Deviation of the mean specific star-formation rate (top) and molecular hydrogen depletion timescale (bottom) from the respective best-fit relations in logarithmic scale as a function of d_fil in SIMBA at z = 0, using different selection criteria for star-forming galaxies. For each panel, the upper right box shows the deviation of the in-bin median from the best-fit relation. The qualitative sSFR and τ_H2 trends with filament distance at z = 0 are robust against variations in the star-forming selection criteria.