Parameter distributions of the orbital period (P_b), the projected semi-major axis (x), the eccentricity (e), the argument of perigee (ω), the true anomaly (ν), and the intrinsic spin frequency derivative (ḟ_int) resulting from the Monte Carlo simulation assuming M_c = 3.6 M_⊙. The median values and the 68% confidence intervals for each parameter are displayed on top of the columns.