SFR_norm ($=\frac{{\mathrm{SFR}}_{\mathrm{AGN}}}{{\mathrm{SFR}}_{\mathrm{non}-\mathrm{AGN}}}$) as a function of L_X. Median values are presented. The errors presented are 1σ, calculated using bootstrap resampling. The top panel presents the SFR_norm-L_X relation for the total AGNs and galaxy control samples (i.e. irrespective of the cosmic environment). For comparison, results from previous studies are also included. The bottom panel presents the SFR_norm-L_X relation for sources in high and low-density fields (see text for more details). The results from Mountrichas et al. (2023) using data in the COSMOS field (open symbols) have been incorporated for comparison.