Summary of results for the nominal setup at the end of the simulations as a function of the initial disc mass and α-viscosity. The horizontal axis also shows the initial mass of dust in the disc. M_P denotes the total planet mass, M_core the core mass, M_env the mass of H-He envelope, and M_peb the total mass of pebbles that drifted through the position of the embryo. All masses in the squares are in M_⊕. f_HHe is the mass fraction of H-He of the planet as a percentage. Cases where planets remain as lunar-mass embryos are colored in grey. Planets that are rocky-dominated (f_HHe < 30%) and gas-dominated (f_HHe > 30%) with masses larger than that of Mars are highlighted in green and yellow, respectively. Boxes with thick borders indicate that the core growth was truncated by reaching the pebble isolation mass (see also Table 3).