Hidden starbursts and active galactic nuclei at $0 < z < 4$ from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback

Brian C. Lemaux (1) , Emeric Le Floc'H (2) , Olivier Le Fèvre (1) , Olivier Ilbert (1) , Laurence Tresse (1) , Lori M. Lubin , Giovanni Zamorani , Roy R. Gal , Paolo Ciliegi , Paolo Cassata (1) , Dale D. Kocevski , Elizabeth J. Mcgrath , Sandro Bardelli , Elena Zucca , Gordon K. Squires

1 LAM - Laboratoire d'Astrophysique de Marseille
2 AIM (UMR7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation

We investigate of the properties of $\sim$2000 Herschel/SPIRE-selected galaxies from $00.5$), the highest $L_{TIR}$ 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.

Mots clés: galaxies: active; galaxies: evolution; galaxies: high-redshift; galaxies: starburst; techniques: spectroscopic; submillimeter: galaxies

Domaines: Astrophysique [astro-ph]

Brian C. Lemaux, Emeric Le Floc'H, Olivier Le Fèvre, Olivier Ilbert, Laurence Tresse, et al.. Hidden starbursts and active galactic nuclei at $0 < z < 4$ from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback. Astronomy and Astrophysics - A&A, 2014, 572, pp.A90. ⟨10.1051/0004-6361/201323089e⟩. ⟨hal-01582860⟩