Bayesian Model Selection and Extrasolar Planet Detection
Eric B. Ford (CfA), Philip C. Gregory (UBC)

TL;DR
This paper explores Bayesian methods, especially importance sampling, for detecting exoplanets via radial velocity data, improving model selection accuracy and efficiency in complex planetary systems.
Contribution
It introduces a new importance sampling-based algorithm for Bayesian model selection in exoplanet detection, addressing convergence issues of previous estimators.
Findings
Importance sampling methods outperform others in efficiency.
A simple algorithm constructs a mixture distribution for posterior approximation.
Recommendations for developing robust estimators of marginal posterior probabilities.
Abstract
Radial velocity (RV) planet searches are increasingly finding planets with small velocity amplitudes, with long orbital periods, or in multiple planet systems. Bayesian inference has the potential to improve the interpretation of existing observations, the planning of future observations and ultimately inferences concerning the overall population of planets. In recent years, the refinement of Markov chain Monte Carlo (MCMC) algorithms has made it practical to accurately characterize orbital parameters and their uncertainties from RV observations of single-planet and weakly interacting multiple-planet systems. Unfortunately, MCMC is not sufficient for Bayesian model selection, i.e., comparing the marginal posterior probability of models, as is necessary to determine how strongly the observational data favor a model with n+1 planets over a model with just n planets. Many of the obvious…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Gamma-ray bursts and supernovae · Diverse Scientific and Engineering Research
