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Development of Microwave Kinetic Inductance Detector for Cosmological Observations
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A precise measurement of Cosmic Microwave Background (CMB) provides us rich information about the universe. In particular, its asymmetric polarization patterns, B-modes, are smoking gun signature of inflationary universe. Magnitude of the B-modes is order of 10 nK. Its measurement requires a high sensitive millimeter-wave telescope with a large number of superconducting detectors on its focal plane. Microwave Kinetic Inductance Detector (MKID) is appropriate detector for this purpose. MKID camera has been developed in cooperation of National Astronomical Observatory of Japan (NAOJ), Institute of Physical and Chemical Research (RIKEN), High Energy Accelerator Research Organization (KEK), and Okayama University. Our developments of MKID include: fabrication of high-quality superconducting film; optical components for a camera use; and readout electronics. For performance evaluation of total integrated system of our MKID camera, a calibration system was also developed. The system was incorporated in a 0.1 K dilution refrigerator with modulated polarization source. These developed technologies are applicable to other types of detectors.
- Publication
- IEICE TRANSACTIONS on Electronics Vol.E98-C No.3 pp.207-218
- Publication Date
- 2015/03/01
- Publicized
- Online ISSN
- 1745-1353
- DOI
- 10.1587/transele.E98.C.207
- Type of Manuscript
- Special Section INVITED PAPER (Special Section on Leading-Edge Applications and Fundamentals of Superconducting Sensors and Detectors)
- Category
Authors
Kenichi KARATSU
National Astronomical Observatory of Japan
Satoru MIMA
RIKEN
Shugo OGURI
High Energy Accelerator Research Organization (KEK)
Jihoon CHOI
Korea University
R. M. THUSHARA DAMAYANTHI
RIKEN
Agnes DOMINJON
National Astronomical Observatory of Japan
Noboru FURUKAWA
RIKEN
Hirokazu ISHINO
Okayama Uiversity
Hikaru ISHITSUKA
Graduate University for Advanced Studies (SOKENDAI)
Atsuko KIBAYASHI
Okayama Uiversity
Yoshiaki KIBE
Okayama Uiversity
Hitoshi KIUCHI
National Astronomical Observatory of Japan
Kensuke KOGA
Tohoku University
Masato NARUSE
Saitama University
Tom NITTA
National Astronomical Observatory of Japan
Takashi NOGUCHI
National Astronomical Observatory of Japan
Takashi OKADA
The University of Tokyo
Chiko OTANI
RIKEN
Shigeyuki SEKIGUCHI
The University of Tokyo
Yutaro SEKIMOTO
National Astronomical Observatory of Japan
Masakazu SEKINE
The University of Tokyo
Shibo SHU
The University of Tokyo
Osamu TAJIMA
High Energy Accelerator Research Organization (KEK)
Kenta TAKAHASHI
Tohoku University
Nozomu TOMITA
The University of Tokyo
Hiroki WATANABE
Graduate University for Advanced Studies (SOKENDAI)
Mitsuhiro YOSHIDA
High Energy Accelerator Research Organization (KEK)
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Kenichi KARATSU, Satoru MIMA, Shugo OGURI, Jihoon CHOI, R. M. THUSHARA DAMAYANTHI, Agnes DOMINJON, Noboru FURUKAWA, Hirokazu ISHINO, Hikaru ISHITSUKA, Atsuko KIBAYASHI, Yoshiaki KIBE, Hitoshi KIUCHI, Kensuke KOGA, Masato NARUSE, Tom NITTA, Takashi NOGUCHI, Takashi OKADA, Chiko OTANI, Shigeyuki SEKIGUCHI, Yutaro SEKIMOTO, Masakazu SEKINE, Shibo SHU, Osamu TAJIMA, Kenta TAKAHASHI, Nozomu TOMITA, Hiroki WATANABE, Mitsuhiro YOSHIDA, "Development of Microwave Kinetic Inductance Detector for Cosmological Observations" in IEICE TRANSACTIONS on Electronics,
vol. E98-C, no. 3, pp. 207-218, March 2015, doi: 10.1587/transele.E98.C.207.
Abstract: A precise measurement of Cosmic Microwave Background (CMB) provides us rich information about the universe. In particular, its asymmetric polarization patterns, B-modes, are smoking gun signature of inflationary universe. Magnitude of the B-modes is order of 10 nK. Its measurement requires a high sensitive millimeter-wave telescope with a large number of superconducting detectors on its focal plane. Microwave Kinetic Inductance Detector (MKID) is appropriate detector for this purpose. MKID camera has been developed in cooperation of National Astronomical Observatory of Japan (NAOJ), Institute of Physical and Chemical Research (RIKEN), High Energy Accelerator Research Organization (KEK), and Okayama University. Our developments of MKID include: fabrication of high-quality superconducting film; optical components for a camera use; and readout electronics. For performance evaluation of total integrated system of our MKID camera, a calibration system was also developed. The system was incorporated in a 0.1 K dilution refrigerator with modulated polarization source. These developed technologies are applicable to other types of detectors.
URL: https://global.ieice.org/en_transactions/electronics/10.1587/transele.E98.C.207/_p
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@ARTICLE{e98-c_3_207,
author={Kenichi KARATSU, Satoru MIMA, Shugo OGURI, Jihoon CHOI, R. M. THUSHARA DAMAYANTHI, Agnes DOMINJON, Noboru FURUKAWA, Hirokazu ISHINO, Hikaru ISHITSUKA, Atsuko KIBAYASHI, Yoshiaki KIBE, Hitoshi KIUCHI, Kensuke KOGA, Masato NARUSE, Tom NITTA, Takashi NOGUCHI, Takashi OKADA, Chiko OTANI, Shigeyuki SEKIGUCHI, Yutaro SEKIMOTO, Masakazu SEKINE, Shibo SHU, Osamu TAJIMA, Kenta TAKAHASHI, Nozomu TOMITA, Hiroki WATANABE, Mitsuhiro YOSHIDA, },
journal={IEICE TRANSACTIONS on Electronics},
title={Development of Microwave Kinetic Inductance Detector for Cosmological Observations},
year={2015},
volume={E98-C},
number={3},
pages={207-218},
abstract={A precise measurement of Cosmic Microwave Background (CMB) provides us rich information about the universe. In particular, its asymmetric polarization patterns, B-modes, are smoking gun signature of inflationary universe. Magnitude of the B-modes is order of 10 nK. Its measurement requires a high sensitive millimeter-wave telescope with a large number of superconducting detectors on its focal plane. Microwave Kinetic Inductance Detector (MKID) is appropriate detector for this purpose. MKID camera has been developed in cooperation of National Astronomical Observatory of Japan (NAOJ), Institute of Physical and Chemical Research (RIKEN), High Energy Accelerator Research Organization (KEK), and Okayama University. Our developments of MKID include: fabrication of high-quality superconducting film; optical components for a camera use; and readout electronics. For performance evaluation of total integrated system of our MKID camera, a calibration system was also developed. The system was incorporated in a 0.1 K dilution refrigerator with modulated polarization source. These developed technologies are applicable to other types of detectors.},
keywords={},
doi={10.1587/transele.E98.C.207},
ISSN={1745-1353},
month={March},}
Copy
TY - JOUR
TI - Development of Microwave Kinetic Inductance Detector for Cosmological Observations
T2 - IEICE TRANSACTIONS on Electronics
SP - 207
EP - 218
AU - Kenichi KARATSU
AU - Satoru MIMA
AU - Shugo OGURI
AU - Jihoon CHOI
AU - R. M. THUSHARA DAMAYANTHI
AU - Agnes DOMINJON
AU - Noboru FURUKAWA
AU - Hirokazu ISHINO
AU - Hikaru ISHITSUKA
AU - Atsuko KIBAYASHI
AU - Yoshiaki KIBE
AU - Hitoshi KIUCHI
AU - Kensuke KOGA
AU - Masato NARUSE
AU - Tom NITTA
AU - Takashi NOGUCHI
AU - Takashi OKADA
AU - Chiko OTANI
AU - Shigeyuki SEKIGUCHI
AU - Yutaro SEKIMOTO
AU - Masakazu SEKINE
AU - Shibo SHU
AU - Osamu TAJIMA
AU - Kenta TAKAHASHI
AU - Nozomu TOMITA
AU - Hiroki WATANABE
AU - Mitsuhiro YOSHIDA
PY - 2015
DO - 10.1587/transele.E98.C.207
JO - IEICE TRANSACTIONS on Electronics
SN - 1745-1353
VL - E98-C
IS - 3
JA - IEICE TRANSACTIONS on Electronics
Y1 - March 2015
AB - A precise measurement of Cosmic Microwave Background (CMB) provides us rich information about the universe. In particular, its asymmetric polarization patterns, B-modes, are smoking gun signature of inflationary universe. Magnitude of the B-modes is order of 10 nK. Its measurement requires a high sensitive millimeter-wave telescope with a large number of superconducting detectors on its focal plane. Microwave Kinetic Inductance Detector (MKID) is appropriate detector for this purpose. MKID camera has been developed in cooperation of National Astronomical Observatory of Japan (NAOJ), Institute of Physical and Chemical Research (RIKEN), High Energy Accelerator Research Organization (KEK), and Okayama University. Our developments of MKID include: fabrication of high-quality superconducting film; optical components for a camera use; and readout electronics. For performance evaluation of total integrated system of our MKID camera, a calibration system was also developed. The system was incorporated in a 0.1 K dilution refrigerator with modulated polarization source. These developed technologies are applicable to other types of detectors.
ER -
English
