Proceedings Paper • new
Characterization of a 0.35 THz aluminum 64-pixel MKID array| Format | Member Price | Non-Member Price |
|---|---|---|
| $17.00 | $21.00 |
Paper Abstract
Microwave Kinetic Inductance Detectors (MKID) are a promising low temperature superconducting detector because of high sensitivity, easy frequency-domain multiplexing and simple structure for large-format arrays. To develop large-format THz detectors for China’s Antarctic THz telescope, we have preliminarily designed an aluminum 64-pixel MKID array operating at the 350 GHz band. In this paper, the characteristics of the MKID array are thoroughly measured.
Paper Details
Date Published: 18 November 2019
PDF: 8 pages
Proc. SPIE 11196, Infrared, Millimeter-Wave, and Terahertz Technologies VI, 111960S (18 November 2019); doi: 10.1117/12.2537092
Published in SPIE Proceedings Vol. 11196:
Infrared, Millimeter-Wave, and Terahertz Technologies VI
Cunlin Zhang; Xi-Cheng Zhang; Masahiko Tani, Editor(s)
PDF: 8 pages
Proc. SPIE 11196, Infrared, Millimeter-Wave, and Terahertz Technologies VI, 111960S (18 November 2019); doi: 10.1117/12.2537092
Show Author Affiliations
Qing Shi, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Wei-tao Lv, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Bowen Fan, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Zhi Li, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Wei-tao Lv, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Bowen Fan, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Zhi Li, Purple Mountain Observatory (China)
Univ. of Science and Technology of China (China)
Key Lab. of Radio Astronomy (China)
Zheng Wang, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Jing Li, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Sheng-Cai Shi, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Zhen-Hui Lin, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Key Lab. of Radio Astronomy (China)
Jing Li, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Sheng-Cai Shi, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Zhen-Hui Lin, Purple Mountain Observatory (China)
Key Lab. of Radio Astronomy (China)
Published in SPIE Proceedings Vol. 11196:
Infrared, Millimeter-Wave, and Terahertz Technologies VI
Cunlin Zhang; Xi-Cheng Zhang; Masahiko Tani, Editor(s)
© SPIE. Terms of Use
