PACS Evolutionary Probe (PEP) - A Herschel key program

被引:390
作者
Lutz, D. [1 ]
Poglitsch, A. [1 ]
Altieri, B. [2 ]
Andreani, P. [3 ,4 ]
Aussel, H. [5 ]
Berta, S. [1 ]
Bongiovanni, A. [6 ,7 ]
Brisbin, D. [8 ]
Cava, A. [12 ]
Cepa, J. [6 ,7 ]
Cimatti, A. [9 ]
Daddi, E. [5 ]
Dominguez-Sanchez, H. [9 ]
Elbaz, D. [5 ]
Schreiber, N. M. Foerster [1 ]
Genzel, R. [1 ]
Grazian, A. [10 ]
Gruppioni, C. [9 ]
Harwit, M. [8 ]
Le Floc'h, E. [5 ]
Magdis, G. [5 ]
Magnelli, B. [1 ]
Maiolino, R. [10 ]
Nordon, R. [1 ]
Perez Garcia, A. M. [6 ,7 ]
Popesso, P. [1 ]
Pozzi, F. [9 ]
Riguccini, L. [5 ]
Rodighiero, G. [11 ]
Saintonge, A. [1 ]
Sanchez Portal, M. [2 ]
Santini, P. [1 ,10 ]
Shao, L. [1 ]
Sturm, E. [1 ]
Tacconi, L. J. [1 ]
Valtchanov, I. [2 ]
Wetzstein, M. [1 ]
Wieprecht, E. [1 ]
机构
[1] MPE, D-85741 Garching, Germany
[2] European Space Astron Ctr, Villafranca Del Castillo, Spain
[3] European So Observ, D-85748 Garching, Germany
[4] INAF Osservatorio Astron Trieste, I-34143 Trieste, Italy
[5] CEA Saclay, IRFU Serv Astrophys, F-91191 Gif Sur Yvette, France
[6] Inst Astrofis Canarias, San Cristobal la Laguna 38205, Spain
[7] Univ La Laguna, Dept Astrofis, E-38207 San Cristobal la Laguna, Spain
[8] Cornell Univ, Ithaca, NY 14853 USA
[9] Osservatorio Astron Bologna, Ist Nazl Astron, I-40127 Bologna, Italy
[10] INAF Osservatorio Astron Roma, I-00040 Monte Porzio Catone, Italy
[11] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[12] Univ Complutense Madrid, Fac CC Fis, Dept Astrofis, E-28040 Madrid, Spain
来源
ASTRONOMY & ASTROPHYSICS | 2011年 / 532卷
关键词
surveys; galaxies: evolution; galaxies: active; infrared: galaxies; STAR-FORMATION HISTORY; DEEP-FIELD-SOUTH; SIMILAR-TO; 3; LUMINOUS INFRARED GALAXIES; ACTIVE GALACTIC NUCLEI; HIGH-REDSHIFT; SUBMILLIMETER GALAXIES; MASSIVE GALAXIES; FORMING GALAXIES; SPITZER VIEW;
D O I
10.1051/0004-6361/201117107
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
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页数:12
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