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Table 6

Bayesian log-evidence for Lalande 21185 and a number of different models based on CARMENES, SOPHIE, and combined data.

Model(a) Periods
CARMENES
0p − 797.5 ± 0.1 0
1p 12.9 − 783.7 ± 0.2 13.8
1p + uGP 12.9 − 748.1 ± 0.2 49.4
SOPHIE
0p − 371.6 ± 0.1 0
1p 12.9 − 362.4 ± 0.2 9.2
1p + uGP 12.9 − 349.0 ± 0.2 22.6
CARMENES + SOPHIE
0p − 1169.5 ± 0.2 0
2p + GP 1.5,12.9 − 1161.8 ± 0.3 7.7
1p 12.9 − 1143.0 ± 0.2 26.5
1cp 12.9 − 1142.2 ± 0.3 27.3
GP − 1125.4 ± 0.2
1p + uGP 12.9 − 1092.3 ± 0.3 77.2
2p + GP 12.9, 364.5 − 1086.2 ± 0.3 83.3
1p + GP 12.9 − 1085.7 ± 0.3 83.8
1cp + GP 12.9 − 1085.3 ± 0.3 84.2
HIRES
0p − 777.7 ± 0.2 0
1p(b) 12.5 − 761.5 16.2
1p(c) 12.9 − 771.8 5.9

Notes. (a) Planetary models based on CARMENES, SOPHIE, HIRES, and combined CARMENES and SOPHIE RV data. 0p: 0 planets, 1p: one planet, 1cp: one planet on a circular orbit (e = 0). GP and uGP: additional constrained and unconstrained GPs, respectively. Orbital periods rounded to one decimal. (b) Priors as in Table A.2. (c)Gaussian priors for planetary parameters based on posterior solution from Table 4.

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