3.7527 -3.2287
## phi 0.6260 0.37561 -0.1102 1.3621
## f -1.1646 0.31579 -1.7836 -0.5457
## sigma 4.3264 0.07189 4.1855 4.4673
## move.a 4.9283 0.20971 4.5172 5.3393
## y -0.6941 0.61933 -1.9080 0.5198
The cumulative effect of differential settlement may be visualised
with function cumMove
by specifying a single mask covariate
with values in the range 0 to 1.
NOTE: Settlement models are a novelty in openCR 2.2.2 and their value is limited because survival and recruitment are not allowed to vary across space. The implementation may change.
Various derived parameters may be computed from a fitted model. Specifically,
HTbysession = TRUE
) the H-T estimate may be
based on the number detected in each session and the corresponding
session-specific estimates of p or a.Both goals are served by the derived
method for
openCR
objects. Among other outputs, this generates a
summary table with point estimates of all relevant parameters. We
demonstrate this with a new dipper model, fitted using conditional
likelihood:
dipperCL <- openCR.fit(dipperCH, type = 'JSSAlCL',
model = list(lambda~t, phi~t))
# only these parameters are in the model and estimated directly,
names(predict(dipperCL))
## [1] "p" "phi" "lambda"
# but we can derive b, f, gamma and N, as well as the super-population N
d <- derived(dipperCL)
print(d, digits = 3, legend = TRUE)
## Total number observed 294
## Parameters in model p, phi, lambda
## Superpopulation size 310.6
## Session-specific counts and estimates:
##
## stratum session t n R m r z time p phi lambda b f gamma kappa N
## 1 1 1 22 22 0 13 0 0 0.902 0.626 2.792 0.0785 2.166 NA NA 24.4
## 1 2 2 60 60 11 25 2 1 0.902 0.454 1.265 0.1701 0.811 0.224 2.23 68.1
## 1 3 3 78 78 26 36 1 2 0.902 0.478 1.026 0.1778 0.548 0.359 2.36 86.2
## 1 4 4 80 80 35 48 2 3 0.902 0.624 1.104 0.1519 0.480 0.466 2.05 88.4
## 1 5 5 88 88 47 51 3 4 0.902 0.608 1.103 0.1365 0.495 0.566 1.86 97.6
## 1 6 6 98 98 52 52 2 5 0.902 0.583 0.958 0.1554 0.375 0.551 2.09 107.6
## 1 7 7 93 93 54 0 0 6 0.902 NA NA 0.1298 NA 0.609 1.77 103.1
##
## Field Definition
## ------- -----------------------------------------
## stratum independent stratum
## session primary session
## t primary session
## n number observed
## R number released
## m number already marked
## r number recaptured in later session
## z number known alive but not caught
## time accumulated time since start
## p detection probability per secondary session
## phi apparent survival per unit time
## lambda population growth rate per unit time
## b entry probabilities
## f per capita recruitment per unit time
## gamma seniority (cf reverse-time phi)
## kappa recruitment parameter of Link and Barker (2005)
## N population size
The print
method for objects from derived
provides some control over formatting, as shown. Use the Dscale argument
to change area units (spatial models only).
derived
does not yet provide delta-method SE or
confidence intervals for derived parameters. A reliable workaround for
abundance paramaters (N, D)14 is to (i) infer the point estimates with
derived
15, (ii) assemble a start vector on the link
scale(s) for an equivalent full-likelihood openCR.fit
model
that includes the derived abundances, and (iii) run
openCR.fit
with method = "none"
to compute the
hessian at the MLE, and hence the full variance-covariance matrix.
The secr functions sim.popn
and
sim.capthist
provide the means to generate spatial
open-population data with known survival probability, population trend
λ and detection parameters.
Open population data are generated by setting nsessions > 1 in
sim.popn
and specifying a value for λ. Turnover settings are controlled
by components of the ‘details’ argument of sim.popn
. The
secr help page ?turnover should be consulted.
sim.capthist
should be called with renumber = FALSE
(otherwise individual capture histories cannot be matched across primary
sessions).
Use the openCR function sim.nonspatial
to generate non-spatial open-population data. openCR
also provides these functions to streamline simulation –
Function | Purpose |
---|---|
runsim.nonspatial |
Generate data with sim.nonspatial and fit models using
openCR.fit |
runsim.spatial |
Generate data with sim.popn and
sim.capthist , and fit models using
openCR.fit |
sumsims |
Summarise list output from runsim.nonspatial or
runsim.spatial |
runsim.nonspatial
and runsim.spatial
are
essentially wrappers; the user must provide appropriate argument values
for each of the nested functions.
It is common for some session-specific parameters of open capture–recapture models to be nonidentifiable, either for structural reasons or because the particular dataset is uninformative (e.g., Gimenez et al. 2004).
The main diagnostic is the rank of the Hessian matrix. If the rank is less than the number of parameters then the model is not fully identifiable and the estimates of some parameters will be confounded or unreliable. Matrix rank is determined numerically by counting non-zero eigenvalues. Computed eigenvalues of non-identifiable parameters may appear as small positive numbers, so it is necessary to apply an arbitrary numerical threshold.
Exactly which parameter estimates are unreliable can usually be
discerned from computed variances (SE and confidence intervals). Data
cloning (Lele et al. 2010) is also helpful; function
cloned.fit
implements the method for nonspatial models.
Session-specific turnover parameters may become nonidentifiable if
home ranges are allowed to move freely between primary sessions
(movementmodel = 'uncorrelated'
). Intuitively, this is
because radical changes in individual detection probability (due to
proximity to detectors) cannot be separated from mortality and
recruitment.
Bad estimates (zero, very large, close to starting values or zero variance) may merely indicate a problem with the maximization algorithm rather than nonidentifiability.
Numerical maximization of the likelihood requires appropriate starting values for the parameters. If starting values are poor then initial evaluations of the likelihood may return an infinite value, or otherwise provide inadequate direction for the numerical algorithm.
openCR.fit
provides a mechanism for recycling earlier
estimates as starting values: simply provide the name of a previously
fitted model as the start
argument. Parameters shared
between the models will be set to the old estimates, while unmatched
parameters will be set to defaults. A list of two previous models may be
provided; values from the first take precedence.
Variance estimation based on the Hessian matrix fails if the estimate lies on a boundary of the parameter space. Computed SE are then extreme, and confidence limits are implausible. This commonly happens when apparent survival (phi) approaches 1.0. Boundary estimates are more benign than other reasons for failure (the estimates themselves may be reliable). Alternative methods for variance estimation in this case have not been implemented.
Using the “sin” link for parameters bounded by 0 and 1 (the probability parameters p and phi) can be helpful.
The default method for maximizing the likelihood function is
Newton-Raphson as implemented in the R function nlm
. This
relies on numerical gradient estimates, which can cause trouble. Avoid
gradient estimation entirely by using the somewhat slower ‘Nelder-Mead’
method of function optim
e.g.,
fitnr <- openCR.fit(ovenCH, type = 'JSSAlCL', model = list(phi ~ t, lambda~t))
fitnm <- openCR.fit(ovenCH, type = 'JSSAlCL', model = list(phi ~ t, lambda~t),
method = "Nelder-Mead", details = list(control = list(maxit = 5000)))
The default maximum number of likelihood evaluations for the
Nelder-Mead algorithm (500) is often too small and results in a
“probable maximization error” warning. Here we increase it to 2000 by
setting the details argument “control” that is passed to
optim
.
Somewhat alarmingly, the NM algorithm settles on a lower log likelihood and different estimates:
## model npar rank logLik AIC AICc dAIC AICwt
## fitnr p~1 phi~t lambda~t 9 9 -656.7 1331 1334 0.000 0.9898
## fitnm p~1 phi~t lambda~t 9 9 -661.3 1341 1344 9.154 0.0102
We can fix that by feeding Nelder-Mead the starting values from another model:
fitnm <- openCR.fit(ovenCH, type = 'JSSAlCL', model = list(phi ~ t, lambda~t),
method = "Nelder-Mead", details = list(control = list(maxit = 2000)),
start = fitnr)
AIC(fitnm,fitnr)
## model npar rank logLik AIC AICc dAIC AICwt
## fitnm p~1 phi~t lambda~t 9 9 -656.7 1331 1334 0 0.5
## fitnr p~1 phi~t lambda~t 9 9 -656.7 1331 1334 0 0.5
In the longer term, better maximizers are needed.
The Newton-Raphson algorithm typically takes a large step in parameter space after a few iterations, and the resulting log-likelihood may be undefined (NA). Recovery is usually automatic, but sometimes maximization gets stuck at this point. From 2.2.6 it is possible to control the step size with the details argument ‘stepmax’. The default stepmax is generally 1000 on the link scale; and often stepmax = 2 works just as well:
Exceeding the iteration limit of nlm
results in code 4.
The default number of iterations was increased to 300 in
openCR 2.1.0 from the previous default of 100. Each
iteration in nlm
completes one evaluation of the gradient
of the likelihood function, and requires multiple likelihood
evaluations. For many parameters 300 iterations may still not be enough:
increase it with the details argument control
(e.g.,
details = list(control = list(iterlim = 500))
). See the
help for optim
for the relevant control settings of other
maximizers such as ‘Nelder-Mead’.
Boundary values of ‘beta’ coefficients may sometimes be avoided by
changing the default factor coding, particularly for session-specific
estimates (~t, ~session). This may be tackled manually, but from 2.1.0
there is a shortcut using the details
argument
‘dummyvariablecoding’. See the section above on Factor coding.
Spatial models are slow to fit. Consider these options
derive
can give
estimates of abundance (superN, N, superD, and D) from PLB models, as
well as alternative measures of recruitment.openCR ≥ 1.2 uses
multiple threads to run some calculations in parallel. Multithreading
uses RcppParallel. A
couple of tuning parameters are available. The number of threads is set
with the ‘ncores’ argument of openCR.fit
, or with the
setNumThreads
function of secr that sets
the environment variable RCPP_PARALLEL_NUM_THREADS. By default
openCR ≥ 1.5.0 uses
only 2 cores, for compliance with CRAN rules. You can increase this up
to the number of (virtual) cores available (i.e. 8 on a quad-core
desktop with hyperthreading), or some lesser number if you want to
multitask:
The
grain size' tuning parameter (see [RcppParallel](https://rcppcore.github.io/RcppParallel/)) may be varied with
details$grain`,
but it seems to have little effect.
Full models (not CL or Pradel) include superpopulation size N as a variable. The default in
openCR for both non-spatial and spatial models is to
treat N as a Poisson variable,
from which it follows that the number of individuals detected at least
once (n) is also Poisson. This
is also the default in secr. However, estimates from
POPAN models in MARK treat N
as fixed and n as binomial.
The assumption of fixed N
leads to narrower confidence intervals and estimates of detection and
turnover parameters that differ slightly from conditional likelihood
models (see e.g. Schofield and Barker 2016). To obtain JSSA estimates
from openCR that match those from MARK it is necessary
to set distribution = "binomial"
.
Several examples of analyses with openCR are given
in the associated vignette openCR-examples.pdf.
These use data already formatted as secr capthist
objects in R; the objects are provided in one or other package. All are
available immediately openCR is loaded with
library
. Each has its own help page.
Table 9. Data objects in openCR. ‘RD’ indicates robust design with multiple secondary sessions. See openCR-examples.pdf for references.
Data object | Spatial | RD | Species etc. | Source |
---|---|---|---|---|
microtusCH etc. | No | Yes* | Meadow vole Microtus pennsylvanicus USA | Nichols et al. (1984), Williams et al. (2002) |
FebpossumCH | No | Yes | Brushtail possum Trichosurus vulpecula New Zealand | M. Efford unpubl. |
dipperCH | No | No | European dipper Cinclus cinclus France | Lebreton et al. (1992), MARK |
gonodontisCH | No | No | Moth Gonodontis bidentata England | Bishop et al. (1978), Crosbie (1979) |
fieldvoleCH | Yes | Yes | Field vole Microtus agrestis Norway | Ergon and Lambin (2013) |
Table 10. Multi-session data objects in secr.
Data object | Spatial | RD | Species etc. | Source |
---|---|---|---|---|
OVpossumCH | Yes | Yes | Brushtail possum Trichosurus vulpecula New Zealand | M. Efford unpubl. |
ovenCHp | Yes | Yes | Ovenbird Seiurus aurocapilla USA | D. Dawson and M. Efford unpubl. |
This is generally an undeveloped field for spatially explicit capture–recapture models. Demonstrating that assumptions were not satisfied may also be of no consequence: we would usually ignore such a finding if the estimator is reasonably robust.
For Cormack-Jolly-Seber (nonspatial) models there is an established suite of tests following Burnham et al. (1987). The tests have been implemented in the U-CARE software of Choquet et al. (2009), recently translated into R by Gimenez et al (2018) as package R2ucare. Program RELEASE (Burnham et al. 1987) also implements the core CJS tests and is available through MARK.
The openCR function ucare.cjs
is a
wrapper for relevant functions in R2ucare, which should
be installed. We briefly demonstrate it here for the dipper data of
Marzolin (1988).
## Loading required namespace: R2ucare
## $Male
## $Male$components
## stat df p_val sign_test
## test3sr 6.778 5 0.238 -1.530
## test3sm 0.000 2 1.000 NA
## test2ct 4.284 2 0.117 -1.035
## test2cl 0.000 0 1.000 NA
##
## $Male$overall_CJS
## chi2 degree_of_freedom p_value
## Gof test for CJS model: 11.06 9 0.271
##
##
## $Female
## $Female$components
## stat df p_val sign_test
## test3sr 4.985 5 0.418 1.428
## test3sm 2.041 3 0.564 NA
## test2ct 3.250 4 0.517 -0.901
## test2cl 0.000 0 1.000 NA
##
## $Female$overall_CJS
## chi2 degree_of_freedom p_value
## Gof test for CJS model: 10.28 12 0.592
This invocation of ucare.cjs
calls the
R2ucare functions test3sr
,
test3sm
, test2ct
, test2cl
and
overall_CJS
for each sex and provides a condensed report.
For interpretation see the original papers, the R2ucare
vignette,
and Chapter 5 of the MARK book (Cooch and White 2019). Lebreton et
al. (1992: 86) indicate only Test 3SR is meaningful for these data (see
also openCR-examples.pdf).
openCR does not do
ucare.cjs
(above).Parameter counting and overdispersion adjustment are probably the most critical omissions. See Cooch and White (2019) for detailed coverage in the context of MARK.
Defaults for some arguments differ between openCR.fit
and secr.fit
. For openCR.fit
–
trace = FALSE
details$multinom = FALSE
)distribution
has been elevated to a full argument rather
than merely a component of details
. This argument describes
the distribution of the number of individuals detected (default
distribution = “poisson”) (see here).
When details$LLonly = TRUE
, openCR.fit
returns a vector with the log likelihood in position 1, followed by the
named starting values of the coefficients (beta parameters)
(secr.fit
returns only the log likelihood).
In secr the argument CL
is used in
secr.fit
to switch between full- and conditional-likelihood
models. In openCR conditional-likelihood models are
given a separate type
with the suffix CL (or use PLB
alias).
The predictor ‘t’ is used in secr models to indicate a factor with one level for each secondary session. In openCR it is a synonym for ‘session’, i.e. a factor with one level for each primary session. This is consistent with the use of ‘t’ in Lebreton et al. (1992) and makes for more compact model specification. In the unlikely event that you want to code a model with one level for each secondary session in openCR, use the ‘timecov’ argument.
Arguments to be passed to nlm() cannot merely be appended as in the
argument of secr.fit(), but must be passed as a named list in the
details argument control
. See here
for an example.
Parts of openCR are coded in C++, via the R package
Rcpp. The Rcpp interface requires less
copying of data, and enables the use of multiple threads via
RcppParallel. openCR also duplicates
some C++ functions in native R code, which is useful for debugging.
Select the R version by setting details = list(R = TRUE)
in
openCR.fit
. This currently works for most models except
those with detector type ‘multi’ and some exotic movement models.
Strata (openCR >=2.0) are analogous to sessions in secr in that they are treated as independent with no re-detections of animals between strata. The total log-likelihood in openCR is the sum of stratum log likelihoods, just as the total is the sum of session loglikelihoods in secr.
These features of secr are not available in openCR
make.table
may do the job)The non-spatial capability of openCR largely duplicates MARK and RMark. Several of the nonspatial model types have exact matches in MARK (Table 11).
Table 11. Relationship of non-spatial openCR models to MARK model types
openCR type | MARK model | Reference |
---|---|---|
CJS | CJS | Seber (1982) |
JSSAb | POPAN | Schwarz and Arnason (1996) |
JSSAfCL | LinkBarker | Link and Barker (2005) |
Pradel | Pradlambda | Pradel (1996) |
Pradelg | Pradsen | Pradel (1996) |
The R package marked (Laake, Johnson and Conn 2013) also overlaps substantially with the non-spatial features of openCR. Its interface echoes RMark just as openCR echoes secr. marked has some fancy features for individual covariates and random effects, and promises fast processing of large datasets. marked 1.2.6 includes full-likelihood JSSA (POPAN) models parameterized in terms of entry probabilities (type JSSAb)16, but not the other JSSA options in Table 3.
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Chandler, R. B. and Clark, J. D. (2014) Spatially explicit integrated population models. Methods in Ecology and Evolution 5, 1351–1360.
Choquet, R., Lebreton, J.-D., Gimenez, O., Reboulet, A.-M. and Pradel, R. (2009) U-CARE: Utilities for performing goodness of fit tests and manipulating CApture-REcapture data. Ecography 32, 1071–1074.
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Efford, M. G. (2004) Density estimation in live-trapping studies. Oikos 106, 598–610.
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Efford, M. G., Borchers D. L. and Mowat, G. (2013) Varying effort in capture–recapture studies. Methods in Ecology and Evolution 4, 629–636.
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Gimenez, O., Viallefont, A., Catchpole, E. A., Choquet, R. and Morgan, B. J. T. (2004) Methods for investigating parameter redundancy. Animal Biodiversity and Conservation 27, 561–572.
Gimenez, O., Lebreton, J.-D., Choquet, R. and Pradel, R. (2018) R2ucare: An R package to perform goodness-of-fit tests for capture–recapture models. Methods in Ecology and Evolution 9, 1749–1754.
Gimenez, O., Lebreton, J.-D., Choquet, R. and Pradel, R. (2022) R2ucare: Goodness-of-Fit Tests for Capture-Recapture Models. R package version 1.0.2. https://github.com/oliviergimenez/R2ucare/
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Code used to generate schematic diagrams of data structure.
onemulti <- function(st = c(0,6,11,15), le = c(5,4,3,5), yb = 7, col=col1, outer = TRUE) {
col <- rep(col, le)
xl <- unlist(mapply(":",st,le+st-1))
yb <- rep(yb,length(xl))
xr <- xl + width
yt <- yb + height
rect(xl,yb,xr,yt,col=col)
text(xl+width/2, yb+height/2, unlist(mapply(":", 1, le)))
xl <- st - margin
yb <- rep(yb[1], length(xl)) - margin
xr <- st+le-1+width+margin
yt <- yb+height+2*margin
rect(xl,yb,xr,yt)
text(st+le/2, rep(yb[1]+2*margin,length(st))+height+0.5, paste('session',1:length(st)))
if (outer) {
rect(st[1]-3*margin, yb[1]-2*margin, tail(st+le-1,1)+width+3*margin,
yb[1]+height+8*margin)
}
}
onejoined <- function(offset = 1.5, le = c(5,4,3,5), yb = 2.2, col=col1, intervals = TRUE,
intlabel = 'intervals', leftlabel = '', outer = TRUE) {
col <- rep(col, le)
xl <- 0:(sum(le)-1)+offset
yb <- rep(yb,length(xl))
xr <- xl + width
yt <- yb + height
rect(xl,yb,xr,yt,col=col)
text(xl+width/2, yb+height/2, c(1:length(xl)))
if (intervals) {
xi <- offset + (1:(length(xl)-1)) - (1-width)/2
xip <- cumsum(le)[-length(le)] # intermediate between primary sessions
intervals <- rep(0,length(xi))
intervals[xip] <- 1
text(xi, yb [-1]-0.8, intervals)
text(-0.2, yb[1]-0.8, intlabel)
segments(xi[xip], rep(yb[1]-0.4,length(xip)), xi[xip], rep(yb[1]+0.4,
length(xip))+height)
}
text (0.4, yb[1]+height/2, leftlabel, adj = c(1,0.5))
if (outer) {
rect(offset-2*margin, yb[1]-2*margin, sum(le)-1+offset+width+2*margin,
yb[1]+height+2*margin)
}
}
# Fig. 1 Single-stratum data
par(cex=1, xpd = TRUE, mfrow = c(1,1), mar=c(1,4,1,4))
width <- 0.85
height <- 1.1
margin <- 0.15
col1 <- c('salmon','pink','brown', 'red')
col2 <- c('green','lightgreen','darkgreen', 'lightblue')
MASS::eqscplot(0,0,xlim=c(0,20), ylim=c(0,8), type='n', axes=F,xlab='',ylab='')
onemulti(col = col1)
text(9, 5.2, 'join()', cex=1.1)
arrows (10.7,6.2,10.7,4.2)
onejoined(leftlabel='')
# Fig. 2 Multi-stratum data
par(cex = 0.9, xpd = TRUE, mfrow = c(1,1), mar = c(1,4,1,4))
MASS::eqscplot(0,0,xlim=c(-3,20), ylim=c(-2,8), type='n', axes=FALSE, xlab = '',ylab='')
onejoined(leftlabel='stratum 1', yb = 6.5, intlabel='')
onejoined(leftlabel='stratum 2', yb = 3, intlabel='')
onejoined(leftlabel='stratum 3', yb = -0.5, le = c(4,3,4,4), intlabel='', col = col2)
rect(-3, -2, 19.3, 8.7)
These supplementary vignettes are not included with the package. It is intended to distribute them on the website https://www.otago.ac.nz/density/. Otherwise contact the author.↩︎
As far as I know, this abbreviation was first used by Pledger et al. (2010). Recognising the contributions of Crosbie and Manly, Schofield and Barker (2009) and Cowen et al. (2010) referred to it the Crosbie-Manly-Arnason-Schwarz (CMAS) model. Link and Barker (2010) used ‘Crosbie-Manly-Schwarz-Arnason’ (CMSA) for the same model. CMSA has since been used by various authors, including Schofield and Barker (2016). JSSA is used in openCR because this highlights its evolution from the widely known Jolly-Seber model. POPAN refers to the software of Schwarz and Arnason (1996), recycled as the name of a data type in MARK.↩︎
A direct spatial implementation of CJS fails because the
distribution of detected animals is not uniform at first detection, but
rather biased towards the vicinity of the detectors. Set
details = list(CJSp1 = TRUE)
to model first detections and
get sensible estimates (model type ‘CJSsecr’).↩︎
This is equivalent of ~t in Lebreton et al. (1992) or
~time in RMark, and openCR recognises ~ t
as a synonym of ~ session
.↩︎
except for some mostly trivial differences relating to removals↩︎
this may not be true for spatial models with spatially varying density, but these models are not considered in openCR.↩︎
strictly, the product over observed histories is only one component of the likelihood↩︎
The terms ‘single-session’ and ‘multi-session’ are here used in the secr sense (secr-multisession). openCR uses these data structures, but interprets them differently as explained here.↩︎
This rectangular (or cuboidal) configuration includes cells that are redundant and unused for a particular model type (e.g., cells corresponding to sessions at or before first capture in CJS models). However, the full complement of rows is required in dframe.↩︎
This does not apply for times when a parameter can never be estimated – for example, openCR understands that seniority (gamma) is not estimated for the first session and uses the second session for the reference level.↩︎
This also works in secr.fit
.↩︎
Helmert contrasts (contr.helmert
) also
yield the mean as the first coefficient, but the coding is more
obscure.↩︎
However, the effect of a constraint (e.g., parameter constant over sessions) will vary depending on the parameter to which it is applied.↩︎
This may sometimes be feasible for derived recruitment parameters, but given the doubts introduced by differing constraints (e.g. constant f vs constant λ) it is better just to refit the model.↩︎
These are also the MLE when distribution = “poisson” (e.g., Schofield and Barker 2016).↩︎
dipper example in openCR-examples.pdf.↩︎