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Table 6

Kepler-74 system parameters.

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

Orbital period P [days] 7.340718 ± 0.000001 7.340711 ± 0.000006
Transit epoch T0 [BJDTDB − 2 454 900] 67.3453 ± 0.0003 287.56737 ± 0.00014
Transit duration T14 [h] 2.699 ± 0.038a 3.082 ± 0.011
Radius ratio Rp/R 0.090 ± 0.002 0.0912 ± 0.0009
Inclination i [deg] 85.55 ± 0.96 87.46 ± 0.07
Limb-darkening coefficient q1
Limb-darkening coefficient q2
Orbital eccentricity e 0.287 ± 0.062 0 (fixed)
Argument of periastron ω [deg] 64 ± 21
Radial-velocity semi-amplitude K [ m s-1] 58 ± 7 59 ± 11
HARPS-N systemic velocity Vr,HN [ km s-1] 19.356 ± 0.008 19.366 ± 0.009
HARPS-N RV jitter [ m s-1] sj,HN < 5
SOPHIE systemic velocity Vr,SO [ km s-1] 19.290 ± 0.014
SOPHIE RV jitter [ m s-1] sj,SO 28 ± 13
Derived transit parameters

a/R 15.47 ± 0.18
Stellar density ρ [gcm-3]
Impact parameter b 0.684 ± 0.032 0.685 ± 0.011
Limb-darkening coefficient ua 0.35 ± 0.17
Limb-darkening coefficient ub 0.6 ± 0.4
Atmospheric parameters of the star

Effective temperature Teff[K] 6050 ± 110 6000 ± 100
Spectroscopic surface gravity log g [cgs] 4.2 ± 0.1 4.5 ± 0.10
Derived surface gravity log g [cgs] 4.2 ± 0.1 4.44 ± 0.01
Metallicity [Fe/H] [dex] 0.34 ± 0.14 0.42 ± 0.11
Stellar rotational velocity Vsini [ km s-1] 5.0 ± 1.0 5.0 ± 1.0
Spectral type F8V F8V
Stellar and planetary physical parameters

Stellar mass [M] 1.18 ± 0.04
Stellar radius [R] 1.51 ± 0.14 1.12 ± 0.04
Planetary mass Mp [MJup] 0.68 ± 0.09 0.63 ± 0.12
Planetary radius Rp [RJup] 1.32 ± 0.14 0.96 ± 0.02
Planetary density ρp [gcm-3] 0.37 ± 0.13 0.88 ± 0.18
Planetary surface gravity log gp [cgs] 2.98 ± 0.11 3.23 ± 0.10
Age t [Gyr]
Orbital semi-major axis a [au] 0.084 ± 0.014 0.0781 ± 0.0007
Equilibrium temperature Teq [K]b 1250 ± 120 1078 ± 19

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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