Work

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

Year: 2012

Type: article

Abstract: Aims. We investigate the global galaxy evolution over ~12 Gyr (0.05 ≤ z ≤ 4.5), from the far ultraviolet (FUV) luminosity function (LF), luminosity density (LD), and star formation rate density (SFRD), using the VIMOS-VLT Deep Survey (VVDS), a single deep galaxy redshift survey with a well controlled selection function.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361/201118010

Authors: O. Cucciati, L. Tresse, O. Ilbert, O. Le Fèvre, B. Garilli, V. Le Brun, P. Cassata, P. Franzetti, D. Maccagni, M. Scodeggio, E. Zucca, G. Zamorani, S. Bardelli, M. Bolzonella, R. M. Bielby, H. J. McCracken, A. Zanichelli, D. Vergani

Institutions: Centre National de la Recherche Scientifique, Trieste Astronomical Observatory, Laboratoire d’Astrophysique de Marseille, Université de Provence Aix-Marseille I, National Institute for Astrophysics, University of Massachusetts Amherst, Osservatorio astronomico di Bologna, Durham University, Institut d'Astrophysique de Paris, Université Pierre-et-Marie-Curie, Istituto di Radioastronomia di Bologna

Language: English

Topic: Galaxies: Formation, Evolution, Phenomena

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funder: Centre National de la Recherche Scientifique

OpenAlex ID: W2048081235

FWCI: 12.77

Cites: 104

Cited by: 299

Related to: 9