Returns an object of class "gamlss", which is a generalized additive model for location scale and shape (GAMLSS).
The function gamlss()
is very similar to the gam()
function in S-plus (now also in R in package gam
), but
can fit more distributions (not only the ones belonging to the exponential family) and can model all the parameters of the
distribution as functions of the explanatory variables (e.g. using linear, non-linear, smoothing, loess
and random effects terms).
This implementation of gamlss()
allows modelling of up to four
parameters in a distribution family, which are conventionally called mu
, sigma
, nu
and tau
.
The function gamlssNews()
shows what is new in the current implementation.
gamlss(formula = formula(data), sigma.formula = ~1,
nu.formula = ~1, tau.formula = ~1, family = NO(),
data, weights = NULL,
contrasts = NULL, method = RS(), start.from = NULL,
mu.start = NULL, sigma.start = NULL,
nu.start = NULL, tau.start = NULL,
mu.fix = FALSE, sigma.fix = FALSE, nu.fix = FALSE,
tau.fix = FALSE, control = gamlss.control(...),
i.control = glim.control(...), ...)
is.gamlss(x)
gamlssNews()
Returns a gamlss object with components
the distribution family of the gamlss object (see gamlss.family)
the name of the fitted parameters i.e. mu
, sigma
, nu
, tau
the call of the gamlss function
the response variable
the gamlss fit control settings
the vector of weights
the global deviance
the number of observations in the fit
a function to calculate the normalized (randomized) quantile residuals of the object
the number of external iterations in the fitting process
the type of the distribution or the response variable (continuous or discrete)
which algorithm is used for the fit, RS(), CG() or mixed()
whether the model fitting has have converged
the normalized (randomized) quantile residuals of the model
the fitted values of the mu model, also sigma.fv, nu.fv, tau.fv for the other parameters if present
the linear predictor of the mu model, also sigma.lp, nu.lp, tau.lp for the other parameters if present
the working variable of the mu model, also sigma.wv
, nu.wv
, tau.wv
for the other parameters if present
the working weights of the mu model, also sigma.wt, nu.wt, tau.wt for the other parameters if present
the link function for the mu model, also sigma.link, nu.link, tau.link for the other parameters if present
the terms for the mu model, also sigma.terms, nu.terms, tau.terms for the other parameters if present
the design matrix for the mu, also sigma.x, nu.x, tau.x for the other parameters if present
the QR decomposition of the mu model, also sigma.qr, nu.qr, tau.qr for the other parameters if present
the linear coefficients of the mu model, also sigma.coefficients, nu.coefficients, tau.coefficients for the other parameters if present
the formula for the mu model, also sigma.formula, nu.formula, tau.formula for the other parameters if present
the mu degrees of freedom also sigma.df, nu.df, tau.df for the other parameters if present
the non linear degrees of freedom, also sigma.nl.df, nu.nl.df, tau.nl.df for the other parameters if present
the total degrees of freedom use by the model
the residual degrees of freedom left after the model is fitted
the Akaike information criterion
the Bayesian information criterion
a formula object, with the response on the left of an ~ operator, and the terms, separated by \(+\) operators, on the right.
Nonparametric smoothing terms are indicated by pb()
for penalised beta splines, cs
for smoothing splines, lo
for loess
smooth terms and random
or ra
for random terms, e.g. y~cs(x,df=5)+x1+x2*x3
. Additional smoothers can be added by creating the appropriate interface.
Interactions with nonparametric smooth terms are not fully supported, but will not produce errors;
they will simply produce the usual parametric interaction
a formula object for fitting a model to the sigma parameter, as in the formula above,
e.g. sigma.formula=~cs(x,df=5)
. It can be abbreviated to sigma.fo=~cs(x,df=5)
.
a formula object for fitting a model to the nu parameter, e.g. nu.fo=~x
a formula object for fitting a model to the tau parameter, e.g. tau.fo=~cs(x,df=2)
a gamlss.family
object, which is used to define the distribution and the link functions of the various parameters.
The distribution families supported by gamlss()
can be found in gamlss.family
.
Functions such as BI() (binomial) produce a family object. Also can be given without the parentheses i.e. BI
.
Family functions can take arguments, as in BI(mu.link=probit)
a data frame containing the variables occurring in the formula, e.g. data=aids
. If this is missing, the variables should be on the search list.
a vector of weights. Note that this is not the same as in the glm() or gam() function.
Here weights can be used to weight out observations (like in subset
) or for a weighted likelihood analysis where
the contribution of the observations to the likelihood differs according to weights
.
The length of weights
must be the same as the number of observations in the data.
By default, the weight is set to one. To set weights to vector w
use weights=w
list of contrasts to be used for some or all of the factors appearing as variables in the model formula. The names of the list should be the names of the corresponding variables. The elements should either be contrast-type matrices (matrices with as many rows as levels of the factor and with columns linearly independent of each other and of a column of ones), or else they should be functions that compute such contrast matrices.
the current algorithms for GAMLSS are RS(), CG() and mixed(). i.e. method=RS()
will use the Rigby and Stasinopoulos algorithm,
method=CG()
will use the Cole and Green algorithm and
mixed(2,10)
will use the RS algorithm twice before switching to the Cole and Green algorithm for up to 10 extra iterations
a fitted GAMLSS model which the fitted values will be used as staring values for the current model
vector or scalar of initial values for the location parameter mu e.g. mu.start=4
vector or scalar of initial values for the scale parameter sigma e.g. sigma.start=1
vector or scalar of initial values for the parameter nu e.g. nu.start=3
vector or scalar of initial values for the location parameter tau e.g. tau.start=2
whether the mu parameter should be kept fixed in the fitting processes e.g. mu.fix=FALSE
whether the sigma parameter should be kept fixed in the fitting processes e.g. sigma.fix=FALSE
whether the nu parameter should be kept fixed in the fitting processes e.g. nu.fix=FALSE
whether the tau parameter should be kept fixed in the fitting processes e.g. tau.fix=FALSE
this sets the control parameters of the outer iterations algorithm. The default setting is the gamlss.control
function
this sets the control parameters of the inner iterations of the RS algorithm. The default setting is the glim.control
function
for extra arguments
an object
Mikis Stasinopoulos d.stasinopoulos@londonmet.ac.uk, Bob Rigby, Calliope Akantziliotou and Vlasios Voudouris
Respect the parameter hierarchy when you are fitting a model. For example a good model for mu
should be fitted before a model for sigma
is fitted
The Generalized Additive Model for Location, Scale and Shape
is a general class of statistical models for a univariate
response variable. The model assumes independent observations of the response variable
y given the parameters, the explanatory variables and the values
of the random effects. The distribution for the response variable
in the GAMLSS can be selected from a very general family of
distributions including highly skew and/or kurtotic continuous and
discrete distributions, see gamlss.family
. The systematic part of the model is
expanded to allow modelling not only of the mean (or location) parameter,
but also of the other parameters of the distribution of y, as
linear parametric and/or additive nonparametric (smooth)
functions of explanatory variables and/or random effects terms.
Maximum (penalized) likelihood estimation is used to fit the
(non)parametric models. A Newton-Raphson/Fisher scoring algorithm
is used to maximize the (penalized) likelihood. The additive terms
in the model are fitted using a backfitting algorithm.
is.gamlss
is a short version is is(object,"gamlss")
Rigby, R. A. and Stasinopoulos D. M. (2005). Generalized additive models for location, scale and shape,(with discussion), Appl. Statist., 54, part 3, pp 507-554.
Rigby, R. A., Stasinopoulos, D. M., Heller, G. Z., and De Bastiani, F. (2019) Distributions for modeling location, scale, and shape: Using GAMLSS in R, Chapman and Hall/CRC. An older version can be found in https://www.gamlss.com/.
Stasinopoulos D. M. Rigby R.A. (2007) Generalized additive models for location scale and shape (GAMLSS) in R. Journal of Statistical Software, Vol. 23, Issue 7, Dec 2007, https://www.jstatsoft.org/v23/i07/.
Stasinopoulos D. M., Rigby R.A., Heller G., Voudouris V., and De Bastiani F., (2017) Flexible Regression and Smoothing: Using GAMLSS in R, Chapman and Hall/CRC.
(see also https://www.gamlss.com/).
gamlss.family
, pdf.plot
, find.hyper
data(abdom)
mod<-gamlss(y~pb(x),sigma.fo=~pb(x),family=BCT, data=abdom, method=mixed(1,20))
plot(mod)
rm(mod)
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