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Table A.1

Priors used for TOI-1235 b in the joint fit with juliet.

Parameter (a) Prior Unit Description
Stellar parameters
ρ g cm−3 Stellar density
Planet parameters
Pb d Period of planet b
t0,b d Time of transit center of planet b
r1,b Parameterization for p and b
r2,b Parameterization for p and b
Kb m s−1 RV semi-amplitude of planet b
eb 0.0 (fixed) Orbital eccentricity of planet b
ωb 90.0 (fixed) deg Periastron angle of planet b
       
Photometry parameters
DTESS 1.0 (fixed) Dilution factor for TESS Sectors 14, 20, and 21
MTESS,S14 Relative flux offset for TESS Sector 14
MTESS,S20 Relative flux offset for TESS Sector 20
MTESS,S21 Relative flux offset for TESS Sector 21
σTESS,S14 ppm Extra jitter term for TESS Sector 14
σTESS,S20 ppm Extra jitter term for TESS Sector 20
σTESS,S21 ppm Extra jitter term TESS Sector 21
q1,TESS Limb-darkening parameterization for TESS Sectors 14, 20, 21
q2,TESS Limb-darkening parameterization for TESS Sectors 14, 20, 21
DLCO 1.0 (fixed) Dilution factor for LCOGT
q1,LCO Limb-darkening parameterization for LCOGT
MLCO Relative flux offset for LCOGT
σLCO ppm Extra jitter term for LCOGT
θ0,LCO Extra jitter term for LCOGT
θ1,LCO Extra jitter term for LCOGT
       
RV parameters
γHARPS-N m s−1 RV zero-point for HARPS-N
σHARPS-N m s−1 Extra jitter term for HARPS-N
γCARMENES m s−1 RV zero point for CARMENES
σCARMENES m s−1 Extra jitter term for CARMENES
       
GP hyperparameters
σGP,RV m s−1 Amplitude of GP component for the RVs
αGP,RV d−2 Inverse length-scale of GP exponential component for the RVs
ΓGP,RV Amplitude of GP sine-squared component for the RVs
Prot;GP,RV d Period of the GP quasi-periodic component for the RVs

Notes. (a) The parameterization for (p, b) was made with (r1, r2) as in Espinoza (2018). The prior labels of , , and represent normal, uniform, and log-uniform distributions, respectively, where is a normal distribution of the mean μ and variance σ2 and and are uniform and log-uniform distributions between a and b.

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