Angular TPCF of mock galaxies and radio sources. Left: Angular TPCF of mock EGG galaxies with stellar mass > 10¹⁰ M_⊙ at different redshift bins. A straight line with power law slope of −1 is also plotted. Middle: Angular TPCF of redistributed mock EGG galaxies with stellar mass > 10¹⁰ M_⊙ at different redshift bins. A straight line with power law slope of −1 is also plotted. Solid and dashed lines represent active and passive galaxies respectively. Right: Angular TPCF of our mock radio AGNs with 3 GHz flux density above 13 μJy. We also plot the best-fit model from Hale et al. (2018) with a slope of −0.8. The vertical dotted line denotes the clump radius of 3′ (see Sect. 2.4).