Can the unresolved X-ray background be explained by the emission from the optically-detected faint galaxies of the GOODS project?

Monthly Notices of the Royal Astronomical Society

Volumn 368, Issue 4, 2006, Pages 1735-1741

  Worsley, M A ^a   Fabian, A C ^a   Bauer, F E ^b   Alexander, D M ^a   Brandt, W N ^c   Lehmer, B D ^c  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b Och Spine at New York Presbyterian Hospitals   (United States)

^c PENNSYLVANIA STATE UNIVERSITY   (United States)

Author keywords

Galaxies: active; Galaxies: starburst; Surveys; X rays: diffuse background; X rays: galaxies

Indexed keywords

ELECTRON SOURCES; GALAXIES; STARS; X RAY APPARATUS;

ACTIVE GALACTIC NUCLEI; CHANDRA; GALAXIES ACTIVE; GALAXIES: STARBURSTS; HARD X RAY; X-RAY BACKGROUND; X-RAY SOURCES; X-RAYS: DIFFUSE BACKGROUND; X-RAYS: GALAXIES; XMM-NEWTON;

SURVEYS;

EID: 33744544508     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10240.x     Document Type: Article

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