Notes. The T_eff is derived from SED-fit. We use 1–5 Gyr isochrones obtained from the Dartmouth stellar evolution database (Dotter et al. 2008) to estimate R1_⋆, log   g₁ and M_⋆. The extinction values (A_v) found in the SED-fit are reported in Col. 6. In the three cases marked with an asterisk, the best-fitting extinction is higher than the total extragalactic extinction and we report the extinction that corresponds to the minimum χ² within the allowed extinction range. The stellar radii R2_⋆ correspond to the best-fitting analytic transit model (see Sect. 5.3). The values of log   g₂ reported in Col. 5 are estimated from the stellar radii R2_⋆, which tend to be higher than R1_⋆, resulting in lower log   g₂. The distances reported in Col. 7 are estimated utilizing the extinction values found in the VOSA analysis, the i-band magnitudes reported in Table 3, and the absolute magnitudes M_i, which are obtained from the isochrones.