Residuals deviation as a function of the distance to the filaments after correcting for stellar-mass effects. We show the SFR (top-left), the sSFR (top-right), the molecular hydrogen depletion timescale (middle-left), the total gas depletion timescale (middle-right), the molecular hydrogen fraction (bottom-left), and the gas fraction (bottom-right) for star-forming galaxies in SIMBA in bins of distance at z = 0 (blue), 1 (green), 2 (red), and 3 (brown). The arrows pointing to the left represent galaxies located at smaller distances than the plotted range, grouped into a single bin. For each panel, the upper right box shows the deviation of the in-bin median from the best-fit relation. Star formation and gas properties vary systematically with filament proximity with enhancement near filaments at high-z, but a V-shaped trend in sSFR and τ_H2 at z = 0.