Architecture of our simulated planetary systems around a 0.6 M_⊙ and a 0.8 M_⊙ K-dwarf star, for two or four different gas surface density values and different initial disk masses (IDM) after 20 Myr of N-body integration using GENGA. Outcomes for the initial disk mass 5 M_⊕ are not displayed. The point size indicates the masses in M_⊕ of the formed planets. The gray zone is the region inside the inner truncation radius, and the dashed gray line shows the inner edge of the gas disk.