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

Autor: R. Shimizu, Ettore Majorana, H. B. Jin, P. Jung, M. Fukunaga, G-Z. Huang, F. E. Peña Arellano, H. Pang, Kunihiro Nagano, John J. Oh, Atsushi Nishizawa, M. Nakano, C. Kozakai, Yasufumi Kojima, S. Saito, Takayuki Tomaru, T. Tomura, Y. Fujikawa, Kazuhiro Hayama, Hajime Sotani, Shigeo Nagano, Masatake Ohashi, S. Otabe, Naoki Aritomi, Chunglee Kim, Tatsuhiro Yamada, Kipp Cannon, Shuen De Wu, Yuhang Zhao, Fumihiro Uraguchi, Hideki Asada, Ryutaro Takahashi, Kei Kotake, Yutaro Enomoto, Naoko Ohishi, L. W. Luo, K. Inayoshi, S. Bae, S. Ha, Sadakazu Haino, T. Narikawa, Yoshiyuki Obuchi, Ryo Yamazaki, K. Hattori, Y. Tomigami, K. Ueno, Zhoujian Cao, Keiko Kokeyama, Kentaro Somiya, G. Ge, K. Yamashita, Wei-Tou Ni, Satoshi Tsuchida, Takashi Sato, M. Zhan, Akiteru Takamori, Masaki Ando, Y. Nakayama, F. K. Lin, W-R. Xu, T. Sawada, Seog Oh, Ray-Kuang Lee, C. P. Ooi, C. Chen, Takahiro Tanaka, S. Ide, H. Vocca, J. Wang, Albert K. H. Kong, T. Yoshioka, Lijing Shao, T. Shimoda, Y. Okutani, R. Flaminio, S. Eguchi, T. Sekiguchi, Y. Sakuno, R. Kozu, Hyang Woon Lee, Zong-Hong Zhu, Y. Hiranuma, Wen-Biao Han, Hideaki Hayakawa, K. Chen, Y. Mori, Yuki Fujii, H. Ohta, Y. Miyazaki, A. Shoda, B. H. Hsieh, Y. Sakai, K. Sakai, S. Oshino, T. Ushiba, Luca Baiotti, Simon Zeidler, Yousuke Itoh, Hiroyuki Nakano, Takaaki Kajita, Yuki Inoue, S. Shibagaki, Hiroyuki Takeda, Chau Ron Wu, Y-K. Chu, M. Kamiizumi, Guo-Chin Liu, Yoshiaki Himemoto, I. M. Pinto, S. Sato, Y. Kuromiya, Yuta Michimura, N. Hirata, A. Miyamoto, Y. Huang, K. L. Li, Yi Chen, Yuichiro Sekiguchi, Kimio Tsubono, Hideyuki Tagoshi, S. Imam, H. L. Lin, M. Chan, Rajesh Kumar, L. C.C. Lin, K. Kusayanagi, K. Okutomi, D. C. Y. Hui, Sachiko Kuroyanagi, K. Kaihotsu, J. Kim, Jinsook Kim, K. Ito, Takashi Uchiyama, Kunihito Ioka, L. Nguyen Quynh, K. Yokogawa, R. Bajpai, K. Shimode, Norikatsu Mio, Koya Arai, Toshihiro Tsuzuki, L. Naticchioni, T. Shishido, R. Nakashima, M. Takeda, Akito Araya, A. Parisi, T. Yokozawa, E. N. Tapia San Martin, Souichi Telada, M. H. P. M. van Putten, Jishnu Suresh, Y. Arai, K. Miyo, K. Oohara, N. Kawai, Soichiro Morisaki, C. Jeon, W. S. Kim, T. Uehara, Jun'ichi Yokoyama, Nobutada Kimura, K. Oh, D. Tuyenbayev, Kentaro Komori, N. Kita, T. Kawasaki, T. Tsang, Hong Wu, Yi Yang, Kuo-Chuan Pan, S. Tanioka, K. Jung, A. Hagiwara, D. Gao, R. Negishi, C-Y. Lin, E. Capocasa, Shinji Miyoki, H. Chu, G. Ueshima, Tomotada Akutsu, M. A. Barton, Y. M. Kim, C-Y. Chiang, Hisa-aki Shinkai, L. Trozzo, Norichika Sago, K. Kwak, J. Kume, Takahiro Yamamoto, Nobuyuki Kanda, S. Nozaki, H. K. Tanaka, H. Yuzurihara, Masako Kakizaki, Eiichi Hirose, Kouji Nakamura, F-L. Lin, M. Leonardi, Haruki Kitazawa, J-S. Tsao, Takuya Tsutsui, M. Marchio, Yoichi Aso, J. Park, K. Izumi, F. Travasso, Hirotaka Takahashi, Nami Uchikata, Mitsuhiro Fukushima, H. Y. Huang, G. Kang, H. Zhang, A. Ueda, Sakae Araki, Osamu Miyakawa, Chin Guo Kuo, Y. Moriwaki, K. Yamamoto, Toshio Suzuki, Hyun Lee, Y. Bae, Masashi Ohkawa, K. Hasegawa, T. Washimi, Kyohei Kawaguchi, B. Ikenoue, H-S. Kuo, P. W. Huang, Kazuyuki Tanaka, Y. Saito, S. Takano, E. J. Son, W. Ogaki, Z. Hong, R. Sugimoto
Přispěvatelé: Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), KAGRA
Jazyk: angličtina
Rok vydání: 2021
Předmět:
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
data acquisition
interferometer
General Physics and Astronomy
FOS: Physical sciences
detector: noise
General Relativity and Quantum Cosmology (gr-qc)
01 natural sciences
General Relativity and Quantum Cosmology
Optics
0103 physical sciences
Calibration
detector: calibration
KAGRA
laser: interferometer
[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
010306 general physics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
Physics
010308 nuclear & particles physics
business.industry
geophysics
Detector
gravitational radiation
KAGRA gravitational wave kamioka
gravitational radiation detector
Characterization (materials science)
detector: sensitivity
Interferometry
F32 Calibration and operation of gravitational wave detector
[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik
Astrophysics - Instrumentation and Methods for Astrophysics
business
detector: sensitivity
data acquisition
interferometer
geophysics
detector: noise
detector: calibration
KAGRA
gravitational radiation detector
gravitational radiation
laser: interferometer
Zdroj: Progress of Theoretical and Experimental Physics [PTEP]
Progress of Theoretical and Experimental Physics [PTEP], Oxford University Press on behalf of the Physical Society of Japan, 2021, 2021 (5), pp.05A102. ⟨10.1093/ptep/ptab018⟩
Progress of Theoretical and Experimental Physics
ISSN: 2050-3911
DOI: 10.1093/ptep/ptab018⟩
Popis: KAGRA is a newly built gravitational wave observatory, a laser interferometer with a 3 km arm length, located in 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 monitors (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.
Comment: 2021/02/08 Accepted by PTEP
Databáze: OpenAIRE