Map highlighting the different migration regimes after 0.1 Myr of disc evolution. Upper two plots: red zones show the outward migration regions. The type I and type II migration regimes are distinguished by the solid black line: above it the planets undergo type II migration and below it they undergo type I migration. These two plots are computed with the planetesimal accretion code (top plot) and the pebble accretion code (middle plot) respectively. Third and bottom plot: relative difference we observe between the top two plots. The darker the outcome, the more similar they are.