Star formation in AEGIS field galaxies since z = 1.1: The dominance of gradually declining star formation, and the main sequence of star-forming galaxies

Astrophysical Journal

Volumn 660, Issue 1 II, 2007, Pages

  Noeske, K G ^a   Weiner, B J ^b   Faber, S M ^a   Papovich, C ^b   Koo, D C ^a   Somerville, R S ^c   Bundy, K ^d   Conselice, C J ^e   Newman, J A ^f   Schiminovich, D ^g   Le Floc'h, E ^b   Coil, A L ^b   Rieke, G H ^b   Lotz, J M ^h   Primack, J R ⁱ   Barmby, P ^j   Cooper, M C ^k   Davis, M ^k   Ellis, R S ^d   Fazio, G G ^j   Guhathakurta, P ^a   Huang, J ^j   Kassin, S A ^a   Martin, D C ^d   Phillips, A C ^a   Rich, R M ^l   Small, T A ^d   Wlllmer, C N A ^b   Wilson, G ^m   more..

^a University of California at Santa Cruz   (United States)

^b UNIVERSITY OF ARIZONA   (United States)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^f LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^g Columbia University ^*  (United States)

^h NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^k UNIVERSITY OF CALIFORNIA   (United States)

^l UNIVERSITY OF CALIFORNIA   (United States)

^m CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Galaxies: starburst

Indexed keywords

EID: 34249041519     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/517926     Document Type: Article

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