Open Access
Table 3
Parameters and adopted priors of the RV models with Gaussian processes and three different kernels (U and N stand for uniform and Gaussian priors, respectively).
Parameter | Symbol | Units | C.I. | Prior |
---|---|---|---|---|
Squared-exponential Gaussian process model [ΔBIC = 56.8] | ||||
RV zero point | γ | m s−1 | −3.2 ± 4.6 | U] – ∞, +∞o[ |
RV jitter | σjit | m s−1 | 3.29 ± 0.24 | U[0, +∞[ |
GP-SE amplitude | h | m s−1 | ![]() |
U[0, +∞[ |
GP-SE decay timescale | λ | days | ![]() |
U[0, 500] |
Eccentricity | e | − | 0.2608 ± 0.0086 | N(0.258, 0.004) |
Stellar argument of periastron | ω⋆ | deg | 13.5 ± 2.7 | N(12, 3) |
Radial-velocity semi-amplitude | K⋆ | m s−1 | 11.20 ± 0.50 | U[0, +∞[ |
Quasi-periodic Gaussian process model [ΔBIC = 18.6] | ||||
RV zero point | γ | m s−1 | ![]() |
U] – ∞, +∞[ |
RV jitter | σjit | ms−1 | 2.16 ± 0.24 | U[0, +∞[ |
GP amplitude | h | ms−1 | ![]() |
U[0, +∞[ |
GP decay timescale | λ | days | ![]() |
U[0, 500] |
GP rotational period | Prot | days | ![]() |
U[25, 40] |
GP harmonic inverse complexity | w | ![]() |
U[0.1, 5] | |
Eccentricity | e | − | 0.2638 ± 0.0090 | N(0.258,0.004) |
Stellar argument of periastron | ω⋆ | deg | 14.2 ± 2.5 | N(12,3) |
Radial-velocity semi-amplitude | K⋆ | m s−1 | 10.72 ± 0.43 | U[0, +∞[ |
Quasi-periodic+squared-exponential Gaussian process model [ΔBIC = 0] | ||||
RV zero point | γ | m s−1 | ![]() |
U] – ∞, +∞[ |
RV jitter | σjit | ms−1 | ![]() |
U[0, +∞[ |
GP rotational amplitude | hrot | ms−1 | ![]() |
U[0, +∞[ |
GP rotational decay timescale | λrot | days | ![]() |
U[0, 500] |
GP rotational period | Prot | days | ![]() |
U[25, 40] |
GP rotational harmonic inverse complexity | wrot | ![]() |
U[0.1,5] | |
GP cycle amplitude | hcycle | ms−1 | ![]() |
U[0, +∞[ |
GP cycle decay timescale | λcycle | days | ![]() |
U[0,1000] |
Eccentricity | e | − | 0.2654 ± 0.0091 | N(0.258,0.004) |
Stellar argument of periastron | ω⋆ | deg | 14.7 ± 2.6 | N(12,3) |
Radial-velocity semi-amplitude | K⋆ | m s−1 | 10.78 ± 0.42 | U[0, +∞[ |
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