Proceedings Paper
Developments of wide field submillimeter optics and lens antenna-coupled MKID cameras| Format | Member Price | Non-Member Price |
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Paper Abstract
Wide field cryogenic optics and millimeter-wave Microwave Kinetic Inductance Detector (MKID) cameras with Si lens array have been developed. MKID is a Cooper-pair breaking photon detector and consists of supercon- ducting resonators which enable microwave (~GHz) frequency multiplexing. Antenna-coupled Aluminum CPW resonators are put in a line on a Si substrate to be read by a pair of coaxial cables. A 220 GHz - 600 pixels MKID camera with anti-reflection (AR) coated Si lens has been demonstrated in an 0.1 K cryostat. A compact cryogenic system with high refractive index materials has been developed for the MKID camera.
Paper Details
Date Published: 23 July 2014
PDF: 6 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91532P (23 July 2014); doi: 10.1117/12.2055666
Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)
PDF: 6 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91532P (23 July 2014); doi: 10.1117/12.2055666
Show Author Affiliations
Y. Sekimoto, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
T. Nitta, National Astronomical Observatory of Japan (Japan)
Univ. of Tsukuba (Japan)
Japan Society for the Promotion of Science (Japan)
K. Karatsu, National Astronomical Observatory of Japan (Japan)
M. Sekine, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
S. Sekiguchi, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
T. Okada, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
S. Shu, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
The Univ. of Tokyo (Japan)
T. Nitta, National Astronomical Observatory of Japan (Japan)
Univ. of Tsukuba (Japan)
Japan Society for the Promotion of Science (Japan)
K. Karatsu, National Astronomical Observatory of Japan (Japan)
M. Sekine, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
S. Sekiguchi, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
T. Okada, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
S. Shu, National Astronomical Observatory of Japan (Japan)
The Univ. of Tokyo (Japan)
T. Noguchi, National Astronomical Observatory of Japan (Japan)
M. Naruse, National Astronomical Observatory of Japan (Japan)
Saitama Univ. (Japan)
K. Mitsui, National Astronomical Observatory of Japan (Japan)
N. Okada, National Astronomical Observatory of Japan (Japan)
T. Tsuzuki, National Astronomical Observatory of Japan (Japan)
A. Dominjon, National Astronomical Observatory of Japan (Japan)
H. Matsuo, National Astronomical Observatory of Japan (Japan)
M. Naruse, National Astronomical Observatory of Japan (Japan)
Saitama Univ. (Japan)
K. Mitsui, National Astronomical Observatory of Japan (Japan)
N. Okada, National Astronomical Observatory of Japan (Japan)
T. Tsuzuki, National Astronomical Observatory of Japan (Japan)
A. Dominjon, National Astronomical Observatory of Japan (Japan)
H. Matsuo, National Astronomical Observatory of Japan (Japan)
Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)
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