%0 Journal Article %T Hidden starbursts and active galactic nuclei at 0 < z < 4 from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback %+ Laboratoire d'Astrophysique de Marseille (LAM) %+ Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)) %A Lemaux, B. C. %A Le Floc’h, E. %A Le Fèvre, O. %A Ilbert, O. %A Tresse, L. %A Lubin, L. M. %A Zamorani, G. %A Gal, R. R. %A Ciliegi, P. %A Cassata, P. %A Kocevski, D. D. %A Mcgrath, E. J. %A Bardelli, S. %A Zucca, E. %A Squires, G. K. %< avec comité de lecture %@ 0004-6361 %J Astronomy and Astrophysics - A&A %I EDP Sciences %V 572 %P A90 %8 2014-12 %D 2014 %R 10.1051/0004-6361/201323089 %K galaxies: active %K galaxies: evolution %K galaxies: high-redshift %K galaxies: starburst %K techniques: spectroscopic %K submillimeter: galaxies %Z Physics [physics]/Astrophysics [astro-ph]Journal articles %X We investigate of the properties of ~2000 Herschel/SPIRE far-infrared-selected galaxies from 0 0.5), the highest LTIR galaxies in a given redshift bin are unobserved by SPIRE at subsequently lower redshifts, a trend linked to downsizing. In conjunction with other results, this evidence is used to argue for prevalent AGN-driven quenching in starburst galaxies across cosmic time. %G English %2 https://cea.hal.science/cea-01290030/document %2 https://cea.hal.science/cea-01290030/file/aa23089-13.pdf %L cea-01290030 %U https://cea.hal.science/cea-01290030 %~ CEA %~ INSU %~ UNIV-PARIS7 %~ CNRS %~ UNIV-AMU %~ CNES %~ LAM %~ OPENAIRE %~ OSU-INSTITUT-PYTHEAS %~ DSM-IRFU %~ IRFU-AIM %~ CERCLE %~ CEA-DRF %~ UNIV-PARIS %~ UP-SCIENCES %~ GS-PHYSIQUE