Carry out the ``starship'' estimation method for the generalised lambda distribution using a grid-based search
Carry out the ``starship'' estimation method for the generalised lambda distribution using a grid-based search
Calculates estimates for the generalised lambda distribution on the basis of data, using the starship method. The starship method is built on the fact that the generalised lambda distribution is a transformation of the uniform distribution. This method finds the parameters that transform the data closest to the uniform distribution. This function uses a grid-based search.
initgrid: A list with elements, lcvect, a vector of values for lambda3, ldvect, a vector of values for lambda4 and levect, a vector of values for lambda5
(levect is only required if param is fm5).
Note: if param=rs, the non-positive values are dropped from lcvect and ldvect.
param: choose parameterisation: fmkl uses Freimer, Mudholkar, Kollia and Lin (1988) (default). rs uses Ramberg and Schmeiser (1974)
fm5 uses the 5 parameter version of the FMKL parameterisation (paper to appear)
Details
The starship method is described in King and MacGillivray, 1999 (see references). It is built on the fact that the generalised lambda distribution is a transformation of the uniform distribution. Thus the inverse of this transformation is the distribution function for the gld. The starship method applies different values of the parameters of the distribution to the distribution function, calculates the depths q corresponding to the data and chooses the parameters that make the depths closest to a uniform distribution.
The closeness to the uniform is assessed by calculating the Anderson-Darling goodness-of-fit test on the transformed data against the uniform, for a sample of size length(data).
This function carries out a grid-based search. This was the original method of King and MacGillivray, 1999, but you are advised to instead use starship which uses a grid-based search together with an optimisation based search.
See references for details on parameterisations.
Returns
response: The minimum ``response value'' --- the result of the internal goodness-of-fit measure. This is the return value of starship.obj. See King and MacGillivray, 1999 for more details
lambda: A vector of length 4 giving the values of lambda1 to lambda4 that produce this minimum response, i.e. the estimates
References
Freimer, M., Mudholkar, G. S., Kollia, G. & Lin, C. T. (1988), A study of the generalized tukey lambda family, Communications in Statistics - Theory and Methods 17 , 3547--3567.
Ramberg, J. S. & Schmeiser, B. W. (1974), An approximate method for generating asymmetric random variables, Communications of the ACM 17 , 78--82.
King, R.A.R. & MacGillivray, H. L. (1999), A starship method for fitting the generalised lambda distributions, Australian and New Zealand Journal of Statistics 41 , 353--374
Owen, D. B. (1988), The starship, Communications in Statistics - Computation and Simulation 17 , 315--323.
Author(s)
Robert King, Darren Wraith
See Also
starship, starship.obj
Examples
data <- rgl(100,0,1,.2,.2) starship.adaptivegrid(data,list(lcvect=(0:4)/10,ldvect=(0:4)/10))