How dead are dead galaxies? Mid-infrared fluxes of quiescent galaxies at redshift 0.3 < z < 2.5: Implications for star formation rates and dust heating

Astrophysical Journal

Volumn 796, Issue 1, 2014, Pages

  Fumagalli, Mattia ^a   Labbé, Ivo ^a   Patel, Shannon G ^a   Franx, Marijn ^a   Van Dokkum, Pieter ^b   Brammer, Gabriel ^c   Da Cunha, Elisabete ^d   Schreiber, Natascha M Förster ^e   Kriek, Mariska ^f   Quadri, Ryan ^g   Rix, Hans Walter ^d   Wake, David ^h,i   Whitaker, Katherine E ^j   Lundgren, Britt ^h   Marchesini, Danilo ^k   Maseda, Michael ^d   Momcheva, Ivelina ^b   Nelson, Erica ^b   Pacifici, Camilla ^l   Skelton, Rosalind E ^m  

^a LEIDEN UNIVERSITY   (Netherlands)

^b YALE UNIVERSITY   (United States)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g CARNEGIE OBSERVATORIES   (United States)

^h UNIVERSITY OF WISCONSIN MADISON   (United States)

ⁱ OPEN UNIVERSITY   (United Kingdom)

^j NASA GODDARD SPACE FLIGHT CENTER   (United States)

^k TUFTS UNIVERSITY   (United States)

^l Yonsei University   (South Korea)

^m SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

more..

Author keywords

galaxies: evolution; galaxies: formation

Indexed keywords

EID: 84909641348     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/796/1/35     Document Type: Article

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