Relative posterior probabilities and log-Bayesian evidences of models ℳk with k = 0, ...,3 Keplerian signals, given the HARPS RVs.
|0||4.7 × 10-45||−6884.1||1.0 × 10-39||−6886.7|
|1||8.4 × 10-29||−6846.0||1.6 × 10-24||−6851.1|
|2||8.1 × 10-18||−6820.0||7.4 × 10-14||−6825.8|
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