Table 3
Model comparison of RV-only fits with juliet.
| Model | Prior Pplanet | GP kernel | Δ ln Z |
|---|---|---|---|
| 1pl |  |
… | 19.93 |
| 2pl |  |
… | 15.51 |
 |
|||
| 3pl |  |
… | 9.03 |
 |
|||
 |
|||
| 4pl |  |
… | −2.15 |
 |
|||
 |
|||
 |
|||
| 1pl+GPexp |  |
Exp (a) | 19.51 |
| 2pl+GPexp |  |
Exp (a) | 9.29 |
 |
|||
| 3pl+GPexp |  |
Exp (a) | 0.00 |
 |
|||
 |
|||
| 4pl+GPexp |  |
Exp (a) | −0.95 |
 |
|||
 |
|||
 |
|||
| 1pl+GPess |  |
ExpSinSq (b) | 18.06 |
| 2pl+GPess |  |
ExpSinSq (b) | 6.32 |
 |
|||
| 3pl+GPess |  |
ExpSinSq (b) | −1.59 |
 |
|||
 |
|||
| 4pl+GPess |  |
ExpSinSq (b) | 3.11 |
 |
|||
 |
|||
 |
|||
Notes. The prior label 
represents a normal distribution. The final model used for the joint fit is marked in boldface (see Sect. 5.2.2 for details about the selection of the final model). (a) Simple exponential kernel of the form 
TGP,RV). (b) Exponential-sine-squared kernel of the form ki,j = 
with a uniform prior in Prot;GP,RV ranging from 30 to 100 d.
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