Redshift evolution of the real-space 2PCF, ξ(r), for the selected sub-samples: Gal-dens, low-Z_cold and high-Z_cold, using the same colour and line style keys as described in Fig. 9. The uppermost panels display clustering for knot galaxies, while the lowermost panels show clustering for filament galaxies. Additionally, the fractional difference of ξ(r) with respect to the clustering of the parent samples, ξ(r)_ref , is also presented. From left to right we include the initial redshift of sample selection, z_ref = 0.56, followed by the same four redshift snapshots marked by vertical lines in Fig. 6.