Fig. 3.
Infrared-to-1.4 GHz radio luminosity ratio (qTOT) vs. redshift for the HLAGN. The data are color-coded by their median values of AGN fractions. The magenta dashed line is the redshift dependent analytic form calibrated by Delhaize et al. (2017) on a sample of SFGs, with ±1σ spread (magenta area). White dots show the peaks (q̄SF,z) of the underlying qTOT distribution calibrated on the star-forming galaxies in the full radio detected sample.
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