This page provides machine-readable posterior probability distributions for the exoplanet and exomoon system parameters, marginalised over the prior volume. These distributions are provided regardless as to whether the system is thought to have a genuine moon or not, and thus may be used to place upper limits for null detection cases. It is our hope that the scientific community will find these posteriors useful for estimating the frequency of large moons around viable planet hosts.

[1] KOI-872b:Null detection [posteriors]

…more coming soon