The HARPS search for southern extra-solar planets - XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles

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Table 8

Summary of the Bayesian evidence computation for each model.


n	log p(D \| M_n,I)−1000	log ₁₀p(M_n \| D,I) /p(M₃ \| D,I)

2	1.26 ± 0.70	− 20.75 ± 0.61
3	49.04 ± 0.62	0.0
4	51.71 ± 0.23	1.16 ± 0.29
5	50.38 ± 3.98	0.6 ± 1.8
6	28.2 ± 20.7	− 9.0 ± 9.0

Notes. The geometric mean between the estimates by CJ01 and P14 is computed. The uncertainties are the quadratic mean between the statistical errors reported in Table 7 and the difference between the two estimates.

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