PACS Evolutionary Probe (PEP)-A Herschel key program

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 scientific motivation for the PACS Evolutionary Probe (PEP) guaranteed time key program and its role within the entire set of H...

Celý popis

Podrobná bibliografie
Hlavní autoři: Lutz, D, Poglitsch, A, Altieri, B, Andreani, P, Aussel, H, Berta, S, Bongiovanni, A, Brisbin, D, Cava, A, Cepa, J, Cimatti, A, Daddi, E, Dominguez-Sanchez, H, Elbaz, D, Förster Schreiber, N, Genzel, R, Grazian, A, Gruppioni, C, Harwit, M, Le Floc'H, E, Magdis, G, Magnelli, B, Maiolino, R, Nordon, R, Pérez García, A
Médium: Journal article
Jazyk:English
Vydáno: 2011
Popis
Shrnutí: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 scientific motivation for the PACS Evolutionary Probe (PEP) guaranteed time key program and its role within the entire set of Herschel surveys, and the field selection that includes popular multiwavelength fields such as GOODS, COSMOS, Lockman Hole, ECDFS, and EGS. We provide an account of the observing strategies and data reduction methods used. An overview of first science results illustrates the potential of PEP in providing calorimetric star formation rates for high-redshift galaxy populations, thus testing and superseding previous extrapolations from other wavelengths, and enabling a wide range of galaxy evolution studies. © 2011 ESO, .