Semi-major axis evolution of single planets starting at 5 or 10 AU in discs with S_peb = 2.5. The bodies migrate at four different speeds: (i) the nominal migration speed (purple), (ii) with a nominal type-I migration but a type-II migration of 1/50 of the nominal type-II migration rate (yellow) and (iii) following the Kanagawa et al. (2018) prescription with α_mig = 0.00054 (green) and α_mig = 0.0001 (blue). Reduction of type-II migration does not change the migration path exterior to 1 AU compared to the nominal migration rates, because the transition to type-II migration is too late. The bodies that cross the 1 AU threshold have roughly masses of typical super-Earths to Neptune mass. We do not show the evolution of bodies crossing interior of 0.2 AU.