Cumulative distribution for the mass-period bins of all stars in this study sample. Blue dots represent the bin sub-sample FFD, which takes to account multiple stars by averaging each portion of the FFD by the number of stars that contribute to it. Initial guess for slope α_{1 ini} and intercept β_ini from MMLE method as before were used to fit the broken power law was to the distribution resulting slopes α₁, α₂ (black dash-dotted lines) and break points indicated by black dashed lines, if the fit was successful. The grey and blue dashed guides corresponding to power law coefficient α = 2.0 and α = 1.5, respectively, are plotted for a range of ED ∈[10⁻², 10⁴] days.