Notes. The estimates correspond to the posterior median (P₅₀) with 1σ uncertainty estimate based on the 16th and 84th posterior percentiles (P₁₆ and P₈₄, respectively) for symmetric, approximately normal posteriors. For asymmetric, unimodal posteriors, the estimates are . ^(a) The semi-major axis and planet candidate radius are based on the scaled semi-major axis and true radius ratio samples, and the stellar radius estimate shown in Table 1. ^(b) The equilibrium temperature of the planet candidate is calculated using the stellar T_Eff estimate, scaled semi-major axis distribution, heat redistribution factor distributed uniformly between 0.25 and 0.5, and planetary albedo distributed uniformly between 0 and 0.4.