Stacked mass evolution profiles of recent crossers (t _FC < 3 Gyr) subsampled based on their closest filament density as in Figure 8 (left) and those of intermediate crossers (4 ≤ t _FC/Gyr < 9) subsampled by the number of orbits (right). Note that the left and right panels are of different halo samples. Each axis is normalized by the value at the first crossing.