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Table 2

Pyaneti model of TOI-733 described in Sect. 4.

Parameter Priors(a) Final value
Fitted parameters
Transit epoch T0 (BJD - 2 450 000) 𝒰[8545.73, 8545.79] days
Orbital period Porb 𝒰[4.8845, 4.8860] days
𝒰[−1, 1] −0.08 ± 0.19
𝒰[−1, 1]
Impact parameter b 𝒰[0, 1]
Scaled semi-major axis a/R 𝒩[14, 1]
Scaled planet radius Rp/R 𝒰[0, 0.05]
Doppler semi-amplitude variation K 𝒰[0, 50] 2.23 ± 0.26 m s−1
Limb-darkening coefficient q1 𝒰[0, 1]

Limb-darkening coefficient q2 𝒰[0, 1]
GP hyperparameters
GP period PGP 𝒰[24.5, 26.5] days
λp 𝒰[0.1, 3]
λe 𝒰[1, 200] days
Vc 𝒰[0, 100] m s−1
Vr 𝒰[0, 500] m s−1 d−1
Fc 𝒰[0, 150] m s−1

Derived parameters
Planet mass Mp M
Planet radius Rp R
Inclination i deg
Eccentricity e
Angle of periastron ω
Semi-major axis a AU
Insolation F F
Planet density ρp g cm−3
Planet surface gravity log(gb) cm s−2
Equilibrium temperature Teq(b) K
Jeans escape parameter Λ (c)
Transmission spectroscopy metric TSM(d)
Total transit duration T14 hours
Full transit duration T23 hours
Ingress and egress transit duration T12 hours

Additional parameters
Offset RV HARPS 𝒰[−24.3256, −23.3089] km s−1
Offset FWHM 𝒰[6.4434, 7.4657] km s−1
RV jitter HARPS 𝒥[0, 1000] m s−1
FWHM jitter 𝒥[0, 1000] m s−1
TESS light curve jitter σTESS (×10−6) 𝒥[0, 1000]

Notes. (a)𝒰[a, b] refers to uniform priors in the range ab, and 𝒥[a, b] to modified Jeffrey’s priors (Eq. (16) in Gregory 2005). (b)Dayside equilibrium temperature, assuming no heat redistribution and zero albedo. (c)Λ = GMpmH/(kBTeqRp) (Fossati et al. 2017). (d)Kempton et al. (2018).

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