PACS Evolutionary Probe (PEP) – A Herschel key program

D. Lutz; A. Poglitsch; B. Altieri; P. Andreani; H. Aussel; S. Berta; A. Bongiovanni; D. Brisbin; A. Cava; J. Cepa; A. Cimatti; E. Daddi; H. Dominguez-Sanchez; D. Elbaz; N. M. Förster Schreiber; R. Genzel; A. Grazian; C. Gruppioni; M. Harwit; E. Le Floc’h; G. Magdis; B. Magnelli; R. Maiolino; R. Nordon; A. M.  Pérez García; P. Popesso; F. Pozzi; L. Riguccini; G. Rodighiero; A. Saintonge; M. Sanchez Portal; P. Santini; L. Shao; E. Sturm; L. J. Tacconi; I. Valtchanov; M. Wetzstein; E. Wieprecht

doi:10.1051/0004-6361/201117107

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Volume 532 (August 2011)

A&A, 532 (2011) A90

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Fig. 12

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Red: Total infrared luminosity of GOODS-N sources detected above 3σ in the PEP SDP data. Blue: Sources from the GOODS-S and COSMOS data illustrate the potential of the full PEP survey.

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