Best-fitting parameters M_min (upper left panel), α (upper right panel), M_exp (lower left panel), and β (lower right panel) of the exponentially tapered power law (Eq. (19)) at every Keplerian orbital period between t = 36 P_K and t = 40 P_K for all five simulations. Standard errors are plotted as error bars. In the case of the simulation with the smallest box size and the lower resolution, run_0.2_320, only parameter values for t = 36 P_K are plotted because afterwards only four sink particles persist, which prevents us from properly fitting the mass distributions with a power law and an exponential tapering.