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Table D.3

GJ 699 RV ESPRESSO model statistics.

Model ln P−ln 𝒵 ln 𝒵 σ^Z${{{\hat \sigma }_Z}}$ BIC χv2${\chi _v^2}$ RMS
𝒢𝒫 3SHO(K0) -28.29±0.01 -230.28±0.01 0.11 499.70±0.11 0.75±0.02 0.58±0.01
𝒢𝒫 3SHO(K1) -13.66±0.30 -230.84±0.25 0.26 482.01±0.09 0.71±0.02 0.44±0.01
𝒢𝒫 rot+SHO(K0) -15.70±0.05 -233.14±0.04 0.07 495.65±0.22 0.77±0.01 0.61±0.01
𝒢𝒫 rot+SHO(K1) -2.38±0.54 -232.56±0.33 0.09 478.10±0.64 0.73±0.07 0.43±0.01
𝒢𝒫 2rot(K0) -19.81±0.05 -232.25±0.05 0.07 505.65±0.21 0.78±0.01 0.61±0.01
𝒢𝒫 2rot(K1) -7.54±0.30 -231.24±0.30 0.09 489.76±0.12 0.80±0.03 0.46±0.01
𝒢𝒫 rot+S (K1) 7.55±0.20 -231.21±0.18 0.11 470.94±0.25 0.72±0.03 0.46±0.01
𝒢𝒫 rot+Mag (K1) 3.67±0.42 -230.58±0.42 0.12 480.55±0.62 0.78±0.01 0.45±0.01
𝒢𝒫 grot+S (K1) 4.34±0.11 -229.86±0.07 0.10 461.31±0.27 0.74±0.03 0.44±0.01
𝒢𝒫 grot+Mag (K1) 1.19±0.32 -230.55±0.28 0.11 472.50±0.40 0.70±0.03 0.44±0.01

Notes. Runs from different models, (Kn) denotes the number of Keplerian signals. In descending order: Gaussian process with 3 SHO kernels, rotation plus SHO kernel, 2 rotation kernels, rotation kernel plus a sinusoid, rotation kernel plus magnetic cycle, and the modified rotation kernel.

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