cUmbrPU: Computes a critical value for the Mack-Wolfe Peak Unknown...

In NSM3: Functions and Datasets to Accompany Hollander, Wolfe, and Chicken - Nonparametric Statistical Methods, Third Edition

Computes a critical value for the Mack-Wolfe Peak Unknown A_p-hat distribution.

Description

This function computes the critical value for the Mack-Wolfe Peak Unknown A_p-hat distribution at (or typically in the "Exact" and "Monte Carlo" cases, close to) the given alpha level.

Usage

cUmbrPU(alpha, n, method=NA, n.mc=10000)

Arguments

alpha	A numeric value between 0 and 1.
n	A vector of numeric values indicating the size of each of the k data groups.
method	Either "Exact", "Monte Carlo" or "Asymptotic", indicating the desired distribution. When method=NA, "Exact" will be used if the number of permutations is 10,000 or less. Otherwise, "Monte Carlo" will be used.
n.mc	If method="Monte Carlo", the number of Monte Carlo samples used to estimate the distribution. Otherwise, not used.

Value

Returns a list with "NSM3Ch6c" class containing the following components:

n	number of observations in the k data groups
cutoff.U	upper tail cutoff at or below user-specified alpha
true.alpha.U	true alpha level corresponding to cutoff.U (if method="Exact" or "Monte Carlo")

Author(s)

Grant Schneider

Examples

##Hollander-Wolfe-Chicken Example 6.4 Learning Comprehension and Age
#cUmbrPU(.0495, c(3, 3, 3, 3, 3))

cUmbrPU(.10, c(2, 4, 2))

NSM3 documentation built on Nov. 4, 2024, 5:08 p.m.