Simulated planetary systems from NGPPS hosting final planets comparable to the observed sample. The criteria are a radius between 2 and 4 R_⊕ and an orbital period between 5 and 60 days. Those planets are marked in the semi-major axis versus total mass plots (left four panels) with larger, dark outlined circles. The rest of the simulated planetary systems containing those planets is shown with transparent circles using the same color-code showing the mass of volatile species accreted as ices compared to the total core mass. The fraction of systems with giants f_giants differs between the two samples. The lower two panels on the left show an earlier stage of the system at the time of disk dispersal. In addition, collision partners of the planets meeting the selection criteria are connected to them with lines. For visual guidance, the mass region from 3 to 20 M_Earth, where most of the (nearly) resonant planets reside, is marked with grey lines.