The XMM-newton wide field survey in the cosmos field: Redshift evolution of agn bias and subdominant role of mergers in triggering moderate-luminosity AGNs at redshifts up to 2.2

Astrophysical Journal

Volumn 736, Issue 2, 2011, Pages

  Allevato, V ^a   Finoguenov, A ^b,c   Cappelluti, N ^c,d   Miyaji, T ^e,f,n   Hasinger, G ^a   Salvato, M ^a,g,h   Brusa, M ^b   Gilli, R ^d   Zamorani, G ^d   Shankar, F ⁱ   James, J B ^j,k   McCracken, H J ^l   Bongiorno, A ^b   Merloni, A ^b,g   Peacock, J A ^j   Silverman, J ^m   Comastri, A ^d  

^a MAX PLANCK INSTITUT FÜR PLASMAPHYSIK   (Germany)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c NATIONAL SPACE SCIENCE AND TECHNOLOGY CENTER   (United States)

^d INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^e UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g EXCELLENCE CLUSTER UNIVERSE   (Germany)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^j UNIVERSITY OF CALIFORNIA   (United States)

^k UNIVERSITY OF COPENHAGEN   (Denmark)

^l OBSERVATOIRE DE PARIS   (France)

^m UNIVERSITY OF TOKYO   (Japan)

ⁿ NONE   (United States)

more..

Author keywords

dark matter; galaxies: active; galaxies: evolution; large scale structure of universe; quasars: general; surveys

Indexed keywords

EID: 80051484340     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/736/2/99     Document Type: Article

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