Notes. The table lists: prior, posterior median, and 68.3% CI, for the analysis of transit photometry and RVs ( juliet, in which the asymmetry of the transit is modelled using GPs, and the chromaticity with dilution factors), and the analysis of transit photometry including a starspot in the model ( starry). If a parameter is estimated from both modellings, the last column specifies the adopted value. There is a degeneracy with (i_⋆ + 180°) and (180° −λ) angles assuming i_p between 0° and 180°. ^† Upper limit, 95% confidence. The parameters q₁ and q₂ are the quadratic limb-darkening coefficients parameterised using Kipping (2013). The planetary equilibrium temperature is computed for zero albedo and full day-night heat redistribution. The true spin-orbit angle is given for the prograde and retrograde configurations, which cannot be distinguished with the available data. IAU 2012: au = 149 597 870 700 m . IAU 2015: = 6.957  × 10⁸ m, = 6.378 1  × 10⁶ m, = 1.327 124 4  × 10²⁰ m³ s⁻², = 3.986 004  × 10¹⁴ m³ s⁻². M_⊙ = /𝒢, M_E = /𝒢. CODATA 2018: 𝒢 = 6.674 30  × 10⁻¹¹ m³ kg⁻¹ s⁻². N(μ, σ): Normal distribution with mean μ, and standard deviation σ. U(a, b): A uniform distribution defined between a lower a and an upper b limit.