Best-fit evolution parameters α_L (upper panel) and α_D (bottom panel) obtained from PLE and PDE fitting forms, respectively. Our estimates (black circles) at each redshift are compared against those by Smolčić et al. (2017c, grey squares), which include both SF and passive hosts of radio-excess AGN. Grey lines by Smolčić et al. (2017c) indicate a declining evolution of (α + z ⋅ β) with redshift, while our data points display a reversal at z ∼ 2 likely ascribed to the lack of passive galaxies that would outnumber SFGs at lower redshifts. See Sect. 4.3 for details.