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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. 6.

Top: 20–100 keV flux distribution of AGNs contributing to the CXB at 30 keV for different bins of redshift (see labels in the bottom panel). Bottom: Fraction of the CXB contributed by sources brighter than the value in abscissa, for the different redshift shells.

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