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  The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM-Newton deep fields

Worsley, M. A., Fabian, A. C., Bauer, F. E., Alexander, D. M., Hasinger, G., Mateos, S., et al. (2005). The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM-Newton deep fields. Monthly Notices of the Royal Astronomical Society, 357(4), 1281-1287. doi:10.1111/j.1365-2966.2005.08731.x.

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Worsley, M. A., Author
Fabian, A. C., Author
Bauer, F. E., Author
Alexander, D. M., Author
Hasinger, G.1, Author           
Mateos, S., Author
Brunner, H.1, Author           
Brandt, W. N., Author
Schneider, D. P., Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2005-03
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 218195
DOI: 10.1111/j.1365-2966.2005.08731.x
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Title: Monthly Notices of the Royal Astronomical Society
  Alternative Title : Mon. Not. R. astr. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 357 (4) Sequence Number: - Start / End Page: 1281 - 1287 Identifier: ISSN: 1364-8711
ISSN: 0035-8711