The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys - Cucciati, O.; Tresse, L.; Ilbert, O.; Le Fèvre, O.; Garilli, B.; Le Brun, V.; Cassata, P.; Franzetti, P.; Maccagni, D.; Scodeggio, M.; Zucca, E.; Zamorani, G.; et al. (Astronomy and astrophysics (Berlin), 2012)
Keywords: Astronomy; cosmology: observations; Earth, ocean, space; Exact sciences and technology; galaxies: evolution; galaxies: high-redshift; galaxies: luminosity function; galaxies: star formation; mass function; Galaxy evolution; Red shift; Uncertainty; Accretion; Galaxies; galaxies: luminosity function; galaxies: evolution; Spectral energy distribution; Absolute magnitude; galaxies: star formation; Formation rate; Selection function; galaxies: high-redshift; Mass function; Star formation; Stellar mass; Feedback; Galaxy formation; Attenuation; Cosmology; Models; cosmology: observations; Photometry; Luminosity function