The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals

被引：147

作者：

Mauduit, J. -C. ^{[1
]}

Lacy, M. ^{[2
]}

Farrah, D. ^{[3
]}

Surace, J. A. ^{[1
]}

Jarvis, M. ^{[4
]}

Oliver, S. ^{[3
]}

Maraston, C. ^{[5
]}

Vaccari, M. ^{[6
,7
]}

Marchetti, L. ^{[6
]}

Zeimann, G. ^{[8
]}

Gonzales-Solares, E. A. ^{[9
]}

Pforr, J. ^{[5
,10
]}

Petric, A. O. ^{[1
]}

Henriques, B. ^{[2
]}

Thomas, P. A. ^{[2
]}

Afonso, J. ^{[11
,12
]}

Rettura, A. ^{[13
]}

Wilson, G. ^{[13
]}

Falder, J. T. ^{[4
]}

Geach, J. E. ^{[14
]}

Huynh, M. ^{[15
]}

Norris, R. P. ^{[16
]}

Seymour, N. ^{[16
]}

Richards, G. T. ^{[17
]}

Stanford, S. A. ^{[8
,18
]}

Alexander, D. M. ^{[19
]}

Becker, R. H. ^{[8
,18
]}

Best, P. N. ^{[20
]}

Bizzocchi, L. ^{[11
,12
]}

Bonfield, D. ^{[4
]}

Castro, N. ^{[21
]}

Cava, A. ^{[21
]}

Chapman, S. ^{[9
]}

Christopher, N. ^{[22
]}

Clements, D. L. ^{[23
]}

Covone, G. ^{[24
,25
]}

Dubois, N. ^{[3
]}

Dunlop, J. S. ^{[20
]}

Dyke, E. ^{[4
]}

Edge, A. ^{[26
]}

Ferguson, H. C. ^{[27
]}

Foucaud, S. ^{[28
]}

Franceschini, A. ^{[6
]}

Gal, R. R. ^{[29
]}

Grant, J. K. ^{[30
]}

Grossi, M. ^{[11
,12
]}

Hatziminaoglou, E. ^{[31
]}

Hickey, S. ^{[4
]}

Hodge, J. A. ^{[32
]}

Huang, J. -S. ^{[32
]}

机构：

[1] CALTECH, Spitzer Sci Ctr, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA

[2] Natl Radio Astron Observ, Charlottesville, VA 22903 USA

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

[4] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England

[5] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

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

[7] Univ Western Cape, Dept Phys, Astrophys Grp, ZA-7535 Cape Town, South Africa

[8] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

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

[10] Natl Opt Astron Observ, Tucson, AZ 85719 USA

[11] Univ Lisbon, Fac Ciencias, Observ Astron Lisboa, P-1349018 Lisbon, Portugal

[12] Univ Lisbon, Ctr Astron & Astrofis, P-1349018 Lisbon, Portugal

[13] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA

[14] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada

[15] Univ Western Australia, Int Ctr Radio Astron Res, Crawley, WA 6009, Australia

[16] Commonwealth Sci & Ind Res Org, Astron & Space Sci, Epping, NSW 1710, Australia

[17] Drexel Univ, Dept Phys, Philadelphia, PA 19014 USA

[18] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94550 USA

[19] Univ Durham, Dept Phys, Durham DH1 3LE, England

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

[21] Inst Astrofis Canarias, Tenerife 38200, Spain

[22] Oxford Astrophys, Oxford OX1 3RH, England

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

[24] Univ Naples Federico II, Dipartimento Sci Fisiche, I-80126 Naples, Italy

[25] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy

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

[27] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[28] Natl Taiwan Normal Univ, Dept Earth Sci, Taipei 11677, Taiwan

[29] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

[30] Univ Calgary, Inst Space Imaging Sci, Calgary, AB T2N 1N4, Canada

[31] European So Observ, D-85748 Garching, Germany

[32] Max Planck Inst Astron, D-69177 Heidelberg, Germany

[33] Lab Astrophys Marseille, F-13376 Marseille 12, France

[34] Observ Paris, UMR8111, Lab Etud Galaxies Etoiles Phys & Instrumentat GEP, F-92195 Meudon, France

[35] Univ Wisconsin, Dept Astron, Madison, WI 53711 USA

[36] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

[37] CEA, F-91191 Gif Sur Yvette, France

[38] CALTECH, Dept Astron, Pasadena, CA 91125 USA

[39] Cerro Tololo Interamer Observ, La Serena, Chile

[40] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[41] Haverford Coll, Dept Phys & Astron, Haverford, PA 19041 USA

[42] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England

[43] Leibniz Inst Astrophys, D-14482 Potsdam, Germany

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 2012年 / 124卷 / 917期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

DEEP FIELD-SOUTH; ACTIVE GALACTIC NUCLEI; X-RAY SOURCES; GALAXY LUMINOSITY FUNCTION; METREWAVE RADIO TELESCOPE; DIGITAL SKY SURVEY; PHOTOMETRIC REDSHIFTS; MASSIVE GALAXIES; SPACE-TELESCOPE; LOCKMAN HOLE;

D O I：

10.1086/666945

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the Spitzer Extragalactic Representative Volume Survey (SERVS), an 18 deg(2) medium-deep survey at 3.6 and 4.5 mu m with the postcryogenic Spitzer Space Telescope to approximate to 2 mu Jy (AB = 23.1) depth of five highly observed astronomical fields (ELAIS-N1, ELAIS-S1, Lockman Hole, Chandra Deep Field South, and XMM-LSS). SERVSis designed to enable the study of galaxy evolution as a function of environment from z similar to 5 to the present day and is the first extragalactic survey that is both large enough and deep enough to put rare objects such as luminous quasars and galaxy clusters at z greater than or similar to 1 into their cosmological context. SERVS is designed to overlap with several key surveys at optical, near-through far-infrared, submillimeter, and radio wavelengths to provide an unprecedented view of the formation and evolution of massive galaxies. In this article, we discuss the SERVS survey design, the data processing flow from image reduction and mosaicking to catalogs, and coverage of ancillary data from other surveys in the SERVS fields. We also highlight a variety of early science results from the survey.

引用

页码：714 / 736

页数：23

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