Image Details
Caption: Figure 1.
0.1–2.4 keV X-ray luminosity vs. redshift for the broad emission line AGN sample in SDSS DR5 determined by Anderson et al. (2007). Black symbols show objects in the redshift range 0.16 < z < 0.36, which define the AGN sample used here. The dashed line corresponds to the common dividing line between low luminous AGNs and high luminous QSOs ( L 0.5–10 keV X = 10 44 erg s −1) defining the low and high luminosity RASS-AGN samples used here.
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