Deviation of the mean star-formation rate, specific star-formation rate, molecular hydrogen depletion time, and gas depletion timescale (top panel, from left to right) 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), 2 (red), and 3 (brown) with the exclusions of galaxies with halo mass M_h > 10¹³ M_⊙. 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. Lower panel: standardised deviation of the same quantities between the values obtained in Fig. 3 and the upper panel. Overall, the results do not deviate significantly from those in Fig. 3.