galaxy

<p>Velocity at which 82 galaxies in the Corona Borealis region are moving away from our galaxy, scaled by 1000.</p>

datasets

A two-step Bayesian approach for mode inference following
Cross, Hoogerheide, Labonne and van Dijk (2024) <doi:10.1016/j.econlet.2024.111579>).
First, a mixture distribution is fitted on the data using a sparse finite
mixture (SFM) Markov chain Monte Carlo (MCMC) algorithm. The number of
mixture components does not have to be known; the size of the mixture is
estimated endogenously through the SFM approach. Second, the modes of the
estimated mixture at each MCMC draw are retrieved using algorithms
specifically tailored for mode detection. These estimates are then used to
construct posterior probabilities for the number of modes, their locations
and uncertainties, providing a powerful tool for mode inference.

Paul Labonne

BayesMultiMode

Bayesian Mode Inference

Nalan Baştürk

Jamie Cross

Peter de Knijff

Lennart Hoogerheide

Herman van Dijk

galaxy function

<p>An object of class <code>numeric</code> of length 82.</p>

Format

Galaxy series — galaxy

Galaxy series

galaxy: Galaxy series

Description

Usage

Arguments

Format

References