The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey

Astronomy and Astrophysics

Volumn 534, Issue , 2011, Pages

  Lusso, E ^a,b   Comastri, A ^b   Vignali, C ^a,b   Zamorani, G ^b   Treister, E ^c,i   Sanders, D ^c   Bolzonella, M ^b   Bongiorno, A ^d   Brusa, M ^d   Civano, F ^f   Gilli, R ^b   Mainieri, V ^g   Nair, P ^b   Aller, M C ^h   Carollo, M ^h   Koekemoer, A M ^k   Merloni, A ^d,e   Trump, J R ^j  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c UNIVERSITY OF HAWAII   (United States)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e EXCELLENCE CLUSTER UNIVERSE   (Germany)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^h ETH ZURICH   (Switzerland)

ⁱ UNIVERSITY OF CONCEPCIÓN   (Chile)

^j University of California Santa Cruz   (United States)

^k STScI   (United States)

more..

Author keywords

Galaxies: active; Galaxy: general; Methods: statistical; Quasars: general; X rays: general

Indexed keywords

GALAXIES : ACTIVE; GALAXY: GENERAL; METHODS: STATISTICAL; QUASARS: GENERAL; X-RAYS: GENERAL;

INFRARED DEVICES; LUMINANCE; SPECTROSCOPY; SPECTRUM ANALYSIS; STARS; SURVEYS; X RAYS;

GALAXIES;

EID: 80054751626     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117175     Document Type: Article

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