galaxy

The observed rotation velocities and their uncertainties of Low Surface Brightness (LSB) galaxies, along with the physical radius of the galaxy.

datasets

A Bayesian data modeling scheme that performs four interconnected tasks: (i) characterizes the uncertainty of the elicited parametric prior; (ii) provides exploratory diagnostic for checking prior-data conflict; (iii) computes the final statistical prior density estimate; and (iv) executes macro- and micro-inference. Primary reference is Mukhopadhyay, S. and Fletcher, D. 2018 paper "Generalized Empirical Bayes via Frequentist Goodness of Fit" (<https://www.nature.com/articles/s41598-018-28130-5 >).

Doug Fletcher

BayesGOF

Bayesian Modeling via Frequentist Goodness-of-Fit

galaxy function

A data frame of \((y_i, se_i, X_i)\) for \(i = 1,...,318\).<dl class="dl-horizontal">
 <dt><code>y</code></dt><dd>actual observed (smoothed) velocity</dd>
 <dt><code>se</code></dt><dd>uncertainty of observed velocity</dd>
 <dt><code>X</code></dt><dd>physical radius of the galaxy</dd>
 </dl>

Format

Galaxy Data — galaxy

A data frame of \((y_i, se_i, X_i)\) for \(i = 1,...,318\).<dl class='dl-horizontal'>
 <dt><code>y</code></dt><dd>actual observed (smoothed) velocity</dd>
 <dt><code>se</code></dt><dd>uncertainty of observed velocity</dd>
 <dt><code>X</code></dt><dd>physical radius of the galaxy</dd>
 </dl>

galaxy: Galaxy Data

Description

Usage

Arguments

Format