As in Fig. 1, but for fixed α_DZ = 10⁻³ and different values of the planet-to-star mass ratio q (see the plot legend). Two cases of the MRI-active viscosity are considered, namely α_MRI = 5 × 10⁻² (top) and 2.5 × 10⁻² (bottom). Dashed lines correspond to simulations in which the torque is evaluated from the whole disk, without any exclusion of the Hill sphere material. Solid lines are affected by the Hill cut (see Eq. (7)). For comparison purposes, the case of TOI-216b is labelled and marked with an arrow.