The 12 μm ISO-ESO-Sculptor* and 24 μm Spitzer faint counts reveal a population of ULIRGs as dusty massive ellipticals Evolution by types and cosmic star formation

Astronomy and Astrophysics

Volumn 475, Issue 3, 2007, Pages 801-812

  Rocca Volmerange, B ^a,b   De Lapparent, V ^a   Seymour, N ^a,c   Fioc, M ^a  

^a INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^b UNIVERSITÉ PARIS SACLAY   (France)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Cosmology: Observations; Galaxies: Evolution; Galaxies: Photometry; Infrared: Galaxies

Indexed keywords

CONSTRAINT THEORY; COSMOLOGY; PHOTOMETRY; STARS; WAVELENGTH;

COSMIC STAR FORMATION; COSMOLOGY OBSERVATIONS; GALAXIES EVOLUTION; INFRARED GALAXIES; SPITZER FAINT COUNTS; STELLAR EMISSION;

GALAXIES;

EID: 36549059673     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065217     Document Type: Article

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