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

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Fig. 1

FIP periodogram of a simulated system with three injected planets. The periods of the peaks are indicated by red points; the −log₁₀FIP and log₁₀TIP are represented as a function of the centre of the period interval considered, in blue and yellow, respectively.

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