Galaxy clustering functions in different environments: in the upper panels, we show the real-space two-point correlation function, ξ(r), at z = 0.56 for galaxies in the parent sample, Gal-dens (left panel), and for sub-samples low-Z_cold (middle panel) and high-Z_cold (right panel). In each panel we show the clustering for all galaxies in the sample (dashed black line), knot galaxies (solid yellow line), and filament galaxies (solid blue line with white dots). In the lower panel, we present the fractional difference in the clustering function of the filament and knot populations (ξ(r)), respectively, with respect to the clustering of the entire sample (‘all’, ξ(r)_ref).