Faint-source contributions to the extragalactic X-ray background in an XMM deep field

Details Faint-source contributions to the extragalactic X-ray background in an XMM deep field Faint-source contributions to the extragalactic X-ray background in an XMM deep field

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..927s&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

Computer Science

Databases

Observatories And Site Testing, X-Ray Sources, X-Ray Bursts, Background Radiations, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Active And Peculiar Galaxies And Related Systems, Characteristics And Properties Of External Galaxies And Extragalactic Objects

Scientific paper

Two 200-ks XMM Deep Field observations are planned to probe the faint-source populations that make up the hard X-ray background (2-10 keV). We use a simulated 200-ks XMM EPIC-PN Deep Field image, as well as simulated EPIC-PN spectra of potential types of faint-source populations, in order to explore the sensitivity of XMM for resolving the contributors to the hard X-ray background. .

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