Tracking down the source population responsible for the unresolved cosmic 6-8keV background

Astrophysical Journal

Volumn 758, Issue 2, 2012, Pages

  Xue, Y Q ^a,b   Wang, S X ^a   Brandt, W N ^a   Luo, B ^a   Alexander, D M ^c   Bauer, F E ^d,e   Comastri, A ^f   Fabian, A C ^g   Gilli, R ^f   Lehmer, B D ^h,i   Schneider, D P ^a   Vignali, C ^j   Young, M ^a  

^a PENNSYLVANIA STATE UNIVERSITY   (United States)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^c DURHAM UNIVERSITY   (United Kingdom)

^d PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^e Center for Extrasolar Planetary Studies   (United States)

^f INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^g UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^h JOHNS HOPKINS UNIVERSITY   (United States)

ⁱ NASA GODDARD SPACE FLIGHT CENTER   (United States)

^j UNIVERSITY OF BOLOGNA   (Italy)

more..

Author keywords

diffuse radiation; galaxies: active; surveys; X rays: diffuse background; X rays: galaxies

Indexed keywords

EID: 84867375228     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/758/2/129     Document Type: Article

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