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Table 3

Different model components that were investigated in this work.

Parameter name Prior Units Description
White noise
γSIM 𝒰(−10, 10) m s−1 Velocity zero-point for simulated data set
σSIM 𝒥(0.01, 10) m s−1 Extra jitter term for simulated data set
GP Prior I (wide priors)
σGP, RV 𝒰(0, 40) m s−1 Amplitude of GP component for RVs
ΓGP,RV 𝒥(10−2, 101) Amplitude of GP sine-squared component for RVs
lGP, RV 𝒥(1, 105) days Length scale of GP exponential component for RVs(a)
Prot, GP,RV 𝒰(3, 110) days Period of the GP quasi-periodic component for RVs
GP Prior II (length scale constrained)
σGP, RV 𝒰(0, 40) m s−1 Amplitude of GP component for RVs
ΓGP, RV 𝒥 (10−1, 101) Amplitude of GP sine-squared component for RVs
lGP,RV days Length scale of GP exponential component for RVs(a)
Prot, GP,RV 𝒰(3, 110) days Period of the GP quasi-periodic component for RVs
GP Prior III (period constrained)
σGP, RV 𝒰(0, 40) m s−1 Amplitude of GP component for RVs
ΓGP, RV 𝒥(10−1, 101) Amplitude of GP sine-squared component for RVs
lGP, RV 𝒥(1, 105) days Length scale of GP exponential component for RVs(a)
Prot, GP,RV 𝒩(22, 2.2) days Period of the GP quasi-periodic component for RVs
GP Prior IV (length scale and period constrained)
σGP, RV 𝒰(0, 40) m s−1 Amplitude of GP component for RVs
ΓGP, RV 𝒥 (10−1, 101) Amplitude of GP sine-squared component for RVs
lGP, RV days Length scale of GP exponential component for RVs(a)
Prot, GP,RV 𝒩(22, 2.2) days Period of the GP quasi-periodic component for RVs
KX (where X is given in days)
Pb 𝒰(X − 0.1X, X + 0.1X) days Period
t0,b − 2450000 𝒰(2458620., 2458620. + 1.1X) days Time of transit center
Kb 𝒰(0, 40) m s−1 RV semi-amplitude
𝒰(−1, 1) Parametrization for e and ω
𝒰(−1, 1) Parametrization for e and ω

Notes. (a)In juliet, the length scale parameter is parameterized by its inverse as described in Appendix A. For better understanding, however, we give the direct length scale. The prior labels 𝒰, 𝒩, and 𝒥 represent uniform, Normal and Jeffrey’s distributions (Jeffreys 1946). The x represents either 5.12 days, 30.35 days or 44 days regarding the period of the Kepler signal. The white noise model is always applied on top of the other models in this table.

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