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PACS Evolutionary Probe (PEP) - A Herschel Key Program
D. Lutz, A. Poglitsch, B. Altieri +35
Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scienti…
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…
Herschel deep far-infrared counts through the Abell 2218 cluster-lens
B. Altieri, S. Berta, D. Lutz +35
Gravitational lensing by massive galaxy clusters allows study of the population of intrinsically faint infrared galaxies that lie below the sensitivity and confusion limits of curr…
Herschel PEP: The star-formation rates of 1.5<z<2.5 massive galaxies
R. Nordon, D. Lutz, L. Shao +31
The star formation rate (SFR) is a key parameter in the study of galaxy evolution. The accuracy of SFR measurements at z~2 has been questioned following a disagreement between obse…
Star formation in AGN hosts in GOODS-N
L. Shao, D. Lutz, R. Nordon +40
Sensitive Herschel far-infrared observations can break degeneracies that were inherent to previous studies of star formation in high-z AGN hosts. Combining PACS 100 and 160um obser…