| Type: | Package |
| Title: | Fast Numerical Maximum Likelihood Estimation for Latent Markov Models |
| Version: | 3.0.0 |
| Description: | A variety of latent Markov models, including hidden Markov models, hidden semi-Markov models, state-space models and continuous-time variants can be formulated and estimated within the same framework via directly maximising the likelihood function using the so-called forward algorithm. Applied researchers often need custom models that standard software does not easily support. Writing tailored 'R' code offers flexibility but suffers from slow estimation speeds. We address these issues by providing easy-to-use functions (written in 'C++' for speed) for common tasks like the forward algorithm. These functions can be combined into custom models in a Lego-type approach, offering up to 10-20 times faster estimation via standard numerical optimisers. To aid in building fully custom likelihood functions, several vignettes are included that show how to simulate data from and estimate all the above model classes. |
| URL: | https://janolefi.github.io/LaMa/ |
| License: | MIT + file LICENSE |
| Encoding: | UTF-8 |
| Imports: | Rcpp, stats, utils, methods, Matrix, splines2, mgcv, MASS, numDeriv, RTMBdist (≥ 1.1.0) |
| LinkingTo: | Rcpp, RcppArmadillo |
| Depends: | R (≥ 3.5.0), RTMB (≥ 2.0) |
| RoxygenNote: | 7.3.3 |
| Suggests: | knitr, rmarkdown, testthat (≥ 3.0.0), PHSMM, MSwM, scales |
| VignetteBuilder: | knitr |
| Config/testthat/edition: | 3 |
| LazyData: | true |
| NeedsCompilation: | yes |
| Packaged: | 2026-10-28 13:04:00 UTC; jan-ole |
| Author: | Jan-Ole Fischer |
| Maintainer: | Jan-Ole Fischer <jan-ole.fischer@mailbox.org> |
| Repository: | CRAN |
| Date/Publication: | 2026-10-28 14:30:08 UTC |
LaMa: Fast Numerical Maximum Likelihood Estimation for Latent Markov Models
Description
A variety of latent Markov models, including hidden Markov models, hidden semi-Markov models, state-space models and continuous-time variants can be formulated and estimated within the same framework via directly maximising the likelihood function using the so-called forward algorithm. Applied researchers often need custom models that standard software does not easily support. Writing tailored 'R' code offers flexibility but suffers from slow estimation speeds. We address these issues by providing easy-to-use functions (written in 'C++' for speed) for common tasks like the forward algorithm. These functions can be combined into custom models in a Lego-type approach, offering up to 10-20 times faster estimation via standard numerical optimisers. To aid in building fully custom likelihood functions, several vignettes are included that show how to simulate data from and estimate all the above model classes.
Author(s)
Maintainer: Jan-Ole Fischer jan-ole.fischer@mailbox.org (ORCID)
See Also
Useful links:
Sparsity-retaining matrix multiplication
Description
Standard matrix multiplication destroys automatic sparsity detection by RTMB which is essential for models with high-dimensional random effects.
This can be mitigated by changing to "plain" with TapeConfig, but this can make AD tape construction very slow.
Here, we provide a different version that retains sparsity. It may be slightly slower than the standard method when constructing the AD tape.
Usage
A %sp% B
Arguments
A |
matrix of dimension n x p |
B |
matrix of dimension p x m |
Value
the matrix product of A and B, which is of dimension n x m
Examples
A <- matrix(1:6, nrow = 2, ncol = 3)
B <- matrix(7:12, nrow = 3, ncol = 2)
A %sp% B
Generate a colour-blind-friendly palette
Description
Generate a colour-blind-friendly palette
Usage
LaMaColors(ncolors)
Arguments
ncolors |
Number of colours to return; at most 10 |
Value
A colour palette of length ncolors
Examples
cb <- LaMaColors(3)
Sample parameters from approximate Gaussian posterior distribution
Description
Efficient Monte Carlo sampling of parameters (and REPORTed quantities) from the approximate posterior of an (R)TMB model.
See sdreport for details on posterior variance-covariance in random effects models.
Usage
MCreport(
obj,
nSamples = 1000,
include_random_pars = TRUE,
report = FALSE,
Q = NULL,
...
)
Arguments
obj |
Optimised |
nSamples |
Number of samples to draw |
include_random_pars |
Logical; Should random parameters be included in the output? |
report |
Logical; Should |
Q |
Optional precalculated sparse precision matrix returned by |
... |
For internal use only |
Details
Caution: This has nothing to do with Bayesian posterior sampling. It is simple Monte Carlo sampling from a Gaussian distribution with mean at the MLE and covariance given by the inverse of the Hessian (for fixed effects models) or the joint precision matrix (for random effects models). This is a common approach to get an approximate idea of parameter uncertainty around the MLE, but it relies on large-sample asymptotics.
Sampling random effects from their posterior as compared to calculating marginal standard devitions like sdreport is particularly useful for multidimensional random effects (e.g. for locations x and y)
where pointwise confidence intervals (e.g. along a path) based on standard deviations are not possible.
Value
A list structured like the original parameter list used in the MakeADFun call (potentially including additional REPORTed quantities). Each entry is a list with nSamples entries.
Examples
step <- trex$step[1:2000] # subsetting trex data
N <- 2 # 2 states
# custom likelihood
nll <- function(par) {
getAll(par)
Gamma <- tpm(eta)
delta <- stationary(Gamma)
mu <- exp(log_mu); REPORT(mu)
sigma <- exp(log_sigma); REPORT(sigma)
allprobs <- matrix(1, length(step), N)
for(j in 1:N) allprobs[,j] <- dgamma2(step, mu[j], sigma[j])
-forward(delta, Gamma, allprobs)
}
# initial parameters in named list
par0 <- list(eta = rep(-1.5,2),
log_mu = log(c(0.3, 2.5)),
log_sigma = log(c(0.3, 1.5)))
# constructing AD object
obj <- MakeADFun(nll, par0, silent = TRUE)
# optimising
opt <- nlminb(obj$par, obj$fn, obj$gr)
# sampling from distribution of the MLE
samples <- MCreport(obj, nSamples = 10, report = TRUE)
Calculate the index of the first observation of each track based on an ID variable
Description
Function to conveniently calculate the trackInd variable that is needed internally when fitting a model to longitudinal data with multiple tracks.
Usage
calc_trackInd(ID)
Arguments
ID |
ID variable of track IDs that is of the same length as the data to be analysed |
Value
A vector of indices of the first observation of each track which can be passed to the forward and forward_g to sum likelihood contributions of each track
Examples
uniqueID = c("Animal1", "Animal2", "Animal3")
ID = rep(uniqueID, c(100, 200, 300))
trackInd = calc_trackInd(ID)
Trigonometric basis expansion
Description
Builds a design matrix of sin/cos pairs for use in models
with periodic predictors. Can be used directly or inside formulas passed
to modmat (where expansion is handled automatically).
Usage
cosinor(x, period = 24)
Arguments
x |
Numeric vector of the periodic variable. |
period |
Numeric vector of period lengths, e.g. |
Details
The resulting columns form the basis for linear predictors of the form
\eta_t = \beta_0 + \sum_k \Bigl(
\beta_{1k} \sin\!\Bigl(\tfrac{2 \pi x_t}{\text{period}_k}\Bigr) +
\beta_{2k} \cos\!\Bigl(\tfrac{2 \pi x_t}{\text{period}_k}\Bigr)
\Bigr).
Value
A numeric matrix with 2 * length(period) columns named
sin(2*pi*x/period) / cos(2*pi*x/period).
Examples
cosinor(1:24, period = 24)
cosinor(1:24, period = c(24, 12, 6))
## In model formulas (expand_cosinor handles the expansion):
form <- ~ x + temp * cosinor(hour, c(24, 12))
data <- data.frame(x = runif(24), temp = rnorm(24, 20), hour = 1:24)
modmat <- modmat(form, data = data)
State dwell-time distributions of periodically inhomogeneous Markov chains
Description
Computes the dwell-time distribution of a periodically inhomogeneous Markov chain for a given transition probability matrix.
Usage
ddwell(x, Gamma, time = NULL, state = NULL)
Arguments
x |
vector of (non-negative) dwell times to compute the dwell-time distribution for |
Gamma |
array of |
time |
integer vector of time points in |
state |
integer vector of state indices for which to compute the dwell-time distribution. If |
Details
For Markov chains whose transition probabilities vary only periodically, which is achieved for example by
expressing the transition probability matrix as a periodic function of the time of day using tpm_p or cosinor, the probability distribution of time spent in a state can be computed analytically.
This function computes said distribution, either for a specific time point (conditioning on transitioning into the state at that time point) or for the overall distribution (conditioning on transitioning into the state at any time point).
Value
either time-varying dwell-time distribution(s) if time is specified, or overall dwell-time distribution if time is NULL.
If more than one state is specified, a named list over states is returned.
References
When using this function, please cite:
Koslik, J. O., Feldmann, C. C., Mews, S., Michels, R., & Langrock, R. (2025). Inference on the state process of periodically inhomogeneous hidden Markov models for animal behavior. The Annals of Applied Statistics, 19(4), 2724–2737.
Examples
# setting parameters for trigonometric link
beta = matrix(c(-1, 2, -1, -2, 1, -1), nrow = 2, byrow = TRUE)
Gamma = tpm_p(beta = beta, degree = 1)
# at specific times and for specific state
ddwell(1:20, Gamma, time = 1:4, state = 1)
# results in 4x20 matrix
# or overall distribution for all states
ddwell(1:20, Gamma)
# results in list of length 2, each element is a vector of length 20
Reparametrised multivariate Gaussian distribution
Description
Density function of the multivariate Gaussian distribution reparametrised in terms of its precision matrix (inverse variance).
This implementation is particularly useful for defining the joint log-likelihood with penalised splines or i.i.d. random effects that have a multivariate Gaussian distribution with fixed precision/ penalty matrix \lambda S.
As S is fixed and only scaled by \lambda, it is more efficient to precompute the determinant of S (for the normalisation constant) and only scale the quadratic form by \lambda
when multiple spline parameters/ random effects with different \lambda's but the same penalty matrix S are evaluated.
Usage
dgmrf2(x, mu = 0, S, lambda, logdetS = NULL, log = FALSE)
Arguments
x |
density evaluation point, either a vector or a matrix |
mu |
mean parameter. Either scalar or vector |
S |
unscaled precision matrix |
lambda |
precision scaling parameter Can be a vector if |
logdetS |
Optional precomputed log determinant of the precision matrix |
log |
logical; if |
Details
This implementation allows for automatic differentiation with RTMB.
Value
vector of density values
Examples
x = matrix(runif(30), nrow = 3)
# iid random effects
S = diag(10)
sigma = c(1, 2, 3) # random effect standard deviations
lambda = 1 / sigma^2
d = dgmrf2(x, 0, S, lambda)
# P-splines
L = diff(diag(10), diff = 2) # second-order difference matrix
S = t(L) %*% L
lambda = c(1,2,3)
d = dgmrf2(x, 0, S, lambda, log = TRUE)
Forward algorithm to calculate the HMM log-likelihood
Description
Calculates the log-likelihood of a sequence of observations under a hidden Markov model using the forward algorithm (Zucchini, MacDonald & Langrock, 2016).
Usage
forward(
delta,
Gamma,
allprobs,
trackID = NULL,
logspace = FALSE,
bw = NULL,
report = TRUE,
ad = NULL,
tod = NULL
)
Arguments
delta |
initial distribution; either
|
Gamma |
transition probability matrix; either
|
allprobs |
matrix of state-dependent probabilities or density values of dimension |
trackID |
optional vector of length |
logspace |
logical; if |
bw |
optional positive integer specifying the bandwidth for a banded approximation of the forward algorithm, inducing a banded Hessian w.r.t. the observations.
Defaults to |
report |
logical; if |
ad |
logical; whether to use automatic differentiation. Determined automatically — for debugging only. |
tod |
optional integer vector of length |
Details
If trackID is provided, the total log-likelihood is the sum of each track's likelihood
contribution. In this case, Gamma can be
a matrix (same transition probabilities for each track),
an array of dimension
c(nStates, nStates, nTracks)(track-specific transition probability matrix), oran array of dimension
c(nStates, nStates, nObs)for time-varying transition probabilities, oran array of dimension
c(nStates, nStates, L)for periodic transition probabilities, iftodis provided.
Additionally, delta can be a vector (same initial distribution for each track) or a
matrix of dimension c(nTracks, nStates) (track-specific initial distributions).
With delta = "stationary", the initial distribution of each track is computed from Gamma:
the stationary distribution of
Gamma(or of its slice for each track, if track-specific),the periodically stationary distribution at the first time point of each track, if
todis provided (seestationary_p),the stationary distribution of the first slice of each track, for time-varying transition probabilities, i.e. at the covariate values of the first observation.
This requires Gamma to contain transition probability matrices (not, e.g., sub-stochastic matrices), which is checked without automatic differentiation.
The computed delta is reported as a matrix of dimension c(nTracks, nStates).
Note: forward should only be called once in the likelihood function, with a trackID argument for multiple tracks.
Downstream functions like lama, viterbi, stateprobs or pseudo_res rely on the quantities it reports,
and only those of the last call are kept.
Value
HMM log-likelihood for given data and parameters
References
Zucchini, W., MacDonald, I.L., & Langrock, R. (2016). Hidden Markov Models for Time Series: An Introduction Using R (2nd ed.). Chapman & Hall/CRC.
Mews, Koslik, & Langrock (2025). How to build your latent Markov model: The role of time and space. Statistical Modelling, 25(6), 481–507.
See Also
Other forward algorithms:
forward_g(),
forward_hsmm(),
forward_ihsmm(),
forward_p(),
forward_phsmm()
Examples
## negative log likelihood function
nll = function(par, step) {
# parameter transformations for unconstrained optimisation
Gamma = tpm(par[1:2]) # multinomial logit link
delta = stationary(Gamma) # stationary HMM
mu = exp(par[3:4])
sigma = exp(par[5:6])
# calculate all state-dependent probabilities
allprobs = matrix(1, length(step), 2)
ind = which(!is.na(step))
for(j in 1:2) allprobs[ind,j] = dgamma2(step[ind], mu[j], sigma[j])
# simple forward algorithm to calculate log-likelihood
-forward(delta, Gamma, allprobs)
}
## fitting an HMM to the trex data
par = c(-2,-2, # initial tpm params (logit-scale)
log(c(0.3, 2.5)), # initial means for step length (log-transformed)
log(c(0.2, 1.5))) # initial sds for step length (log-transformed)
mod = nlm(nll, par, step = trex$step[1:1000])
Forward algorithm with time-varying transition probability matrix
Description
Calculates the log-likelihood of a sequence of observations under a hidden Markov model with time-varying transition probabilities using the forward algorithm (Zucchini, MacDonald & Langrock, 2016).
Usage
forward_g(
delta,
Gamma,
allprobs,
trackID = NULL,
logspace = FALSE,
bw = NULL,
report = TRUE,
ad = NULL
)
Arguments
delta |
initial distribution; either
|
Gamma |
array of transition probability matrices of dimension For a single track, an array of dimension This function also supports continuous-time HMMs, where each slice is a Markov semigroup
|
allprobs |
matrix of state-dependent probabilities or density values of dimension |
trackID |
optional vector of length |
logspace |
logical; if |
bw |
optional positive integer specifying the bandwidth for a banded approximation of the forward algorithm, inducing a banded Hessian w.r.t. the observations.
Defaults to |
report |
logical; if |
ad |
logical; whether to use automatic differentiation. Determined automatically — for debugging only. |
Details
Deprecated: please use forward for all model types instead.
If trackID is provided, the total log-likelihood will be the sum of each track's likelihood contribution.
In this case, Gamma must be an array of dimension c(nStates, nStates, nObs), matching the number of rows of allprobs. For each track, the transition matrix at the beginning of the track will be ignored (as there is no transition between tracks).
Additionally, delta can be a vector (same initial distribution for each track) or a matrix of dimension c(nTracks, nStates) (different initial distribution for each track).
Note: When there are multiple tracks, for compatibility with downstream functions like viterbi_g, stateprobs_g or pseudo_res,
forward_g should only be called once with a trackID argument.
Value
HMM log-likelihood for given data and parameters
References
Zucchini, W., MacDonald, I.L., & Langrock, R. (2016). Hidden Markov Models for Time Series: An Introduction Using R (2nd ed.). Chapman & Hall/CRC.
Mews, Koslik, & Langrock (2025). How to build your latent Markov model: The role of time and space. Statistical Modelling, 25(6), 481–507.
See Also
Other forward algorithms:
forward(),
forward_hsmm(),
forward_ihsmm(),
forward_p(),
forward_phsmm()
Examples
## Simple usage
Gamma = array(c(0.9, 0.2, 0.1, 0.8), dim = c(2,2,10))
delta = c(0.5, 0.5)
allprobs = matrix(0.5, 10, 2)
forward_g(delta, Gamma, allprobs)
## Full model fitting example
## negative log likelihood function
nll = function(par, step, Z) {
# parameter transformations for unconstrained optimisation
beta = matrix(par[1:6], nrow = 2)
Gamma = tpm_g(Z, beta) # multinomial logit link for each time point
delta = stationary(Gamma[,,1]) # stationary HMM
mu = exp(par[7:8])
sigma = exp(par[9:10])
# calculate all state-dependent probabilities
allprobs = matrix(1, length(step), 2)
ind = which(!is.na(step))
for(j in 1:2) allprobs[ind,j] = dgamma2(step[ind], mu[j], sigma[j])
# simple forward algorithm to calculate log-likelihood
-forward_g(delta, Gamma, allprobs)
}
## fitting an HMM to the trex data
par = c(-1.5,-1.5, # initial tpm intercepts (logit-scale)
rep(0, 4), # initial tpm slopes
log(c(0.3, 2.5)), # initial means for step length (log-transformed)
log(c(0.2, 1.5))) # initial sds for step length (log-transformed)
mod = nlm(nll, par, step = trex$step[1:500], Z = cosinor(trex$tod[1:500]))
Forward algorithm for homogeneous hidden semi-Markov models
Description
Calculates the (approximate) log-likelihood of a sequence of observations under a homogeneous hidden semi-Markov model using a modified forward algorithm.
Usage
forward_hsmm(
dm,
omega,
allprobs,
trackID = NULL,
delta = NULL,
eps = 1e-10,
report = TRUE
)
Arguments
dm |
list of length |
omega |
matrix of dimension Contains the transition probabilities given that the current state is left. Hence, the diagonal elements need to be zero and the rows need to sum to one. Can be constructed using |
allprobs |
matrix of state-dependent probabilities/ density values of dimension |
trackID |
optional vector of length If provided, the total log-likelihood will be the sum of each track's likelihood contribution.
In this case, |
delta |
optional vector of initial state probabilities of length By default, the stationary distribution is computed (which is typically recommended). |
eps |
small value to avoid numerical issues in the approximating transition matrix construction. Usually, this should not be changed. |
report |
logical, indicating whether initial distribution, approximating transition probability matrix and |
Details
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs, where the state duration distribution is explicitly modelled by a distribution on the positive integers.
For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function is designed to be used with automatic differentiation based on the R package RTMB. It will be very slow without it!
Value
HSMM log-likelihood for given data and parameters
References
Langrock, R., & Zucchini, W. (2011). Hidden Markov models with arbitrary state dwell-time distributions. Computational Statistics & Data Analysis, 55(1), 715-724.
Koslik, J. O. (2025). Hidden semi-Markov models with inhomogeneous state dwell-time distributions. Computational Statistics & Data Analysis, 209, 108171.
See Also
Other forward algorithms:
forward(),
forward_g(),
forward_ihsmm(),
forward_p(),
forward_phsmm()
Examples
# currently no examples
Forward algorithm for hidden semi-Markov models with inhomogeneous state durations and/ or conditional transition probabilities
Description
Calculates the (approximate) log-likelihood of a sequence of observations under an inhomogeneous hidden semi-Markov model using a modified forward algorithm.
Usage
forward_ihsmm(
dm,
omega,
allprobs,
trackID = NULL,
delta = NULL,
startInd = NULL,
eps = 1e-10,
report = TRUE
)
Arguments
dm |
list of length If the dwell-time PMFs are constant, the vectors are the PMF of the dwell-time distribution fixed in time. The vector lengths correspond to the approximating state aggregate sizes, hence there should be little probablity mass not covered by these. If the dwell-time PMFs are inhomogeneous, the matrices need to have n rows, where n is the number of observations. The number of columns again correponds to the size of the approximating state aggregates. In the latter case, the first |
omega |
matrix of dimension It contains the transition probabilities given the current state is left. Hence, the diagonal elements need to be zero and the rows need to sum to one. Such a matrix can be constructed using |
allprobs |
matrix of state-dependent probabilities/ density values of dimension |
trackID |
trackID optional vector of length If provided, the total log-likelihood will be the sum of each track's likelihood contribution.
Instead of a single vector |
delta |
optional vector of initial state probabilities of length N By default, instead of this, the stationary distribution is computed corresponding to the first approximating transition probability matrix of each track is computed. Contrary to the homogeneous case, this is not theoretically motivated but just for convenience. |
startInd |
optional integer index at which the forward algorithm starts. When approximating inhomogeneous HSMMs by inhomogeneous HMMs, the first transition probability matrix that can be constructed is at time |
eps |
small value to avoid numerical issues in the approximating transition matrix construction. Usually, this should not be changed. |
report |
logical, indicating whether initial distribution, approximating transition probability matrix and |
Details
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs, where the state duration distribution is explicitly modelled by a distribution on the positive integers. This function can be used to fit HSMMs where the state-duration distribution and/ or the conditional transition probabilities vary with covariates.
For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function is designed to be used with automatic differentiation based on the R package RTMB. It will be very slow without it!
Value
HSMM log-likelihood for given data and parameters
References
Koslik, J. O. (2025). Hidden semi-Markov models with inhomogeneous state dwell-time distributions. Computational Statistics & Data Analysis, 209, 108171.
See Also
Other forward algorithms:
forward(),
forward_g(),
forward_hsmm(),
forward_p(),
forward_phsmm()
Examples
# currently no examples
Forward algorithm with for periodically varying transition probability matrices
Description
Calculates the log-likelihood of a sequence of observations under a hidden Markov model with periodically varying transition probabilities using the forward algorithm.
Usage
forward_p(
delta,
Gamma,
allprobs,
tod,
trackID = NULL,
ad = NULL,
report = TRUE,
logspace = FALSE
)
Arguments
delta |
initial or stationary distribution of length |
Gamma |
array of transition probability matrices of dimension Here we use the definition |
allprobs |
matrix of state-dependent probabilities/ density values of dimension |
tod |
(Integer valued) variable for cycle indexing in 1, ..., L, mapping the data index to a generalised time of day (length For half-hourly data L = 48. It could, however, also be day of year for daily data and L = 365. |
trackID |
optional vector of length If provided, the total log-likelihood will be the sum of each track's likelihood contribution.
Instead of a single vector |
ad |
optional logical, indicating whether automatic differentiation with |
report |
logical, indicating whether Caution: When there are multiple tracks, for compatibility with downstream functions like |
logspace |
logical, indicating whether the probabilities/ densities in the |
Details
Deprecated: please use forward with argument tod instead.
When the transition probability matrix only varies periodically (e.g. as a function of time of day), there are only L unique matrices if L is the period length (e.g. L=24 for hourly data and time-of-day variation).
Thus, it is much more efficient to only calculate these L matrices and index them by a time variable (e.g. time of day or day of year) instead of calculating such a matrix for each index in the data set (which would be redundant).
This function allows for that by only expecting a transition probability matrix for each time point in a period and an integer valued (1, \dots, L) time variable that maps the data index to the according time.
Value
HMM log-likelihood for given data and parameters
See Also
Other forward algorithms:
forward(),
forward_g(),
forward_hsmm(),
forward_ihsmm(),
forward_phsmm()
Examples
## negative log likelihood function
nll = function(par, step, tod) {
# parameter transformations for unconstrained optimisation
beta = matrix(par[1:6], nrow = 2)
Gamma = tpm_p(1:24, beta = beta) # multinomial logit link for each time point
delta = stationary_p(Gamma, tod[1] %% 24 + 1) # stationary HMM
mu = exp(par[7:8])
sigma = exp(par[9:10])
# calculate all state-dependent probabilities
allprobs = matrix(1, length(step), 2)
ind = which(!is.na(step))
for(j in 1:2) allprobs[ind,j] = dgamma2(step[ind], mu[j], sigma[j])
# simple forward algorithm to calculate log-likelihood
-forward_p(delta, Gamma, allprobs, tod)
}
## fitting an HMM to the nessi data
par = c(-2,-2, # initial tpm intercepts (logit-scale)
rep(0, 4), # initial tpm slopes
log(c(0.3, 2.5)), # initial means for step length (log-transformed)
log(c(0.2, 1.5))) # initial sds for step length (log-transformed)
mod = nlm(nll, par, step = trex$step[1:500], tod = trex$tod[1:500])
Forward algorithm for hidden semi-Markov models with periodically inhomogeneous state durations and/ or conditional transition probabilities
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs, where the state duration distribution is explicitly modelled by a distribution on the positive integers. This function can be used to fit HSMMs where the state-duration distribution and/ or the conditional transition probabilities vary with covariates.
For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function can be used to fit HSMMs where the state-duration distribution and/ or the conditional transition probabilities vary periodically.
In the special case of periodic variation (as compared to arbitrary covariate influence), this version is to be preferred over forward_ihsmm because it computes the correct periodically stationary distribution and no observations are lost for the approximation.
This function is designed to be used with automatic differentiation based on the R package RTMB. It will be very slow without it!
Usage
forward_phsmm(
dm,
omega,
allprobs,
tod,
trackID = NULL,
delta = NULL,
eps = 1e-10,
report = TRUE
)
Arguments
dm |
list of length If the dwell-time PMFs are constant, the vectors are the PMF of the dwell-time distribution fixed in time. The vector lengths correspond to the approximating state aggregate sizes, hence there should be little probablity mass not covered by these. If the dwell-time PMFs are inhomogeneous, the matrices need to have L rows, where L is the cycle length. The number of columns again correpond to the size of the approximating state aggregates. |
omega |
matrix of dimension It contains the transition probabilities given the current state is left. Hence, the diagonal elements need to be zero and the rows need to sum to one. Such a matrix can be constructed using |
allprobs |
matrix of state-dependent probabilities/ density values of dimension |
tod |
(Integer valued) variable for cycle indexing in 1, ..., L, mapping the data index to a generalised time of day (length |
trackID |
optional vector of length If provided, the total log-likelihood will be the sum of each track's likelihood contribution.
Instead of a single vector |
delta |
Optional vector of initial state probabilities of length |
eps |
small value to avoid numerical issues in the approximating transition matrix construction. Usually, this should not be changed. |
report |
logical, indicating whether initial distribution, approximating transition probability matrix and |
Details
Calculates the (approximate) log-likelihood of a sequence of observations under a periodically inhomogeneous hidden semi-Markov model using a modified forward algorithm.
Value
HSMM log-likelihood for given data and parameters
References
Koslik, J. O. (2025). Hidden semi-Markov models with inhomogeneous state dwell-time distributions. Computational Statistics & Data Analysis, 209, 108171.
See Also
Other forward algorithms:
forward(),
forward_g(),
forward_hsmm(),
forward_ihsmm(),
forward_p()
Examples
# currently no examples
Forward algorithm for hidden semi-Markov models with homogeneous transition probability matrix
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs that can be approximated by HMMs on an enlarged state space (of size M) and with structured transition probabilities.
Usage
forward_s(delta, Gamma, allprobs, sizes)
Arguments
delta |
initial or stationary distribution of length N, or matrix of dimension c(k,N) for k independent tracks, if |
Gamma |
transition probability matrix of dimension c(M,M) |
allprobs |
matrix of state-dependent probabilities/ density values of dimension c(n, N) which will automatically be converted to the appropriate dimension. |
sizes |
state aggregate sizes that are used for the approximation of the semi-Markov chain. |
Value
log-likelihood for given data and parameters
Examples
## generating data from homogeneous 2-state HSMM
mu = c(0, 6)
lambda = c(6, 12)
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE)
# simulation
# for a 2-state HSMM the embedded chain always alternates between 1 and 2
s = rep(1:2, 100)
C = x = numeric(0)
for(t in 1:100){
dt = rpois(1, lambda[s[t]])+1 # shifted Poisson
C = c(C, rep(s[t], dt))
x = c(x, rnorm(dt, mu[s[t]], 1.5)) # fixed sd 2 for both states
}
## negative log likelihood function
mllk = function(theta.star, x, sizes){
# parameter transformations for unconstraint optimization
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE) # omega fixed (2-states)
lambda = exp(theta.star[1:2]) # dwell time means
dm = list(dpois(1:sizes[1]-1, lambda[1]), dpois(1:sizes[2]-1, lambda[2]))
Gamma = tpm_hsmm2(omega, dm)
delta = stationary(Gamma) # stationary
mu = theta.star[3:4]
sigma = exp(theta.star[5:6])
# calculate all state-dependent probabilities
allprobs = matrix(1, length(x), 2)
for(j in 1:2){ allprobs[,j] = dnorm(x, mu[j], sigma[j]) }
# return negative for minimization
-forward_s(delta, Gamma, allprobs, sizes)
}
## fitting an HSMM to the data
theta.star = c(log(5), log(10), 1, 4, log(2), log(2))
mod = nlm(mllk, theta.star, x = x, sizes = c(20, 30), stepmax = 5)
Forward algorithm for hidden semi-Markov models with periodically varying transition probability matrices
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs that can be approximated by HMMs on an enlarged state space (of size M) and with structured transition probabilities.
Recently, this inference procedure has been generalised to allow either the dwell-time distributions or the conditional transition probabilities to depend on external covariates such as the time of day. This special case is implemented here.
This function allows for that, by expecting a transition probability matrix for each time point in a period, and an integer valued (1, \dots, L) time variable that maps the data index to the according time.
Usage
forward_sp(delta, Gamma, allprobs, sizes, tod)
Arguments
delta |
initial or stationary distribution of length N, or matrix of dimension c(k,N) for k independent tracks, if |
Gamma |
array of transition probability matrices of dimension c(M,M,L). Here we use the definition |
allprobs |
matrix of state-dependent probabilities/ density values of dimension c(n, N) which will automatically be converted to the appropriate dimension. |
sizes |
state aggregate sizes that are used for the approximation of the semi-Markov chain. |
tod |
(Integer valued) variable for cycle indexing in 1, ..., L, mapping the data index to a generalised time of day (length n). For half-hourly data L = 48. It could, however, also be day of year for daily data and L = 365. |
Value
log-likelihood for given data and parameters
Examples
## generating data from homogeneous 2-state HSMM
mu = c(0, 6)
beta = matrix(c(log(4),log(6),-0.2,0.2,-0.1,0.4), nrow=2)
# time varying mean dwell time
Lambda = exp(cbind(1, cosinor(1:24))%*%t(beta))
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE)
# simulation
# for a 2-state HSMM the embedded chain always alternates between 1 and 2
s = rep(1:2, 100)
C = x = numeric(0)
tod = rep(1:24, 50) # time of day variable
time = 1
for(t in 1:100){
dt = rpois(1, Lambda[tod[time], s[t]])+1 # dwell time depending on time of day
time = time + dt
C = c(C, rep(s[t], dt))
x = c(x, rnorm(dt, mu[s[t]], 1.5)) # fixed sd 2 for both states
}
tod = tod[1:length(x)]
## negative log likelihood function
mllk = function(theta.star, x, sizes, tod){
# parameter transformations for unconstraint optimization
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE) # omega fixed (2-states)
mu = theta.star[1:2]
sigma = exp(theta.star[3:4])
beta = matrix(theta.star[5:10], nrow=2)
# time varying mean dwell time
Lambda = exp(cbind(1, cosinor(1:24))%*%t(beta))
dm = list()
for(j in 1:2){
dm[[j]] = sapply(1:sizes[j]-1, dpois, lambda = Lambda[,j])
}
Gamma = tpm_phsmm2(omega, dm)
delta = stationary_p(Gamma, tod[1])
# calculate all state-dependent probabilities
allprobs = matrix(1, length(x), 2)
for(j in 1:2){ allprobs[,j] = dnorm(x, mu[j], sigma[j]) }
# return negative for minimization
-forward_sp(delta, Gamma, allprobs, sizes, tod)
}
## fitting an HSMM to the data
theta.star = c(1, 4, log(2), log(2), # state-dependent parameters
log(4), log(6), rep(0,4)) # state process parameters dm
# mod = nlm(mllk, theta.star, x = x, sizes = c(10, 15), tod = tod, stepmax = 5)
Reparametrised gamma distribution
Description
Density, distribution function, quantile function and random generation for the gamma distribution reparametrised in terms of mean and standard deviation.
Usage
dgamma2(x, mean = 1, sd = 1, log = FALSE)
pgamma2(q, mean = 1, sd = 1, lower.tail = TRUE, log.p = FALSE)
qgamma2(p, mean = 1, sd = 1, lower.tail = TRUE, log.p = FALSE)
rgamma2(n, mean = 1, sd = 1)
Arguments
x, q |
vector of quantiles |
mean |
mean parameter, must be positive scalar. |
sd |
standard deviation parameter, must be positive scalar. |
log, log.p |
logical; if |
lower.tail |
logical; if |
p |
vector of probabilities |
n |
number of observations. If |
Details
This implementation allows for automatic differentiation with RTMB.
Value
dgamma2 gives the density, pgamma2 gives the distribution function, qgamma2 gives the quantile function, and rgamma2 generates random deviates.
Examples
x = rgamma2(1)
d = dgamma2(x)
p = pgamma2(x)
q = qgamma2(p)
Computes generalised determinant
Description
Computes generalised determinant
Usage
gdeterminant(x, eps = NULL, log = TRUE)
Arguments
x |
symmetric matrix |
eps |
eigenvalues smaller than this will be treated as zero |
log |
logical. If |
Value
generalised log-determinant of x
Build the generator matrix of a continuous-time Markov chain
Description
This function builds the infinitesimal generator matrix for a continuous-time Markov chain from an unconstrained parameter vector.
Usage
generator(
beta,
Z = NULL,
Eta = NULL,
byrow = FALSE,
report = TRUE,
param = NULL
)
Arguments
beta |
parameters; either
|
Z |
optional covariate design matrix with or without intercept column, i.e. of dimension |
Eta |
optional pre-calculated matrix of linear predictors of dimension |
byrow |
logical indicating if the generator matrix should be filled by row |
report |
logical, indicating whether the generator matrix |
param |
depricated, please use argument |
Details
Off-diagonal entries are calculated as \exp(\beta_i) to ensure positivity. The diagonal entries are then set to the negative row sums, which is required for generator matrices.
If a design matrix Z or a matrix of linear predictors Eta is provided, the function will automatically call generator_g to build the generator matrix based on the design matrix and coefficient matrix.
In that case, the argument beta needs to be a matrix of coefficients of dimension c(nStates * (nStates-1), p+1), where the first column contains the intercepts.
Value
infinitesimal generator matrix of dimension c(nStates, nStates) or array of such matrices of dimension c(nStates, nStates, nObs) if Z or Eta is provided.
See Also
Other transition probability matrix functions:
generator_g(),
tpm(),
tpm_ct(),
tpm_emb(),
tpm_emb_g(),
tpm_g(),
tpm_g2(),
tpm_p()
Examples
# 2 states: 2 free off-diagonal elements
generator(rep(-1, 2))
# 3 states: 6 free off-diagonal elements
generator(rep(-2, 6))
Build generator matrices of a continuous-time Markov chain
Description
This function builds infinitesimal generator matrices for a continuous-time Markov chain based on a design matrix and coefficient matrix.
Usage
generator_g(Z, beta, Eta = NULL, byrow = FALSE, report = TRUE)
Arguments
Z |
Covariate design matrix with or without intercept column, i.e. of dimension |
beta |
Matrix of coefficients for the off-diagonal elements of the generator matrix
of dimension |
Eta |
optional pre-calculated matrix of linear predictors of dimension |
byrow |
logical indicating if the generator matrices should be filled by row |
report |
logical, indicating whether the generator matrices |
Details
Deprecated: please use generator(beta, Z) for all model types instead.
Off-diagonal entries are calculated as \exp(Z \beta_i) to ensure positivity. The diagonal entries are then set to the negative row sums, which is required for generator matrices.
Value
array of infinitesimal generator matrices of dimension c(nStates, nStates, nObs)
See Also
Other transition probability matrix functions:
generator(),
tpm(),
tpm_ct(),
tpm_emb(),
tpm_emb_g(),
tpm_g(),
tpm_g2(),
tpm_p()
Examples
# 2 states: 2 free off-diagonal elements
generator(rep(-1, 2))
# 3 states: 6 free off-diagonal elements
generator(rep(-2, 6))
Build a LaMaModel from an optimised RTMB object
Description
Having fitted a latent Markov model using automatic differentiation via RTMB, this function calls RTMB's obj$report() and does some additional processing.
This then yields estimated parameters on their natural scale, allows for convenient calculation of AIC and BIC, state-decoding, and residual calculation.
print() gives a short overview of the model, summary() the estimates.
report() is the deprecated old name of lama().
Usage
lama(obj)
report(obj)
Arguments
obj |
Optimised |
Details
The number of observations (used by BIC) is the number of rows of the reported allprobs that are not all 1,
i.e. missing observations are not counted. This assumes that forward is called only once in the likelihood function.
Value
A model object of class "LaMaModel" containing a list with the reported quantities from the RTMB object, along estimated parameters (par),
the log-likelihood (llk), number of parameters (df) and observations (nobs), and the maximum gradient component (mgc) at the estimate.
It also contains obj itself (not a copy), so that functions like MCreport or scores can be called on the model object.
Examples
data <- trex[1:200,]
# initial parameters and observations
par <- list(
log_mu = log(c(0.3, 1)), # initial means for step length (log-transformed)
log_sigma = log(c(0.2, 0.7)), # initial sds for step length (log-transformed)
eta = rep(-2, 2) # initial t.p.m. parameters (on logit scale)
)
dat <- list(
step = data$step, # hourly step lengths
nStates = 2 # number of hidden states
)
# likelihood function
nll <- function(par) {
getAll(par, dat)
Gamma <- tpm(eta)
delta <- stationary(Gamma)
mu <- exp(log_mu); REPORT(mu)
sigma <- exp(log_sigma); REPORT(sigma)
allprobs <- matrix(1, length(step), nStates)
ind <- which(!is.na(step))
for(j in 1:nStates) {
allprobs[ind,j] <- dgamma2(step[ind], mu[j], sigma[j])
}
-forward(delta, Gamma, allprobs)
}
# automatic differentiation and optimisation
obj <- MakeADFun(nll, par, silent = TRUE)
opt <- nlminb(obj$par, obj$fn, obj$gr)
### reporting ###
mod <- lama(obj)
mod # short overview
summary(mod) # estimated state process and reported quantities
# estimated parameters
mod$par
# estimated quantities on natural scale
mod$mu
mod$sigma
mod$Gamma
# information criteria
AIC(mod)
BIC(mod)
# state decoding
states <- viterbi(mod = mod) # global decoding
probs <- stateprobs(mod = mod) # local decoding
# residual calculation
pres <- pseudo_res(data$step, # observation sequence
"gamma2", # distribution family
list(mean = mod$mu, sd = mod$sigma), # parameters for that family
mod = mod) # model object
# or from the model object alone, and plotted
plot(mod)
Extract log-likelihood from LaMaModel object
Description
Extract log-likelihood from LaMaModel object
Usage
## S3 method for class 'LaMaModel'
logLik(object, ...)
Arguments
object |
A model fitted using RTMB and obtained via |
... |
Additional arguments (not used) |
Value
An object of class "logLik"
Build a standardised P-Spline design matrix and the associated P-Spline penalty matrix
Description
This function builds the B-spline design matrix for a given data vector. Importantly, the B-spline basis functions are normalised such that the integral of each basis function is 1, hence this basis can be used for spline-based density estimation, when the basis functions are weighted by non-negative weights summing to one.
Usage
make_matrices_dens(
x,
k,
type = "real",
degree = 3,
knots = NULL,
diff_order = 2,
pow = 0.5,
npoints = 10000
)
Arguments
x |
data vector |
k |
number of basis functions |
type |
type of the data, either |
degree |
degree of the B-spline basis functions, defaults to cubic B-splines |
knots |
optional vector of knots (including the boundary knots) to be used for basis construction.
If not provided, the knots are placed equidistantly for For |
diff_order |
order of differencing used for the P-Spline penalty matrix. Defaults to second-order differences. |
pow |
power for polynomial knot spacing, only used for |
npoints |
number of points used in the numerical integration for normalizing the B-spline basis functions |
Value
list containing the design matrix Z, the penalty matrix S, the prediction design matrix Z_predict, the prediction grid xseq, and details for the basis expansion.
The penalty matrix leaves out the last coefficient, which is fixed at zero for identifiability.
Examples
set.seed(1)
# real-valued
x <- rnorm(100)
modmat <- make_matrices_dens(x, k = 20)
# positive-continuouos
x <- rgamma2(100, mean = 5, sd = 2)
modmat <- make_matrices_dens(x, k = 20, type = "positive")
# circular
x <- rvm(100, mu = 0, kappa = 2)
modmat <- make_matrices_dens(x, k = 20, type = "circular")
# bounded in an interval
x <- rbeta(100, 1, 2)
modmat <- make_matrices_dens(x, k = 20)
AD-compatible minimum and maximum functions
Description
These functions compute the parallel minimum/ maximum of two vector-valued inputs and are compatible with automatic differentiation using RTMB.
Usage
min2(x, y)
max2(x, y)
Arguments
x |
first vector |
y |
second vector |
Value
min2 returns the parallel minimum and max2 the parallel maximum of x and y
Examples
x <- c(1, 4, 8, 2)
y <- c(2, 5, 3, 7)
min2(x, y)
max2(x, y)
Smooth approximations to max(x, 0) and min(x, 0)
Description
Smooth approximations to max(x, 0) and min(x, 0)
Usage
max0_smooth(x, rho = 20)
min0_smooth(x, rho = 20)
Arguments
x |
a vector of values |
rho |
smoothing parameter, larger values lead to closer approximation |
Value
the approximate maximum or minimum of x and 0
Examples
x <- seq(-1, 1, by = 0.1)
min0_smooth(x)
max0_smooth(x)
Build the design and the penalty matrix for models involving penalised splines based on a formula and a data set
Description
Build the design and the penalty matrix for models involving penalised splines based on a formula and a data set
Usage
modmat(formula, data, knots = NULL)
make_matrices(formula, data, knots = NULL)
Arguments
formula |
formula as used in Can also be a list of formulas, which are then processed separately. In that case, both a named list of right-side only formulas or a list of formulas with response variables can be provided. |
data |
data frame containing all the variables on the right side of the formula(s) |
knots |
optional list containing user specified knot values for each covariate to be used for basis construction.
For most bases the user simply supplies the If |
Details
make_matrices() is the former name of modmat() and still works.
Value
a list of class LaMa_matrices containing:
Z |
design matrix (or list of such matrices if |
S |
list of penalty matrices (with names based on the response terms of the formulas as well as the smooth terms and covariates). For tensorproduct smooths, corresponding entries are themselves lists, containing the |
pardim |
list of parameter dimensions (fixed and penalised separately) for each formula, for ease of setting up initial parameters |
coef |
list of coefficient vectors filled with zeros of the correct length for each formula, for ease of setting up initial parameters |
sp0 |
named vector of initial penalty strengths, with one entry per penalty matrix and names matching These are It can be passed straight to |
formula |
the formula(s) as supplied, in the same nesting as |
data |
the data frame used for the model(s) |
gam |
unfitted |
gam0 |
fitted |
knots |
knot list used in the basis construction (or named list over such lists if |
See Also
predict.LaMa_matrices for prediction design matrix construction based on the model matrices object created by this function.
Examples
data = data.frame(x = runif(100),
y = runif(100),
g = factor(rep(1:10, each = 10)))
# unvariate thin plate regression spline
modmat = modmat(~ s(x), data)
# univariate P-spline
modmat = modmat(~ s(x, bs = "ps"), data)
# adding random intercept
modmat = modmat(~ s(g, bs = "re") + s(x, bs = "ps"), data)
# tensorproduct of x and y
modmat = modmat(~ s(x) + s(y) + ti(x,y), data)
# multiple formulas at once
modmat = modmat(list(mu ~ s(x) + y, sigma ~ s(g, bs = "re")), data = data)
Optimise an RTMB object from several starting values
Description
Latent Markov models often have several local optima of the likelihood. multistart() optimises
obj from several starting values: the first is obj$par (the initial parameters), the others
are random perturbations of it on the working scale. Afterwards, lama(obj) builds the model
from the best fit, as RTMB keeps the parameters with the lowest negative log-likelihood it evaluated.
Usage
multistart(
obj,
nstarts = 20,
sd = 1,
starts = NULL,
scale = c("fixed", "unit_info"),
stop = c("bayes", "hits", "none"),
hits = 3,
sd_max = 2,
tol = 1e-06,
seed = NULL,
optimizer = stats::nlminb,
silent = FALSE,
...
)
Arguments
obj |
|
nstarts |
maximum number of starts, including |
sd |
standard deviation of the perturbations on the working scale: a number, a vector of the length of |
starts |
optional matrix of starting values, one per row, with columns as |
scale |
|
stop |
stopping rule: |
hits |
number of times the best optimum needs to be reached for |
sd_max |
largest standard deviation for |
tol |
relative tolerance for two runs to reach the same optimum |
seed |
optional seed for the random number generator |
optimizer |
optimisation function called as |
silent |
logical; if |
... |
further arguments passed to |
Details
Stopping. Two runs reach the same optimum if their negative log-likelihoods differ by less than
tol (relative), so permuted states (label switching) count as the same optimum.
Only converged runs (convergence code 0 and maximum gradient component below 0.01) count for stopping.
In any case, at most nstarts starts are run.
-
stop = "bayes"uses the Bayesian stopping rule of Boender and Rinnooy Kan (1987): afterkruns withwdistinct optima, the expected number of optima isw(k-1)/(k-w-2), andmultistart()stops when this is beloww + 0.5, i.e. probably no optimum is missed. The rule assumes that the starts are independent draws from one distribution, so only the random starts count, not the first run fromobj$par, and it is not used for givenstarts. It needs at least 8 converged random starts. -
stop = "hits"stops once the best optimum was reachedhitstimes.
Caution. Stopping does not mean that the global optimum was found. "No optimum missed" only refers to the
distribution of the starts: optima far away from it, or with a small basin of attraction, can be missed.
For example, with a very small sd, all starts converge to the same optimum and the rule stops quickly,
although other starts might find a better one. So choose sd wide enough and still check the fit.
Scatter.
With
scale = "fixed", the starts areobj$parplus normal noise with standard deviationsd. As most working parameters are on log or logit scale,sd = 1is a relative change, so one value usually fits all parameters. Parameters on identity scale (e.g. means of normal distributions) may need their ownsd, given as a named list likelist(eta = 1, mu = 5).With
scale = "unit_info", the starts are drawn around the first fit from a normal distribution with covariancen H^{-1}, whereHis the Hessian of the negative log-likelihood andnthe number of observations. This is the information of a single observation (unit information), which does not shrink withnand takes correlations of the parameters into account. Standard deviations are capped atsd_max, for weakly identified parameters. If the Hessian is not positive definite (orallprobsis not reported, sonis unknown), the fixedsdis used instead.
Value
output of optimizer for the best run, with two more elements: runs, a data frame
with the negative log-likelihood nll, convergence code and maximum gradient component mgc of each run,
and starts, the matrix of starting values used.
References
Boender, C. G. E., & Rinnooy Kan, A. H. G. (1987). Bayesian stopping rules for multistart global optimization methods. Mathematical Programming, 37(1), 59-80.
Examples
nll <- function(par) {
getAll(par, dat)
Gamma <- tpm(eta)
mu <- exp(log_mu); REPORT(mu)
allprobs <- cbind(dgamma2(step, mu[1], exp(log_sigma[1])),
dgamma2(step, mu[2], exp(log_sigma[2])))
-forward(stationary(Gamma), Gamma, allprobs)
}
dat <- list(step = trex$step[1:500])
par <- list(eta = c(-2, -2), log_mu = log(c(0.3, 2.5)), log_sigma = log(c(0.2, 1.5)))
obj <- MakeADFun(nll, par, silent = TRUE)
opt <- multistart(obj, seed = 1)
opt$runs
mod <- lama(obj) # best fit
# starts scaled by the first fit
opt <- multistart(obj, scale = "unit_info", seed = 1)
Loch Ness Monster Acceleration Data
Description
A small group of researchers managed to put an accelerometer on the Loch Ness Monster and collected data for a few days. Now we have a data set of the overall dynamic body acceleration (ODBA) of the creature.
Usage
nessi
Format
A data frame with 5.000 rows and 3 variables:
- ODBA
overall dynamci body acceleration
- logODBA
logarithm of overall dynamic body acceleration
- state
hidden state variable
Source
Generated for example purposes.
Computes penalty based on quadratic form
Description
This function computes quadratic penalties of the form
0.5 \sum_{i} \lambda_i b_i^T S_i b_i,
with smoothing parameters \lambda_i, coefficient vectors b_i, and fixed penalty matrices S_i.
It is intended to be used inside the penalised negative log-likelihood function when fitting models with penalised splines or simple random effects via quasi restricted maximum likelihood (qREML) with the qreml function.
For qreml to work, the likelihood function needs to be compatible with the RTMB R package to enable automatic differentiation.
Usage
penalty(re_coef, S, sp, lambda)
Arguments
re_coef |
coefficient vector/ matrix or list of coefficient vectors/ matrices Each list entry corresponds to a different smooth/ random effect with its own associated penalty matrix in |
S |
fixed penalty matrix or list of penalty matrices matching the structure of |
sp |
penalty strength parameter vector that has a length corresponding to the total number of random effects/ spline coefficients in E.g. if |
lambda |
former name of |
Details
Caution: The formatting of re_coef needs to match the structure of the parameter list in your penalised negative log-likelihood function,
i.e. you cannot have two random effect vectors of different names (different list elements in the parameter list), combine them into a matrix inside your likelihood and pass the matrix to penalty.
If these are seperate random effects, each with its own name, they need to be passed as a list to penalty. Moreover, the ordering of re_coef needs to match the character vector random specified in qreml.
Value
returns the penalty value and reports to qreml.
References
Koslik, J. O. (2024). Efficient smoothness selection for nonparametric Markov-switching models via quasi restricted maximum likelihood. arXiv preprint arXiv:2411.11498.
See Also
qreml for the qREML algorithm
Examples
# Example with a single random effect
re = rep(0, 5)
S = diag(5)
sp = 1
penalty(re, S, sp)
# Example with two random effects,
# where one element contains two random effects of similar structure
re = list(matrix(0, 2, 5), rep(0, 4))
S = list(diag(5), diag(4))
sp = c(1,1,2) # length = total number of random effects
penalty(re, S, sp)
# Full model-fitting example
data = trex[1:1000,] # subset
# initial parameter list
par = list(logmu = log(c(0.3, 2.5)), # step mean
logsigma = log(c(0.3, 1.5)), # step sd
beta0 = c(-2,-2), # state process intercept
betaspline = matrix(rep(0, 18), nrow = 2)) # state process spline coefs
# data object with initial penalty strength sp
dat = list(step = data$step, # step length
tod = data$tod, # time of day covariate
N = 2, # number of states
sp = rep(10,2)) # initial penalty strength
# building model matrices
modmat = modmat(~ s(tod, bs = "cp"),
data = data.frame(tod = 1:24),
knots = list(tod = c(0,24))) # wrapping points
dat$Z = modmat$Z # spline design matrix
dat$S = modmat$S # penalty matrix
# penalised negative log-likelihood function
pnll = function(par) {
getAll(par, dat) # makes everything contained available without $
Gamma = tpm_g(Z, cbind(beta0, betaspline)) # transition probabilities
delta = stationary_p(Gamma, t = tod[1] %% 24 + 1) # initial distribution
mu = exp(logmu) # step mean
sigma = exp(logsigma) # step sd
# calculating all state-dependent densities
allprobs = matrix(1, nrow = length(step), ncol = N)
ind = which(!is.na(step)) # only for non-NA obs.
for(j in 1:N) allprobs[ind,j] = dgamma2(step[ind],mu[j],sigma[j])
-forward_g(delta, Gamma[,,tod], allprobs) +
penalty(betaspline, S, sp) # this does all the penalization work
}
# model fitting
mod = qreml(pnll, par, dat, random = "betaspline")
Computes generalised quadratic-form penalties
Description
This function computes a quadratic penalty of the form
0.5 \sum_{i} \lambda_i b^T S_i b,
with smoothing parameters \lambda_i, coefficient vector b, and fixed penalty matrices S_i.
This generalises the penalty by allowing subsets of the coefficient vector b to be penalised multiple times with different smoothing parameters, which is necessary for tensor products, functional random effects or adaptive smoothing.
It is intended to be used inside the penalised negative log-likelihood function when fitting models with penalised splines or simple random effects via quasi restricted maximum likelihood (qREML) with the qreml function.
For qreml to work, the likelihood function needs to be compatible with the RTMB R package to enable automatic differentiation.
Usage
penalty2(re_coef, S, sp, lambda)
Arguments
re_coef |
list of coefficient vectors/ matrices Each list entry corresponds to a different smooth/ random effect with its own associated penalty matrix or penalty-matrix list in |
S |
list of fixed penalty matrices matching the structure of This means if |
sp |
penalty strength parameter vector that has a length corresponding to the provided Specifically, for entries with one penalty matrix, E.g. if |
lambda |
former name of |
Details
Caution: The formatting of re_coef needs to match the structure of the parameter list in your penalised negative log-likelihood function,
i.e. you cannot have two random effect vectors of different names (different list elements in the parameter list), combine them into a matrix inside your likelihood and pass the matrix to penalty.
If these are seperate random effects, each with its own name, they need to be passed as a list to penalty. Moreover, the ordering of re_coef needs to match the character vector random specified in qreml.
Value
returns the penalty value and reports to qreml.
See Also
qreml for the qREML algorithm
Examples
# Example with a single random effect
re = rep(0, 5)
S = diag(5)
sp = 1
penalty(re, S, sp)
# Example with two random effects,
# where one element contains two random effects of similar structure
re = list(matrix(0, 2, 5), rep(0, 4))
S = list(diag(5), diag(4))
sp = c(1,1,2) # length = total number of random effects
penalty(re, S, sp)
# Full model-fitting example
data = trex[1:1000,] # subset
# initial parameter list
par = list(logmu = log(c(0.3, 2.5)), # step mean
logsigma = log(c(0.3, 1.5)), # step sd
beta0 = c(-2,-2), # state process intercept
betaspline = matrix(rep(0, 18), nrow = 2)) # state process spline coefs
# data object with initial penalty strength sp
dat = list(step = data$step, # step length
tod = data$tod, # time of day covariate
N = 2, # number of states
sp = rep(10,2)) # initial penalty strength
# building model matrices
modmat = modmat(~ s(tod, bs = "cp"),
data = data.frame(tod = 1:24),
knots = list(tod = c(0,24))) # wrapping points
dat$Z = modmat$Z # spline design matrix
dat$S = modmat$S # penalty matrix
# penalised negative log-likelihood function
pnll = function(par) {
getAll(par, dat) # makes everything contained available without $
Gamma = tpm_g(Z, cbind(beta0, betaspline)) # transition probabilities
delta = stationary_p(Gamma, t = tod[1] %% 24 + 1) # initial distribution
mu = exp(logmu) # step mean
sigma = exp(logsigma) # step sd
# calculating all state-dependent densities
allprobs = matrix(1, nrow = length(step), ncol = N)
ind = which(!is.na(step)) # only for non-NA obs.
for(j in 1:N) allprobs[ind,j] = dgamma2(step[ind],mu[j],sigma[j])
-forward_g(delta, Gamma[,,tod], allprobs) +
penalty(betaspline, S, sp) # this does all the penalisation work
}
# model fitting
mod = qreml(pnll, par, dat, random = "betaspline")
Penalty approximation of unimodality constraints for univariates smooths
Description
Penalty approximation of unimodality constraints for univariates smooths
Usage
penalty_uni(coef, m, kappa = 1000, concave = TRUE, rho = 20)
Arguments
coef |
coefficient vector of matrix on which to apply the unimodality penalty |
m |
vector of indices for the position of the coefficient mode.
If |
kappa |
global scaling factor for the penalty |
concave |
logical; if |
rho |
control parameter for smooth approximation to |
Value
a numeric value of the penalty for the given coefficients
Examples
## coefficient vector
coef <- c(1, 2, 3, 2, 1)
# mode at position 3
penalty_uni(coef, m = 3) # basically zero
#' # mode at position 2
penalty_uni(coef, m = 2) # large positive penalty
## coefficient matrix
coef <- rbind(coef, coef)
m <- c(1, 4)
penalty_uni(coef, m)
Plot a LaMaModel object
Description
Plots the pseudo-residuals of a model from lama or qreml,
computed by pseudo_res from the model object alone, with one row of plots per data stream,
or the estimated state-dependent densities of each data stream built with statedens.
Usage
## S3 method for class 'LaMaModel'
plot(x, type = c("residuals", "statedens"), stream = NULL, ...)
Arguments
x |
model object of class |
type |
|
stream |
optional names of the data streams to plot, by default all |
... |
further arguments passed to |
Details
For type = "statedens", each data stream is shown as a histogram with the state-dependent densities
(probabilities for discrete distributions) weighted by the state probabilities, and their sum, the marginal density, as a dashed line.
The weighted density of state j is the mean over the observations of p_{tj} f_j(x; \theta_{tj}),
which allows for parameters that depend on covariates, several tracks and inhomogeneous state processes.
This needs allprobs to be the product of matrices from statedens, which is checked.
Further arguments for type = "statedens":
weightsstate probabilities
p_{tj}:"stateprobs"(default) for the local state probabilities fromstateprobs,"viterbi"for the states decoded byviterbi,"stationary"for the stationary distribution (averaged over tracks, or over the cycle for periodic models), or a vector of lengthnStatescolcolours of the states, defaults to
LaMaColorslwdline width
nnumber of grid points for continuous distributions
legendposition of the legend, e.g.
"topright"(default), orFALSEfor none- ...
arguments passed to
plot()of the histogram, e.g.breaks,main,xlab,xlim,ylimorborder
Several streams are shown side by side, unless par(mfrow) has been set.
Value
for type = "residuals" the pseudo-residuals, for type = "statedens" a list with the grid x,
the weighted state-dependent densities density (one column per state), the state weights and the observations data
(or a list of these for several streams), invisibly
Examples
dat <- list(step = trex$step[1:500], angle = trex$angle[1:500])
nll <- function(par) {
getAll(par, dat)
Gamma <- tpm(eta)
allprobs <- statedens(step, dgamma2, exp(log_mu), exp(log_sigma)) *
statedens(angle, dvm, 0, exp(log_kappa))
-forward(stationary(Gamma), Gamma, allprobs)
}
par <- list(eta = c(-2, -2), log_mu = log(c(0.3, 2.5)), log_sigma = log(c(0.2, 1.5)),
log_kappa = log(c(0.2, 1.5)))
obj <- MakeADFun(nll, par, silent = TRUE)
opt <- nlminb(obj$par, obj$fn, obj$gr)
mod <- lama(obj)
plot(mod) # pseudo-residuals
plot(mod, type = "statedens") # state-dependent densities of both streams
plot(mod, type = "statedens", stream = "step", weights = "viterbi",
breaks = 40, xlab = "step length")
Plot pseudo-residuals
Description
Plot pseudo-residuals computed by pseudo_res.
The QQ plot shows a pointwise 95% band (in gray) for the sample quantiles under a correct model.
Usage
## S3 method for class 'LaMaResiduals'
plot(
x,
col = "darkblue",
lwd = 1.5,
main = NULL,
breaks = "Sturges",
axis.lab = list(qq = c("Theoretical quantiles", "Sample quantiles"), hist =
c("Pseudo-residuals", "Density"), acf = c("Lag", "ACF")),
...
)
Arguments
x |
pseudo-residuals as returned by |
col |
character, color for the QQ-line (and density curve if |
lwd |
numeric, line width for the QQ-line (and density curve if |
main |
optional character vector of main titles for the plots of length 2 (or 3 if |
breaks |
|
axis.lab |
labels used for the x and y axis of each plot (named list) |
... |
currently ignored. For method consistency |
Value
NULL, plots the pseudo-residuals in a 3-panel layout
Examples
## pseudo-residuals for the trex data
step = trex$step[1:1000]
angle = trex$angle[1:1000]
nll = function(par){
getAll(par)
Gamma = tpm(logitGamma)
delta = stationary(Gamma)
mu = exp(logMu); REPORT(mu)
sigma = exp(logSigma); REPORT(sigma)
kappa = exp(logKappa); REPORT(kappa)
allprobs = matrix(1, length(step), 2)
ind = which(!is.na(step) & !is.na(angle))
for(j in 1:2) {
allprobs[ind,j] = dgamma2(step[ind], mu[j], sigma[j]) *
dvm(angle[ind], 0, kappa[j])
}
-forward(delta, Gamma, allprobs)
}
par = list(logitGamma = c(-2,-2),
logMu = log(c(0.3, 2.5)),
logSigma = log(c(0.3, 1.5)),
logKappa = log(c(0.1, 1.7)))
obj = MakeADFun(nll, par, silent = TRUE)
opt = nlminb(obj$par, obj$fn, obj$gr)
mod = lama(obj)
pres_step = pseudo_res(step, # observations
"gamma2", # family that is used
list(mean = mod$mu, sd = mod$sigma), # the family's parameters
mod = mod) # model object
pres_angle = pseudo_res(angle,
"vm",
list(mu = 0, kappa = mod$kappa),
mod = mod)
# separate plots
plot(pres_step)
plot(pres_angle)
# together
par(mfrow = c(2,3))
plot(pres_step, main = c("", "Step Length", ""),
axis.lab = list(hist = c("Step residuals", "Density")))
plot(pres_angle, main = c("", "Turning Angle", ""),
axis.lab = list(hist = c("Angle residuals", "Density")))
# or from the model object alone, one row per stream
plot(pseudo_res(mod))
Build the prediction design matrix based on new data and model_matrices object created by modmat
Description
Deprecated. Use predict on the object returned by modmat instead, which does the same thing:
predict(modmat, newdata) in place of pred_matrix(modmat, newdata).
Usage
pred_matrix(model_matrices, newdata, what = NULL, exclude = NULL)
Arguments
model_matrices |
model_matrices object as returned from |
newdata |
data frame containing the variables in the formula and new data for which to evaluate the basis |
what |
optional character string specifying which formula to use for prediction if |
exclude |
optional vector of terms to set to zero in the predicted design matrix. Useful for predicting main effects only when e.g. |
Value
prediction design matrix for newdata with the same basis as used for model_matrices
See Also
predict, which replaces this function
Examples
modmat = modmat(~ s(x), data.frame(x = 1:10))
# deprecated:
# Z_p = pred_matrix(modmat, data.frame(x = 1:10 - 0.5))
# use instead:
Z_p = predict(modmat, data.frame(x = 1:10 - 0.5))
Build the prediction design matrix based on new data and model_matrices object created by modmat
Description
Build the prediction design matrix based on new data and model_matrices object created by modmat
Usage
## S3 method for class 'LaMa_matrices'
predict(object, newdata, what = NULL, exclude = NULL, ...)
Arguments
object |
model matrices object as returned from |
newdata |
data frame containing the variables in the formula and new data for which to evaluate the basis |
what |
optional character string specifying which formula to use for prediction if |
exclude |
optional vector of terms to set to zero in the predicted design matrix. Useful for predicting main effects only when e.g. |
... |
for method consistency only |
Value
prediction design matrix for newdata with the same basis as used for object
See Also
modmat for creating objects of class LaMa_matrices which can be used for prediction by this function.
Examples
# single formula
modmat = modmat(~ s(x), data.frame(x = 1:10))
Z_p = predict(modmat, data.frame(x = 1:10 - 0.5))
# with multiple formulas
modmat = modmat(list(mu ~ s(x), sigma ~ s(x, bs = "ps")), data = data.frame(x = 1:10))
Z_p = predict(modmat, data.frame(x = 1:10 - 0.5), what = "mu")
# nested formula list
form = list(stream1 = list(mu ~ s(x), sigma ~ s(x, bs = "ps")))
modmat = modmat(form, data = data.frame(x = 1:10))
Z_p = predict(modmat, data.frame(x = 1:10 - 0.5), what = c("stream1", "mu"))
Estimated smooth densities
Description
Evaluates the smooth densities built with smoothdens for given spline coefficients, e.g. to plot the estimated state-dependent densities.
Usage
## S3 method for class 'smoothdens'
predict(object, coef, x = NULL, ...)
Arguments
object |
object of class |
coef |
coefficient matrix, one row per state, without the last column fixed at zero |
x |
optional points to evaluate the densities at, defaults to the prediction grid |
... |
unused |
Value
list with the points x and the matrix density of densities, one row per point and one column per state
Examples
x = c(rnorm(100, 0, 1), rnorm(100, 5, 1))
dens = smoothdens(x, par = list(mean = c(0, 5), sd = c(1, 1)))
# densities at the initial coefficients
pred = predict(dens, coef = dens$coef)
matplot(pred$x, pred$density, type = "l", lty = 1)
Print a LaMaModel object
Description
Prints a short overview of a model from lama or qreml:
the state process, observations, parameters, log-likelihood, AIC and BIC, and the names of the reported quantities.
Use summary() for the estimates.
Usage
## S3 method for class 'LaMaModel'
print(x, ...)
Arguments
x |
model object of class |
... |
additional arguments (not used) |
Value
x, invisibly
Print a LaMa_matrices object
Description
Print a LaMa_matrices object
Usage
## S3 method for class 'LaMa_matrices'
print(x, ...)
Arguments
x |
object of class |
... |
ignored |
Value
x, invisibly. Called for its side effect of printing.
See Also
Process and standardise formulas for the state process of hidden Markov models
Description
Process and standardise formulas for the state process of hidden Markov models
Usage
process_hid_formulas(formulas, nStates, ref = NULL)
Arguments
formulas |
formulas for the transition process of a hidden Markov model, either as a single formula, a list of formulas, or a matrix. |
nStates |
number of states of the Markov chain |
ref |
optional vector of reference categories for each state, defaults to |
Value
named list of formulas of length nStates * (nStates - 1), where each formula corresponds to a transition from state i to state j, excluding transitions from i to ref[i].
Examples
# single formula for all non-reference category elements
formulas = process_hid_formulas(~ s(x), nStates = 3)
# now a list of length 6 with names tr.ij, not including reference categories
# different reference categories
formulas = process_hid_formulas(~ s(x), nStates = 3, ref = c(1,1,1))
# different formulas for different entries (and only for 2 of 6)
formulas = list(tr.12 ~ s(x), tr.23 ~ s(y))
formulas = process_hid_formulas(formulas, nStates = 3, ref = c(1,1,1))
# also a list of length 6, remaining entries filled with tr.ij ~ 1
# matrix input with reference categories
formulas = matrix(c(".", "~ s(x)", "~ s(y)",
"~ g", ".", "~ I(x^2)",
"~ y", "~ 1", "."),
nrow = 3, byrow = TRUE)
# dots define reference categories
formulas = process_hid_formulas(formulas, nStates = 3)
Calculate pseudo-residuals
Description
For HMMs, pseudo-residuals are used to assess the overall goodness-of-fit of the model. These are based on the cumulative distribution function (CDF)
F_{X_t}(x_t) = F(x_t \mid x_1, \dots, x_{t-1})
and can be used to quantify whether an observation is extreme relative to its model-implied distribution.
This function calculates such residuals via the probability integral transform, based on the local state probabilities obtained by stateprobs and the respective parametric family.
Usage
pseudo_res(
obs,
dist,
par,
stateprobs = NULL,
mod = NULL,
normal = TRUE,
discrete = NULL,
randomise = TRUE
)
Arguments
obs |
vector of observations (of length |
dist |
character string specifying which parametric CDF to use (e.g., |
par |
named parameter list for the parametric CDF Names need to correspond to the parameter names in the specified distribution (e.g. |
stateprobs |
matrix of local state probabilities for each observation (of dimension c(nObs, nStates)) as computed by |
mod |
optional model object containing required quantities When using automatic differentiation either with |
normal |
logical, if These will be approximately standard normally distributed if the model is correct. |
discrete |
logical, if By default, will be determined using |
randomise |
for discrete pseudo residuals only. Logical, if |
Details
Pseudo-residuals are based on the probability integral transform.
If the cumulative distribution function (CDF) F of a random variable
X is known, then F(X) is uniformly distributed on [0,1].
Applying the standard normal quantile function \Phi^{-1} then gives
a residual that is approximately standard normal under the model.
For discrete-valued observations, the CDF is a step function, so the residual
is not uniquely defined. One can compute a "lower" and "upper" pseudo-residual
corresponding to F(X-1) and F(X), respectively.
If randomise = TRUE, a value is drawn uniformly
between the lower and upper bounds. In this case, the resulting pseudo-residuals
are again approximately standard normal after applying the standard normal quantile function.
Model object only: pseudo_res(mod) needs no observations, family or parameters.
It evaluates the likelihood function stored in the model again, with each density
(e.g. dgamma2()) replaced by its CDF (pgamma2()) with the same arguments, so
that the likelihood function itself builds the CDFs in place of allprobs. This works for
loops over states or time, cbind(), covariate-dependent parameters, densities on the log scale,
mixtures within a state and several data streams (multiplied, or summed on the log scale),
giving one set of residuals per stream, named after the data variable.
Before, it checks that the densities enter allprobs as a product or mixture, so that
swapping in CDFs is valid. If not, e.g. for densities transformed by hand (truncation, Jacobians,
zero inflation via indicators) or a latent variable integrated out inside allprobs, it stops, and
pseudo_res(obs, dist, par, mod = mod) needs to be used instead.
Densities in your own helper functions called by the likelihood function are found as well,
and qreml models work like models from lama.
The likelihood function needs to call forward once (use trackID for several tracks),
and it is evaluated with the data as they are when pseudo_res() is called.
Value
vector of pseudo residuals of class LaMaResiduals or list containing lower, upper, and mean if discrete residuals are not randomised.
For pseudo_res(mod) with several data streams, a named list of these, one per stream, also of class LaMaResiduals.
See Also
plot.LaMaResiduals for plotting pseudo-residuals.
Examples
## continuous-valued observations
obs = rnorm(100)
stateprobs = matrix(0.5, nrow = 100, ncol = 2)
par = list(mean = c(1,2), sd = c(1,1))
pres = pseudo_res(obs, "norm", par, stateprobs)
## discrete-valued observations
obs = rpois(100, lambda = 1)
par = list(lambda = c(1,2))
pres = pseudo_res(obs, "pois", par, stateprobs)
## custom CDF function
obs = rnbinom(100, size = 1, prob = 0.5)
par = list(size = c(0.5, 2), prob = c(0.4, 0.6))
pres = pseudo_res(obs, pnbinom, par, stateprobs,
discrete = TRUE)
# if discrete CDF function is passed, 'discrete' needs to be set to TRUE
## no CDF function available, only density (artificial example)
obs = rnorm(100)
par = list(mean = c(1,2), sd = c(1,1))
# construct CDF using numerical integration
cdf = function(x, mean, sd) integrate(dnorm, -Inf, x, mean = mean, sd = sd)$value
pres = pseudo_res(obs, cdf, par, stateprobs)
### Full model fit example ###
step = trex$step[1:500]
nll = function(par){
getAll(par)
Gamma = tpm(logitGamma)
delta = stationary(Gamma)
mu = exp(logMu); REPORT(mu)
sigma = exp(logSigma); REPORT(sigma)
allprobs = matrix(1, length(step), 2)
ind = which(!is.na(step))
for(j in 1:2) allprobs[ind,j] = dgamma2(step[ind], mu[j], sigma[j])
-forward(delta, Gamma, allprobs)
}
par = list(logitGamma = c(-2,-2),
logMu = log(c(0.3, 2.5)),
logSigma = log(c(0.3, 1.5)))
obj = MakeADFun(nll, par, silent = TRUE)
opt = nlminb(obj$par, obj$fn, obj$gr)
mod = lama(obj)
pres = pseudo_res(step, # observation sequence
"gamma2", # parametric family that was used
list(mean = mod$mu, sd = mod$sigma), # parameters for that family
mod = mod) # model object
# or, from the model object alone
pres = pseudo_res(mod)
plot(pres)
Automatic smoothness selection for arbitrary statistical models with penalised splines, simple random effects, or tensorproducts
Description
Efficiently fits models involving quadratic penalties of the form
\sum_{i} \lambda_i b^T S_i b,
by combining automatic differentiation via RTMB with a custom implementation of the extended Fellner-Schall update.
Users only need to supply a custom penalised log-likelihood function that calls penalty() or penalty2().
Usage
qreml(
pnll,
par,
dat,
random,
map = NULL,
silent = 1,
spname = NULL,
tol_edf = 0.01,
maxiter = 100,
alpha = 0.1,
tol = 0.01,
smoothing = 1,
method = "BFGS",
lsp_max = 15,
step_small = 0.05,
max_halve = 6,
control = list(),
spHess = FALSE,
joint_unc = FALSE,
saveall = FALSE
)
Arguments
pnll |
penalised negative log-likelihood function that is structured as dictated by |
par |
named list of initial parameters |
dat |
initial data list that contains the data used in the likelihood function, hyperparameters, and the initial penalty strength vector,
called |
random |
vector of names of the random effects/ penalised parameters in Caution: The ordering of |
map |
optional map argument, containing factor vectors to indicate parameter sharing or fixing |
silent |
integer silencing level: 0 corresponds to full printing of inner and outer iterations, 1 to printing of outer iterations only, and 2 to no printing |
spname |
optional name of the penalty strength vector in By default, |
tol_edf |
convergence tolerance on the effective degrees of freedom. This is the primary convergence criterion. The iteration stops once no smooth's effective degrees of freedom has changed by more than |
maxiter |
maximum number of outer iterations |
alpha |
smallest factor by which a penalty strength may decrease in one outer iteration, a number in [0, 1). Defaults to 0.1. Penalty strengths are free to increase as fast as the update proposes, but cannot collapse faster than this per iteration.
Reducing a penalty strength too quickly can push the inner optimisation into a local optimum or a numerically awkward region, which matters more here than in a GAM because the likelihood is user-written.
Set to zero to remove the floor entirely. Step length is handled separately, by |
tol |
fallback convergence tolerance, on the restricted log-likelihood. Defaults to 0.01. Used only when the effective degrees of freedom are not trustworthy, i.e.\ when they fall outside |
smoothing |
optional scaling factor for the final penalty strength parameters. Increasing this beyond one leads to a smoother final model |
method |
inner optimisation method to be used by |
lsp_max |
largest value allowed for |
step_small |
size of a step in |
max_halve |
maximum number of times a step that decreases the restricted likelihood is halved before it is accepted anyway. Defaults to 6.
|
control |
list of control parameters for |
spHess |
logical, if |
joint_unc |
logical, if |
saveall |
logical, if |
Details
Step size control follows the extended Fellner-Schall implementation in mgcv while convergence is judged on the effective degrees of freedom (differing from mgcv).
The criterion. The penalty strengths are chosen to maximise the Laplace-approximate restricted log-likelihood
V(\lambda) = \ell_p(\hat{b}; \lambda) + \tfrac{1}{2} \log |S_\lambda|_+ - \tfrac{1}{2} \log |J|,
where \ell_p is the penalised log-likelihood at its mode \hat{b}, S_\lambda = \sum_i \lambda_i S_i, |\cdot|_+ denotes the product of the positive eigenvalues, and J is the Hessian of the penalised negative log-likelihood at \hat{b}.
Every outer iteration refits the inner problem to obtain \hat{b} and J, so one call is a sequence of complete model fits, each warm started at the previous one.
The update. The penalty strengths are updated multiplicatively, \lambda_i \leftarrow \lambda_i r_i, by the extended Fellner-Schall ratio
r_i = \frac{\mathrm{tr}(S_\lambda^- S_i) - \mathrm{tr}(J^{-1} S_i)}{\hat{b}^T S_i \hat{b}},
which equals one exactly where \partial V / \partial \lambda_i = 0 and otherwise moves \lambda_i in the direction of the gradient, without ever making it negative.
For a smooth carrying a single penalty the first trace is \mathrm{rank}(S_i) / \lambda_i, obtained once from an eigendecomposition instead of at every iteration.
Only the diagonal blocks of J^{-1} enter, and these come from the Cholesky factor by triangular solves rather than from a full inverse.
Step control. The step is taken in \log \lambda and scaled by a multiplier that persists across iterations: it doubles while the criterion keeps improving and is halved, up to max_halve times, while it does not.
A step that still worsens the criterion after that many halvings is accepted, which is the only way the iteration can move downhill.
In addition no penalty strength may fall by more than a factor alpha in one iteration, and \log \lambda is capped at lsp_max.
The fit returned is the best iterate seen, not necessarily the last one.
Convergence. The iteration stops once no smooth's effective degrees of freedom
\mathrm{edf}_i = K_i - \mathrm{tr}(J^{-1} \lambda_i S_i)
has moved by more than tol_edf over the last four iterations, provided the step in \log \lambda is also small; see tol_edf.
Being eigenvalue sums, the effective degrees of freedom must lie in [0, K_i], and they leave that range only if the data Hessian is indefinite, in which case the traces driving the update are not the quantities the method assumes.
That is reported rather than repaired, through the returned edf_valid and a warning, and the criterion then falls back to tol on the restricted log-likelihood.
Numerics. J is the exact automatic differentiation Hessian, which matters because the finite differencing error of optimHess is of the same order as the criterion differences the convergence test has to resolve.
It is factorised by a pivoted Cholesky decomposition after scaling to a unit diagonal; should it not be positive definite, a ridge is added and reported through the returned hessian_repaired.
Uncertainty. The returned outer_hessian() gives the Hessian of the negative restricted log-likelihood in the penalty strengths, which sdreport_outer turns into standard errors.
Note that these describe the curvature of V only, and treat the approximation to it as exact.
Value
model object of class "qremlModel", inheriting from "LaMaModel" (see lama), carrying the fitted quantities, the smoothness selection diagnostics shown by summary.qremlModel, and outer_hessian(), the outer Hessian that sdreport_outer turns into standard errors
References
Wood, S. N., & Fasiolo, M. (2017). A generalized Fellner-Schall method for smoothing parameter optimization with application to Tweedie location, scale and shape models. Biometrics, 73(4), 1071-1081.
Koslik, J. O. (2024). Efficient smoothness selection for nonparametric Markov-switching models via quasi restricted maximum likelihood. arXiv preprint arXiv:2411.11498.
See Also
penalty and penalty2 to compute the penalty inside the likelihood function, and qreml_old for the original algorithm
Examples
data = trex[1:2000,] # subset of the data
# initial parameter list
par = list(logmu = log(c(0.3, 2.5)), # step mean
logsigma = log(c(0.3, 1.5)), # step sd
beta0 = c(-2,-2), # state process intercept
beta_spline = matrix(rep(0, 18), nrow = 2)) # state process spline coefs
# data object with initial penalty strength sp
dat = list(step = data$step, # step length
tod = data$tod, # time of day covariate
N = 2, # number of states
sp = rep(20,2)) # initial penalty strength
# building model matrices
modmat = modmat(~ s(tod, bs = "cp"),
data = data.frame(tod = 1:24),
knots = list(tod = c(0,24))) # wrapping points
dat$Z = modmat$Z # spline design matrix
dat$S = modmat$S # penalty matrix
# penalised negative log-likelihood function
pnll = function(par) {
getAll(par, dat) # makes everything contained available without $
Gamma = tpm(cbind(beta0, beta_spline), Z) # transition probabilities
delta = stationary_p(Gamma, t = tod[1] %% 24 + 1) # initial distribution
mu = exp(logmu) # step mean
sigma = exp(logsigma) # step sd
# calculating all state-dependent densities
allprobs = matrix(1, nrow = length(step), ncol = N)
ind = which(!is.na(step)) # only for non-NA obs.
for(j in 1:N) allprobs[ind,j] = dgamma2(step[ind],mu[j],sigma[j])
-forward(delta, Gamma[,,tod], allprobs) +
penalty(beta_spline, S, sp) # this does all the penalization work
}
# model fitting
mod = qreml(pnll, par, dat, random = "beta_spline", silent = 2)
Quasi restricted maximum likelihood (qREML) algorithm, previous version
Description
This algorithm can be used very flexibly to fit statistical models that involve penalised splines or simple i.i.d. random effects, i.e. that have penalties of the form
0.5 \sum_{i} \lambda_i b_i^T S_i b_i,
with smoothing parameters \lambda_i, coefficient vectors b_i, and fixed penalty matrices S_i.
The qREML algorithm is typically much faster than REML or marginal ML using the full Laplace approximation method, but may be slightly less accurate regarding the estimation of the penalty strength parameters.
qreml_old is the previous implementation, kept for reference. Use qreml, which estimates the same quantities with a better behaved outer iteration.
Under the hood, qreml_old uses the R package RTMB for automatic differentiation in the inner optimisation.
The user has to specify the penalised negative log-likelihood function pnll structured as dictated by RTMB and use the penalty function to compute the quadratic-form penalty inside the likelihood.
Usage
qreml_old(
pnll,
par,
dat,
random,
map = NULL,
silent = 1,
psname = "lambda",
alpha = 0.3,
smoothing = 1,
maxiter = 100,
tol = 1e-04,
max_halve = 5,
method = "BFGS",
control = list(),
conv_crit = "relchange",
spHess = FALSE,
joint_unc = FALSE,
saveall = FALSE
)
Arguments
pnll |
penalised negative log-likelihood function that is structured as dictated by Needs to be a function of the named list of initial parameters |
par |
named list of initial parameters The random effects/ spline coefficients can be vectors or matrices, the latter summarising several random effects of the same structure, each one being a row in the matrix. |
dat |
initial data list that contains the data used in the likelihood function, hyperparameters, and the initial penalty strength vector If the initial penalty strength vector is not called |
random |
vector of names of the random effects/ penalised parameters in Caution: The ordering of |
map |
optional map argument, containing factor vectors to indicate parameter sharing or fixing. Needs to be a named list for a subset of fixed effect parameters or penalty strength parameters.
For example, if the model has four penalty strength parameters, |
silent |
integer silencing level: 0 corresponds to full printing of inner and outer iterations, 1 to printing of outer iterations only, and 2 to no printing. |
psname |
optional name given to the penalty strength parameter in |
alpha |
optional hyperparamater for exponential smoothing of the penalty strengths. For larger values smoother convergence is to be expected but the algorithm may need more iterations. |
smoothing |
optional scaling factor for the final penalty strength parameters Increasing this beyond one will lead to a smoother final model. Can be an integer or a vector of length equal to the length of the penalty strength parameter. |
maxiter |
maximum number of iterations in the outer optimisation over the penalty strength parameters. |
tol |
Convergence tolerance for the penalty strength parameters. |
max_halve |
maximum number of step halvings per outer iteration. After each update of the penalty strength parameters, the restricted log-likelihood is compared to its value in the previous iteration.
If it decreased, the step (on the log scale) is repeatedly halved until it does not, or until |
method |
optimisation method to be used by |
control |
list of control parameters for We advise against changing the default values of |
conv_crit |
character, convergence criterion for the penalty strength parameters. Can be |
spHess |
logical, if |
joint_unc |
logical, if |
saveall |
logical, if |
Value
model object of class 'qremlModel'. This is a list containing:
... |
everything that is reported inside |
obj |
|
psname |
final penalty strength parameter vector |
all_psname |
list of all penalty strength parameter vectors over the iterations |
par |
named estimated parameter list in the same structure as the initial |
relist_par |
function to convert the estimated parameter vector to the estimated parameter list. This is useful for uncertainty quantification based on sampling from a multivariate normal distribution. |
par_vec |
estimated parameter vector |
llk |
unpenalised log-likelihood at the optimum |
n_fixpar |
number of fixed, i.e. unpenalised, parameters |
edf |
overall effective number of parameters |
all_edf |
list of effective number of parameters for each smooth |
Hessian_condtional |
final Hessian of the conditional penalised fit |
obj_joint |
if |
References
Koslik, J. O. (2024). Efficient smoothness selection for nonparametric Markov-switching models via quasi restricted maximum likelihood. arXiv preprint arXiv:2411.11498.
See Also
penalty and penalty2 to compute the penalty inside the likelihood function
Examples
data = trex[1:1000,] # subset
# initial parameter list
par = list(logmu = log(c(0.3, 2.5)), # step mean
logsigma = log(c(0.3, 1.5)), # step sd
beta0 = c(-2,-2), # state process intercept
betaspline = matrix(rep(0, 18), nrow = 2)) # state process spline coefs
# data object with initial penalty strength lambda
dat = list(step = data$step, # step length
tod = data$tod, # time of day covariate
N = 2, # number of states
lambda = rep(10,2)) # initial penalty strength
# building model matrices
modmat = modmat(~ s(tod, bs = "cp"),
data = data.frame(tod = 1:24),
knots = list(tod = c(0,24))) # wrapping points
dat$Z = modmat$Z # spline design matrix
dat$S = modmat$S # penalty matrix
# penalised negative log-likelihood function
pnll = function(par) {
getAll(par, dat) # makes everything contained available without $
Gamma = tpm_g(Z, cbind(beta0, betaspline), ad = TRUE) # transition probabilities
delta = stationary_p(Gamma, t = tod[1] %% 24 + 1, ad = TRUE) # initial distribution
mu = exp(logmu) # step mean
sigma = exp(logsigma) # step sd
# calculating all state-dependent densities
allprobs = matrix(1, nrow = length(step), ncol = N)
ind = which(!is.na(step)) # only for non-NA obs.
for(j in 1:N) allprobs[ind,j] = dgamma2(step[ind],mu[j],sigma[j])
-forward_g(delta, Gamma[,,tod], allprobs) +
penalty(betaspline, S, lambda) # this does all the penalization work
}
# model fitting
mod = qreml_old(pnll, par, dat, random = "betaspline", silent = 2)
Repeat initial penalty strengths for replicated smooths
Description
Expands the sp0 element of a modmat object into a
sp vector for penalty or penalty2, when each smooth is
used more than once, for example one spline per state or per off-diagonal element of the
transition probability matrix.
Usage
rep_sp(model_matrices, N)
Arguments
model_matrices |
object of class |
N |
number of replicates. Either a single number used for every smooth, or one number per
smooth, i.e. per element of |
Details
sp runs over replicates within each smooth, so for a tensor product the
margins vary fastest. A single rep() over sp0 therefore only gives the right
answer for some models, silently producing the right length but the wrong values for others.
This function repeats each smooth's penalty strengths separately, which is always correct.
Value
named numeric vector of initial penalty strengths, of the length and in the order
expected for sp
See Also
modmat, which computes sp0
Examples
modmat = modmat(~ s(x) + ti(x, y), data.frame(x = runif(100), y = runif(100)))
modmat$sp0 # one value per penalty
rep_sp(modmat, 2) # ready to use as 'sp' for two replicates of each smooth
Per-observation score contributions
Description
Computes the score contribution of each observation,
u_t = \frac{\partial}{\partial \theta} \log p(x_t \mid x_1, \dots, x_{t-1}),
for a model whose negative log-likelihood function calls forward.
Their column sums are the gradient of the log-likelihood. They are the building block for
robust (sandwich) standard errors, e.g. cluster-robust ones via rowsum(U, ID).
Usage
scores(obj, par = NULL)
Arguments
obj |
optimised |
par |
optional parameter vector like |
Details
Each log-likelihood contribution in forward gets a weight w_t.
The gradient of the weighted log-likelihood is linear in the weights, so its derivative
w.r.t. w_t is u_t. This needs one tape of the gradient and one reverse sweep
per parameter. The weights are handed to forward internally, so the
likelihood function does not need to change.
The likelihood function is taken from obj and evaluated again, with the data as they are
when scores() is called. Parameters fixed via map are respected, and the columns
correspond to obj$par, like obj$gr() and obj$he().
If the likelihood function calls forward several times, e.g. once per track, the rows of the
result follow the order of these calls. Only forward (and its deprecated
_g and _p versions) is supported, and models with random effects are not.
Value
matrix of score contributions of dimension c(nObs, length(obj$par))
Examples
nll <- function(par) {
getAll(par)
Gamma <- tpm(eta)
delta <- stationary(Gamma)
allprobs <- cbind(dgamma2(step, mu[1], sigma[1]),
dgamma2(step, mu[2], sigma[2]))
-forward(delta, Gamma, allprobs)
}
step <- trex$step[1:200]
par <- list(eta = c(-2, -2), mu = c(0.3, 2.5), sigma = c(0.2, 1.5))
obj <- MakeADFun(nll, par, silent = TRUE)
opt <- nlminb(obj$par, obj$fn, obj$gr)
mod <- lama(obj)
U <- scores(mod)
colSums(U) # ~ 0 at the MLE
Monte Carlo version of sdreport
Description
After optimisation of an AD model, sdreportMC can be used to calculate samples of confidence intervals of all model parameters and REPORT()ed quantities
including nonlinear functions of random effects and parameters.
Usage
sdreportMC(
obj,
what,
nSamples = 1000,
Hessian = NULL,
CI = FALSE,
probs = c(0.025, 0.975)
)
Arguments
obj |
object returned by |
what |
vector of strings with names of parameters and/or |
nSamples |
number of samples to draw from the multivariate normal distribution of the MLE |
Hessian |
optional Hessian matrix. If not provided, it will be computed from the object |
CI |
logical. If |
probs |
vector of probabilities for the confidence intervals (ignored if no CIs are computed) |
Details
This function simply samples from the approximate multivariate normal distribution of the maximum likelihood estimate (MLE) of the parameters
\hat{\theta} \sim N(\theta, H^{-1}),
where H is the Hessian matrix of the negative log-likelihood function at the MLE.
It then returns either the sampled parameters or REPORT()ed transformations of them. If CI = TRUE, it does not return the samples but directly computes confidence intervals.
If you are interested in several quantities, calling sdreportMC once with a vector what will generally be faster than calling it several times with single elements of what.
Value
named list corresponding to the elements of what. Each element has the structure of the corresponding quantity with an additional dimension added for the samples.
For example, if a quantity is a vector, the list contains a matrix. If a quantity is a matrix, the list contains an array. If quantity is an array, the list contains an array with one extra dimension.
Examples
# fitting an HMM to the trex data and running sdreportMC
## negative log-likelihood function
nll = function(par) {
getAll(par, dat) # makes everything contained available without $
Gamma = tpm(eta) # computes transition probability matrix from unconstrained eta
delta = stationary(Gamma) # computes stationary distribution
# exponentiating because all parameters strictly positive
mu = exp(logmu)
sigma = exp(logsigma)
kappa = exp(logkappa)
# reporting statements for sdreportMC
REPORT(mu)
REPORT(sigma)
REPORT(kappa)
# calculating all state-dependent densities
allprobs = matrix(1, nrow = length(step), ncol = N)
ind = which(!is.na(step) & !is.na(angle)) # only for non-NA obs.
for(j in 1:N){
allprobs[ind,j] = dgamma2(step[ind],mu[j],sigma[j])*dvm(angle[ind],0,kappa[j])
}
-forward(delta, Gamma, allprobs) # simple forward algorithm
}
## initial parameter list
par = list(
logmu = log(c(0.3, 1)), # initial means for step length (log-transformed)
logsigma = log(c(0.2, 0.7)), # initial sds for step length (log-transformed)
logkappa = log(c(0.2, 0.7)), # initial concentration for turning angle (log-transformed)
eta = rep(-2, 2) # initial t.p.m. parameters (on logit scale)
)
## data and hyperparameters
dat = list(
step = trex$step[1:500], # hourly step lengths
angle = trex$angle[1:500], # hourly turning angles
N = 2
)
## creating AD function
obj = MakeADFun(nll, par, silent = TRUE) # creating the objective function
## optimising
opt = nlminb(obj$par, obj$fn, obj$gr) # optimization
## running sdreportMC
# `mu` has report statement, `delta` is automatically reported by `forward()`
sdrMC = sdreportMC(obj,
what = c("mu", "delta"),
nSamples = 50)
dim(sdrMC$delta)
# now a matrix with 50 samples (rows)
Report uncertainty of the estimated smoothing parameters or variances
Description
Computes standard deviations for the smoothing parameters of a model object returned by qreml using the delta method.
Usage
sdreport_outer(mod, invert = FALSE)
Arguments
mod |
model objects as returned by |
invert |
optional logical; if |
Details
The computations are based on the approximate gradient of the restricted log likelihood. The outer Hessian is computed by finite differencing of this gradient. If the inverse smoothing parameters are requested, the standard deviations are transformed to the variances using the delta method.
Value
list containing report matrix summarising parameters and standard deviations as well as the outer Hessian matrix.
Examples
## no examples
Simulate from a fitted model
Description
Simulates states and observations from a model fitted with forward and statedens.
By default, this is done on the observed design: the tracks and their lengths, the initial distribution delta,
the transition probabilities Gamma and the parameters of the state-dependent densities
are those reported by the model, i.e. conditional on the observed covariates.
Simulating for new covariates is not possible; instead, rebuild the likelihood function for the new data
and call lama on the resulting object.
Usage
## S3 method for class 'LaMaModel'
simulate(
object,
nsim = 1,
seed = NULL,
rdens = NULL,
random = FALSE,
fill_na = FALSE,
...
)
Arguments
object |
model object from |
nsim |
number of simulations |
seed |
optional seed for the random number generator |
rdens |
optional named list of random number generators of the data streams, for densities without one named
by replacing the leading |
random |
logical; if |
fill_na |
logical; if |
... |
currently not used |
Details
The states are drawn as in the decoding functions, so that all types of Gamma that forward accepts
(homogeneous, track-specific, time-varying, periodic) work, as does a continuous-time model with one transition matrix
per time interval (the simulation is then conditional on the observed time points).
Each data stream is drawn from the random number generator belonging to its density, e.g. rgamma2 for dgamma2.
Missing observations of the data stay missing (unless fill_na = TRUE), except for a stream that is missing completely: such a placeholder
(e.g. step = rep(NA, n)) lets you simulate from a likelihood function without data, see the examples.
Models with random effects are by default simulated conditional on the estimated random effects.
With random = TRUE, RTMB draws the random effects first, which requires that the density of each random effect
is evaluated in the likelihood function before the random effect is used, either by u %~% dnorm(...)
or by nll <- nll - sum(dnorm(u, ..., log = TRUE)) (or another density).
The states and data are then simulated given these draws, so that every simulation has new random effects.
This also requires that allprobs is the product of the data streams built by statedens,
with each data stream passed once.
Value
data frame with the columns trackID (index of the track, if used), state and one column per data stream,
for nsim = 1, else a list of nsim such data frames.
Examples
nll <- function(par) {
getAll(par, dat)
Gamma <- tpm(eta)
allprobs <- statedens(step, dgamma2, exp(log_mu), exp(log_sigma)) *
statedens(angle, dvm, 0, exp(log_kappa))
-forward(stationary(Gamma), Gamma, allprobs)
}
dat <- list(step = trex$step[1:500], angle = trex$angle[1:500])
par <- list(eta = c(-2, -2), log_mu = log(c(0.3, 2.5)), log_sigma = log(c(0.2, 1.5)),
log_kappa = log(c(0.2, 1.5)))
obj <- MakeADFun(nll, par, silent = TRUE)
opt <- nlminb(obj$par, obj$fn, obj$gr)
mod <- lama(obj)
sim <- simulate(mod, seed = 1)
head(sim)
# simulate without data: all-NA streams as placeholders, parameters of your choice, then refit
dat$step <- dat$angle <- rep(NA, 500)
obj0 <- MakeADFun(nll, par, silent = TRUE)
sim <- simulate(lama(obj0), seed = 1)
dat$step <- sim$step; dat$angle <- sim$angle
obj1 <- MakeADFun(nll, par, silent = TRUE)
opt1 <- nlminb(obj1$par, obj1$fn, obj1$gr)
# random effects: RTMB draws them first, then the states and data are simulated given them
nll_re <- function(par) {
getAll(par, dat)
u %~% dnorm(0, exp(log_su)) # track-level random effect on the mean step length in state 1
mu <- exp(cbind(log_mu[1] + u[id], log_mu[2]))
Gamma <- tpm(eta)
.nll <- .nll - forward(stationary(Gamma), Gamma, statedens(step, dgamma2, mu, exp(log_sigma)), id)
.nll
}
dat <- list(step = trex$step[1:500], id = rep(1:5, each = 100))
par_re <- list(eta = c(-2, -2), log_mu = log(c(0.3, 2.5)), log_sigma = log(c(0.2, 1.5)),
log_su = log(0.3), u = rep(0, 5))
obj_re <- MakeADFun(nll_re, par_re, random = "u", silent = TRUE)
sim_re <- simulate(lama(obj_re), random = TRUE, seed = 1)
Skew normal distribution
Description
Density, distribution function, quantile function and random generation for the skew normal distribution.
Usage
dskewnorm(x, xi = 0, omega = 1, alpha = 0, log = FALSE)
pskewnorm(q, xi = 0, omega = 1, alpha = 0, lower.tail = TRUE, log.p = FALSE)
qskewnorm(p, xi = 0, omega = 1, alpha = 0, lower.tail = TRUE, log.p = FALSE)
rskewnorm(n, xi = 0, omega = 1, alpha = 0)
Arguments
x, q |
vector of quantiles |
xi |
location parameter |
omega |
scale parameter, must be positive. |
alpha |
skewness parameter, +/- |
log, log.p |
logical; if |
lower.tail |
logical; if |
p |
vector of probabilities |
n |
number of observations. If |
Details
This implementation of dskewnorm allows for automatic differentiation with RTMB while the other functions are imported from the sn package.
Value
dskewnorm gives the density, pskewnorm gives the distribution function, qskewnorm gives the quantile function, and rskewnorm generates random deviates.
Examples
x = rskewnorm(1)
d = dskewnorm(x)
p = pskewnorm(x)
q = qskewnorm(p)
Build the design and penalty matrices for smooth density estimation
Description
smooth_dens_construct() is deprecated, use smoothdens instead.
It returns the same objects, but ordered by component first and data stream second.
Usage
smooth_dens_construct(
data,
par,
type = "real",
k = 25,
knots = NULL,
degree = 3,
diff_order = 2
)
Arguments
data |
named data frame of 1 or multiple data streams |
par |
list of initial means and sds ( |
type |
type of each data stream, either |
k |
number of basis functions for each data stream |
knots |
optional vector of knots (including the boundary knots) to be used for basis construction, for several data streams a named list of such vectors.
If not provided, the knots are placed equidistantly for For |
degree |
degree of the B-spline basis functions for each data stream, defaults to cubic B-splines |
diff_order |
order of differencing used for the P-Spline penalty matrix for each data stream. Defaults to second-order differences. |
Value
a nested list containing the design matrices Z, the penalty matrices S, the initial coefficients coef the prediction design matrices Z_predict, the prediction grids xseq, and details for the basis expansion for each data stream.
Examples
data = data.frame(x = rnorm(100))
# deprecated:
# SmoothDens = smooth_dens_construct(data, par = list(x = list(mean = 0, sd = 1)))
# use instead:
dens = smoothdens(data$x, par = list(mean = 0, sd = 1))
Build the design and penalty matrices for smooth density estimation
Description
This high-level function can be used to prepare objects needed to estimate mixture models of smooth densities using P-Splines.
Usage
smoothdens(
x,
par,
type = "real",
k = 25,
knots = NULL,
degree = 3,
diff_order = 2,
pow = 0.5,
npoints = 10000
)
Arguments
x |
data vector for one data stream, or named data frame or list of several data streams |
par |
list of initial means and sds ( |
type |
type of each data stream, either |
k |
number of basis functions for each data stream |
knots |
optional vector of knots (including the boundary knots) to be used for basis construction, for several data streams a named list of such vectors.
If not provided, the knots are placed equidistantly for For |
degree |
degree of the B-spline basis functions for each data stream, defaults to cubic B-splines |
diff_order |
order of differencing used for the P-Spline penalty matrix for each data stream. Defaults to second-order differences. |
pow |
power for polynomial knot spacing, only used for |
npoints |
number of points used in the numerical integration for normalizing the B-spline basis functions
|
Details
Under the hood, make_matrices_dens is used for the actual construction of the design and penalty matrices.
You can provide one or multiple data streams of different types (real, positive, circular) and specify initial means and standard deviations/ concentrations for each data stream. This information is then converted into suitable spline coefficients.
smoothdens then constructs the design and penalty matrices for standardised B-splines basis functions (integrating to one) for each data stream.
For types "real" and "circular" the knots are placed equidistant in the range of the data, for type "positive" the knots are placed using polynomial spacing.
The last spline coefficient of each state is fixed at zero for identifiability, hence coef has k - 1 columns.
density(beta) takes care of this: it maps the coefficient matrix to the allprobs matrix, with rows of missing observations equal to one.
Value
For one data stream, an object of class "smoothdens": a list containing the design matrix Z, the penalty matrix S, the initial coefficients coef, the prediction design matrix Z_predict, the prediction grid xseq, details for the basis expansion basis, and the function density(beta).
For several data streams, a named list of such objects.
See Also
predict for the estimated densities
Examples
## one data stream, mixture of two normals
x = c(rnorm(100, 0, 1), rnorm(100, 5, 1))
dens = smoothdens(x, par = list(mean = c(0, 5), sd = c(1, 1)))
Z = dens$Z # design matrix
S = dens$S # penalty matrix
beta = dens$coef # initial coefficients
allprobs = dens$density(beta) # use this in the likelihood function
## 3 data streams
data = data.frame(x1 = rnorm(100, mean = 0, sd = 1),
x2 = rgamma2(100, mean = 5, sd = 3),
x3 = rvm(100, mu = 0, kappa = 2))
par = list(x1 = list(mean = 0, sd = 1),
x2 = list(mean = 5, sd = 3),
x3 = list(mean = 0, kappa = 2))
dens = smoothdens(data, par, type = c("real", "positive", "circular"))
# objects for x1
Z1 = dens$x1$Z
allprobs = dens$x1$density(dens$x1$coef) *
dens$x2$density(dens$x2$coef) *
dens$x3$density(dens$x3$coef)
State-dependent densities of one data stream
Description
Builds the matrix of state-dependent densities (or probabilities) of one data stream,
as used in the allprobs matrix of forward.
Several data streams that are conditionally independent given the state are combined by multiplying their matrices.
Usage
statedens(x, dens, ..., nStates = NULL, log = FALSE)
Arguments
x |
vector of observations of length |
dens |
density function, e.g. |
... |
parameters of |
nStates |
number of states. Only needed if all parameters are single values. |
log |
logical; if |
Details
Each parameter in ... can be
a single value, used for all states,
a vector of length
nStates, one value per state, ora matrix of dimension
c(nObs, nStates), one value per observation and state, e.g. from a regression on covariates.
Missing observations contribute nothing to the likelihood, so their rows are 1 (0 with log = TRUE).
As each data stream gets its own matrix, a missing value in one stream does not remove the observations of the others.
With log = TRUE, the log-densities are returned, to be added over data streams and used with forward(..., logspace = TRUE).
They are computed by dens(..., log = TRUE) if dens has an argument log, otherwise as log(dens(...))
(e.g. for densities from zero_inflate).
In obj$simulate() of RTMB, x is registered as data and simulated by forward, see simulate.LaMaModel.
Writing the loop over states by hand is equally valid and gives the same result. statedens() is just a shortcut.
Value
matrix of dimension c(nObs, nStates)
Examples
step <- trex$step[1:200]
angle <- trex$angle[1:200]
mu <- c(0.3, 2.5); sigma <- c(0.2, 1.5); kappa <- c(0.2, 1.5)
# one data stream
allprobs <- statedens(step, dgamma2, mu, sigma)
# the same by hand
allprobs2 <- matrix(1, length(step), 2)
ind <- which(!is.na(step))
for(j in 1:2) allprobs2[ind, j] <- dgamma2(step[ind], mu[j], sigma[j])
all.equal(allprobs, allprobs2)
# two data streams, mean of the turning angle the same in both states
allprobs <- statedens(step, dgamma2, mu, sigma) * statedens(angle, dvm, 0, kappa)
# on the log scale, for forward(..., logspace = TRUE)
logprobs <- statedens(step, dgamma2, mu, sigma, log = TRUE) +
statedens(angle, dvm, 0, kappa, log = TRUE)
Calculate conditional local state probabilities in HMMs
Description
Computes
\Pr(\text{State}_t = j \mid X_1, ..., X_T)
for a given HMM.
Usage
stateprobs(
delta,
Gamma,
allprobs,
trackID = NULL,
mod = NULL,
forecast = FALSE,
tod = NULL
)
Arguments
delta |
initial distribution; either
|
Gamma |
transition probability matrix; either
|
allprobs |
matrix of state-dependent probabilities or density values of dimension |
trackID |
optional vector of length |
mod |
optional model object containing |
forecast |
logical, indicating if forecast probabilities |
tod |
optional integer vector of length |
Value
matrix of conditional state probabilities of dimension c(nObs, nStates)
See Also
Other decoding functions:
stateprobs_g(),
stateprobs_p(),
viterbi(),
viterbi_g(),
viterbi_p()
Examples
Gamma = tpm(c(-1,-2))
delta = stationary(Gamma)
allprobs = matrix(runif(10), nrow = 10, ncol = 2)
probs = stateprobs(delta, Gamma, allprobs)
Calculate conditional local state probabilities for inhomogeneous HMMs
Description
Computes
\Pr(\text{State}_t = j \mid X_1, ..., X_T)
for inhomogeneous HMMs
Usage
stateprobs_g(
delta,
Gamma,
allprobs,
trackID = NULL,
mod = NULL,
forecast = FALSE
)
Arguments
delta |
initial distribution; either
|
Gamma |
array of transition probability matrices of dimension |
allprobs |
matrix of state-dependent probabilities or density values of dimension |
trackID |
optional vector of length |
mod |
optional model object containing |
forecast |
logical, indicating if forecast probabilities |
Details
Deprecated: please use stateprobs for all model types instead.
Value
matrix of conditional state probabilities of dimension c(nObs, nStates)
See Also
Other decoding functions:
stateprobs(),
stateprobs_p(),
viterbi(),
viterbi_g(),
viterbi_p()
Examples
Gamma = tpm_g(runif(10), matrix(c(-1,-1,1,-2), nrow = 2, byrow = TRUE))
delta = c(0.5, 0.5)
allprobs = matrix(runif(20), nrow = 10, ncol = 2)
probs = stateprobs_g(delta, Gamma[,,-1], allprobs)
Calculate conditional local state probabilities for periodically inhomogeneous HMMs
Description
Computes
\Pr(S_t = j \mid X_1, ..., X_T)
for periodically inhomogeneous HMMs
Usage
stateprobs_p(
delta,
Gamma,
allprobs,
tod,
trackID = NULL,
mod = NULL,
forecast = FALSE
)
Arguments
delta |
initial or stationary distribution of length N, or matrix of dimension c(k,N) for k independent tracks, if This could e.g. be the periodically stationary distribution (for each track) as computed by |
Gamma |
array of transition probability matrices for each time point in the cycle of dimension c(N,N,L), where L is the length of the cycle. |
allprobs |
matrix of state-dependent probabilities/ density values of dimension c(n, N) |
tod |
(Integer valued) variable for cycle indexing in 1, ..., L, mapping the data index to a generalised time of day (length n). For half-hourly data L = 48. It could, however, also be day of year for daily data and L = 365. |
trackID |
optional vector of k track IDs, if multiple tracks need to be decoded separately. The observations of each track need to be consecutive. |
mod |
optional model object containing initial distribution If you are using automatic differentiation either with |
forecast |
logical, indicating if forecast probabilities |
Details
Deprecated: please use stateprobs with argument tod instead.
Value
matrix of conditional state probabilities of dimension c(n,N)
See Also
Other decoding functions:
stateprobs(),
stateprobs_g(),
viterbi(),
viterbi_g(),
viterbi_p()
Examples
L = 24
beta = matrix(c(-1, 2, -1, -2, 1, -1), nrow = 2, byrow = TRUE)
Gamma = tpm_p(1:L, L, beta, degree = 1)
delta = stationary_p(Gamma, 2) # for tod[1] = 1
allprobs = matrix(runif(200), nrow = 100, ncol = 2)
tod = rep(1:24, 5)[1:100]
probs = stateprobs_p(delta, Gamma, allprobs, tod)
Compute the stationary distribution of a homogeneous Markov chain
Description
A homogeneous, finite state Markov chain that is irreducible and aperiodic converges to a unique stationary distribution, here called \delta.
As it is stationary, this distribution satisfies
\delta \Gamma = \delta,
subject to \sum_{j=1}^N \delta_j = 1,
where \Gamma is the transition probability matrix.
This function solves the linear system of equations above.
Usage
stationary(Gamma)
Arguments
Gamma |
transition probability matrix of dimension |
Value
either a single stationary distribution of the Markov chain (vector of length N) or a matrix of stationary distributions of dimension c(nTracks,N) with one stationary distribution in each row
See Also
tpm to create a transition probabilty matrix using the multinomial logistic link (softmax)
Other stationary distribution functions:
stationary_ct(),
stationary_p()
Examples
# single matrix
Gamma = tpm(c(rep(-2,3), rep(-3,3)))
delta = stationary(Gamma)
# multiple matrices
Gamma = array(Gamma, dim = c(3,3,10))
Delta = stationary(Gamma)
Compute the stationary distribution of a continuous-time Markov chain
Description
A well-behaved continuous-time Markov chain converges to a unique stationary distribution, here called \pi.
This distribution satisfies
\pi Q = 0,
subject to \sum_{j=1}^N \pi_j = 1,
where Q is the infinitesimal generator of the Markov chain.
This function solves the linear system of equations above for a given generator matrix.
Usage
stationary_ct(Q)
stationary_cont(Q)
Arguments
Q |
infinitesimal generator matrix of dimension |
Value
either a single stationary distribution of the continuous-time Markov chain (vector of length N) or a matrix of stationary distributions of dimension c(nTracks,N) with one stationary distribution in each row
See Also
generator to create a generator matrix
Other stationary distribution functions:
stationary(),
stationary_p()
Examples
# single matrix
Q = generator(c(-2,-2))
Pi = stationary_ct(Q)
# multiple matrices
Q = array(Q, dim = c(2,2,10))
Pi = stationary_ct(Q)
Periodically stationary distribution of a periodically inhomogeneous Markov chain
Description
Computes the periodically stationary distribution of a periodically inhomogeneous Markov chain.
Usage
stationary_p(Gamma, t = NULL, ad = NULL)
Arguments
Gamma |
array of transition probability matrices of dimension c(N,N,L) |
t |
integer index of the time point in the cycle, for which to calculate the stationary distribution If |
ad |
optional logical, indicating whether automatic differentiation with |
Details
If the transition probability matrix of an inhomogeneous Markov chain varies only periodically (with period length L), it converges to a so-called periodically stationary distribution.
This happens, because the thinned Markov chain, which has a full cycle as each time step, has homogeneous transition probability matrix
\Gamma_t = \Gamma^{(t)} \Gamma^{(t+1)} \dots \Gamma^{(t+L-1)}
for all t = 1, \dots, L.
The stationary distribution for time t satifies \delta^{(t)} \Gamma_t = \delta^{(t)}.
Here, Gamma[,,t] is the transition from t to t+1. forward with tod uses Gamma[,,tod[t]] for the transition into t,
so there, the initial distribution is stationary_p(Gamma, tod[1] %% L + 1), and stationary_p(Gamma)[c(2:L, 1), ] has the distribution at tod = k in row k.
This function calculates said periodically stationary distribution.
Value
either the periodically stationary distribution at time t or all periodically stationary distributions.
References
When using this function, please cite:
Koslik, J. O., Feldmann, C. C., Mews, S., Michels, R., & Langrock, R. (2025). Inference on the state process of periodically inhomogeneous hidden Markov models for animal behavior. The Annals of Applied Statistics, 19(4), 2724–2737.
See Also
tpm_p and tpm_g to create multiple transition matrices based on a cyclic variable or design matrix
Other stationary distribution functions:
stationary(),
stationary_ct()
Examples
# setting parameters for trigonometric link
beta = matrix(c(-1, 2, -1, -2, 1, -1), nrow = 2, byrow = TRUE)
Gamma = tpm_p(beta = beta, degree = 1)
# periodically stationary distribution for specific time point
delta = stationary_p(Gamma, 4)
# all periodically stationary distributions
Delta = stationary_p(Gamma)
Sparse version of stationary_p
Description
This is function computes the periodically stationary distribution of a Markov chain given a list of L sparse transition probability matrices.
Compatible with automatic differentiation by RTMB
Usage
stationary_p_sparse(Gamma, t = NULL)
Arguments
Gamma |
sist of length L containing sparse transition probability matrices for one cycle. |
t |
integer index of the time point in the cycle, for which to calculate the stationary distribution If t is not provided, the function calculates all stationary distributions for each time point in the cycle. |
Value
either the periodically stationary distribution at time t or all periodically stationary distributions.
Examples
## periodic HSMM example (here the approximating tpm is sparse)
N = 2 # number of states
L = 24 # cycle length
# time-varying mean dwell times
Z = cosinor(1:L, period = L) # trigonometric basis functions design matrix
beta = matrix(c(2, 2, 0.1, -0.1, -0.2, 0.2), nrow = 2)
Lambda = exp(cbind(1, Z) %*% t(beta))
sizes = c(20, 20) # approximating chain with 40 states
# state dwell-time distributions
dm = lapply(1:N, function(i) sapply(1:sizes[i]-1, dpois, lambda = Lambda[,i]))
omega = matrix(c(0,1,1,0), nrow = N, byrow = TRUE) # embedded t.p.m.
# calculating extended-state-space t.p.m.s
Gamma = tpm_phsmm(omega, dm)
# Periodically stationary distribution for specific time point
delta = stationary_p_sparse(Gamma, 4)
# All periodically stationary distributions
Delta = stationary_p_sparse(Gamma)
Sparse version of stationary
Description
This is function computes the stationary distribution of a Markov chain with a given sparse transition probability matrix.
Compatible with automatic differentiation by RTMB
Usage
stationary_sparse(Gamma)
Arguments
Gamma |
sparse transition probability matrix of dimension c(N,N) |
Value
stationary distribution of the Markov chain with the given transition probability matrix
Examples
## HSMM example (here the approximating tpm is sparse)
# building the t.p.m. of the embedded Markov chain
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE)
# defining state aggregate sizes
sizes = c(20, 30)
# defining state dwell-time distributions
lambda = c(5, 11)
dm = list(dpois(1:sizes[1]-1, lambda[1]), dpois(1:sizes[2]-1, lambda[2]))
# calculating extended-state-space t.p.m.
Gamma = tpm_hsmm(omega, dm)
delta = stationary_sparse(Gamma)
Summary of a LaMaModel object
Description
Summarises a model from lama or qreml.
Besides the overview of print(), this contains
for a homogeneous state process (or one per track) with at most 10 states: the transition probability matrix (or generator matrix
Qin continuous time, if reported, e.g. bytpm_ct), its stationary distribution and mean dwell times, averaged over tracks if there is one per track,for a periodic state process: the stationary distribution averaged over the cycle, i.e. the long-run proportion of time spent in each state,
the quantities reported by the likelihood function via
REPORT(): numeric vectors of length equal to the number of states are shown as one table with a column per state, other small objects separately, and large ones only by name,log-likelihood, AIC, BIC and the maximum gradient component at the estimate.
Usage
## S3 method for class 'LaMaModel'
summary(object, ...)
## S3 method for class 'summary.LaMaModel'
print(x, digits = max(3, getOption("digits") - 3), ...)
Arguments
object |
model object of class |
... |
additional arguments (not used) |
x |
object of class |
digits |
number of significant digits to print |
Value
summary() returns an object of class "summary.LaMaModel", a list containing the quantities shown,
e.g. Gamma, stationary, dwell and bystate. print() returns x invisibly.
Summary of a qremlModel object
Description
Summarises a model from qreml: the summary of summary.LaMaModel,
plus the effective degrees of freedom and smoothing parameters of the smooth terms and diagnostics of the smoothness selection.
Usage
## S3 method for class 'qremlModel'
summary(object, ...)
## S3 method for class 'summary.qremlModel'
print(x, digits = max(3, getOption("digits") - 3), ...)
Arguments
object |
model object of class |
... |
additional arguments (not used) |
x |
object of class |
digits |
number of significant digits to print |
Value
summary() returns an object of class "summary.qremlModel",
extending "summary.LaMaModel" by edf, lambda and selection. print() returns x invisibly.
Build the transition probability matrix from unconstrained parameter vector
Description
Markov chains are parametrised in terms of a transition probability matrix \Gamma, for which each row contains a conditional probability distribution of the next state given the current state.
Hence, each row has entries between 0 and 1 that need to sum to one.
For numerical optimisation, we parameterise in terms of unconstrained parameters, thus this function computes said matrix from an unconstrained parameter vector via the inverse multinomial logistic link (also known as softmax) applied to each row.
Usage
tpm(
beta,
Z = NULL,
Eta = NULL,
byrow = FALSE,
ref = NULL,
ad = NULL,
report = TRUE,
param = NULL
)
Arguments
beta |
parameters; either
|
Z |
optional covariate design matrix with or without intercept column, i.e. of dimension |
Eta |
optional pre-calculated matrix of linear predictors of dimension |
byrow |
logical indicating if each transition probability matrix should be filled by row.
Defaults to |
ref |
optional integer vector of length |
ad |
logical; whether to use automatic differentiation. Determined automatically — for debugging only. |
report |
logical; if |
param |
depricated, please use argument |
Value
Transition probability matrix of dimension c(nStates, nStates) or array of such matrices of dimension c(nStates, nStates, nObs) if Z or Eta is provided.
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm_ct(),
tpm_emb(),
tpm_emb_g(),
tpm_g(),
tpm_g2(),
tpm_p()
Examples
## homogeneous Markov chain
# 2 states: 2 = 2*(2-1) free off-diagonal elements
par <- rep(-2, 2)
Gamma <- tpm(par)
# 3 states: 6 = 3*(3-1) free off-diagonal elements
par <- rep(-3, 6)
Gamma <- tpm(par)
# 4 states: 12 = 4*(4-1) free off-diagonal elements
par <- rep(-4, 12)
Gamma <- tpm(par)
## inhomogeneous Markov chain
# t.p.m. depends on covariates
z1 <- runif(100); z2 <- runif(100) # 2 covariates
Z <- cbind(1, z1, z2) # design matrix
beta0 <- c(-2, -2); beta1 = c(1, -2); beta2 = c(2, -1) # coefficients for intercept and covariates
beta <- cbind(beta0, beta1, beta2) # coefficient matrix; with intercepts!
Gamma <- tpm(beta, Z) # array with 100 slices
Calculate continuous time transition probabilities
Description
A continuous-time Markov chain is described by an infinitesimal generator matrix Q.
When observing data at time points t_1, \dots, t_n the transition probabilites between t_i and t_{i+1} are caluclated as
\Gamma(\Delta t_i) = \exp(Q \Delta t_i),
where \exp() is the matrix exponential. The mapping \Gamma(\Delta t) is also called the Markov semigroup.
This function calculates all transition matrices based on a given generator and time differences.
Usage
tpm_ct(Q, timediff, rates = NULL, ad = NULL, report = TRUE)
tpm_cont(Q, timediff, rates = NULL, ad = NULL, report = TRUE)
Arguments
Q |
infinitesimal generator matrix of the continuous-time Markov chain of dimension |
timediff |
time differences between observations of length |
rates |
optional vector of state-dependent rates for MM(M)PP fitting.
For the MM(M)PP likelihood, the matrices needed in the forward algorithm are |
ad |
optional logical, indicating whether automatic differentiation with |
report |
logical, indicating whether |
Value
array of continuous-time transition matrices of dimension c(nStates, nStates, nObs-1)
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm(),
tpm_emb(),
tpm_emb_g(),
tpm_g(),
tpm_g2(),
tpm_p()
Examples
# building a Q matrix for a 3-state cont.-time Markov chain
Q = generator(rep(-2, 6))
# draw random time differences
timediff = rexp(100, 10)
# compute all transition matrices
Gamma = tpm_cont(Q, timediff)
Build the embedded transition probability matrix of an HSMM from unconstrained parameter vector
Description
Hidden semi-Markov models are defined in terms of state durations and an embedded transition probability matrix that contains the conditional transition probabilities given that the current state is left. This matrix necessarily has diagonal entries all equal to zero as self-transitions are impossible.
This function builds such an embedded/ conditional transition probability matrix from an unconstrained parameter vector. For each row of the matrix, the inverse multinomial logistic link is applied.
For a matrix of dimension c(nStates, nStates), the number of free off-diagonal elements is nStates * (nStates-2), hence also the length of param.
This means, for 2 states, the function needs to be called without any arguments, for 3-states with a vector of length 3, for 4 states with a vector of length 8, etc.
Compatible with automatic differentiation by RTMB
Usage
tpm_emb(param = NULL)
Arguments
param |
unconstrained parameter vector of length If the function is called without |
Value
embedded/ conditional transition probability matrix of dimension c(nStates, nStates)
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm(),
tpm_ct(),
tpm_emb_g(),
tpm_g(),
tpm_g2(),
tpm_p()
Examples
# 2 states: no free off-diagonal elements
omega = tpm_emb()
# 3 states: 3 free off-diagonal elements
param = rep(0, 3)
omega = tpm_emb(param)
# 4 states: 8 free off-diagonal elements
param = rep(0, 8)
omega = tpm_emb(param)
Build all embedded transition probability matrices of an inhomogeneous HSMM
Description
Hidden semi-Markov models are defined in terms of state durations and an embedded transition probability matrix that contains the conditional transition probabilities given that the current state is left. This matrix necessarily has diagonal entries all equal to zero as self-transitions are impossible. We can allow this matrix to vary with covariates, which is the purpose of this function.
It builds all embedded/ conditional transition probability matrices based on a design and parameter matrix. For each row of the matrix, the inverse multinomial logistic link is applied.
For a matrix of dimension c(nStates, nStates), the number of free off-diagonal elements is nStates * (nStates-2) which determines the number of rows of the parameter matrix.
Compatible with automatic differentiation by RTMB
Usage
tpm_emb_g(Z, beta, report = TRUE)
Arguments
Z |
covariate design matrix with or without intercept column, i.e. of dimension If |
beta |
matrix of coefficients for the off-diagonal elements of the embedded transition probability matrix Needs to be of dimension |
report |
logical, indicating whether the coefficient matrix beta should be reported from the fitted model. Defaults to |
Value
array of embedded/ conditional transition probability matrices of dimension c(nStates, nStates, nObs)
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm(),
tpm_ct(),
tpm_emb(),
tpm_g(),
tpm_g2(),
tpm_p()
Examples
## parameter matrix for 3-state HSMM
beta = matrix(c(rep(0, 3), -0.2, 0.2, 0.1), nrow = 3)
# no intercept
Z = rnorm(100)
omega = tpm_emb_g(Z, beta)
# intercept
Z = cbind(1, Z)
omega = tpm_emb_g(Z, beta)
Build all transition probability matrices of an inhomogeneous HMM
Description
In an HMM, we often model the influence of covariates on the state process by linking them to the transition probabiltiy matrix. Most commonly, this is done by specifying a linear predictor
\eta_{ij}^{(t)} = \beta^{(ij)}_0 + \beta^{(ij)}_1 z_{t1} + \dots + \beta^{(ij)}_p z_{tp}
for each off-diagonal element (i \neq j) of the transition probability matrix and then applying the inverse multinomial logistic link (also known as softmax) to each row.
This function efficiently calculates all transition probabilty matrices for a given design matrix Z and parameter matrix beta.
Usage
tpm_g(Z, beta, Eta = NULL, byrow = FALSE, ref = NULL, ad = NULL, report = TRUE)
Arguments
Z |
Covariate design matrix with or without intercept column, i.e. of dimension |
beta |
Matrix of coefficients for the off-diagonal elements of the transition probability matrix
of dimension |
Eta |
optional pre-calculated matrix of linear predictors of dimension |
byrow |
logical indicating if each transition probability matrix should be filled by row.
Defaults to |
ref |
optional integer vector of length |
ad |
logical; whether to use automatic differentiation. Determined automatically — for debugging only. |
report |
logical; if |
Details
Deprecated: please use tpm(beta, Z) for all model types instead.
Value
array of transition probability matrices of dimension c(nStates, nStates, nObs)
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm(),
tpm_ct(),
tpm_emb(),
tpm_emb_g(),
tpm_g2(),
tpm_p()
Examples
## inhomogeneous Markov chain
# t.p.m. depends on covariates
z1 <- runif(100); z2 <- runif(100) # 2 covariates
Z <- cbind(1, z1, z2) # design matrix
beta0 <- c(-2, -2); beta1 = c(1, -2); beta2 = c(2, -1) # coefficients for intercept and covariates
beta <- cbind(beta0, beta1, beta2) # coefficient matrix; with intercepts!
#' Gamma <- tpm(beta, Z) # array with 100 slices
Build all transition probability matrices of an inhomogeneous HMM
Description
In an HMM, we often model the influence of covariates on the state process by linking them to the transition probabiltiy matrix. Most commonly, this is done by specifying linear predictors
\eta_{ij}^{(t)} = \beta^{(ij)}_0 + \beta^{(ij)}_1 z_{t1} + \dots + \beta^{(ij)}_p z_{tp}
for each off-diagonal element (i \neq j) of the transition probability matrix and then applying the inverse multinomial logistic link (also known as softmax) to each row.
This function efficiently calculates all transition probabilty matrices for a given design matrix Z and parameter matrix beta.
Usage
tpm_g2(Z, beta, byrow = FALSE, ad = NULL, report = TRUE, ref = NULL)
Arguments
Z |
covariate design matrix with or without intercept column, i.e. of dimension c(n, p) or c(n, p+1) If Can also be a list of N*(N-1) design matrices with different number of columns but the same number of rows. In that case, no intercept column will be added. |
beta |
matrix of coefficients for the off-diagonal elements of the transition probability matrix Needs to be of dimension c(N*(N-1), p+1), where the first column contains the intercepts. If |
byrow |
logical indicating if each transition probability matrix should be filled by row Defaults to |
ad |
optional logical, indicating whether automatic differentiation with |
report |
logical, indicating whether the coefficient matrix |
ref |
optional vector of length N with the reference state indices for each column of the transition probability matrix. Each row in the transition matrix corresponds to a multinomial regression, hence one state needs to be the reference category. Defaults to off-diagonal elements ( |
Value
array of transition probability matrices of dimension c(N,N,n)
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm(),
tpm_ct(),
tpm_emb(),
tpm_emb_g(),
tpm_g(),
tpm_p()
Examples
Z = matrix(runif(200), ncol = 2)
beta = matrix(c(-1, 1, 2, -2, 1, -2), nrow = 2, byrow = TRUE)
Gamma = tpm_g(Z, beta)
Builds the transition probability matrix of an HSMM-approximating HMM
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs, where the state duration distribution is explicitly modelled.
For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function computes the transition matrix to approximate a given HSMM by an HMM with a larger state space.
Usage
tpm_hsmm(omega, dm, Fm = NULL, sparse = TRUE, eps = 1e-10)
Arguments
omega |
embedded transition probability matrix of dimension |
dm |
state dwell-time distributions arranged in a list of length |
Fm |
optional list of length |
sparse |
logical, indicating whether the output should be a sparse matrix. Defaults to |
eps |
rounding value: If an entry of the transition probabily matrix is smaller, than it is rounded to zero. Usually, this should not be changed. |
Value
extended-state-space transition probability matrix of the approximating HMM
Examples
# building the t.p.m. of the embedded Markov chain
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE)
# defining state aggregate sizes
sizes = c(20, 30)
# defining state dwell-time distributions
lambda = c(5, 11)
dm = list(dpois(1:sizes[1]-1, lambda[1]), dpois(1:sizes[2]-1, lambda[2]))
# calculating extended-state-space t.p.m.
Gamma = tpm_hsmm(omega, dm)
Build the transition probability matrix of an HSMM-approximating HMM
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs.
For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function computes the transition matrix of an HSMM.
Usage
tpm_hsmm2(omega, dm, eps = 1e-10)
Arguments
omega |
embedded transition probability matrix of dimension c(N,N) |
dm |
state dwell-time distributions arranged in a list of length(N). Each list element needs to be a vector of length N_i, where N_i is the state aggregate size. |
eps |
rounding value: If an entry of the transition probabily matrix is smaller, than it is rounded to zero. |
Value
extended-state-space transition probability matrix of the approximating HMM
Examples
# building the t.p.m. of the embedded Markov chain
omega = matrix(c(0,1,1,0), nrow = 2, byrow = TRUE)
# defining state aggregate sizes
sizes = c(20, 30)
# defining state dwell-time distributions
lambda = c(5, 11)
dm = list(dpois(1:sizes[1]-1, lambda[1]), dpois(1:sizes[2]-1, lambda[2]))
# calculating extended-state-space t.p.m.
Gamma = tpm_hsmm(omega, dm)
Builds all transition probability matrices of an inhomogeneous-HSMM-approximating HMM
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs. For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function computes the transition matrices of a periodically inhomogeneos HSMMs.
Usage
tpm_ihsmm(omega, dm, eps = 1e-10)
Arguments
omega |
embedded transition probability matrix Either a matrix of dimension |
dm |
state dwell-time distributions arranged in a list of length Each list element needs to be a matrix of dimension c(n, N_i), where each row t is the (approximate) probability mass function of state i at time t. |
eps |
rounding value: If an entry of the transition probabily matrix is smaller, than it is rounded to zero. Usually, this should not be changed. |
Value
list of dimension length n - max(sapply(dm, ncol)), containing sparse extended-state-space transition probability matrices for each time point (except the first max(sapply(dm, ncol)) - 1).
Examples
N = 2
# time-varying mean dwell times
n = 100
z = runif(n)
beta = matrix(c(2, 2, 0.1, -0.1), nrow = 2)
Lambda = exp(cbind(1, z) %*% t(beta))
sizes = c(15, 15) # approximating chain with 30 states
# state dwell-time distributions
dm = lapply(1:N, function(i) sapply(1:sizes[i]-1, dpois, lambda = Lambda[,i]))
## homogeneous conditional transition probabilites
# diagonal elements are zero, rowsums are one
omega = matrix(c(0,1,1,0), nrow = N, byrow = TRUE)
# calculating extended-state-space t.p.m.s
Gamma = tpm_ihsmm(omega, dm)
## inhomogeneous conditional transition probabilites
# omega can be an array
omega = array(omega, dim = c(N,N,n))
# calculating extended-state-space t.p.m.s
Gamma = tpm_ihsmm(omega, dm)
Build all transition probability matrices of a periodically inhomogeneous HMM
Description
Given a periodically varying variable such as time of day or day of year and the associated cycle length, this function calculates the transition probability matrices by applying the inverse multinomial logistic link (also known as softmax) to linear predictors of the form
\eta^{(t)}_{ij} = \beta_0^{(ij)} + \sum_{k=1}^K \bigl( \beta_{1k}^{(ij)} \sin(\frac{2 \pi k t}{L}) + \beta_{2k}^{(ij)} \cos(\frac{2 \pi k t}{L}) \bigr)
for the off-diagonal elements (i \neq j) of the transition probability matrix.
This is relevant for modeling e.g. diurnal variation and the flexibility can be increased by adding smaller frequencies (i.e. increasing K).
Usage
tpm_p(
tod = 1:24,
L = 24,
beta,
degree = 1,
Z = NULL,
byrow = FALSE,
ad = NULL,
report = TRUE
)
Arguments
tod |
equidistant sequence of a cyclic variable For time of day and e.g. half-hourly data, this could be 1, ..., L and L = 48, or 0.5, 1, 1.5, ..., 24 and L = 24. |
L |
length of one full cycle, on the scale of tod |
beta |
matrix of coefficients for the off-diagonal elements of the transition probability matrix Needs to be of dimension |
degree |
degree of the trigonometric link function For each additional degree, one sine and one cosine frequency are added. |
Z |
pre-calculated design matrix (excluding intercept column) Defaults to |
byrow |
logical indicating if each transition probability matrix should be filled by row Defaults to |
ad |
optional logical, indicating whether automatic differentiation with RTMB should be used. By default, the function determines this itself. |
report |
logical, indicating whether the coefficient matrix |
Details
Note that using this function inside the negative log-likelihood function is convenient, but it performs the basis expansion into sine and cosine terms each time it is called.
As these do not change during the optimisation, using tpm_g with a pre-calculated (by trigBasisExp) design matrix would be more efficient.
Value
array of transition probability matrices of dimension c(nStates, nStates, length(tod))
See Also
Other transition probability matrix functions:
generator(),
generator_g(),
tpm(),
tpm_ct(),
tpm_emb(),
tpm_emb_g(),
tpm_g(),
tpm_g2()
Examples
# hourly data
tod = seq(1, 24, by = 1)
L = 24
beta = matrix(c(-1, 2, -1, -2, 1, -1), nrow = 2, byrow = TRUE)
Gamma = tpm_p(tod, L, beta, degree = 1)
# half-hourly data
## integer tod sequence
tod = seq(1, 48, by = 1)
L = 48
beta = matrix(c(-1, 2, -1, -2, 1, -1), nrow = 2, byrow = TRUE)
Gamma1 = tpm_p(tod, L, beta, degree = 1)
## equivalent specification
tod = seq(0.5, 24, by = 0.5)
L = 24
beta = matrix(c(-1, 2, -1, -2, 1, -1), nrow = 2, byrow = TRUE)
Gamma2 = tpm_p(tod, L, beta, degree = 1)
all(Gamma1 == Gamma2) # same result
Builds all transition probability matrices of an periodic-HSMM-approximating HMM
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs. For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function computes the transition matrices of a periodically inhomogeneos HSMMs.
Usage
tpm_phsmm(omega, dm, eps = 1e-10)
Arguments
omega |
embedded transition probability matrix Either a matrix of dimension |
dm |
state dwell-time distributions arranged in a list of length Each list element needs to be a matrix of dimension c(L, N_i), where each row t is the (approximate) probability mass function of state i at time t. |
eps |
rounding value: If an entry of the transition probabily matrix is smaller, than it is rounded to zero. Usually, this should not be changed. |
Value
list of dimension length L, containing sparse extended-state-space transition probability matrices of the approximating HMM for each time point of the cycle.
Examples
N = 2 # number of states
L = 24 # cycle length
# time-varying mean dwell times
Z = cosinor(1:L, period = L) # trigonometric basis functions design matrix
beta = matrix(c(2, 2, 0.1, -0.1, -0.2, 0.2), nrow = 2)
Lambda = exp(cbind(1, Z) %*% t(beta))
sizes = c(20, 20) # approximating chain with 40 states
# state dwell-time distributions
dm = lapply(1:N, function(i) sapply(1:sizes[i]-1, dpois, lambda = Lambda[,i]))
## homogeneous conditional transition probabilites
# diagonal elements are zero, rowsums are one
omega = matrix(c(0,1,1,0), nrow = N, byrow = TRUE)
# calculating extended-state-space t.p.m.s
Gamma = tpm_phsmm(omega, dm)
## inhomogeneous conditional transition probabilites
# omega can be an array
omega = array(omega, dim = c(N,N,L))
# calculating extended-state-space t.p.m.s
Gamma = tpm_phsmm(omega, dm)
Build all transition probability matrices of an periodic-HSMM-approximating HMM
Description
Hidden semi-Markov models (HSMMs) are a flexible extension of HMMs. For direct numerical maximum likelhood estimation, HSMMs can be represented as HMMs on an enlarged state space (of size M) and with structured transition probabilities.
This function computes the transition matrices of a periodically inhomogeneos HSMMs.
Usage
tpm_phsmm2(omega, dm, eps = 1e-10)
Arguments
omega |
embedded transition probability matrix Either a matrix of dimension c(N,N) for homogeneous conditional transition probabilities, or an array of dimension c(N,N,L) for inhomogeneous conditional transition probabilities. |
dm |
state dwell-time distributions arranged in a list of length(N) Each list element needs to be a matrix of dimension c(L, N_i), where each row t is the (approximate) probability mass function of state i at time t. |
eps |
rounding value: If an entry of the transition probabily matrix is smaller, than it is rounded to zero. |
Value
array of dimension c(N,N,L), containing the extended-state-space transition probability matrices of the approximating HMM for each time point of the cycle.
Examples
N = 3
L = 24
# time-varying mean dwell times
Lambda = exp(matrix(rnorm(L*N, 2, 0.5), nrow = L))
sizes = c(25, 25, 25) # approximating chain with 75 states
# state dwell-time distributions
dm = list()
for(i in 1:3){
dmi = matrix(nrow = L, ncol = sizes[i])
for(t in 1:L){
dmi[t,] = dpois(1:sizes[i]-1, Lambda[t,i])
}
dm[[i]] = dmi
}
## homogeneous conditional transition probabilites
# diagonal elements are zero, rowsums are one
omega = matrix(c(0,0.5,0.5,0.2,0,0.8,0.7,0.3,0), nrow = N, byrow = TRUE)
# calculating extended-state-space t.p.m.s
Gamma = tpm_phsmm(omega, dm)
## inhomogeneous conditional transition probabilites
# omega can be an array
omega = array(rep(omega,L), dim = c(N,N,L))
omega[1,,4] = c(0, 0.2, 0.8) # small change for inhomogeneity
# calculating extended-state-space t.p.m.s
Gamma = tpm_phsmm(omega, dm)
Compute the transition probability matrix of a thinned periodically inhomogeneous Markov chain.
Description
If the transition probability matrix of an inhomogeneous Markov chain varies only periodically (with period length L), it converges to a so-called periodically stationary distribution.
This happens, because the thinned Markov chain, which has a full cycle as each time step, has homogeneous transition probability matrix
\Gamma_t = \Gamma^{(t)} \Gamma^{(t+1)} \dots \Gamma^{(t+L-1)}
for all t = 1, \dots, L.
This function calculates the matrix above efficiently as a preliminery step to calculating the periodically stationary distribution.
Usage
tpm_thinned(Gamma, t)
Arguments
Gamma |
array of transition probability matrices of dimension |
t |
integer index of the time point in the cycle, for which to calculate the thinned transition probility matrix |
Value
thinned transition probabilty matrix of dimension c(nStates, nStates)
Examples
# setting parameters for trigonometric link
beta = matrix(c(-1, -2, 2, -1, 2, -4), nrow = 2, byrow = TRUE)
# calculating periodically varying t.p.m. array (of length 24 here)
Gamma = tpm_p(beta = beta)
# calculating t.p.m. of thinned Markov chain
tpm_thinned(Gamma, 4)
T-Rex Movement Data
Description
Hourly step lengths and turning angles of a Tyrannosaurus rex, living 66 million years ago.
Usage
trex
Format
A data frame with 10.000 rows and 4 variables:
- tod
time of day variable ranging from 1 to 24
- step
hourly step lengths in kilometres
- angle
hourly turning angles in radians
- state
hidden state variable
Source
Generated for example purposes.
Compute the design matrix for a trigonometric basis expansion
Description
Given a periodically varying variable such as time of day or day of year and the associated cycle length, this function performs a basis expansion to efficiently calculate a linear predictor of the form
\eta^{(t)} = \beta_0 + \sum_{k=1}^K \bigl( \beta_{1k} \sin(\frac{2 \pi k t}{L}) + \beta_{2k} \cos(\frac{2 \pi k t}{L}) \bigr).
This is relevant for modeling e.g. diurnal variation and the flexibility can be increased by adding smaller frequencies (i.e. increasing K).
Usage
trigBasisExp(tod, L = 24, degree = 1)
Arguments
tod |
equidistant sequence of a cyclic variable For time of day and e.g. half-hourly data, this could be 1, ..., L and L = 48, or 0.5, 1, 1.5, ..., 24 and L = 24. |
L |
length of one cycle on the scale of the time variable. For time of day, this would be 24. |
degree |
degree K of the trigonometric link above. Increasing K increases the flexibility. |
Value
design matrix (without intercept column), ordered as sin1, cos1, sin2, cos2, ...
Examples
# no examples
Viterbi algorithm for state decoding in HMMs
Description
The Viterbi algorithm decodes the most probable state sequence of an HMM.
Usage
viterbi(delta, Gamma, allprobs, trackID = NULL, mod = NULL, tod = NULL)
Arguments
delta |
initial distribution; either
|
Gamma |
transition probability matrix; either
|
allprobs |
matrix of state-dependent probabilities or density values of dimension |
trackID |
optional vector of length |
mod |
optional model object containing |
tod |
optional integer vector of length |
Value
vector of decoded states of length nObs
See Also
Other decoding functions:
stateprobs(),
stateprobs_g(),
stateprobs_p(),
viterbi_g(),
viterbi_p()
Examples
delta = c(0.5, 0.5)
Gamma = matrix(c(0.9, 0.1, 0.2, 0.8), nrow = 2, byrow = TRUE)
allprobs = matrix(runif(200), nrow = 100, ncol = 2)
states = viterbi(delta, Gamma, allprobs)
Viterbi algorithm for state decoding in inhomogeneous HMMs
Description
The Viterbi algorithm decodes the most probable state sequence of an HMM.
Usage
viterbi_g(delta, Gamma, allprobs, trackID = NULL, mod = NULL)
Arguments
delta |
initial distribution; either
|
Gamma |
array of transition probability matrices of dimension |
allprobs |
matrix of state-dependent probabilities or density values of dimension |
trackID |
optional vector of length |
mod |
optional model object containing |
Details
Deprecated: please use viterbi for all model types instead.
Value
vector of decoded states of length nObs
See Also
Other decoding functions:
stateprobs(),
stateprobs_g(),
stateprobs_p(),
viterbi(),
viterbi_p()
Examples
delta = c(0.5, 0.5)
Gamma = tpm_g(runif(10), matrix(c(-2,-2,1,-1), nrow = 2))
allprobs = matrix(runif(20), nrow = 10, ncol = 2)
states = viterbi_g(delta, Gamma[,,-1], allprobs)
Viterbi algorithm for state decoding in periodically inhomogeneous HMMs
Description
The Viterbi algorithm allows one to decode the most probable state sequence of an HMM.
Usage
viterbi_p(delta, Gamma, allprobs, tod, trackID = NULL, mod = NULL)
Arguments
delta |
initial distribution of length N, or matrix of dimension c(k,N) for k independent tracks, if This could e.g. be the periodically stationary distribution (for each track). |
Gamma |
array of transition probability matrices for each time point in the cycle of dimension c(N,N,L), where L is the length of the cycle |
allprobs |
matrix of state-dependent probabilities/ density values of dimension c(n, N) |
tod |
(Integer valued) variable for cycle indexing in 1, ..., L, mapping the data index to a generalised time of day (length n) For half-hourly data L = 48. It could, however, also be day of year for daily data and L = 365. |
trackID |
optional vector of k track IDs, if multiple tracks need to be decoded separately. The observations of each track need to be consecutive. |
mod |
optional model object containing initial distribution If you are using automatic differentiation either with |
Details
Deprecated: please use viterbi with argument tod instead.
Value
vector of decoded states of length n
See Also
Other decoding functions:
stateprobs(),
stateprobs_g(),
stateprobs_p(),
viterbi(),
viterbi_g()
Examples
delta = c(0.5, 0.5)
beta = matrix(c(-2, 1, -1,
-2, -1, 1), nrow = 2, byrow = TRUE)
Gamma = tpm_p(1:24, 24, beta)
tod = rep(1:24, 5)
n = length(tod)
allprobs = matrix(runif(2*n), nrow = n, ncol = 2)
states = viterbi_p(delta, Gamma, allprobs, tod)
Von Mises distribution
Description
Density, distribution function and random generation for the von Mises distribution.
Usage
dvm(x, mu = 0, kappa = 1, log = FALSE)
pvm(q, mu = 0, kappa = 1, from = NULL, tol = 1e-20)
rvm(n, mu = 0, kappa = 1, wrap = TRUE)
Arguments
x, q |
vector of angles measured in radians at which to evaluate the density function. |
mu |
mean direction of the distribution measured in radians. |
kappa |
non-negative numeric value for the concentration parameter of the distribution. |
log |
logical; if |
from |
value from which the integration for CDF starts. If |
tol |
the precision in evaluating the distribution function |
n |
number of observations. If |
wrap |
logical; if |
Details
This implementation of dvm allows for automatic differentiation with RTMB.
rvm and pvm are simply wrappers of the corresponding functions from circular.
Value
dvm gives the density, pvm gives the distribution function, and rvm generates random deviates.
Examples
set.seed(1)
x = rvm(10, 0, 1)
d = dvm(x, 0, 1)
p = pvm(x, 0, 1)
Wrapped Cauchy distribution
Description
Density and random generation for the wrapped Cauchy distribution.
Usage
dwrpcauchy(x, mu = 0, rho, log = FALSE)
rwrpcauchy(n, mu = 0, rho, wrap = TRUE)
Arguments
x |
vector of angles measured in radians at which to evaluate the density function. |
mu |
mean direction of the distribution measured in radians. |
rho |
concentration parameter of the distribution, must be in the interval from 0 to 1. |
log |
logical; if |
n |
number of observations. If |
wrap |
logical; if |
Details
This implementation of dwrpcauchy allows for automatic differentiation with RTMB.
rwrpcauchy is simply a wrapper for rwrappedcauchy imported from circular.
Value
dwrpcauchy gives the density and rwrpcauchy generates random deviates.
Examples
set.seed(1)
x = rwrpcauchy(10, 0, 0.3)
d = dwrpcauchy(x, 0, 0.3)
Zero-inflated density constructer
Description
Constructs a zero-inflated density function from a given probability density function
Usage
zero_inflate(dist, discrete = NULL)
Arguments
dist |
either a probability density function or a probability mass function |
discrete |
logical; if |
Details
The definition of zero-inflation is different for discrete and continuous distributions.
For discrete distributions with p.m.f. f and zero-inflation probability p, we have
\Pr(X = 0) = p + (1 - p) \cdot f(0),
and
\Pr(X = x) = (1 - p) \cdot f(x), \quad x > 0.
For continuous distributions with p.d.f. f, we have
f_{\text{zinfl}}(x) = p \cdot \delta_0(x) + (1 - p) \cdot f(x),
where \delta_0 is the Dirac delta function at zero.
Value
zero-inflated density function with first argument x, second argument zeroprob, and additional arguments ... that will be passed to dist.
Examples
dzinorm <- zero_inflate(dnorm)
dzinorm(c(NA, 0, 2), 0.5, mean = 1, sd = 1)
zipois <- zero_inflate(dpois)
zipois(c(NA, 0, 1), 0.5, 1)