Table A.1
Parameters used for the standard reduction and retrievals, with priors and posteriors from the white light curve fit.
| Name | Symbol | Unit | Order | Prior | Posterior | Note |
|---|---|---|---|---|---|---|
| Star | ||||||
| Mass | M* | M⊙ | 0.691 | |||
| Radius | R* | R⊙ | 0.679 | [1], (a) | ||
| Effective temperature | ![]() |
K | 4665 | |||
| Surface gravity | log g* | log(g cm−3) | 4.614 (4.5) | [1], (a), (b) | ||
| Metallicity | [Fe/H] | −0.20 | [1], (a) | |||
| Distance | d | pc | 142.751 | |||
| Orbit | ||||||
| Period | P | d | 3.21305751 | [2], [A] | ||
| Transit mid-time | t0 | BMJD | 60115 + U(0.3,0.6) | 60115.447938(12) | [B], (c), (d) | |
| Semimajor axis | a | au | 0.03767 | [1] | ||
| Scaled semimajor axis | a/R* | N (11.9,0.3) | 11.69(3) | [1], [B], (e) | ||
| Impact parameter | b | N (0.19,0.05) | 0.258(11) | |||
| Eccentricity Argument of periastron |
e ω |
° | 0 90 |
[1], [A], (f) | ||
| Planet | ||||||
| Mass | Mp | MJup | 0.201 | [1] | ||
| Radius ratio | Rp/R* | 1 2 |
U(0.01,0.9) | 0.13794(17) 0.13825(23) |
[A], (d) | |
| Limb darkening | ||||||
| Quadratic LDCs |
q1 q2 |
1 2 1 2 |
q1 ∈ [0, 1] q2 ∈ [0, 1] |
0.115(11) 0.282(17) 0.57(5) 0.59(3) |
[C], (d), (g) | |
| Systematic | ||||||
| Dilution factor | D | 1,2 | 1 | |||
| Relative out-of-transit flux Jitter term |
M σω |
ppm | 1,2 1 2 |
N (0.0,0.1) L(10−1,104) |
|M| < 10−5 95(5) 146(10) |
[A] |
Notes. Uncertainties are given in parentheses for brevity and correspond to the 1σ errors in the last digits. Priors: U = Uniform, N = Normal, L = Log-uniform; References: [1] Mancini et al. (2018), [2] Kokori et al. (2022); Spectral light curves: [A] Same prior used, [B] Fixed to median value from white light curves, [C] Fixed to values from theoretical models; Minor remarks: (a) Used for wavelength calibration & calculation of spectral light curve LDCs, (b) Value of 4.5 used for spectral LDCs due to grid limitations, (c) BMJD := BJD - 2400000.5, (d) Wide uninformative prior, (e) Prior calculated from literature values, (f) Assumption of circular orbit (based on Bonomo et al. 2017), (g) Use of Kipping (2013) parametrization.
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