The Herschel Multi-tiered Extragalactic Survey: HerMES

被引：668

作者：

Oliver, S. J. ^{[1
]}

Bock, J. ^{[2
,3
]}

Altieri, B. ^{[4
]}

Amblard, A. ^{[4
,5
,6
,7
,10
]}

Arumugam, V. ^{[6
]}

Aussel, H. ^{[7
]}

Babbedge, T. ^{[8
]}

Beelen, A. ^{[9
,10
]}

Bethermin, M. ^{[9
,10
]}

Blain, A. ^{[2
]}

Boselli, A. ^{[11
]}

Bridge, C. ^{[2
]}

Brisbin, D. ^{[12
]}

Buat, V. ^{[11
]}

Burgarella, D. ^{[11
]}

Castro-Rodriguez, N. ^{[13
,14
]}

Cava, A. ^{[15
]}

Chania, P.

Cirasuolo, M. ^{[16
]}

Clements, D. L. ^{[8
]}

Conley, A. ^{[17
]}

Conversi, L. ^{[4
]}

Cooray, A. ^{[2
,18
]}

Dowell, C. D. ^{[2
,3
]}

Dubois, E. N. ^{[1
]}

Dwek, E. ^{[19
]}

Dye, S. ^{[20
]}

Eales, S. ^{[21
]}

Elbaz, D. ^{[7
]}

Farrah, D. ^{[1
]}

Feltre, A. ^{[22
]}

Ferrero, P. ^{[13
,14
]}

Fiolet, N. ^{[9
,10
,23
]}

Fox, M. ^{[8
]}

Franceschini, A. ^{[22
]}

Gear, W. ^{[21
]}

Giovannoli, E. ^{[11
]}

Glenn, J. ^{[17
,24
]}

Gong, Y. ^{[18
]}

Solares, E. A. Gonzalez ^{[25
]}

Griffin, M. ^{[21
]}

Halpern, M. ^{[26
]}

Harwit, M.

Hatziminaoglou, E. ^{[27
]}

Heinis, S. ^{[11
]}

Hurley, P. ^{[1
]}

Hwang, H. S. ^{[7
]}

Hyde, A. ^{[8
]}

Ibar, E. ^{[16
]}

Ilbert, O. ^{[11
]}

机构：

[1] Univ Sussex, Dept Phys & Astron, Ctr Astron, Brighton BN1 9QH, E Sussex, England

[2] CALTECH, Pasadena, CA 91125 USA

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

[4] European Space Astron Ctr, Herschel Sci Ctr, Madrid 28691, Spain

[5] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

[6] Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland

[7] Univ Paris Diderot, CE Saclay, Lab AIM Paris Saclay, F-91191 Gif Sur Yvette, France

[8] Univ London Imperial Coll Sci Technol & Med, Astrophys Grp, Blackett Lab, London SW7 2AZ, England

[9] Univ Paris 11, IAS, F-91405 Orsay, France

[10] CNRS, UMR 8617, F-91405 Orsay, France

[11] Univ Aix marseille, CNRS, OAMP, Lab Astrophys Marseille, F-13388 Marseille 13, France

[12] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

[13] IAC, E-38200 San Cristobal la Laguna, Tenerife, Spain

[14] ULL, Dept Astrofis, E-38205 San Cristobal la Laguna, Tenerife, Spain

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

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

[17] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA

[18] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[19] NASA, Observ Cosmol Lab, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[20] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England

[21] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[22] Univ Padua, Dipartmento Astron, I-35122 Padua, Italy

[23] Univ Paris 06, CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France

[24] Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USA

[25] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England

[26] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada

[27] ESO, Garching, Germany

[28] ESTEC SRE SA, ESA Res & Sci Support Dept, NL-2201 AZ Noordwijk, Netherlands

[29] CALTECH, JPL, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA

[30] Univ Manchester, Sch Phys & Astron, Oxford, England

[31] Univ Coll London, Space Sci Lab, Dorking RH5 6NT, Surrey, England

[32] Rutherford Appleton Lab, RAL Space, Chilton, England

[33] Univ Lethbridge, Inst Space Imaging Sci, Lethbridge, AB T1K 3M4, Canada

[34] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England

[35] CSIRO Astron & Space Sci, Epping, NSW 1710, Australia

[36] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2012年 / 424卷 / 03期

基金：

英国科学技术设施理事会;

关键词：

surveys; galaxies: evolution; infrared: galaxies; submillimetre: galaxies; DEEP-FIELD-SOUTH; SPECTRAL ENERGY-DISTRIBUTIONS; STAR-FORMATION HISTORY; LARGE-SCALE STRUCTURE; GOODS-N FIELD; 160; MU-M; ULTRALUMINOUS INFRARED GALAXIES; SUBMILLIMETER-SELECTED GALAXIES; 1200-MU-M MAMBO SURVEY; POLE TELESCOPE SURVEY;

D O I：

10.1111/j.1365-2966.2012.20912.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme designed to map a set of nested fields totalling similar to 380?deg2. Fields range in size from 0.01 to similar to 20?deg2, using the Herschel-Spectral and Photometric Imaging Receiver (SPIRE) (at 250, 350 and 500?mu m) and the Herschel-Photodetector Array Camera and Spectrometer (PACS) (at 100 and 160?mu m), with an additional wider component of 270?deg2 with SPIRE alone. These bands cover the peak of the redshifted thermal spectral energy distribution from interstellar dust and thus capture the reprocessed optical and ultraviolet radiation from star formation that has been absorbed by dust, and are critical for forming a complete multiwavelength understanding of galaxy formation and evolution. The survey will detect of the order of 100?000 galaxies at 5 sigma in some of the best-studied fields in the sky. Additionally, HerMES is closely coordinated with the PACS Evolutionary Probe survey. Making maximum use of the full spectrum of ancillary data, from radio to X-ray wavelengths, it is designed to facilitate redshift determination, rapidly identify unusual objects and understand the relationships between thermal emission from dust and other processes. Scientific questions HerMES will be used to answer include the total infrared emission of galaxies, the evolution of the luminosity function, the clustering properties of dusty galaxies and the properties of populations of galaxies which lie below the confusion limit through lensing and statistical techniques. This paper defines the survey observations and data products, outlines the primary scientific goals of the HerMES team, and reviews some of the early results.

引用

页码：1614 / 1635

页数：22

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