False inclusion probability periodograms of the Kepler-10 HARPS-N data processed with YARARA-v2 for different priors on semiamplitude. (a) was obtained with a log-uniform prior on semiamplitude, (b) with a Gaussian mixture model on mass. In yellow we represent the true inclusion probability (TIP), the probability of having a planet in the range [ω−Δ ω, ω+Δ ω] as a function of ω. In blue, we represent −log ₁₀ FIP, where FIP =1 – TIP is the false inclusion probability.