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Table 3

Priors and results of the model of planet b from the combined analysis of the light curve and RV series (Case 1).

Stellar activity
Parameter Unit Prior Value
Common RV+log RHK+light curve Rotational period (Prot) days U(8.0, 10.0) 8.83 ± 0.08
Quasi-periodic kernel
Decay Timescale of activity (Pdec) days U(10.0, 100.0)
Coherence scale (w)
Amplitude of the RV signal m s−1 U(0.01, 1500.00)
Uncorrelated RV iitter () m s−1
RV offset (γRV) m s−1 −6838.3 ± 4.2
SHOTterm+RotationTerm kernel
Standard deviation of the rotation ppt
Granulation period days U(0.05, 5.00)
Standard deviation of granulation ppt 0.067 ± 0.010
Photometric jitter () 303 ± 7
Planet b
Parameter Unit Prior Value
Orbital Period (Pb) days U(0.549, 0.550)
Central time of the first transit (T0,b) BJD U(21458899.3, 2458899.4)
Duration of the transit (T14,b) hours
Limb darkening (u1) N (0.47,0.05) 0.46 ± 0.05
Limb darkening (u2) N (0.18,0.05) 0.17 ± 0.05
Impact factor (bb)
Orbital inclination (ib) deg 82.0 ± 2.0
Orbital eccentricity (eb) fixed 0
Semi-major-axis-to-stellar-radius ratio ((ab/R*)) 3.8 ± 0.2
Orbital Semi-major axis (ab) au 0.0120 ± 0.0003
Planetary-to-stellar-radius ratio ((RP,b/R*)) 0.0182 ± 0.0006
Planetary radius (RP,b) R 1.37 ± 0.09
RV semi-amplitude (Kb) m s−1 U(0.01, 10)
Planetary mass (MP,b) M 2.57 ± 0.50
Planetary density (ρb) ρ 1.00 ± 0.29
Stellar density (ρ*) ρ N(2.3, 0.4) 2.4 ± 0.4

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