Relative posterior probabilities and log-Bayesian evidences for different noise models using the HARPS RVs.
|G+MA(3)||1.1 × 10-48||−6994.0|
|G+MA(5)||2.8 × 10-14||−6914.8|
|G+MA(7)||1.9 × 10-9||−6903.7|
Notes. No Keplerian signals were included in the model. The noise models are Gaussian (G), Cauchy (C), Uniform (U), AR(q), and MA(p).
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