First use of the learned harmonic mean estimator for Bayesian model selection across circular/eccentric, white-noise/GP, and trend variants in radial velocity exoplanet analyses.
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Reanalysis retracts TOI-1272c as a planet due to stellar activity, finds slightly eccentric orbits for TOI-1694b and c, and provides updated parameters with smaller uncertainties for both systems.
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Improving exoplanet mass characterisation with Bayesian model selection using the Learned Harmonic Mean Estimator
First use of the learned harmonic mean estimator for Bayesian model selection across circular/eccentric, white-noise/GP, and trend variants in radial velocity exoplanet analyses.
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The GAPS Programme at TNG LXXIV. A reanalysis of the planetary systems TOI-1272 and TOI-1694 with HARPS-N and retraction of the planetary interpretation of TOI-1272 c
Reanalysis retracts TOI-1272c as a planet due to stellar activity, finds slightly eccentric orbits for TOI-1694b and c, and provides updated parameters with smaller uncertainties for both systems.