Trajectories of pebbles in UP-m001-hw01 case (top) and PI-Stokes-m001-hw01 case (bottom) with different Stokes numbers at the midplane of the disk. We set z_s = 0 for all cases. The red and blue solid lines correspond to the trajectories of pebbles which accreted and did not accrete onto the planet, respectively. The dashed circles show the Hill radius of the planet. The sizes of the Hill and Bondi radii are 0.15 [H] and 0.01 [H]. The black dot at the center of each panel denotes the position of the planet. The interval of pebbles at their initial locations is 0.05 [H]. The regimes of pebble accretion and the planet-induced gas flow are determined by Eqs. (A.4) and (28).