Median cumulative fraction of stellar mass M_star/M_{star, z = 0} for today’s low-mass (first and second rows) and massive (third and fourth rows) members of filaments categorised by environmental history and infall time into filaments compared to the field galaxies (stellar mass is controlled in each panel). Results are shown for two models with solid lines representing the median and shaded regions indicating uncertainty limits across 100 stellar mass-matched realisations. The vertical lines represent the median time when galaxies build 70% of their mass, with a standard deviation between 100 stellar mass fittings. The number of galaxies in each bin of stellar mass and infall time is given in the top-left corner of each panel.