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Table B.1

Priors for each of the parameters fitted in the global photometric analysis of CHEOPS and TESS data.

Parameter Prior
Star
ρ [kg m−3] TN(1790, 110, 1680, 1900)
q1, TESS N (0.34, 0.05)
q2, TESS N (0.27, 0.05)
q1, CHEOPS N (0.46, 0.05)
q2, CHEOPS N (0.32, 0.05)
Planet b
Rp/R N (0.01688, 0.01)
T0-2 450 000. [BJD] N (8572.1128, 0.01)
P[d] N (3.796, 0.001)
Planet c
Rp/R N (0.0217, 0.01)
T0-2 450 000. [BJD] N (8572.3949, 0.01)
P [d] N (6.203, 0.001)
Planet d
Rp/R N (0.0266, 0.01)
T0-2450000. [BJD] N (8571.3368, 0.01)
P [d] N (14.1758, 0.001)
Planet e
Rp/R N (0.0322, 0.01)
T0-2450000. [BJD] N (8586.5677, 0.01)
P [d] N (19.59, 0.001)
Planet f
Rp/R N (0.0211, 0.01)
T0-2450000. [BJD] N (8616.039, 0.01)
P [d] N (29.5398, 0.001)
All planets
b [R] U(0.001, 0.99)
U(−0.3, 0.3)
U(−0.3, 0.3)
Instrumental
mflux_TESSi N (0.0, 0.1)
σw_TESS; [ppm] logU(0.1, 1000)
mflux__CHEOPSi N (0.0, 0.1)
σw_CHEOPSi [ppm] logU(0.1, 1000)
c1(t)_CHEOPSi U(−1.0, 1.0)
c2(t2)_CHEOPSi U(−1.0, 1.0)

Notes. The following distributions were used: Normal (N(µ0, σ0)), Truncated Normal (TN(µ0, σ0, limit_low, limit_upper)), Uniform (U(limit_low, limit_upper)), log-Uniform (logU(limit_low, limit_upper)). The instrumental parameters are defined for each fitted light curve.

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