The GAPS programme at TNG - L. TOI-4515 b: An eccentric warm Jupiter orbiting a 1.2 Gyr-old G-star

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Table 2

Comparison between the joint models.

Model	No trend	Linear trend	Quadratic trend
1p	0.00 ± 0.35	−10.98 ± 0.37	−324.93 ± 0.35
1p+GP	1.65 ± 0.35	−10.52 ± 0.38	−271.48 ± 0.36
2p	0.92 ± 0.36	−9.01 ± 0.38	−496.27 ± 0.40
2p+GP	1.89 ± 0.36	−9.55 ± 0.37	−170.27 ± 0.36

Notes. The Bayesian evidence log 𝒵 for the 12 investigated models are listed. To improve the readability of the table, we subtracted the log 𝒵 = 25071.20 from the first model. The models with no trend are preferred.

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