The Herschel Lensing Survey (HLS): Overview

被引：91

作者：

Egami, E. ^{[1
]}

Rex, M. ^{[1
]}

Rawle, T. D. ^{[1
]}

Perez-Gonzalez, P. G. ^{[1
,2
]}

Richard, J. ^{[3
]}

Kneib, J. -P. ^{[4
]}

Schaerer, D. ^{[5
,6
]}

Altieri, B. ^{[7
]}

Valtchanov, I. ^{[7
]}

Blain, A. W.

Fadda, D. ^{[17
]}

Zemcov, M. ^{[18
]}

Bock, J. J. ^{[18
]}

Boone, F. ^{[6
,8
]}

Bridge, C. R.

Clement, B. ^{[4
]}

Combes, F. ^{[8
]}

Dessauges-Zavadsky, M. ^{[5
]}

Dowell, C. D. ^{[8
]}

Ilbert, O. ^{[4
]}

Ivison, R. J. ^{[15
,16
]}

Jauzac, M. ^{[4
]}

Lutz, D. ^{[14
]}

Metcalfe, L. ^{[7
]}

Omont, A. ^{[12
,13
]}

Pello, R. ^{[6
]}

Pereira, M. J. ^{[1
]}

Rieke, G. H. ^{[1
]}

Rodighiero, G. ^{[11
]}

Smail, I. ^{[3
]}

Smith, G. P. ^{[10
]}

Tramoy, G. ^{[4
]}

Walth, G. L. ^{[1
]}

van der Werf, P. ^{[9
]}

Werner, Andm. W. ^{[18
]}

机构：

[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[2] Univ Complutense Madrid, Dept Astrofis, Fac CC Fis, E-28040 Madrid, Spain

[3] Univ Durham, Inst Computat Cosmol, Dept Phys, Durham DH1 3LE, England

[4] Univ Aix Marseille, CNRS, Lab Astrophys Marseille, F-13388 Marseille 13, France

[5] Univ Geneva, Observ Geneva, CH-1290 Versoix, Switzerland

[6] Univ Toulouse, CNRS, Lab Astrophys Toulouse Tarbes, F-31400 Toulouse, France

[7] ESA, ESAC, Herschel Sci Ctr, Madrid 28691, Spain

[8] Observ Paris, LERMA, F-75014 Paris, France

[9] Leiden Univ, Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands

[10] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[11] Univ Padua, Dept Astron, I-35122 Padua, Italy

[12] Univ Paris 06, F-75014 Paris, France

[13] CNRS, Inst Astrophys Paris, F-75014 Paris, France

[14] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany

[15] Univ Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland

[16] Royal Observ, Sci & Technol Facil Council, UK Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland

[17] CALTECH, NASA Herschel Sci Ctr, Pasadena, CA 91125 USA

[18] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2010年 / 518卷

关键词：

infrared: galaxies; submillimeter: galaxies; galaxies: evolution; galaxies: high-redshift; galaxies: clusters: general; BULLET CLUSTER 1E0657-56; STAR-FORMATION; SUBMILLIMETER GALAXIES; INFRARED GALAXY; SPITZER VIEW; BRIGHT; COUNTS;

D O I：

10.1051/0004-6361/201014696

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Herschel Lensing Survey (HLS) will conduct deep PACS and SPIRE imaging of similar to 40 massive clusters of galaxies. The strong gravitational lensing power of these clusters will enable us to penetrate through the confusion noise, which sets the ultimate limit on our ability to probe the Universe with Herschel. Here we present an overview of our survey and a summary of the major results from our science demonstration phase (SDP) observations of the Bullet cluster (z = 0.297). The SDP data are rich and allow us to study not only the background high-redshift galaxies (e. g., strongly lensed and distorted galaxies at z = 2.8 and 3.2) but also the properties of cluster-member galaxies. Our preliminary analysis shows a great diversity of far-infrared/submillimeter spectral energy distributions (SEDs), indicating that we have much to learn with Herschel about the properties of galaxy SEDs. We have also detected the Sunyaev-Zel'dovich (SZ) effect increment with the SPIRE data. The success of this SDP program demonstrates the great potential of the Herschel Lensing Survey to produce exciting results in a variety of science areas.

引用

页数：5

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