Fig. 3: FPP calculation for Kepler-1708 b-i.
From: An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i

Histogram of the log Bayes factor between a planet–moon and a planet-only model from 200 fake planet-only signals injected into the light curve. Two signals pass the threshold (=loge10) and have positive radii, indicating a 1% FPP.