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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. 4.

Energy spectrum of the predicted CXB for ﹩E\geq 30﹩ keV, for different ranges of luminosity of the contributing sources. Symbols are as in Fig. 1. Data are from Gruber et al. (1999).

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