Fig. B.1.
Distribution of L2 keV (top panel) and L3000 Å (bottom panel) in the luminosity-redshift plane of the 379 sources of our XMM-XXL sample (red and blue respectively), with respect to the parent sample of BLAGN from L16 (black). The dashed red lines broadly represent the sensitivity of the survey at the related frequency (see the text for a description).
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