Comparison of the cumulative mass distributions after 100 Myr for different populations of planets with K ≳ 10 m s^-1. The black solid line denotes the distribution for observed exoplanets, the red dashed line for the reference population (R), the blue dot-dashed line for the population without eccentricity and inclination damping (ND), and the green dotted line for the population with 20 intial embryo seeds (E20).