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

Volumn 357, Issue 4, 2005, Pages 1281-1287

  Worsley, M A ^a   Fabian, A C ^a   Bauer, F E ^a   Alexander, D M ^a   Hasinger, G ^b   Mateos, S ^c   Brunner, H ^b   Brandt, W N ^d   Schneider, D P ^d  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^d PENNSYLVANIA STATE UNIVERSITY   (United States)

Author keywords

Diffuse radiation; Galaxies: active; Surveys; X rays: diffuse background; X rays: galaxies

Indexed keywords

CHANDRA; CHANDRA DEEP FIELD SOUTHS; DIFFUSE RADIATION; GALAXIES ACTIVE; HARD X RAY; SOURCE POPULATION; X-RAY BACKGROUND; X-RAYS: DIFFUSE BACKGROUND; X-RAYS: GALAXIES; XMM-NEWTON;

GALAXIES;

EID: 15244348085     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08731.x     Document Type: Article

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