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

B. C. Lemaux (1) , E. Le Floc’h (2) , O. Le Fèvre (1) , O. Ilbert (1) , L. Tresse (1) , L. M. Lubin , G. Zamorani , R. R. Gal , P. Ciliegi , P. Cassata (1) , D. D. Kocevski , E. J. Mcgrath , S. Bardelli , E. Zucca , G. 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 ~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.

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

Domains: Astrophysics [astro-ph]

B. C. Lemaux, E. Le Floc’h, O. Le Fèvre, O. Ilbert, L. 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. ⟨10.1051/0004-6361/201323089⟩. ⟨cea-01290030⟩