X-ray counts of Active Galactic Nuclei in Einstein extended medium sensitivity survey

Details X-ray counts of Active Galactic Nuclei in Einstein extended medium sensitivity survey X-ray counts of Active Galactic Nuclei in Einstein extended medium sensitivity survey

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acasn..33..341l&link_type=abstract

Acta Astronomica Sinica (ISSN 0001-5245), vol. 33, no. 4, p. 341-345.

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Sky Surveys (Astronomy), X Ray Astronomy, Background Radiation, Cosmic Rays, Flux Density

Scientific paper

An AGN subsample extracted from an Eistein extended medium sensitivity
survey sample is used to study AGN number density-limiting flux for
fluxes from 5 x 10 exp -14 to 1 x 10 exp -11 erg/sq cm/s in an 0.3-3.5
energy band. It is estimated that 13.5 percent of X-ray background comes
from AGN which are are brighter than 5 x 10 exp -14 erg/sq cm/s.

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