View source: R/halfnorm.like.R
halfnorm.like | R Documentation |
This function computes the likelihood contributions for sighting distances, scaled appropriately, for use as a distance likelihood.
halfnorm.like(
a,
dist,
covars = NULL,
w.lo = units::set_units(0, "m"),
w.hi = max(dist),
series = "cosine",
expansions = 0,
scale = TRUE,
pointSurvey = FALSE
)
a |
A vector of likelihood parameter values. Length and
meaning depend on |
dist |
A numeric vector containing the observed distances. |
covars |
Data frame containing values of covariates at
each observation in |
w.lo |
Scalar value of the lowest observable distance.
This is the left truncation of sighting distances
in |
w.hi |
Scalar value of the largest observable distance.
This is the right truncation of sighting distances
in |
series |
A string specifying the type of expansion to use.
Currently, valid values are 'simple', 'hermite', and 'cosine'; but, see
|
expansions |
A scalar specifying the number of terms
in |
scale |
Logical scalar indicating whether or not to
scale the likelihood so it integrates to 1. This parameter is
used to stop recursion in other functions. If |
pointSurvey |
Boolean. TRUE if distances in |
The half-normal likelihood is
f(x|a) = \exp(-x^2 / (2*a^2))
where a
is the parameter to be estimated.
Some half-normal distance functions in the literature
do not use a "2" in the
denominator of the exponent. Rdistance
uses a
"2" in the denominator of the exponent to make quantiles of this
function agree with
the standard normal which means a can be interpreted as a
normal standard error. e.g., approximately 95% of all observations
will occur between 0 and 2a.
Expansion Terms: If expansions
= k (k > 0), the expansion function specified by series
is called (see for example
cosine.expansion
). Assuming h_{ij}(x)
is the j^{th}
expansion term for the i^{th}
distance and that
c_1, c_2, \dots, c_k
are (estimated) coefficients for the expansion terms, the likelihood contribution for the i^{th}
distance is,
f(x|a,b,c_1,c_2,\dots,c_k) = f(x|a,b)(1 + \sum_{j=1}^{k} c_j h_{ij}(x)).
f(x|a,b,c_1,c_2,...,c_k) = f(x|a,b)(1 + c(1) h_i1(x) + c(2) h_i2(x) + ... + c(k) h_ik(x)).
A numeric vector the same length and order as dist
containing the
likelihood contribution for corresponding distances in dist
.
Assuming L
is the returned vector from one of these functions,
the negative log likelihood of all the data is -sum(log(L), na.rm=T)
.
Note that the returned likelihood value for distances less
than w.lo
or greater than w.hi
is NA
,
hence na.rm=TRUE
in the sum.
If scale
= TRUE, the integral of the likelihood from
w.lo
to w.hi
is 1.0. If scale
= FALSE,
the integral of the likelihood is something else.
Values are always greater than or equal to zero.
dfuncEstim
,
hazrate.like
,
uniform.like
,
negexp.like
,
Gamma.like
## Not run:
set.seed(238642)
x <- seq(0, 100, length=100)
# Plots showing effects of changes in parameter Sigma
plot(x, halfnorm.like(20, x), type="l", col="red")
plot(x, halfnorm.like(40, x), type="l", col="blue")
# Estimate 'halfnorm' distance function
a <- 5
x <- rnorm(1000, mean=0, sd=a)
x <- x[x >= 0]
dfunc <- dfuncEstim(x~1, likelihood="halfnorm")
plot(dfunc)
# evaluate the log Likelihood
L <- halfnorm.like(dfunc$parameters, dfunc$detections$dist, covars=dfunc$covars,
w.lo=dfunc$w.lo, w.hi=dfunc$w.hi,
series=dfunc$series, expansions=dfunc$expansions,
scale=TRUE)
-sum(log(L), na.rm=TRUE) # the negative log likelihood
## End(Not run)
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