Distributions of ⟨M^*⟩, ⟨SFR⟩, ⟨sSFR⟩, ⟨θ⟩, ⟨cos(4θ)⟩, fraction of quenched galaxies (f_Q), fraction of ordered galaxies (f_Ord), fraction of parallel galaxies (f_∥), and fraction of perpendicular galaxies (f_⊥) as a function of the distances from the features of the cosmic web d_fil (dashed red line in every panel), d_CP (dotted blue line in every panel), and d_skel (solid orange line in every panel). In the case of d_CP and d_skel, only galaxies outside of filaments (d_fil ≥ 1 Mpc) and inside filaments (d_fil ≤ 1 Mpc) have been considered, respectively. Error bars on the distributions have been computed through bootstrap resampling. The dashed black line in every panel is the average of the considered quantity in the full simulation box. In the top and middle panels of the right column, the grey line is and , computed given Eqs. (3) and (4) for the total subhalo sample. In this figure, the dashed grey line corresponding to is hidden behind the dashed black line in the same panel. In every panel, the first distance bin we considered extends all the way to 0 for all distances, but it is cut because the x-axis in in logarithmic scale. In the f_∥ and f_⊥ cases, the y-axes of the plots cover very different ranges.