The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys

Astronomy and Astrophysics

Volumn 539, Issue , 2012, Pages

  Cucciati, O ^a,b   Tresse, L ^a   Ilbert, O ^a   Le Fevre O ^a   Garilli, B ^a,c   Le Brun, V ^a   Cassata, P ^d   Franzetti, P ^c   MacCagni, D ^a,c   Scodeggio, M ^c   Zucca, E ^e   Zamorani, G ^e   Bardelli, S ^e   Bolzonella, M ^e   Bielby, R M ^f,g   McCracken, H J ^g   Zanichelli, A ^h   Vergani, D ^e  

^a CNRS   (France)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c INAF IASF MILANO   (Italy)

^d UNIVERSITY OF MASSACHUSETTS   (United States)

^e INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^f DURHAM UNIVERSITY   (United Kingdom)

^g INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^h OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

Author keywords

Cosmology: observations; Galaxies: evolution; Galaxies: high redshift; Galaxies: luminosity function, mass function; Galaxies: star formation

Indexed keywords

COSMOLOGY: OBSERVATION; GALAXIES: EVOLUTION; GALAXIES: HIGH-REDSHIFT; GALAXIES: LUMINOSITY FUNCTION, MASS FUNCTION; GALAXIES: STAR FORMATION;

COSMOLOGY; DUST; LUMINANCE; STARS; SURVEYS;

GALAXIES;

EID: 84857546993     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118010     Document Type: Review

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