Table A.4
Parameters used in the analysis.
Parameter | Prior | Posterior | |
---|---|---|---|
Dartmouth | PARSEC | ||
(adopted) | |||
Stellar parameters | |||
Effective temperature Teff [K] | ![]() |
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Surface gravity log g [cgs] | ![]() |
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Metallicity [M/H] [dex] | ![]() |
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Distance to Earth D [pc] | ![]() |
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Interstellar extinction E(B− V) [mag] | ![]() |
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Systemic radial velocity γ [km s−1 ] | ![]() |
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Linear limb-darkening coefficient ua | (Derived) | ![]() |
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Quadratic limb-darkening coefficient ub | (Derived) | ![]() |
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Stellar density ρ⋆ ∕ρ⊙ | (Derived) | ![]() |
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Stellar mass M⋆ [M⊙ ] | (Derived) | ![]() |
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Stellar radius R⋆ [R⊙ ] | (Derived) | ![]() |
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Stellar age τ [Gyr] | (Derived) | ![]() |
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Planet b parameters | |||
Orbital period Pb [d] | ![]() |
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Transit epoch T0,b [BJD - 2 450 000] | ![]() |
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Radial velocity semi-amplitude Kb [km s−1 ] | ![]() |
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Orbital inclination ib [°] | ![]() |
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Planet-to-star radius ratio kb | ![]() |
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Orbital eccentricity eb | ![]() |
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Argument of periastron ωb [°] | ![]() |
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System scale ab ∕R⋆ | (Derived) | ![]() |
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Impact parameter bb | (Derived) | ![]() |
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Transit duration T14,b [h] | (Derived) | ![]() |
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Semi-major axis ab [AU] | (Derived) | ![]() |
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Planet mass Mb [M⊕ ] | (Derived) | ![]() |
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Planet radius Rb [R⊕ ] | (Derived) | ![]() |
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Planet bulk density ρb [g cm−3] | (Derived) | ![]() |
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Planet c parameters | |||
Orbital period Pc [d] | ![]() |
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Transit epoch T0,c [BJD - 2 450 000] | ![]() |
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Radial velocity semi-amplitude Kc [km s−1 ] | ![]() |
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Orbital inclination ic [°] | ![]() |
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Planet-to-star radius ratio kc | ![]() |
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Orbital eccentricity ec | ![]() |
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Argument of periastron ωc [°] | ![]() |
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System scale ac ∕R⋆ | (Derived) | ![]() |
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Impact parameter bc | (Derived) | ![]() |
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Transit duration14,c [h] | (Derived) | ![]() |
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Semi-major axis ac [AU] | (Derived) | ![]() |
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Planet mass Mc [M⊕ ] | (Derived) | ![]() |
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Planet radius Rc [R⊕ ] | (Derived) | ![]() |
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Planet bulk density ρc [g cm−3] | (Derived) | ![]() |
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Planet d parameters | |||
Orbital period Pd [d] | ![]() |
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Transit epoch T0,d [BJD - 2 450 000] | ![]() |
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Radial velocity semi-amplitude Kd [km s−1 ] | ![]() |
0.00303 ± 0.00052 | 0.00303 ± 0.00051 |
Orbital inclination id [°] | ![]() |
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Planet-to-star radius ratio kd | ![]() |
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Orbital eccentricity ed | ![]() |
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Argument of periastron ωd [°] | ![]() |
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System scale ad ∕R⋆ | (Derived) | ![]() |
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Impact parameter bd | (Derived) | ![]() |
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Transit duration T14,d [h] | (Derived) | ![]() |
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Semi-major axis ad [AU] | (Derived) | ![]() |
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Planet mass Md [M⊕ ] | (Derived) | ![]() |
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Planet radius Rd [R⊕ ] | (Derived) | ![]() |
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Planet bulk density ρd [g cm−3] | (Derived) | ![]() |
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Planet e parameters | |||
Orbital period Pe [d] | ![]() |
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Transit epoch T0,e [BJD - 2 450 000] | ![]() |
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Radial velocity semi-amplitude Ke [km s−1 ] | ![]() |
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Orbital inclination ie [°] | ![]() |
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Planet-to-star radius ratio ke | ![]() |
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Orbital eccentricity ee | ![]() |
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Argument of periastron ωe [°] | ![]() |
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System scale ae ∕R⋆ | (Derived) | ![]() |
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Impact parameter be | (Derived) | ![]() |
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Transit duration T14,e [h] | (Derived) | 2.97 ± 0.05 | 2.97 ± 0.05 |
Semi-major axis ae [AU] | (Derived) | ![]() |
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Planet mass Me [M⊕ ] | (Derived) | ![]() |
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Planet radius Re [R⊕ ] | (Derived) | ![]() |
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Planet bulk density ρe [g cm−3] | (Derived) | ![]() |
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Planet f parameters | |||
Orbital period Pf [d] | ![]() |
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Transit epoch T0,f [BJD - 2 450 000] | ![]() |
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Radial velocity semi-amplitude Kf [km s−1 ] | ![]() |
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Orbital inclination if [°] | ![]() |
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Planet-to-star radius ratio kf | ![]() |
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Orbital eccentricity ef | ![]() |
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Argument of periastron ωf [°] | ![]() |
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System scale af ∕R⋆ | (Derived) | ![]() |
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Impact parameter bf | (Derived) | ![]() |
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Transit duration T14,f [h] | (Derived) | 3.20 ± 0.08 | 3.20 ± 0.08 |
Semi-major axis af [AU] | (Derived) | ![]() |
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Planet mass Mf [M⊕ ] | (Derived) | ![]() |
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Planet radius Rf [R⊕ ] | (Derived) | ![]() |
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Planet bulk density ρf [g cm−3] | (Derived) | ![]() |
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Planet g parameters | |||
Orbital period Pg [d] | ![]() |
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Transit epoch T0,g [BJD - 2 450 000] | ![]() |
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Radial velocity semi-amplitude Kg [km s−1 ] | ![]() |
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Orbital inclination ig [°] | ![]() |
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Planet-to-star radius ratio kg | ![]() |
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Orbital eccentricity eg | ![]() |
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Argument of periastron ωg [°] | ![]() |
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System scale ag ∕R⋆ | (Derived) | ![]() |
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Impact parameter bg | (Derived) | ![]() |
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Transit duration T14,g [h] | (Derived) | ![]() |
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Semi-major axis ag [AU] | (Derived) | ![]() |
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Planet mass Mg [M⊕ ] | (Derived) | ![]() |
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Planet radius Rg [R⊕ ] | (Derived) | ![]() |
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Planet bulk density ρg [g cm−3] | (Derived) | ![]() |
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Instrument-related parameters | |||
HARPS jitter σj, RV [km s−1 ] | ![]() |
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K2 contamination [%] | ![]() |
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K2 jitter σj, K2 [ppm] | ![]() |
185.8 ± 2.6 | 186.0 ± 2.6 |
K2 out-of-transit flux | ![]() |
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SED jitter [mag] | ![]() |
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Gaussian process hyperparameters | |||
Radial-velocities (joint analysis) | |||
A2 [m s−1 ] | ![]() |
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λ1 [d] | ![]() |
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λ2 | ![]() |
1.88 ± 0.79 | 1.72 ± 0.88 |
Prot [d] | ![]() |
25.5 ± 1.7 | ![]() |
Photometry (learning on the light curve for activity filtering) | |||
A1 | ![]() |
0.00293 ± 0.00032 | |
l[d] | ![]() |
1.444 ± 0.056 | |
Photometry (period learning on the light curve) | |||
A2 | ![]() |
0.00315 ± 0.00044 | |
λ1 [d] | ![]() |
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|
λ2 | ![]() |
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|
Prot [d] | ![]() |
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Full width half maximum (period learning on the FWHM time series) | |||
A2 [km s−1 ] | ![]() |
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λ1 [d] | ![]() |
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|
λ2 | ![]() |
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|
Prot [d] | ![]() |
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Bisector inverse slope (period learning on the BIS time series) | |||
A2 [km s−1 ] | ![]() |
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|
λ1 [d] | ![]() |
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|
λ2 | ![]() |
453 ± 380 | |
Prot [d] | ![]() |
22 ± 13 | |
Hα index (period learning on the Hα index time series) | |||
A2 | ![]() |
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|
λ1 [d] | ![]() |
737 ± 260 | |
λ2 | ![]() |
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|
Prot [d] | ![]() |
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Na I D index (period learning on the Na I D index time series) | |||
A2 | ![]() |
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|
λ1 [d] | ![]() |
10.8 ± 2.7 | |
λ2 | ![]() |
435 ± 390 | |
Prot [d] | ![]() |
22 ± 12 | |
SMW index (period learning on the SMW index time series) | |||
A2 | ![]() |
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|
λ1 [d] | ![]() |
7.7 ± 1.7 | |
λ2 | ![]() |
482 ± 360 | |
Prot [d] | ![]() |
23 ± 12 |
Notes. The respective priors are provided together with the posteriors for the Dartmouth and PARSEC stellar evolution tracks. The posterior values represent the median and 68.3% credible interval. 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.
: sine distribution between a and b.
: truncated normal distribution with mean μ and width σ2, between a and b.
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