Fig. 3.
Distribution of absolute magnitude Mλ310 for each AGN sample. AGNs for which the absolute magnitude was not measured owing to saturation or other selection criteria are counted in the brightest bin. (Color online)
Distribution of absolute magnitude Mλ310 for each AGN sample. AGNs for which the absolute magnitude was not measured owing to saturation or other selection criteria are counted in the brightest bin. (Color online)
