Paper
0
The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveys
Authors
O. Cucciati,L. Tresse
O. Ilbert,O. Le Fevre,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,O. Fèvre,V. Brun,R. Bielby,H. McCracken
+20 authors
,C. AdamiJournal
Published
Jan 6, 2012
Show more
Save
Tip0
TipSave
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.
Paper PDF
This paper's license is marked as closed access or non-commercial and cannot be viewed on ResearchHub. Visit the paper's external site.