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DOI	10.1117/12.2056530
	The Cosmology Large Angular Scale Surveyor (CLASS): 38-GHz detector array of bolometric polarimeters
	Appel, John W.1; Ali, Aamir 1; Amiri, Mandana 5; Araujo, Derek 6; Bennett, Charles L.1; Boone, Fletcher 1; Chan, Manwei 1; Cho, Hsiao-Mei 4; Chuss, David T.2; Colazo, Felipe 2; Crowe, Erik 2; Denis, Kevin 2; Duenner, Rolando 3; Eimer, Joseph 1; Essinger-Hileman, Thomas 1; Gothe, Dominik 1; Halpern, Mark 5; Harrington, Kathleen 1; Hilton, Gene 4; Hinshaw, Gary F.5; Huang, Caroline 1; Irwin, Kent 7; Jones, Glenn 6; Karakla, John 1; Kogut, Alan J.2; Larson, David 1; Limon, Michele 6; Lowry, Lindsay 1; Marriage, Tobias 1; Mehrle, Nicholas 1; Miller, Amber D.6; Miller, Nathan 2; Moseley, Samuel H.2; Novak, Giles 8; Reintsema, Carl 4; Rostem, Karwan 2; Stevenson, Thomas 2; Towner, Deborah 2; U-Yen, Kongpop 2; Wagner, Emily 1; Watts, Duncan 1; Wollack, Edward 2; Xu, Zhilei 1; Zeng, Lingzhen 9
通讯作者	Appel, John W.
会议名称	Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
会议日期	JUN 24-27, 2014
会议地点	Montreal, CANADA
英文摘要	The Cosmology Large Angular Scale Surveyor (CLASS) experiment aims to map the polarization of the Cosmic Microwave Background (CMB) at angular scales larger than a few degrees. Operating from Cerro Toco in the Atacama Desert of Chile, it will observe over 65% of the sky at 38, 93, 148, and 217 GHz. In this paper we discuss the design, construction, and characterization of the CLASS 38 GHz detector focal plane, the first ever Q-band bolometric polarimeter array.
英文关键词	CMB Polarimeter Bolometer TES
来源出版物	MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VII
ISSN	0277-786X
EISSN	1996-756X
出版年	2014
卷号	9153
EISBN	978-0-8194-9621-8
出版者	SPIE-INT SOC OPTICAL ENGINEERING
类型	Proceedings Paper
语种	英语
国家	USA;Chile;Canada
收录类别	CPCI-S
WOS记录号	WOS:000354387400040
WOS关键词	POLARIZATION POWER SPECTRA ; PROBE WMAP OBSERVATIONS ; INFLATIONARY UNIVERSE ; MICROWAVE ; PERFORMANCE ; FLATNESS ; HORIZON ; DESIGN ; NOISE ; MAPS
WOS类目	Astronomy & Astrophysics ; Optics
WOS研究方向	Astronomy & Astrophysics ; Optics
资源类型	会议论文
条目标识符	http://119.78.100.177/qdio/handle/2XILL650/303268
作者单位	1.Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA; 2.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA; 3.Pontificia Univ Catolica Chile, Inst Astrofis, Santiago, Chile; 4.NIST, Boulder, CO 80305 USA; 5.Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada; 6.Columbia Univ, Dept Phys, New York, NY USA; 7.Stanford Univ, Dept Phys, Stanford, CA 94305 USA; 8.Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA; 9.Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
推荐引用方式 GB/T 7714	Appel, John W.,Ali, Aamir,Amiri, Mandana,et al. The Cosmology Large Angular Scale Surveyor (CLASS): 38-GHz detector array of bolometric polarimeters[C]:SPIE-INT SOC OPTICAL ENGINEERING,2014.