Evolution of the dusty infrared luminosity function from z = 0 to z = 2.3 using observations from Spitzer

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Magnelli, B ^a,b   Elbaz, D ^a   Chary, R R ^c   Dickinson, M ^d   Le Borgne, D ^e,f   Frayer, D T ^g   Willmer, C N A ^h  

^a CEA SACLAY   (France)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^e SORBONNE UNIVERSITÉ   (France)

^f INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^g NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^h UNIVERSITY OF ARIZONA   (United States)

Author keywords

cosmology: observations; galaxies: starburst; galaxy: evolution; infrared: galaxies

Indexed keywords

A-DENSITY; BEST FIT; COSMOLOGY: OBSERVATION; EXTRACTION TECHNIQUES; FORMATION RATES; GALAXIES: STARBURSTS; GALAXY: EVOLUTION; INFRARED LUMINOSITY; INFRARED: GALAXIES; ON-LINE MATERIALS; RED SHIFT; REDSHIFT RANGE; SHORTER WAVELENGTH; SOURCE POSITION; SPECTRAL ENERGY DISTRIBUTION; SPITZER;

COSMOLOGY; GALAXIES; LIBRARIES; SPECTROSCOPY;

LUMINANCE;

EID: 79952180729     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913941     Document Type: Article

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