Distribution of ablated mass as a function of semimajor axis (left) and time (right) for the same three simulations as in Fig. E.1. Left: Distribution of ablated mass across the disk after 1 Myr. The values on the y-axis represent the amount of mass that has been ablated in a 0.2 au semimajor axis bin. The dotted lines mark the semimajor axes of the planets. The distribution of ablated mass is very similar in all three simulations, with the majority of mass being lost either just within or just outside of Jupiter’s orbit. Right: Total amount of mass that has been ablated as a function of time for the same data as in the left plot. The colored lines show the average over the five simulations and the colored region shows the one standard deviation away from this value. The ablation rate decreases as the planetesimal formation location with regard to the planet increases; however, the ablation continues for a longer period of time.