| ebnm_flat {ebnm} | R Documentation |
Solve the EBNM problem using a flat prior
Description
Solves the empirical Bayes normal means (EBNM) problem using a "non-informative" improper uniform prior, which yields posteriors
\theta_j | x_j, s_j \sim N(x_j, s_j^2).
Identical to function
ebnm with argument prior_family = "flat". For details
about the model, see ebnm.
Usage
ebnm_flat(
x,
s = 1,
g_init = NULL,
fix_g = FALSE,
output = ebnm_output_default()
)
Arguments
x |
A vector of observations. Missing observations ( |
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. |
g_init |
Not used by |
fix_g |
Not used by |
output |
A character vector indicating which values are to be returned.
Function |
Value
An ebnm object. Depending on the argument to output, the
object is a list containing elements:
dataA data frame containing the observations
xand standard errorss.posteriorA data frame of summary results (posterior means, standard deviations, second moments, and local false sign rates).
fitted_gThe fitted prior
\hat{g}.log_likelihoodThe optimal log likelihood attained,
L(\hat{g}).posterior_samplerA 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.
See Also
See ebnm for examples of usage and model details.
Available S3 methods include coef.ebnm,
confint.ebnm,
fitted.ebnm, logLik.ebnm,
nobs.ebnm, plot.ebnm,
predict.ebnm, print.ebnm,
print.summary.ebnm, quantile.ebnm,
residuals.ebnm, simulate.ebnm,
summary.ebnm, and vcov.ebnm.