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Table 5

Kepler-423 system parameters.

Model parameters

Planet orbital period Porb (day) 2.68432850 ± 0.00000007
Planetary mid-transit epochaT0(BJDTDB-2 450 000 day) 4966.35480997 ± 0.00002124
Planet-to-star area ratio 0.015872 ± 0.000062
Planet-to-star surface brightness ratio f (8.93 ± 4.13) × 10-4
Impact parameter b 0.3006 ± 0.0100
Bulk stellar density ρ (g cm-3) 1.398 ± 0.096
Linear limb-darkening coefficient u1 0.4650 ± 0.0100
Quadratic limb-darkening coefficient u2 0.1518 ± 0.0228
Radial velocity semi-amplitude K (km s-1) 0.0967 ± 0.0118
Systemic radial velocity Vγ (km s-1) −3.0410 ± 0.0081
Orbit eccentricity e
Argument of periastron ω (degree)
Kepler LC data scatter σLC (ppm) 292.2 ± 2.4
Kepler SC data scatter σSC (ppm) 1145.7 ± 2.1
Derived parameters

Planet-to-star radius ratio Rp/R 0.12599 ± 0.00024
Planetary eclipse depth ΔFec (ppm) 14.2 ± 6.6
Scaled semi-major axis of the planetary orbit ap/R
Semi-major axis of the planetary orbit ap (AU)
Orbital inclination angle ip (degree) 87.828 ± 0.126
Planetary transit duration T14 (h) 2.7220 ± 0.0019
Transit ingress and egress duration T12 = T34 (h) 0.3330 ± 0.0024
Stellar fundamental parameters

Effective temperature Teff (K) 5560 ± 80
Surface gravityb log g (log10  cm s-2) 4.44 ± 0.10
Surface gravityc log g (log10  cm s-2) 4.41 ± 0.04
Metallicity [M/H] (dex) −0.10 ± 0.05
Microturbulent velocitydvmicro (km s-1) 1.0 ± 0.1
Macroturbulent velocitydvmacro (km s-1) 2.8 ± 0.4
Projected stellar rotational velocity v sin i (km s-1) 2.5 ± 0.5
Spectral typee G4 V
Star mass M (M) 0.85 ± 0.04
Star radius R (R) 0.95 ± 0.04
Star age t (Gyr) 11 ± 2
Star rotation periodfProt (day) 22.047 ± 0.121
Interstellar extinction AV (mag) 0.044 ± 0.044
Distance of the system d (pc) 725 ± 75
Planetary fundamental parameters

Planet massgMp (MJup) 0.595 ± 0.081
Planet radiusgRp (RJup) 1.192 ± 0.052
Planet density ρp (g cm-3) 0.459 ± 0.083
Equilibrium temperature Teq (K) 1605 ± 120
Brightness temperaturehTbr (K) 1950 ± 250
Geometric albedohAg 0.055 ± 0.028
Bond albedohAB 0.037 ± 0.019

Notes.

(a)

BJDTDB is the barycentric Julian date in barycentric dynamical time.

(b)

Obtained from the spectroscopic analysis.

(c)

Obtained from Teff, [M/H], and ρ, along with the Pisa Stellar Evolution Data Base for low-mass stars.

(d)

Using the calibration equations of Bruntt et al. (2010) and Doyle et al. (2014).

(e)

With an accuracy of ± 1 sub-class.

(g)

Radius and mass of Jupiter taken as 6.9911 × 109 cm and 1.89896 × 1030 g, respectively.

(h)

Assuming Ag = 1.5 × AB and heat redistribution factor between 1/4 and 2/3.

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