Histograms of the matching fraction for disk mass, characteristic radius, stellar mass, and fragmentation velocity. The matching fraction shows the percentage of the simulations that remained on the SLR for the chosen time span (300 kyr − 3 Myr). Top left: dependence on the α-value. There is a preference to low α-values (10⁻⁴ ≤ α ≤ 10⁻³). Top right: dependence on the disk mass. There is a preference to high disk masses . Middle left: dependence on the characteristic radius. Smooth disks do not depend on the r_c. Middle right: dependence on the stellar mass. There is a slight preference to higher values. Bottom left: dependence on the fragmentation velocity. There is a slight preference to higher values.