pastis: Bayesian extrasolar planet validation – I. General framework, models, and performance

Citations Over TimeTop 1% of 2014 papers

Abstract

A large fraction of the smallest transiting planet candidates discovered by the Kepler and CoRoT space missions cannot be confirmed by a dynamical measurement of the mass using currently available observing facilities. To establish their planetary nature, the con-cept of planet validation has been advanced. This technique compares the probability of the planetary hypothesis against that of all reasonably conceivable alternative false-positive (FP) hypotheses. The candidate is considered as validated if the posterior probability of the plan-etary hypothesis is sufficiently larger than the sum of the probabilities of all FP scenarios. In this paper, we present PASTIS, the Planet Analysis and Small Transit Investigation Software, a tool designed to perform a rigorous model comparison of the hypotheses involved in the problem of planet validation, and to fully exploit the information available in the candidate light curves. PASTIS self-consistently models the transit light curves and follow-up obser-vations. Its object-oriented structure offers a large flexibility for defining the scenarios to be compared. The performance is explored using artificial transit light curves of planets and FPs with a realistic error distribution obtained from a Kepler light curve. We find that data support

Related Papers

• → Analyses of some exoplanets’ transits and transit timing variations(2017)1 cited
• → The Transit Monitoring in the South (TraMoS) project(2013)
• Beyond Exoplanets: Taking advantage of Kepler Object of Interest fields after the presence or absence of an exoplanet has been documented(2013)
• → An optimized search for exoplanets with Kepler data(2017)
• → Analyzing light curves to highlight phenomena and trends in planetary systems that house terrestrial exoplanets(2023)