Reduction of the pebble flux through accreting planets. Each line shows the pebble flux in a given heliocentric distance bin at a given time averaged over all simulations for an initial configuration of planetesimals. The panels are as follows: narrow rings (top), wide rings (middle), and high-mass wide rings (bottom). The initial location of the planetesimals (grey area) and the 50 and 80% reduction levels (dashed lines) are shown for reference.