Antenna-coupled TES Arrays For The BICEP2/Keck and SPIDER polarimeters

被引:8
|
作者
Orlando, A. [1 ]
Aikin, R. W. [1 ]
Amiri, M. [3 ]
Bock, J. J. [1 ,2 ]
Bonetti, J. A. [2 ]
Brevik, J. A. [1 ]
Burger, B. [3 ]
Day, P. K. [2 ]
Filippini, J. P. [1 ]
Golwala, S. R. [1 ]
Halpern, M. [3 ]
Hasselfield, M. [3 ]
Hilton, G. [4 ]
Irwin, K. [4 ]
Jones, W. C. [5 ]
Kenyon, M. [2 ]
Kuo, C. L. [6 ]
Lange, A. E. [1 ]
LeDuc, H. G. [2 ]
Mates, B. [4 ]
Morford, T. [1 ]
Nguyen, H. T. [2 ]
Ogburn, R. W. [1 ]
Reintsema, C. [4 ]
Runyan, M. [1 ]
Sudiwala, R. [1 ]
Trangsrud, A. [1 ]
Turner, A. D. [2 ]
Wilson, P. [2 ]
机构
[1] CALTECH, Dept Phys, 1200 E Calif Blvd, Pasadena, CA 91125 USA
[2] Jet Prop Lab, Pasadena, CA 91109 USA
[3] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T IZL, Canada
[4] NIST, Quantum Devices Grp, Boulder, CO 80305 USA
[5] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[6] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
来源
基金
美国国家航空航天局;
关键词
Cosmic Microwave Background; polarization; TES bolometers; arrays;
D O I
10.1063/1.3292380
中图分类号
O59 [应用物理学];
学科分类号
摘要
The upcoming Cosmic Microwave Background (CMB) experiments BICEP2/Keck and SPIDER will be using planar arrays of polarization sensitive antenna-coupled TES bolometers, operating at frequencies between 960Hz and 220 GHz. At 145 GHz each array consists of 64 polarimeters (128 TES sensors) and four of these arrays are assembled together to make a focal plane. The detector arrays are integrated with a time-domain SQUID multiplexer developed at NIST and read out using the Multi-Channel Electronics (MCE) developed at the University of British Columbia. We present our progress in characterizing focal plane arrays and SQUID multiplexed readout for BICEP2 and SPIDER, describing testing procedures and giving a summary of dark measurements results, as well as preliminary optical measurements.
引用
收藏
页码:471 / +
页数:2
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