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Table A.4

Parameters used in the analysis.

Parameter Prior Posterior
Dartmouth PARSEC
(Adopted)
Stellar parameters
Effective temperature Teff (K) 5477 ± 27 5480 ± 24
Surface gravity log g (cgs) 4.419 ± 0.053 4.429 ± 0.045
Iron abundance [Fe/H] (dex) 0.078 ± 0.020 0.079 ± 0.020
Distance to Earth D (pc) 145 ± 8 141 ± 6
Interstellar extinction E(BV) (mag)
Systemic radial velocity γ (km s−1) − 18.186 ± 0.002 − 18.186 ± 0.002
Linear limb-darkening coefficient ua (Derived) 0.4631 ± 0.0061 0.4625 ± 0.0057
Quadratic limb-darkening coefficient ub (Derived) 0.2270 ± 0.0041 0.2273 ± 0.0037
Stellar density ρρ (Derived) 0.98 ± 0.19 1.03 ± 0.16
Stellar mass M (M) (Derived) 0.915 ± 0.017 0.884 ± 0.018
Stellar radius R (R) (Derived) 0.977 ± 0.053 0.950 ± 0.040
Stellar age τ (Gyr) (Derived) 9.7 ± 3.0 10.8 ± 2.8

Planet b parameters
Orbital period P (d) 2.369172 ± 8.9 × 10−5 2.369173 ± 9.0 × 10−5
Transit epoch T0 (BJD - 2456000) 981.6431 ± 1.6 × 10−3 981.6431 ± 1.6 × 10−3
Radial velocity semi-amplitude K (m s−1) 3.34 ± 0.43 3.33 ± 0.43
Orbital inclination i (°) 87.7 ± 1.6 88.1 ± 1.4
Planet-to-star radius ratio k 0.01604 ± 0.00041 0.01599 ± 0.00035
Orbital eccentricity e 0.084 ± 0.079 0.080 ± 0.068
Argument of periastron ω (°)
System scale aR (Derived) 7.43 ± 0.45 7.56 ± 3.8
Impact parameter b (Derived) 0.30 ± 0.20 0.25 ± 0.19
Transit duration T14 (h) (Derived) 2.266 ± 0.050 2.264 ± 0.049
Semi-major axis a (AU) (Derived) 0.03376 ± 0.00021 0.03337 ± 0.00023
Planet mass Mp (M) (Derived) 6.54 ± 0.84 6.38 ± 0.83
Planet radius Rp (R) (Derived) 1.71 ± 0.11 1.654 ± 0.84
Planet bulk density ρp (g cm−3) (Derived) 7.1 ± 1.8 7.7 ± 1.7

Gaussian process hyperparameters
A(m s−1) 5.96 ± 1.2
λ1 (d) 34 ± 12 34 ± 12
λ2 0.46 ± 0.12 0.46 ± 0.12
Prot (d) 32.2 ± 0.5 32.2 ± 0.5

Instrument-related parameters
HARPS jitter (m s−1) 1.9 ± 0.4 1.9 ± 0.4
K2 contamination (%) 0.952 ± 0.024 0.952 ± 0.024
K2 jitter (ppm) 59 ± 1 59 ± 1
K2 out-of-transit flux 1.000006 ± 2 × 10−6 1.000006 ± 2 × 10−6
SED jitter (mag) 0.054 ± 0.021 0.054 ± 0.022

Notes. The respective priors are provided together with the posteriors for both the Dartmouth and PARSEC stellar evolution tracks. The posterior values represent the median and 68.3% credible interval. Fixed and derived values that might be useful for follow-up work are also reported. : normal distribution with mean μ and width σ2. : uniform distribution between a and b. : normal distribution with mean μ and width σ2 multiplied with a uniform distribution between a and b. : sine distribution between a and b.

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