Best-fit solution for the planetary system orbiting Gl 378.
|Param.||Units||Gl 378 b|
|M sin i||(MEarth)||13.02|
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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