Detecting exoplanets with the false inclusion probability - Comparison with other detection criteria in the context of radial velocities

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Fig. 4

FIP periodogram of 190 HARPS measurements of HD 10180 computed with a log-uniform prior on semi-amplitude on [0.1,20] m s⁻¹. In blue, pink, and green: FIP periodograms corresponding to different runs of calculations of posterior distributions of the parameters of a seven-planet model.

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