Same as Fig. 5 but with a Jupiter mass planet and its Type II migration. The purple and light blue plots represent the profiles with Ṁ_peb = 10⁻⁵ and 10⁻⁴ M_E yr⁻¹ in Disc A, respectively. The rate to insert the super-particles of pebbles is 10 times lower and the duration of the time step is 10 times longerthan those of the normal cases to make the calculation time shorter. The calculations are stopped when the planets reach about 0.9 au. The time of the snapshots in the lower panel are t = 1.1 × 10⁶, 2.3 × 10⁶, and 2.7 × 10⁶ yr.