Fig. 1.
AGN bolometric luminosity (Lbol) as a function of redshift (z) of our sample (red triangles). Also plotted are the known high redshift quasars from the compiled catalogue of Bañados et al. (2016), the catalogue of SDSS detections of Jiang et al. (2016) and the new detections of Mazzucchelli et al. (2017), from which the majority of our sample has been selected.
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