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.; Brunner, H.; Brandt, W. N.; Schneider, D. P.

doi:10.1111/j.1365-2966.2005.08731.x

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

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Hasinger, G.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Brunner, H.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-DAF8-C

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