A unified empirical model for infrared galaxy counts based on the observed physical evolution of distant galaxies

Astrophysical Journal Letters

Volumn 757, Issue 2, 2012, Pages

  Béthermin, Matthieu ^a   Daddi, Emanuele ^a   Magdis, Georgios ^b   Sargent, Mark T ^a   Hezaveh, Yashar ^c   Elbaz, David ^a   Le Borgne, Damien ^d,e   Mullaney, James ^a   Pannella, Maurilio ^a   Buat, Véronique ^f   Charmandaris, Vassilis ^g   Lagache, Guilaine ^h   Scott, Douglas ⁱ  

^a CEA SACLAY   (France)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c MCGILL UNIVERSITY   (Canada)

^d SORBONNE UNIVERSITÉ   (France)

^e INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^f OBSERVATOIRE DE MARSEILLE   (France)

^g UNIVERSITY OF CRETE   (Greece)

^h CNRS   (France)

ⁱ UNIVERSITY OF BRITISH COLUMBIA   (Canada)

Author keywords

galaxies: evolution; galaxies: star formation; galaxies: statistics; infrared: galaxies; submillimeter: galaxies

Indexed keywords

EID: 84866549447     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/757/2/L23     Document Type: Article

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