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X‐Ray Evolution of Active Galactic Nuclei and Hierarchical Galaxy Formation

  • Authors: N. Menci, F. Fiore, G. C. Perola, and A. Cavaliere

Menci et al. 2004 The Astrophysical Journal 606 58.

  • Provider: AAS Journals

Caption: Fig. 8.

Top: Evolution of the number density of X‐ray AGNs in three bins of luminosity (in units of ergs s−1, in the band 2–10 keV): ﹩43< \mathrm{log}\,L_{\mathrm{X}\,}< 44﹩ (dotted line), ﹩44< \mathrm{log}\,L_{\mathrm{X}\,}< 44.5﹩ (solid line), and ﹩44.5< \mathrm{log}\,L_{\mathrm{X}\,}﹩ (dashed line). The data for the above luminosity bins (squares, triangles, and circles, respectively) are taken from Fiore et al. (2003). Bottom: Evolution of the X‐ray luminosity density for the same luminosity bins.

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