The CARMENES search for exoplanets around M dwarfs - Three temperate-to-warm super-Earths

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Table 5

Bayesian log-evidence for HD 238090 and a number for different models based on CARMENES data.

Model^(a)	Periods (d)
0p	…	− 287.3 ± 0.1	0
GP	…	− 284.9 ± 0.1	2.4
1p	13.7	− 273.0 ± 0.2	14.3
1cp	13.7	− 273.3 ± 0.2	14.3
1p + 1cp	13.7,106.6	− 267.8 ± 0.2	19.5
2p + GP	7.0, 13.7	− 267.7 ± 0.2	19.4
1p + uGP	13.7	− 267.0 ± 0.2	20.3
1p + GP	13.7	− 267.1 ± 0.2	20.2
1cp + GP	13.7	− 267.0 ± 0.2	20.3
2p + GP	13.7, 389.8	− 265.1 ± 0.2	22.2

Notes. ^(a) Planetary models based on CARMENES RV data. 0p: 0 planets, 1p: one planet, 1cp: one planet in circular orbit (e = 0). GP and uGP: additional constrained and unconstrained GPs, respectively. Sin: additional sinusoidal model. Orbital periods rounded to one decimal.

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