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The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel
P. Popesso, A. Biviano, G. Rodighiero +40
Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolu…
GOODS-Herschel and CANDELS: The Morphologies of Ultraluminous Infrared Galaxies at z~2
Jeyhan S. Kartaltepe, Mark Dickinson, David M. Alexander +40
Using deep 100-160 micron observations in GOODS-S from the GOODS-H survey, combined with HST/WFC3 NIR imaging from CANDELS, we present the first morphological analysis of a complet…
The zCOSMOS-SINFONI Project I: Sample Selection and Natural-Seeing Observations
Chiara Mancini, Natascha Foerster Schreiber, Alvio Renzini +21
The zCOSMOS SINFONI project is aimed at studying the physical and kinematical properties of a sample of massive z~1.4-2.5 star-forming galaxies, through SINFONI near-IR integral fi…
Enriched haloes at redshift with no star-formation: Implications for accretion and wind scenarios
N. Bouche, M. T. Murphy, C. Peroux +9
[Abridged] In order to understand which process (e.g. galactic winds, cold accretion) is responsible for the cool (T~10^4 K) halo gas around galaxies, we embarked on a program to s…
FIR measurements of Ly- emitters at z1.0: dust attenuation from PACS-\emph{Herschel}
I. Oteo, A. Bongiovanni, A. M. Pérez García +24
One remaining open question regarding the physical properties of Ly emitters (LAEs) is their dust content and its evolution with redshift. The variety of results is large and wi…
The lesser role of starbursts for star formation at z=2
G. Rodighiero, E. Daddi, I. Baronchelli +31
Two main modes of star formation are know to control the growth of galaxies: a relatively steady one in disk-like galaxies, defining a tight star formation rate (SFR)-stellar mass…