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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Accounting for radial correlations in SPARC rotation curves as nuisance parameters eliminates the preference for pISO over NFW dark matter halo models.
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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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Consequences of radially correlated rotation curves for galaxy mass models
Accounting for radial correlations in SPARC rotation curves as nuisance parameters eliminates the preference for pISO over NFW dark matter halo models.