Deviation of the gas mass accretion rate (left panel) and baryonic mass accretion rate (right panel) from the respective best-fit relations in logarithmic scale as a function of the distance to the closest filament for star-forming galaxies in SIMBA in bins of distance at z = 0 (blue), 1 (green), and 2 (red) for, from top to bottom, all star-forming galaxies, only central star-forming galaxies, and only satellite star-forming galaxies. The arrows pointing to the left give the value for a bin containing all the galaxies not included in the distance range we study here. For each quantity, the upper right box shows the deviation of the in-bin median from the best-fit relation. Gas and baryonic accretion rates closely track sSFR trends, with a dip at intermediate distances and a recovery in filament cores, especially at z ≤ 1.