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26 April 2024
 
  » arxiv » astro-ph/0105524

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The BeppoSAX High Energy Large Area Survey HELLAS, II: Number counts and X-ray spectral properties
F. Fiore ; P. Giommi ; C. Vignali ; A. Comastri ; G. Matt ; G.C. Perola ; F. La Franca ; S. Molendi ; F. Tamburelli ; L.A. Antonelli ;
Date 30 May 2001
Journal Mon.Not.Roy.Astron.Soc. 327 (2001) 771
Subject astro-ph
AbstractThe BeppoSAX High Energy Large Area Survey (HELLAS) has surveyed about 85 deg^2 of sky in the 5-10 keV band down to a flux of 4-5 10^-14 erg cm-2 s-1. The source surface density of 16.9+-6.4 deg$^{-2}$ at the survey limit corresponds to a resolved fraction of the 5-10 keV X-ray background (XRB) of the order of 20-30 %. Hardness ratios analysis indicates that the spectra of a substantial fraction of the HELLAS sources (at least one third) are harder than a alpha_E = 0.6 power law. This hardness may be due to large absorbing columns. The hardness ratio analysis also indicates that many HELLAS sources may have a spectrum more complex than a single absorbed power law. A soft component, superimposed to a strongly cut-off power law, is likely to be present in several sources.
Source arXiv, astro-ph/0105524
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