Simulation set A: disk mass after truncation versus dust-to-gas ratio (top panel) and disk viscosity parameter versus the ratio between the disk characteristic radius and the disk truncation radius, r_char/R_trunc (bottom panel). We show planets that became at least more massive than Mars and their color reflects their final planet mass. The shaded contours highlight regions of highest planet density, obtained through a two-dimensional kernel density estimation (KDE) considering planets with masses above 10 M_⊕.