Table D.1
GJ 699 FWHM ESPRESSO model statistics.
| Model | ln P−ln 𝒵 | ln 𝒵 |  |
BIC |  |
RMS |
|---|---|---|---|---|---|---|
| WN (K1) | 3.36±0.11 | -354.58±0.11 | 0.11 | 705.65±0.23 | 1.07±0.01 | 2.23±0.02 |
| WN (K2) | 10.05±0.13 | -326.64±0.12 | 0.12 | 640.48±1.03 | 1.11±0.02 | 1.66±0.01 |
| WN (K3) | 7.13±0.46 | -316.01±0.44 | 0.13 | 627.35±0.34 | 1.16±0.01 | 1.45±0.01 |
| 𝒢𝒫 grot(K0) | -10.36±0.62 | -217.46±0.06 | 0.09 | 445.72±0.31 | 0.62±0.01 | 0.36±0.01 |
| 𝒢𝒫rot (K0 ) | -4.17±0.02 | -215.86±0.01 | 0.08 | 446.75±0.07 | 0.67±0.01 | 0.38±0.01 |
| 𝒢𝒫 rot+(K1 ) | -6.61±0.09 | -216.20±0.08 | 0.08 | 453.24±0.16 | 0.76±0.01 | 0.41±0.01 |
| 𝒢𝒫rot + Mag(a) | -11.12±0.99 | -219.33±0.06 | 0.10 | 449.53±1.98 | 0.69±0.04 | 0.41±0.01 |
| 𝒢𝒫rot Mag(b) | -18.92±0.22 | -219.49±0.08 | 0.09 | 465.48±0.38 | 0.68±0.04 | 0.37±0.01 |
Notes. Runs from different models: (Kn) denotes the number of Keplerian signals. In descending order: white noise onzly (WN), Gaussian process with different parameterisations of the rotation kernel 𝒢𝒫rot and 𝒢𝒫 grot, and the inclusion of a magnetic cycle (Mag). This last model was tested with two different boundaries for the magnetic cycle: (a)∼ 𝒰 (0.5, 5000), (b)∼U(800, 5000).
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