Final planetary core mass M_core and corresponding envelope mass M_env, as well as total mass M_tot = M_c + M_env and final orbital distance r_f of planets in the evolving disc at a disc dissipation time of 3 Myr. The light blue line represents the initial orbital distance r₀. Planets inside the grey area are subject to very strong migration, so they end up in the inner parts of the disc with r_f< 0.1 AU and become hot gas giants. The divide between ice and gas giants can be seen easily at ~22 AU, where M_c<M_env. All data lines for one r₀ location in this plot give the final result of an individual growth track as in Fig. 2.