Distributions of the mean galaxy stellar mass (top) and SFR (bottom) as a function of the distance to the filaments (d_fil) for galaxies with logM_⋆/M_⊙ >  9.0. Results are shown for the C1 (R = 1000) and the C2 (R = 2000) configurations. The vertical dashed line indicates the reconstruction scales of 4 and 2.5 Mpc for the C1 and C2 configuration, respectively. The dotted black lines show the mass gradient in the original field when all the filaments (not only the densest 50%) are kept in the analysis.