Solve the EBNM problem using an ash family of distributions

A wrapper to function ash in package ashr. Identical to function ebnm with argument prior_family = "ash".

ebnm_ash(
  x,
  s = 1,
  mode = 0,
  scale = "estimate",
  g_init = NULL,
  fix_g = FALSE,
  output = ebnm_output_default(),
  control = NULL,
  ...
)

Arguments

x: A vector of observations. Missing observations (NAs) are not allowed.
s: A vector of standard errors (or a scalar if all are equal). Standard errors may not be exactly zero, and missing standard errors are not allowed.
mode: Passed to ash as parameter mode.
scale: Passed to ash as parameter mixsd.
g_init: Passed to ash as parameter g.
fix_g: Passed to ash as parameter fixg.
output: A character vector indicating which values are to be returned. Function ebnm_output_default() provides the default return values, while ebnm_output_all() lists all possible return values. See Value below.
control: Passed to ash as parameter control.
...: Additional parameters to be passed to ash.

Value

An ebnm object. Depending on the argument to output, the object is a list containing elements:

data: A data frame containing the observations x and standard errors s.
posterior: A data frame of summary results (posterior means, standard deviations, second moments, and local false sign rates).
fitted_g: The fitted prior \(\hat{g}\).
log_likelihood: The optimal log likelihood attained, \(L(\hat{g})\).
posterior_sampler: A function that can be used to produce samples from the posterior. The sampler takes a single parameter nsamp, the number of posterior samples to return per observation.

S3 methods coef, confint, fitted, logLik,

nobs, plot, predict, print, quantile,

residuals, simulate, summary, and vcov

have been implemented for ebnm objects. For details, see the respective help pages, linked below under See Also.

Solve the EBNM problem using an ash family of distributions

Arguments

Value

See also