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Table 3

Best-fit model and derived parameters of the transit, occultation, and phase curve fit.

Parameter Unit CHEOPS TESS
Transit

Stellar density ρ gcm−3
Orbital frequency f day−1 0.28784401 ± 0.00000033 0.28784433 ± 0.000000023
Orbital period P days 3.4741039 ± 0.0000040 3.47409999 ± 0.00000028
Orbital period [G.D.] days 3.47410075 ± 0.00000056 3.4741004 ± 0.0000004
Time of transit Tc BJDTDB – 2457000 2406.927174 ± 0.000024 1698.210775 ± 0.000052
Time of transit [G.D.] 1312.5853 ± 0.0002 1312.5849 ± 0.0001
Planet-star radius ratio Rp/R 0.11572 ± 0.00018 0.11588 ± 0.00006
Planet–star radius ratio [G.D.](1) Rp/Req 0.1131 ± 0.0008
Impact parameter b 0.515 ± 0.005 0.523 ± 0.004
Impact parameter [G.D.] 0.498 ± 0.005 0.510 ± 0.006
Quadratic limb darkening q1 0.257 ± 0.018 0.12 ± 0.05
Quadratic limb darkening q2 0.39 ± 0.26
Quadratic limb darkening [G.D.] ua + ub 0.516 ± 0.021 0.18 ± 0.03
Quadratic limb darkening [G.D.] uaub 0.05 ± 0.10 0.39 ± 0.02
Scaled semi-major axis a/R
Scaled semi major axis [G.D.] 7.46 ± 0.02 7.43 ± 0.02
Stellar rotation axis i deg
Nodal longitude Ω deg 86.12 ± 1.1 81 ± 1
Orbital inclination ip deg 86.03 ± 0.05 85.96 ± 0.04
Orbital inclination [G.D.] deg 86.17 ± 0.04 86.064 ± 0.047
Transit depth δtr % 1.3391 ± 0.0042 1.3428 ± 0.0013
Transit depth [G.D.](1) % 1.3187 ± 0.019 1.2955 ± 0.0116
Sky-projected spin-orbit angle λ deg 3.9 ± 1.1 9 ± 1
Spin-orbit angle Ψ deg 5.0 ± 11 32 ± 7
Jitter σw ppm 123 ± 2 303 ± 4
Red noise σr ppm 1947 ± 107 7862 ± 284

Occultation and phase-curve

Transit/eclipse duration(2) T14/T14 h 3.540 ± 0.003 3.537 ± 0.003
Phase offset φ deg
Dayside phase amplitude Aday ppm 122.2 ± 4.9
Nightside phase amplitude Anight ppm
Occultation depth δocc ppm 82.4 ± 5.6
Brightness temperature (100% NIR)(3) Tday K
Geometric albedo (100% NIR)(3) Ag 0.19 ± 0.08 0.19 ± 0.16

Lambertian grey-sky (CHEOPS-TESS)

Brightness temperature Tday K
Geometric albedo Ag 0.26 ± 0.04
Dayside temperature Td K
Nightside temperature Tn K
Bond albedo AB
Heat re-circulation efficiency ϵ

Notes. G.D. represents gravity-darkening fit. (1)Req and Rpol are the equatorial and the polar radius of the star, respectively. (2)T14 = t14: The transit and occultation duration are the same, as eccentricity is set to zero for a circular orbit.(3) 100% NIR: 1D retrieval model without scattering.

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