Notes. The top part of the table lists the fitted parameters with their corresponding prior probabilities. Uniform prior probabilities are represented with U(x _min, x _max), where x _min and x _max are the minimum and maximum allowed values, respectively. Normal (Gaussian) prior probabilities are written as N(μ, σ), where μ and σ are the mean and standard deviation of the normal distribution, respectively. The lower part of the table shows the values of parameters derived from the sampled parameter space. ^(*)We fixed the eccentricity to 0 despite the non-zero values reported in the literature (Hellier et al. 2009; Triaud et al. 2010; Nymeyer et al. 2011; Csizmadia et al. 2019) because of the small eccentricity value and the possible tidal origin of the eccentric radial-velocity signal (see discussion in Section 4.3). ^(†)The maximum values of the phase curve F _max are equal to the dayside fluxes because the phase offset Δφ was fixed to 0. ^(‡)Equilibrium dayside temperature assuming full absorption of the incoming radiation (AB = 0), no heat redistribution (ε = 0, i.e. immediate re-radiation) and black-body spectral energy distributions for both the planet and the star, i.e. $T_{\text{day,,max}}={\left(2/3\right)}^{0.25}\sqrt{R_{\star }/a}{T}_{\text{eff}}$.