glm
is used to fit generalized linear models, specified by
giving a symbolic description of the linear predictor and a
description of the error distribution.glm(formula, family = gaussian, data, weights, subset,
na.action, start = NULL, etastart, mustart, offset,
control = list(…), model = TRUE, method = "glm.fit",
x = FALSE, y = TRUE, contrasts = NULL, …)glm.fit(x, y, weights = rep(1, nobs),
start = NULL, etastart = NULL, mustart = NULL,
offset = rep(0, nobs), family = gaussian(),
control = list(), intercept = TRUE)
# S3 method for glm
weights(object, type = c("prior", "working"), …)
"formula"
(or one that
can be coerced to that class): a symbolic description of the
model to be fitted. The details of model specification are given
under ‘Details’.glm
this can be a
character string naming a family function, a family function or the
result of a call to a family function. For glm.fit
only the
third option is supported. (See family
for details of
family functions.)as.data.frame
to a data frame) containing
the variables in the model. If not found in data
, the
variables are taken from environment(formula)
,
typically the environment from which glm
is called.NULL
or a numeric vector.NA
s. The default is set by
the na.action
setting of options
, and is
na.fail
if that is unset. The ‘factory-fresh’
default is na.omit
. Another possible value is
NULL
, no action. Value na.exclude
can be useful.NULL
or a numeric vector of length equal to
the number of cases. One or more offset
terms can be
included in the formula instead or as well, and if more than one is
specified their sum is used. See model.offset
.glm.fit
this is passed to
glm.control
."glm.fit"
uses iteratively reweighted least squares
(IWLS): the alternative "model.frame"
returns the model frame
and does no fitting. User-supplied fitting functions can be supplied either as a function
or a character string naming a function, with a function which takes
the same arguments as glm.fit
. If specified as a character
string it is looked up from within the stats namespace.
glm
:
logical values indicating whether the response vector and model
matrix used in the fitting process should be returned as components
of the returned value. For glm.fit
: x
is a design matrix of dimension
n * p
, and y
is a vector of observations of length
n
.
contrasts.arg
of model.matrix.default
."glm"
.glm
: arguments to be used to form the default
control
argument if it is not supplied directly. For weights
: further arguments passed to or from other methods.
glm
returns an object of class inheriting from "glm"
which inherits from the class "lm"
. See later in this section.
If a non-standard method
is used, the object will also inherit
from the class (if any) returned by that function. The function summary
(i.e., summary.glm
) can
be used to obtain or print a summary of the results and the function
anova
(i.e., anova.glm
)
to produce an analysis of variance table. The generic accessor functions coefficients
,
effects
, fitted.values
and residuals
can be used to
extract various useful features of the value returned by glm
. weights
extracts a vector of weights, one for each case in the
fit (after subsetting and na.action
). An object of class "glm"
is a list containing at least the
following components: NA
.family
object used.aic
component of the family.
For binomial and Poison families the dispersion is
fixed at one and the number of parameters is the number of
coefficients. For gaussian, Gamma and inverse gaussian families the
dispersion is estimated from the residual deviance, and the number
of parameters is the number of coefficients plus one. For a
gaussian family the MLE of the dispersion is used so this is a valid
value of AIC, but for Gamma and inverse gaussian families it is not.
For families fitted by quasi-likelihood the value is NA
.deviance
. The null model will include the offset, and an
intercept if there is one in the model. Note that this will be
incorrect if the link function depends on the data other than
through the fitted mean: specify a zero offset to force a correct
calculation.1
s if none were.y
vector
used. (It is a vector even for a binomial model.)terms
object used.data argument
.control
argument used."glm.fit"
.model.frame
on the special handling of NA
s.qr
, R
and effects
relating to the final weighted linear fit. Objects of class "glm"
are normally of class c("glm",
"lm")
, that is inherit from class "lm"
, and well-designed
methods for class "lm"
will be applied to the weighted linear
model at the final iteration of IWLS. However, care is needed, as
extractor functions for class "glm"
such as
residuals
and weights
do not just pick out
the component of the fit with the same name. If a binomial
glm
model was specified by giving a
two-column response, the weights returned by prior.weights
are
the total numbers of cases (factored by the supplied case weights) and
the component y
of the result is the proportion of successes.method
serves two purposes. One is to allow the
model frame to be recreated with no fitting. The other is to allow
the default fitting function glm.fit
to be replaced by a
function which takes the same arguments and uses a different fitting
algorithm. If glm.fit
is supplied as a character string it is
used to search for a function of that name, starting in the
stats namespace. The class of the object return by the fitter (if any) will be
prepended to the class returned by glm
.response ~ terms
where
response
is the (numeric) response vector and terms
is a
series of terms which specifies a linear predictor for
response
. For binomial
and quasibinomial
families the response can also be specified as a factor
(when the first level denotes failure and all others success) or as a
two-column matrix with the columns giving the numbers of successes and
failures. A terms specification of the form first + second
indicates all the terms in first
together with all the terms in
second
with any duplicates removed. A specification of the form first:second
indicates the set
of terms obtained by taking the interactions of all terms in
first
with all terms in second
. The specification
first*second
indicates the cross of first
and
second
. This is the same as first + second +
first:second
. The terms in the formula will be re-ordered so that main effects come
first, followed by the interactions, all second-order, all third-order
and so on: to avoid this pass a terms
object as the formula. Non-NULL
weights
can be used to indicate that different
observations have different dispersions (with the values in
weights
being inversely proportional to the dispersions); or
equivalently, when the elements of weights
are positive
integers \(w_i\), that each response \(y_i\) is the mean of
\(w_i\) unit-weight observations. For a binomial GLM prior weights
are used to give the number of trials when the response is the
proportion of successes: they would rarely be used for a Poisson GLM. glm.fit
is the workhorse function: it is not normally called
directly but can be more efficient where the response vector, design
matrix and family have already been calculated. If more than one of etastart
, start
and mustart
is specified, the first in the list will be used. It is often
advisable to supply starting values for a quasi
family,
and also for families with unusual links such as gaussian("log")
. All of weights
, subset
, offset
, etastart
and mustart
are evaluated in the same way as variables in
formula
, that is first in data
and then in the
environment of formula
. For the background to warning messages about ‘fitted probabilities
numerically 0 or 1 occurred’ for binomial GLMs, see Venables &
Ripley (2002, pp. 197--8).anova.glm
, summary.glm
, etc. for
glm
methods,
and the generic functions anova
, summary
,
effects
, fitted.values
,
and residuals
. lm
for non-generalized linear models (which SAS
calls GLMs, for ‘general’ linear models). loglin
and loglm
(package
https://CRAN.R-project.org/package=MASS) for fitting log-linear models (which binomial and
Poisson GLMs are) to contingency tables. bigglm
in package https://CRAN.R-project.org/package=biglm for an alternative
way to fit GLMs to large datasets (especially those with many cases). esoph
, infert
and
predict.glm
have examples of fitting binomial glms.## Dobson (1990) Page 93: Randomized Controlled Trial :
counts <- c(18,17,15,20,10,20,25,13,12)
outcome <- gl(3,1,9)
treatment <- gl(3,3)
print(d.AD <- data.frame(treatment, outcome, counts))
glm.D93 <- glm(counts ~ outcome + treatment, family = poisson())
anova(glm.D93)
summary(glm.D93)
## an example with offsets from Venables & Ripley (2002, p.189)
utils::data(anorexia, package = "MASS")
anorex.1 <- glm(Postwt ~ Prewt + Treat + offset(Prewt),
family = gaussian, data = anorexia)
summary(anorex.1)
# A Gamma example, from McCullagh & Nelder (1989, pp. 300-2)
clotting <- data.frame(
u = c(5,10,15,20,30,40,60,80,100),
lot1 = c(118,58,42,35,27,25,21,19,18),
lot2 = c(69,35,26,21,18,16,13,12,12))
summary(glm(lot1 ~ log(u), data = clotting, family = Gamma))
summary(glm(lot2 ~ log(u), data = clotting, family = Gamma))
## Not run: ------------------------------------
# ## for an example of the use of a terms object as a formula
# demo(glm.vr)
## ---------------------------------------------
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