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Table 7

Kepler-75 system parameters.

Fitted system parameters Hébrard et al. (2013) This work

Orbital period P [days] 8.884924 ± 0.000002 8.8849116 ± 0.0000034
Transit epoch T0 [BJDTDB − 2 454 900] 102.9910 ± 0.0002 840.44030 ± 0.00012
Transit duration T14 [h] 1.872 ± 0.025a 2.0778 ± 0.0084
Radius ratio Rp/R 0.121 ± 0.002
Inclination i [deg]
Limb-darkening coefficient q1 0.36 ± 0.08
Limb-darkening coefficient q2
0.337 ± 0.020
0.676 ± 0.013
Orbital eccentricity e 0.569 ± 0.010 0.570 ± 0.010
Argument of periastron ω [deg] 63.6 ± 1.4 63.5 ± 1.7
Radial-velocity semi-amplitude K [ km s-1] 1.288 ± 0.024 1.287 ± 0.025
HARPS-N systemic velocity Vr,HN [ km s-1] −64.175 ± 0.050 −64.180 ± 0.056
HARPS-N RV jitter [ m s-1] sj,HN < 17 < 54
SOPHIE systemic velocity Vr,SO [ km s-1] −64.235 ± 0.012 −64.236 ± 0.014
SOPHIE RV jitter [ m s-1] sj,SO < 8 < 8
Derived transit parameters

a / R 19.6 ± 0.6
Stellar density ρ [gcm-3] 1.79 ± 0.17
Impact parameter b 0.14 ± 0.14
Limb-darkening coefficient ua 0.53 ± 0.09 0.50 ± 0.05
Limb-darkening coefficient ub 0.13 ± 0.26 0.09 ± 0.12
Atmospheric parameters of the star

Effective temperature Teff[K] 5330 ± 120 5200 ± 100
Spectroscopic surface gravity log g [cgs] 4.55 ± 0.14 4.60 ± 0.15
Derived surface gravity log g [cgs] 4.5 ± 0.1 4.50 ± 0.02
Metallicity [Fe/H] [dex] –0.07 ± 0.15 0.30 ± 0.12
Stellar rotational velocity Vsini [ km s-1] 3.5 ± 1.5 3.5 ± 1.5
Spectral type G8V K0V
Stellar and planetary physical parameters

Stellar mass [M] 0.88 ± 0.06 0.91 ± 0.04
Stellar radius [R] 0.88 ± 0.04 0.89 ± 0.02
Planetary mass Mp [MJup] 9.9 ± 0.5 10.1 ± 0.4
Planetary radius Rp [RJup] 1.03 ± 0.06 1.05 ± 0.03
Planetary density ρp [gcm-3] 11 ± 2
Planetary surface gravity log gp [cgs] 4.36 ± 0.03 4.36 ± 0.03
Age t [Gyr] 6 ± 3
Orbital semi-major axis a [au] 0.080 ± 0.005 0.0818 ± 0.0012
Equilibrium temperature at the averaged distance Teq [K]b 850 ± 40 767 ± 16

Notes.

(a)

This value of transit duration is not accurate enough because it was estimated with the approximated formula reported in Winn (2010). Indeed, the transit duration is not a free parameter in the transit model adopted by Hébrard et al. (2013).

(b)

Black-body equilibrium temperature assuming a null Bond albedo and uniform heat redistribution to the night side.

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