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DOI | 10.1088/0067-0049/194/2/41 |
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
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ISSN | 0067-0049 |
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 |
推荐引用方式 GB/T 7714 | 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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