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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…
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…
On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3
Stijn Wuyts, Natascha M. Forster Schreiber, Dieter Lutz +23
We compare multi-wavelength SFR indicators out to z~3 in GOODS-South. Our analysis uniquely combines U-to-8um photometry from FIREWORKS, MIPS 24um and PACS 70, 100, and 160um photo…
The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimates
R. Nordon, D. Lutz, R. Genzel +27
We combine Herschel-PACS data from the PEP program with Spitzer 24 um and 16 um photometry and ultra deep IRS mid-infrared spectra, to measure the mid- to far-infrared spectral ene…
The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South
M. Magliocchetti, P. Santini, G. Rodighiero +23
ABRIDGED-This paper presents the first direct estimate of the 3D clustering properties of far-infrared sources up to z~3. This has been possible thanks to the Pacs Evolutionary Pro…
The effect of environment on star forming galaxies at redshift 1 - First insight from PACS
P. Popesso, G. Rodighiero, A. Saintonge +4
We use deep 70, 100 and 160 um observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS Evolutionary Probe (PEP) guar…