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Fig. 5

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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, ωω] as a function of ω. In blue, we represent −log 10 FIP, where FIP =1 – TIP is the false inclusion probability.

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