干旱区生态环境知识资源中心(Arid): Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory

Arid

DOI	10.1007/s10909-020-02386-6
	Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory
	Li, Yaqiong 1; Arnold, Kam 2; Atkins, Zachary 1; Bruno, Sarah Marie 1; Cothard, Nicholas F.3; Dober, Bradley 4; Duell, Cody J.3; Duff, Shannon M.5; Gallardo, Patricio A.3; Healy, Erin 1; Ho, Shuay-Pwu Patty 1; Hubmayr, Johannes 5; Keating, Brian 2; Lee, Adrian T.6; Mangu, Aashrita 6; McCarrick, Heather 1; Niemack, Michael D.3; Newburgh, Laura 7; Raum, Christopher 6; Salatino, Maria 8; Sasse, Trevor 6; Silva-Feaver, Maximiliano 2; Simon, Sara M.9; Staggs, Suzanne 1; Suzuki, Aritoki 10; Ullom, Joel 5; Vavagiakis, Eve M.3; Vissers, Michael R.5; Wang, Yuhan 1; Westbrook, Benjamin 6; Wollack, Edward J.11; Xu, Zhilei 12; Zheng, Kaiwen 1; Zhu, Ningfeng 12
通讯作者	Li, Yaqiong
来源期刊	JOURNAL OF LOW TEMPERATURE PHYSICS
ISSN	0022-2291
EISSN	1573-7357
出版年	2020
卷号	199 期号:3-4 页码:985-993
英文摘要	The Simons Observatory will measure the cosmic microwave background temperature and polarization using a suite of new telescopes in the Atacama Desert in Chile. The Simons Observatory will use dichroic transition edge sensor (TES) bolometer arrays spanning six frequency bands from 27 to 280 GHz. The Simons Observatory will pioneer the use of a densely packed multiplexing architecture based on the microwave SQUID multiplexer (mu microwave resonators, each coupled to a TES. The Simons Observatory aims to multiplex each array of similar to 2000 detectors with a single pair of coaxial cables and requires a multiplexing factor of similar to 1000 The Simons Observatory cryogenic readout system is called the universal microwave multiplexing module (UMM). The UMM couples to both horn and lenslet-coupled detector arrays and is integrated into the universal focal-plane module (UFM) after being independently characterized. We present processes we have developed for highly repeatable and automated integration methods of UMMs, which will be needed for the production of the 49 UFMs required for the first stage of the Simons Observatory.
英文关键词	CMB Packaging Multiplexing RF-SQUID Readout TES bolometers
类型	Article
语种	英语
国家	USA
收录类别	SCI-E
WOS记录号	WOS:000531902200051
WOS类目	Physics, Applied ; Physics, Condensed Matter
WOS研究方向	Physics
来源机构	University of California, Berkeley
资源类型	期刊论文
条目标识符	http://119.78.100.177/qdio/handle/2XILL650/318607
作者单位	1.Princeton Univ, Princeton, NJ 08544 USA; 2.Univ Calif San Diego, San Diego, CA 92093 USA; 3.Cornell Univ, Ithaca, NY 14853 USA; 4.Univ Colorado, Boulder, CO 80302 USA; 5.NIST, Boulder, CO 80305 USA; 6.Univ Calif Berkeley, Berkeley, CA 94720 USA; 7.Yale Univ, New Haven, CT 06520 USA; 8.Stanford Univ, Stanford, CA 94305 USA; 9.Univ Michigan, Ann Arbor, MI 48109 USA; 10.Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA; 11.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA; 12.Univ Penn, Philadelphia, PA 19104 USA
推荐引用方式 GB/T 7714	Li, Yaqiong,Arnold, Kam,Atkins, Zachary,et al. Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory[J]. University of California, Berkeley,2020,199(3-4):985-993.
APA	Li, Yaqiong.,Arnold, Kam.,Atkins, Zachary.,Bruno, Sarah Marie.,Cothard, Nicholas F..,...&Zhu, Ningfeng.(2020).Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory.JOURNAL OF LOW TEMPERATURE PHYSICS,199(3-4),985-993.
MLA	Li, Yaqiong,et al."Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory".JOURNAL OF LOW TEMPERATURE PHYSICS 199.3-4(2020):985-993.