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The properties of X-ray-selected active galactic nuclei. I - Luminosity function, cosmological evolution, and contribution to the diffuse X-ray background

Journal Article · · Astrophysical Journal; (United States)
DOI:https://doi.org/10.1086/170102· OSTI ID:5392766
; ; ; ;  [1]
  1. Osservatorio Astronomico, Bologna (Italy) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA) Bologna, Universita (Italy) CNR, Istituto di Radioastronomia, Bologna (Italy) Observatories of the Carnegie Institution of Washington, Pasadena, CA (USA) Colorado, University, Boulder (USA)
X-ray luminosity functions (XLFs) and their implications for cosmological evolution are determined for 420 X-ray-selected active galactic nuclei (AGN). The local XLFs flatten considerably when L(x) is less than or equal to 5 x 10 to the 42nd ergs/s, and higher-luminosity XLF are demonstrated to fit a power-law approximation. Cosmological evolution in terms of two pure-luminosity evolutionary models is directly supported by model-independent AGN XLF, showing weak evolution when z is less than 0.4 and more pronounced evolution at higher z. The parameter C is determined for the two models, and the values support the 'slower' evolution of these AGN relative to QSOs selected optically. The deevolved XLF best-fit slope is found to be 3.05 for high luminosities and 1.35 for low luminosities, with no evidence of slope changes for other luminosities. 38 refs.
OSTI ID:
5392766
Journal Information:
Astrophysical Journal; (United States), Journal Name: Astrophysical Journal; (United States) Vol. 374; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English