Fast Bayesian Inference for Exoplanet Discovery in Radial Velocity Data
Brendon J. Brewer, Courtney P. Donovan

TL;DR
This paper introduces a trans-dimensional Bayesian inference method using Nested Sampling to efficiently determine the number of exoplanets from radial velocity data, even with complex, multimodal posteriors.
Contribution
It presents a novel approach combining trans-dimensional MCMC with Nested Sampling to infer the number of planets and their parameters in a single analysis.
Findings
Detected multiple signals in $ u$ Oph with high posterior probability.
Identified many potential planets in Gliese 581, with some having well-determined periods.
Demonstrated the presence of phase transitions that challenge traditional sampling methods.
Abstract
Inferring the number of planets in an exoplanetary system from radial velocity (RV) data is a challenging task. Recently, it has become clear that RV data can contain periodic signals due to stellar activity, which can be difficult to distinguish from planetary signals. However, even doing the inference under a given set of simplifying assumptions (e.g. no stellar activity) can be difficult. It is common for the posterior distribution for the planet parameters, such as orbital periods, to be multimodal and to have other awkward features. In addition, when is unknown, the marginal likelihood (or evidence) as a function of is required. Rather than doing separate runs with different trial values of , we propose an alternative approach using a trans-dimensional Markov Chain Monte Carlo method within Nested Sampling. The posterior distribution for can be obtained with a…
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