Cumulative distribution plotted for the mass-period bins for young (age < 800 Myr) stars in the sample. Blue dots represent the bin sub-sample FFD, which combines multiple stars by averaging each portion of the FFD by the number of stars that contribute to it. We first calculated initial guess for slope, α_1 ini, and intercept, β_ini, using MMLE method (Maschberger & Kroupa 2009). The initial guess for α_{2 ini} is fixed at 2.0. Then the broken power law was fitted to the distribution, resulting slopes α₁, α₂ (black dash-dotted lines) and break points (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, plotted for a range of ED ∈ [10⁻², 10⁴] days.