A Bayesian Approach to Calibrating Period-Luminosity Relations of RR Lyrae Stars in the Mid-Infrared
Christopher R. Klein, Joseph W. Richards, Nathaniel R. Butler, and, Joshua S. Bloom

TL;DR
This paper presents a Bayesian method for calibrating period-luminosity relations of RR Lyrae stars in the mid-infrared, demonstrating improved accuracy and consistency over traditional methods.
Contribution
It introduces a generalized Bayesian model fitting approach for PL relations, specifically applied to mid-infrared RR Lyrae data, showing enhanced calibration and agreement with parallax measurements.
Findings
Bayesian approach improves PL relation calibration accuracy.
Method yields distances consistent with Hubble Space Telescope parallaxes.
Bayesian model reduces scatter in multi-waveband PL fits.
Abstract
A Bayesian approach to calibrating period-luminosity (PL) relations has substantial benefits over generic least-squares fits. In particular, the Bayesian approach takes into account the full prior distribution of the model parameters, such as the a priori distances, and refits these parameters as part of the process of settling on the most highly-constrained final fit. Additionally, the Bayesian approach can naturally ingest data from multiple wavebands and simultaneously fit the parameters of PL relations for each waveband in a procedure that constrains the parameter posterior distributions so as to minimize the scatter of the final fits appropriately in all wavebands. Here we describe the generalized approach to Bayesian model fitting and then specialize to a detailed description of applying Bayesian linear model fitting to the mid-infrared PL relations of RR Lyrae variable stars. For…
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