No clear submillimeter signature of suppressed star formation among X-ray luminous active galactic nuclei

Astrophysical Journal Letters

Volumn 760, Issue 1, 2012, Pages

  Harrison, C M ^a   Alexander, D M ^a   Mullaney, J R ^a   Altieri, B ^b   Coia, D ^b   Charmandaris, V ^c   Daddi, E ^d   Dannerbauer, H ^e   Dasyra, K ^f   Del Moro, A ^a   Dickinson, M ^g   Hickox, R C ^h   Ivison, R J ⁱ   Kartaltepe, J ^g   Le Floc'H, E ^d   Leiton, R ^d,j   Magnelli, B ^k   Popesso, P ^k   Rovilos, E ^a   Rosario, D ^k   Swinbank, A M ^a   more..

^a DURHAM UNIVERSITY   (United Kingdom)

^b EUROPEAN SPACE AGENCY   (Spain)

^c UNIVERSITY OF CRETE   (Greece)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e UNIVERSITY OF VIENNA   (Austria)

^f OBSERVATOIRE DE PARIS   (France)

^g NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^h Dartmouth College   (United States)

ⁱ UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^j UNIVERSITY OF CONCEPCIÓN   (Chile)

^k MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

more..

Author keywords

galaxies: active; galaxies: evolution; galaxies: star formation; X rays: general

Indexed keywords

EID: 84868330445     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/760/1/L15     Document Type: Article

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