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Table 2

Best-fit solution for the planetary system orbiting Gl 378.

Param. Units Gl 378 b
P (d) 3.822
K (m s−1) 7.96
e 0.109
ω (deg) 210.6
TP (d) 2455500.02
TC (d) 2455502.564

a (AU) 0.039435
M sin i (MEarth) 13.02

γSOPHIE (m s−1) −9697.333
σJIT (m s−1) 4.610
σ(O–C) (m s−1) 4.86
log(Likelihood) −138.07

Notes. For each parameter the median of the posterior is given, with error bars computed from the MCMC analysis using a 68.3% confidence interval. σO–C corresponds to the weighted standard deviation of the residuals around the best solutions. All the parameters probed by the MCMC can be found in Table B.1.

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