Dust densities distributions with the planet masses reduced by one-half and two-thirds in the Spread configuration (top row) and in the Three-Giants configuration (bottom row). In these simulations, the disk has the smaller aspect ratio and α = 10⁻⁴ with v_frag = 1 m s⁻¹. The masses of the planets mainly change the gap shapes, allowing more or less dust to flow to the inner regions. In the Three-Giants configuration, we also see that more massive planets create more traffic jams in the disk and therefore present more substructures.