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Table A.1

Priors used for the joint fit model 3pl+GPexp presented in Sect. 5.2.3 using juliet.

Parameter name Prior Units Description
Stellar parameters
ρ kg m−3 Stellar density
Planet parameters
Pb d Period of planet b
Pc d Period of planet c
Pd d Period of planet d
t0,b − 24 50 000 d Time of transit-center of planet b
t0,c − 24 50 000 d Time of transit-center of planet c
t0,d − 24 50 000 d Time of transit-center of planet d
r1,b Parametrization for p and b
r2,b Parametrization for p and b
Kb m s−1 RV semi-amplitude of planet b
Kc m s−1 RV semi-amplitude of planet c
Kd m s−1 RV semi-amplitude of planet d
0.0 (fixed) Parametrization for e and ω
0.0 (fixed) Parametrization for e and ω
Photometry parameters
DTESS 1.0 (fixed) Dilution factor
MTESS ppm Relative flux offset for TESS
σTESS ppm Extra jitter term for TESS
q1,TESS Quadratic limb-darkening parametrization for TESS
q2,TESS Quadratic limb-darkening parametrization for TESS
MLCO ppm Relative flux offset for LCO
σLCO ppm Extra jitter term for LCO
q1,LCO Linear limb-darkening parametrization for LCO
RV parameters
μHIRES m s−1 Systemic velocity for HIRES
σHIRES m s−1 Extra jitter term for HIRES
μUVES m s−1 Systemic velocity for UVES
σUVES m s−1 Extra jitter term for UVES
μHARPS m s−1 Systemic velocity for HARPS
σHARPS m s−1 Extra jitter term for HARPS
μPFSpre m s−1 Systemic velocity for PFSpre
σPFSpre m s−1 Extra jitter term for PFSpre
μPFSpost m s−1 Systemic velocity for PFSpost
σPFSpost m s−1 Extra jitter term for PFSpost
μCARMENES m s−1 Systemic velocity for CARMENES
σCARMENES m s−1 Extra jitter term for CARMENES
GP hyperparameters
σGP,TESS ppm Amplitude of GP component for TESS
TGP,TESS d Length scale of GP component for TESS
σGP,RV m s−1 Amplitude of GP component for the RVs
TGP,RV d Length scale of GP component for the RVs

Notes. The prior labels of , , and represent normal, uniform, and Jeffrey’s distributions. The parametrization for (p, b) using (r1, r2) (Espinoza 2018) and the linear (q1) and quadratic (q1, q2) limb-darkening parametrization (Kipping 2013) are both described in Sect. 5.2.1.

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