lms(y, x, families = LMS, data = NULL, k = 2,
cent = 100 * pnorm((-4:4) * 2/3),
calibration = TRUE, trans.x = FALSE,
lim.trans = c(0.001, 1.5),
legend = FALSE, mu.df = NULL,
sigma.df = NULL, nu.df = NULL,
tau.df = NULL, method.pb = c("ML", "GAIC"), ...)
gamlss.families
with default LMS=c("BCCGo", "BCPEo", "BCTo")
TRUE
FALSE
FALSE
mu
effective degrees of freedom if required otherwise are estimatedsigma
effective degrees of freedom if required otherwise are estimatednu
effective degrees of freedom if required otherwise are estimatedtau
effective degrees of freedom if required otherwise are estimatedpb()
for estimating the smoothing
parameters. The default is local maximum likelihood "ML"
. "GAIC"
is also permitted where k
is taken from the k
argument of the fungamlss
gamlss
fitted objectThe model assumes that the response variable has a flexible distribution i.e. $y ~ D(\mu, \sigma, \nu, \tau)$ where the parameters of the distribution are smooth functions of the explanatory variable i.e. $g(\mu)= s(x)$, where $g()$ is a link function and $s()$ is a smooth function. Occasionally a power transformation in the x-axis helps the construction of the centile curves. That is, in this case the parameters are modelled by $x^p$ rather than just x, i.e.$g(\mu)= s(x^p)$. The function lms()
uses P-splines (pb()
) as a smoother.
If a transformation is needed for x
the function lms()
starts by finding an optimum value for p
using the simple model $NO(\mu=s(x^p))$. (Note that this value of p
is not the optimum for the final chosen model but it works well in practice.)
After fitting a Normal error model for staring values the function proceeds by fitting several "appropriate" distributions for the response variable.
The set of gamlss.family
distributions to fit is specified by the argument families
.
The default families
arguments is LMS=c("BCCGo", "BCPEo", "BCTo")
that is the LMS class of distributions, Cole and Green (1992).
Note that this class is only appropriate when y is positive (with no zeros). If the response variable contains negative values and zeros then use the argument families=theSHASH
where theSHASH <- c("NO", "SHASHo")
or add any other list of distributions which you may think is appropriate.
Justification of using the specific centile (0.38 2.27 9.1211220 25.25, 50, 74.75, 90.88, 97.72, 99.62) is given in Cole (1994).
Cole, T. J. and Green, P. J. (1992) Smoothing reference centile curves: the LMS method and penalized likelihood, Statist. Med. 11, 1305--1319
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.
Stasinopoulos D. M., Rigby R.A. and Akantziliotou C. (2006) Instructions on how to use the GAMLSS package in R.
Accompanying documentation in the current GAMLSS help files, (see also
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,
gamlss
, centiles
, calibration
data(abdom)
m1 <- lms(y,x , data=abdom, n.cyc=30)
m2 <- lms(y,x ,data=abdom, method.pb="GAIC", k=log(610))
# this example takes time
data(db)
m1 <- lms(y=head, x=age, data=db, trans.x=TRUE)
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