DancGLOB_pv:

Usage Arguments Examples

Usage

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DancGLOB_pv(n, est = tmean, fr1 = 1, fr2 = 1, nboot = 500, SEED = TRUE, iter = 1000, nmin = 12, MC = TRUE, alpha = 0.05, PRM = FALSE, qvals = c(0.25, 0.5, 0.75), cpp = FALSE, ...)

Arguments

n
est
fr1
fr2
nboot
SEED
iter
nmin
MC
alpha
PRM
qvals
cpp
...

Examples

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##---- Should be DIRECTLY executable !! ----
##-- ==>  Define data, use random,
##--	or do  help(data=index)  for the standard data sets.

## The function is currently defined as
function (n, est = tmean, fr1 = 1, fr2 = 1, nboot = 500, SEED = TRUE, 
    iter = 1000, nmin = 12, MC = TRUE, alpha = 0.05, PRM = FALSE, 
    qvals = c(0.25, 0.5, 0.75), cpp = FALSE, ...) 
{
    if (!cpp) {
        if (SEED) 
            set.seed(45)
        bvec = list()
        for (i in 1:iter) bvec[[i]] = rmul(n, p = 4)
        prm = NA
        pv = lapply(bvec, DancGLOBv2, est = est, fr1 = fr1, fr2 = fr2, 
            nboot = nboot, SEED = FALSE, nmin = nmin, MC = MC, 
            qvals = qvals, plotit = FALSE, ...)
        pv = as.vector(matl(pv))
        p = hd(pv, q = alpha)
    }
    if (cpp) {
        library(WRScpp)
        p = DancGLOB_pv_C(n = n, est = est, fr1 = fr1, fr2 = fr2, 
            SEED = SEED, nboot = nboot, qvals = qvals, nmin = nmin, 
            alpha = alpha, PRM = PRM, ...)$p.crit
    }
    list(p.crit = p)
  }

musto101/wilcox_R documentation built on May 23, 2019, 10:52 a.m.