Fabrication of Antenna-Coupled KID Array for Cosmic Microwave Background Detection

被引：2
|
作者：
Tang, Q. Y. [1 ]
Barry, P. S. [1 ]
Thakur, R. Basu [1 ]
Kofman, A. [2 ]
Nadolski, A. [2 ]
Vieira, J. [2 ]
Shirokoff, E. [1 ]
机构：
[1] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[2] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
来源：
JOURNAL OF LOW TEMPERATURE PHYSICS | 2018年 / 193卷 / 3-4期
基金：
美国国家科学基金会;
关键词：
Fabrication; Kinetic inductance detector; Resonators; Sub-mm wavelength;
D O I：
10.1007/s10909-018-1941-0
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
Kinetic inductance detectors (KIDs) have become an attractive alternative to traditional bolometers in the sub-mm and mm observing community due to their innate frequency multiplexing capabilities and simple lithographic processes. These advantages make KIDs a viable option for the O(500,000) detectors needed for the upcoming Cosmic Microwave Background-Stage 4 experiment. We have fabricated an antenna-coupled MKID array in the 150GHz band optimized for CMB detection. Our design uses a twin-slot antenna coupled to an inverted microstrip made from a superconducting Nb/Al bilayer as the strip, a Nb ground plane and a SiN microstrip resonators.
引用
收藏
页码：149 / 156
页数：8
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