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DOI10.1088/0067-0049/194/2/41
OVERVIEW OF THE ATACAMA COSMOLOGY TELESCOPE: RECEIVER, INSTRUMENTATION, AND TELESCOPE SYSTEMS
Swetz, D. S.1,2; Ade, P. A. R.3; Amiri, M.4; Appel, J. W.5; Battistelli, E. S.4,6; Burger, B.4; Chervenak, J.7; Devlin, M. J.1; Dicker, S. R.1; Doriese, W. B.2; Duenner, R.8; Essinger-Hileman, T.5; Fisher, R. P.5; Fowler, J. W.5; Halpern, M.4; Hasselfield, M.4; Hilton, G. C.2; Hincks, A. D.5; Irwin, K. D.2; Jarosik, N.5; Kaul, M.1; Klein, J.1; Lau, J. M.5,9,10; Limon, M.1,5,11; Marriage, T. A.12; Marsden, D.1; Martocci, K.5,13; Mauskopf, P.3; Moseley, H.7; Netterfield, C. B.14; Niemack, M. D.2,5; Nolta, M. R.15; Page, L. A.5; Parker, L.5; Staggs, S. T.5; Stryzak, O.5; Switzer, E. R.5,13; Thornton, R.1,16; Tucker, C.3; Wollack, E.7; Zhao, Y.5
通讯作者Swetz, D. S.
来源期刊ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
ISSN0067-0049
出版年2011
卷号194期号:2
英文摘要

The Atacama Cosmology Telescope was designed to measure small-scale anisotropies in the cosmic microwave background and detect galaxy clusters through the Sunyaev-Zel’dovich effect. The instrument is located on Cerro Toco in the Atacama Desert, at an altitude of 5190 m. A 6 m off-axis Gregorian telescope feeds a new type of cryogenic receiver, the Millimeter Bolometer Array Camera. The receiver features three 1000-element arrays of transition-edge sensor bolometers for observations at 148 GHz, 218 GHz, and 277 GHz. Each detector array is fed by free space millimeter-wave optics. Each frequency band has a field of view of approximately 22’ x 26’. The telescope was commissioned in 2007 and has completed its third year of operations. We discuss the major components of the telescope, camera, and related systems, and summarize the instrument performance.


英文关键词cosmic background radiation cosmology: observations instrumentation: detectors instrumentation: miscellaneous telescopes
类型Article
语种英语
国家USA ; Wales ; Canada ; Italy ; Chile
收录类别SCI-E
WOS记录号WOS:000291675700025
WOS关键词MICROWAVE-ANISOTROPY-PROBE ; BACKGROUND POWER SPECTRUM ; OPTICAL DESIGN ; ARRAY CAMERA ; 148 GHZ ; ACT ; POLARIZATION ; FABRICATION
WOS类目Astronomy & Astrophysics
WOS研究方向Astronomy & Astrophysics
资源类型期刊论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/167205
作者单位1.Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA;
2.NIST Quantum Devices Grp, Boulder, CO 80305 USA;
3.Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales;
4.Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada;
5.Princeton Univ, Joseph Henry Labs Phys, Princeton, NJ 08544 USA;
6.Univ Roma La Sapienza, Dept Phys, I-00185 Rome, Italy;
7.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA;
8.Pontificia Univ Catolica Chile, Fac Fis, Dept Astron & Astrofis, Santiago 22, Chile;
9.Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA;
10.Stanford Univ, Dept Phys, Stanford, CA 94305 USA;
11.Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA;
12.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA;
13.Kavli Inst Cosmol Phys, Chicago, IL 60637 USA;
14.Univ Toronto, Dept Phys, Toronto, ON M5S 1A7, Canada;
15.Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada;
16.W Chester Univ Penn, Dept Phys, W Chester, PA 19383 USA
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Swetz, D. S.,Ade, P. A. R.,Amiri, M.,et al. OVERVIEW OF THE ATACAMA COSMOLOGY TELESCOPE: RECEIVER, INSTRUMENTATION, AND TELESCOPE SYSTEMS[J],2011,194(2).
APA Swetz, D. S..,Ade, P. A. R..,Amiri, M..,Appel, J. W..,Battistelli, E. S..,...&Zhao, Y..(2011).OVERVIEW OF THE ATACAMA COSMOLOGY TELESCOPE: RECEIVER, INSTRUMENTATION, AND TELESCOPE SYSTEMS.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,194(2).
MLA Swetz, D. S.,et al."OVERVIEW OF THE ATACAMA COSMOLOGY TELESCOPE: RECEIVER, INSTRUMENTATION, AND TELESCOPE SYSTEMS".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 194.2(2011).
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