Differences between the original distributions H_O and the re-shuffled ones H_R, normalised to the sum in quadrature of their errors (σ_O and σ_R, respectively) for the quantities ⟨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. In all panels except for ⟨M^*⟩ and ⟨sSFR⟩ (where they would have encompassed the whole range on the y-axis), light grey and dark grey areas show the 0.5σ and 0.2σ range, respectively.