Development of dual-polarization LEKIDs for CMB observations

被引:3
作者
McCarrick, Heather [1 ]
Abitbol, Maximilian H. [1 ]
Ade, Peter A. R. [5 ]
Barry, Peter [5 ]
Bryan, Sean [2 ]
Che, George [2 ]
Day, Peter [3 ]
Doyle, Simon [5 ]
Flanigan, Daniel [1 ]
Johnson, Bradley R. [1 ]
Jones, Glenn [1 ]
LeDuc, Henry G. [3 ]
Limon, Michele [1 ]
Mauskop, Philip [2 ]
Miller, Amber [1 ]
Tucker, Carole [5 ]
Zmuidzinas, Jonas [3 ,4 ]
机构
[1] Columbia Univ, Dept Phys, New York, NY 10025 USA
[2] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
[3] Jet Prop Lab, Pasadena, CA 91109 USA
[4] CALTECH, Pasadena, CA 91109 USA
[5] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales
来源
MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII | 2016年 / 9914卷
关键词
Lumped element kinetic inductance detectors; cosmic microwave background; polarimetry; dual-polarization;
D O I
10.1117/12.2231830
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the design considerations and initial measurements from arrays of dual-polarization, lumped-element kinetic inductance detectors (LEKIDs) nominally designed for cosmic microwave background (CMB) studies. The detectors are horn-coupled, and each array element contains two single-polarization LEKIDs, which are made from thin-film aluminum and optimized for a single spectral band centered on 150 GHz. We are developing two array architectures, one based on 160 micron thick silicon wafers and the other based on silicon-on-insulator (SOI) wafers with a 30 micron thick device layer. The 20-element test arrays (40 LEKIDs) are characterized with both a linearly-polarized electronic millimeter wave source and a thermal source. We present initial measurements including the noise spectra, noise-equivalent temperature, and responsivity. We discuss future testing and further design optimizations to be implemented.
引用
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页数:7
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