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

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Table 3

Parameters of the different runs of POLYCHORD on the HD 10180 dataset, when using a log-uniform prior on semi-amplitude.

Planets	log(Z)	σ_log(Z)	PNP	Runtime
0	−882.52	0.32	1.71e–108	12s
1	−837.39	0.11	3.69e–93	2 min 10 s
2	−785.31	0.15	7.26e–75	9 min 36 s
3	−731.86	0.09	9.15e–56	28 min 11 s
4	−670.76	0.16	3.08e–33	1 h 06 min 20 s
5	−595.12	0.26	4.15e–25	2 h 22 min 37 s
6	−587.60	0.97	0.396	9 h 42 min 25 s
7	−587.18	2.00	0.603	34 h 14 min 9 s

Notes. For a given number of planets in the model (Col. (1)) we performed three runs. The other columns give the log Bayesian evidence (log(Z), median), the standard deviation of log(Z) amongst runs (σ_log(Z)), the PNP, and the runtime.

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