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Table 2

Model comparison for the RV-only analysis of HD 63433 USING the difference between log-evidence (Δ ln Z).

Activity model

GP (QP kernel) 3 sin (P1 ~ 6.4 days, P2 ~ 3.2 days, P3 ~2.1d)


Dataset Planets Kb (ms−1) Kc (ms−1) Δ ln Z Kb (ms−1) Kc (ms−1) Δ ln Z
VIS 0 −2.2 –41.2
VIS 1 3.42 ± 2.95 −4.2 1.89 ± 1.76 −41.5
VIS 1 3.72 ± 1.12 0 6.13 ± 1.69 −37.8
VIS 2 2.68 ± 2.51 3.62 ± 1.11 −1.6 1.86 ± 1.55 6.30 ± 1.70 −42.0

VIS+NIR 0 –3.8
VIS+NIR 1 2.20 ± 2.05 –6.8
VIS+NIR 1 3.77 ± 0.97 0
VIS+NIR 2 1.77 ± 1.76 3.69 ± 0.98 –2.1

Notes. In the model name, “3 sin” refers to three sinusoidal functions and its periods. All models assume circular orbits, and the amplitudes are given with their 1σ uncertainty.

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