Deviation of the mean specific star-formation rate for central and satellite galaxies (red, blue: top panel), field and cluster central galaxies (orange-red, orange: middle panel), and satellite of quenched central and star-forming central galaxies (green, purple: bottom panel) from the best-fit relation 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. For each panel, the upper right box shows the deviations of the in-bin medians from the best-fit relation. The V-shaped sSFR–filament distance trend at z = 0 is driven primarily by satellites, particularly those orbiting quenched centrals.