Masses versus semimajor axes of planets of our simulated planetary systems (in magenta) compared to the currently known systems around K dwarfs (in blue). Only planets with known masses are presented. Known planets with masses above the super-Earths mass range (above 10 M_⊕) are indicated in light gray. Here, we use the classification of planets by mass proposed by Stevens & Gaudi (2013). The point size indicates the masses in M_⊕ of the planets. The sample of the known systems around K-dwarf stars was retrieved from https://exoplanetarchive.ipac.caltech.edu/ on December 4, 2022.