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Table 4

Bandpass-specific priors and best-fit values for the model and detrending parameters as described in Sect. 3, along with the derived parameters.

Parameter Unit Prior Best-fit value
CHEOPS
Fitted parameters
Zero transit epoch t0 BJD time - 2459095.2 U(−0.01, 0.01)
Transit depth depth U(0.0049, 1)
Transit scaling factor f0 U(0.9,1.1)
1st quadratic limb darkening component q1 N(0.34052, 0.01)(a)
2nd quadratic limb darkening component q2 N(0.22030, 0.01)(a)

Hotspot offset Δϕ deg U(−180, 29) −14.1 ± 2.4
Cm{ power coefficient C1,1 U(0, 1)
Mean background temperature K U(2890, 5780)(d)
Derived parameters
Planetary radius Rp R*
1st quadratic limb darkening component u1
2nd quadratic limb darkening component u2 0.320 ± 0.012

TESS
Fitted parameters
Zero transit epoch t0 BJD time - 2458693.8 U(−0.01, 0.01)
Transit depth depth U(0.0049, 1) 0 006263 ± 0 000016
Transit scaling factor f0 U(0.9, 1.1) 1.00017 ± 0.00012
1st quadratic limb darkening component q1 N(0.1690, 0.01)(b)
2nd quadratic limb darkening component q2 N(0.2082, 0.01)(b)
Hotspot offset Δϕ deg U(−180, 29) −12.32 ± 0.97
Cmℓ power coefficient C1,1 U(0, 1)
Mean background temperature T K U(2890, 5780)(d)
Derived parameters
Planetary radius Rp R* 0.079142 ± 0.000099
1st quadratic limb darkening component u1
2nd quadratic limb darkening component u2 0.2216 ± 0.0096
Spitzer
Fitted parameters
Zero transit epoch t0 BJD time - 2458415.36 U(−0.01, 0.01) 0.00206 ± 0.00015
Transit depth depth U(0.0049, 1) 0.006152 ± 0.000068
Transit scaling factor f0 U(0.9, 1.1) 0.99993 ± 0.00020
1st quadratic limb darkening component q1 N(0.0097, 0.01)(c)
2nd quadratic limb darkening component q2 N(0.1463,0.01)(c)
Hotspot offset Δϕ deg U(−180, 29)
Cmℓ power coefficient C1,1 U(0, 1) 0 2453 ± 0 0092
Mean background temperature T K U(2890, 5780)(d)
Derived parameters
Planetary radius Rp R* 0 0 843 ± 0 00043
1st quadratic limb darkening component u1
2nd quadratic limb darkening component u2

Notes. The reported errors are the 16th and 84th percentile interval for every parameter. Priors based on previous results from (a)Claret (2021), (b)Claret (2017), (c)Claret & Bloemen (2011), (d)Morris et al. (2022).

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