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 in bins of distance at z = 0 (blue), 1 (green), and 2 (red). 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. From left to right, the columns give the results for the full physics, no X-ray feedback, no AGN feedback, and no AGN and stellar feedback in the 50 cMpc³ runs. Removing stellar feedback processes flattens sSFR–distance trends.