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Table A.2
K2-18 model parameters from the HARPS+CARMENES joint RV analysis.
Parameter | Point estimate |
---|---|
Stellar Parameters | |
2MASS Photometry | J = 9.763 ± 0.028, H = 9.135 ± 0.026, Ks = 8.899 ± 0.019 |
Stellar mass, Ms [M⊙] | 0.495 ± 0.004 |
Stellar radius, Rs [R⊙] | 0.469 ± 0.010 |
Effective temperature, Teff [K] | 3503 ± 60 |
Stellar parallax, p [mas] | 26.299 ± 0.055 |
Distance, d [pc] | 38.025 ± 0.079 |
HARPS systemic velocity, γ0,HARPS [m s−1] | 652.51 ± 1.0 |
CARMENES systemic velocity, γ0,CARMENES [m s−1] | − 2.87 ± 0.9 |
GP hyperparameters | |
HARPS covariance amplitude, aHARPS [m s−1] | ![]() |
CARMENES covariance amplitude, aCARMENES [m s−1] | ![]() |
Exponential timescale, λ [days] | 448.8 ± 67.3 |
Coherence, Γ | ![]() |
Periodic timescale, PGP [days] | ![]() |
HARPS additive jitter, sHARPS [m s−1] | 0.48 ± 0.42 |
CARMENES additive jitter, sCARMENES [m s−1] | 0.58 ± 0.53 |
K2-18c | |
Period, Pc [days] | 8.997 ± 0.007 |
Time of inferior conjunction, T0,c [BJD-2 450 000] | 7263.69 ± 0.44 |
Radial velocity semi-amplitude, Kc [m s−1] | 2.76 ± 0.41 |
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Semi-major axis, ac [AU] | 0.0670 ± 0.0002 |
Minimum planet mass, mp,c sinic [M⊕] | 5.62 ± 0.84 |
Equilibrium temperature, Teq,c [K] | |
Bond albedo of 0.3 | 409 ± 8 |
K2-18b | |
Period, Pb [days] | 32.93962 ± 1.0 × 10−4 |
Time of inferior conjunction, T0,b [BJD-2 450 000] | 7264.39142 ± 6.4 × 10−4 |
Radial velocity semi-amplitude, Kb [m s−1] | 2.75 ± 0.43 |
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Semi-major axis, ab [AU] | 0.1591 ± 0.0004 |
Planet radius, rp,b [R⊕]a | 2.711 ± 0.065 |
Planet mass, mp,b [M⊕]b | 8.63 ± 1.35 |
Planet density, ρp,b [g cm-3] | 2.4 ± 0.4 |
Surface gravity, g [m s-2] | 11.5 ± 1.9 |
Escape velocity, vesc,b [km s-1] | 19.9 ± 1.6 |
Equilibrium temperature, Teq,b [K] | |
Bond albedo of 0.3 | 265 ± 5 |
Notes. (a) Based on the measured rp,b ∕Rs of K2-18b from Benneke et al. (2017); rp,b∕Rs = 0.05295 ± 0.00060. (b) Assuming the measured orbital inclination of K2-18b from Benneke et al. (2017); degrees.
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