Related Researcher

Author's Photo

Kwak, Kyujin
Computational Astrophysics Lab
Research Interests
  • Computational Fluid Dynamics
  • Astrophysical and Laboratory Plasma
  • Hydrodynamics with Radiation
  • Nuclear, Atomic, and Molecular Reactions


Overview of KAGRA: Calibration, detector characterization, physical environmental monitors, and the geophysics interferometer

DC Field Value Language Akutsu, T. ko Ando, M. ko Arai, K. ko Arai, Y. ko Araki, S. ko Araya, A. ko Aritomi, N. ko Asada, H. ko Aso, Y. ko Bae, S. ko Baiotti, L. ko Bajpai, R. ko Barton, M. A. ko Cannon, K. ko Cao, Z. ko Capocasa, E. ko Chan, M. ko Chen, C. ko Chen, K. ko Chen, Y. ko Chiang, C-Y ko Chu, H. ko Chu, Y-K ko Eguchi, S. ko Enomoto, Y. ko Flaminio, R. ko Fujii, Y. ko Fujikawa, Y. ko Fukunaga, M. ko Fukushima, M. ko Gao, D. ko Ge, G. ko Ha, S. ko Hagiwara, A. ko Haino, S. ko Han, W-B ko Hasegawa, K. ko Hattori, K. ko Hayakawa, H. ko Hayama, K. ko Himemoto, Y. ko Hiranuma, Y. ko Hirata, N. ko Hirose, E. ko Hong, Z. ko Hsieh, B. ko Huang, G-Z ko Huang, H-Y ko Huang, P. ko Huang, Y-C ko Huang, Y. ko Hui, D. C. Y. ko Ide, S. ko Ikenoue, B. ko Imam, S. ko Inayoshi, K. ko Inoue, Y. ko Ioka, K. ko Ito, K. ko Itoh, Y. ko Izumi, K. ko Jeon, C. ko Jin, H-B ko Jung, K. ko Jung, P. ko Kaihotsu, K. ko Kajita, T. ko Kakizaki, M. ko Kamiizumi, M. ko Kanda, N. ko Kang, G. ko Kawaguchi, K. ko Kawai, N. ko Kawasaki, T. ko Kim, C. ko Kim, J. ko Kim, J. C. ko Kim, S. ko Kim, Y-M ko Kimura, N. ko Kita, N. ko Kitazawa, H. ko Kojima, Y. ko Kokeyama, K. ko Komori, K. ko Kong, A. K. H. ko Kotake, K. ko Kozakai, C. ko Kozu, R. ko Kumar, R. ko Kume, J. ko Kuo, C. ko Kuo, H-S ko Kuromiya, Y. ko Kuroyanagi, S. ko Kusayanagi, K. ko Kwak, Kyujin ko Lee, K. ko Lee, H. W. ko Lee, R. ko Leonardi, M. ko Li, K. L. ko Lin, L. C-C ko Lin, F-K ko Lin, C-Y ko Lin, F-L ko Lin, H. L. ko Liu, C. ko Luo, L-W ko Majorana, E. ko Marchio, M. ko Michimura, Y. ko Mio, N. ko Miyakawa, O. ko Miyamoto, A. ko Miyazaki, Y. ko Miyo, K. ko Miyoki, S. ko Mori, Y. ko Morisaki, S. ko Moriwaki, Y. ko Nagano, K. ko Nagano, S. ko Nakamura, K. ko Nakano, H. ko Nakano, M. ko Nakashima, R. ko Nakayama, Y. ko Narikawa, T. ko Naticchioni, L. ko Negishi, R. ko Quynh, L. Nguyen ko Ni, W-T ko Nishizawa, A. ko Nozaki, S. ko Obuchi, Y. ko Ogaki, W. ko Oh, J. J. ko Oh, K. ko Oh, S. H. ko Ohashi, M. ko Ohishi, N. ko Ohkawa, M. ko Ohta, H. ko Okutani, Y. ko Okutomi, K. ko Oohara, K. ko Ooi, C. ko Oshino, S. ko Otabe, S. ko Pan, K. ko Pang, H. ko Parisi, A. ko Park, J. ko Arellano, F. E. Pena ko Pinto, I ko Sago, N. ko Saito, S. ko Saito, Y. ko Sakai, K. ko Sakai, Y. ko Sakuno, Y. ko Sato, S. ko Sato, T. ko Sawada, T. ko Sekiguchi, T. ko Sekiguchi, Y. ko Shao, L. ko Shibagaki, S. ko Shimizu, R. ko Shimoda, T. ko Shimode, K. ko Shinkai, H. ko Shishido, T. ko Shoda, A. ko Somiya, K. ko Son, J. ko Sotani, H. ko Sugimoto, R. ko Suresh, J. ko Suzuki, T. ko Tagoshi, H. ko Takahashi, H. ko Takahashi, R. ko Takamori, A. ko Takano, S. ko Takeda, H. ko Takeda, M. ko Tanaka, H. ko Tanaka, K. ko Tanaka, T. ko Tanioka, S. ko San Martin, E. N. Tapia ko Telada, S. ko Tomaru, T. ko Tomigami, Y. ko Tomura, T. ko Travasso, F. ko Trozzo, L. ko Tsang, T. ko Tsao, J-S ko Tsubono, K. ko Tsuchida, S. ko Tsutsui, T. ko Tsuzuki, T. ko Tuyenbayev, D. ko Uchikata, N. ko Uchiyama, T. ko Ueda, A. ko Uehara, T. ko Ueno, K. ko Ueshima, G. ko Uraguchi, F. ko Ushiba, T. ko van Putten, M. H. P. M. ko Vocca, H. ko Wang, J. ko Washimi, T. ko Wu, C. ko Wu, H. ko Wu, S. ko Xu, W-R ko Yamada, T. ko Yamamoto, K. ko Yamamoto, T. ko Yamashita, K. ko Yamazaki, R. ko Yang, Y. ko Yokogawa, K. ko Yokoyama, J. ko Yokozawa, T. ko Yoshioka, T. ko Yuzurihara, H. ko Zeidler, S. ko Zhan, M. ko Zhang, H. ko Zhao, Y. ko Zhu, Z-H ko 2021-08-12T08:32:49Z - 2021-08-09 ko 2021-05 ko
dc.identifier.citation PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS, v.2021, no.5, pp.05A102 ko
dc.identifier.issn 2050-3911 ko
dc.identifier.uri -
dc.description.abstract KAGRA is a newly built gravitational wave observatory, a laser interferometer with a 3 km arm length, located at Kamioka, Gifu, Japan. In this series of articles we present an overview of the baseline KAGRA, for which we finished installing the designed configuration in 2019. This article describes the method of calibration (CAL) used for reconstructing gravitational wave signals from the detector outputs, as well as the characterization of the detector (DET). We also review the physical environmental monitoring (PEM) system and the geophysics interferometer (GIF). Both are used for characterizing and evaluating the data quality of the gravitational wave channel. They play important roles in utilizing the detector output for gravitational wave searches. These characterization investigations will be even more important in the near future, once gravitational wave detection has been achieved, and in using KAGRA in the gravitational wave astronomy era. ko
dc.language 영어 ko
dc.publisher OXFORD UNIV PRESS INC ko
dc.title Overview of KAGRA: Calibration, detector characterization, physical environmental monitors, and the geophysics interferometer ko
dc.type ARTICLE ko
dc.identifier.scopusid 2-s2.0-85106375886 ko
dc.identifier.wosid 000671556400008 ko
dc.type.rims ART ko
dc.identifier.doi 10.1093/ptep/ptab018 ko
dc.identifier.url ko
Appears in Collections:
PHY_Journal Papers

find_unist can give you direct access to the published full text of this article. (UNISTARs only)

Show simple item record


  • mendeley


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.