Core and envelope mass fractions for different planetary masses immediately before the disc dissipation (at 4 Myr, left panel), and at the end of the simulations (at 50 Myr, right panel). Orange and blue circles represent mass fractions of cores M_core/M_pl and envelopes M_env/M_pl, respectively. Mass ratios for the core and envelope change significantly for Es/SEs due to the planet-planet collisions after disc dissipation.