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

@article{TAkutsu2020OverviewOK,
  title={Overview of KAGRA: Calibration, detector characterization, physical environmental monitors, and the geophysics interferometer},
  author={T.Akutsu and M.Ando and K.Arai and Y.Arai and S.Araki and A.Araya and N.Aritomi and H.Asada and Y.Aso and S.Bae and Y.Bae and L.Baiotti and R.Bajpai and M.A.Barton and K.Cannon and Z.Cao and E.Capocasa and M.Chan and C.Chen and K.Chen and Y.Chen and C-Y.Chiang and H.Chu and Y-K.Chu and S.Eguchi and Y.Enomoto and R.Flaminio and Y.Fujii and Y.FUJIKAWA and M.Fukunaga and M.Fukushima and D.Gao and G.Ge and S.Ha and A.Hagiwara and S.Haino and W.-B.Han and K.Hasegawa and K.Hattori and H.Hayakawa and K.Hayama and Y.Himemoto and Y.Hiranuma and N.Hirata and E.Hirose and Z.Hong and B.Hsieh and G.-Z.Huang and H-Y.Huang and P.Huang and Y-C.Huang and Y.Huang and D.C.Y.Hui and Side and B.Ikenoue and S.Imam and K.Inayoshi and Y.Inoue and K.Ioka and Kito and Y.Itoh and K.Izumi and C.Jeon and H.-B.Jin and K.Jung and P.Jung and K.Kaihotsu and T.Kajita and M.Kakizaki and M.Kamiizumi and N.Kanda and G.Kang and K.Kawaguchi and N.Kawai and T.Kawasaki and C.Kim and J.Kim and J.C.Kim and W.S.Kim and Y.-M.Kim and N.Kimura and N.Kita and H.Kitazawa and Y.Kojima and K.Kokeyama and K.Komori and A.K.H.Kong and K.Kotake and C.Kozakai and R.Kozu and R.Kumar and J.Kume and C.Kuo and H.-S.Kuo and Y.Kuromiya and S.Kuroyanagi and K.Kusayanagi and K.Kwak and H.-K.Lee and H.-W.Lee and R.Lee and M.Leonardi and K.L.Li and L.C.-C.Lin and C.-Y.Lin and F-K.Lin and H.L.Lin and G.-C.Liu and L.-W.Luo and E.Majorana and M.Marchio and Y.Michimura and N.Mio and O.Miyakawa and A.Miyamoto and Y.Miyazaki and K.Miyo and S.Miyoki and Y.Mori and S.Morisaki and Y.Moriwaki and K.Nagano and S.Nagano and K.Nakamura and H.Nakano and M.Nakano and R.Nakashima and Y.Nakayama and T.Narikawa and L.Naticchioni and R.Negishi and L. Quynh and W.-T.Ni and A.Nishizawa and S.Nozaki and Y.Obuchi and W.Ogaki and J.J.Oh and K.Oh and S.-H.Oh and M.Ohashi and N.Ohishi and M.Ohkawa and H.Ohta and Y.Okutani and K.Okutomi and K.Oohara and C.Ooi and S.Oshino and S.Otabe and K.Pan and H.Pang and Aparisi and J.Park and F. Arellano and I.Pinto and N.Sago and S.Saito and Y.Saito and K.Sakai and Y.Sakai and Y.Sakuno and S.Sato and T.Sato and T.Sawada and T.Sekiguchi and Y.Sekiguchi and L.Shao and S.Shibagaki and R.Shimizu and T.Shimoda and K.Shimode and H.Shinkai and T.Shishido and A.Shoda and K.Somiya and E.J.Son and H.Sotani and R.Sugimoto and J.Suresh and T.Suzuki and H.Tagoshi and H.Takahashi and R.Takahashi and A.Takamori and S.Takano and H.Takeda and M.Takeda and H.Tanaka and K.Tanaka and T.Tanaka and S.Tanioka and E. Martin and S.Telada and T.Tomaru and Y.Tomigami and T.Tomura and F.Travasso and L.Trozzo and T.Tsang and J-S.Tsao and K.Tsubono and S.Tsuchida and T.Tsutsui and T.Tsuzuki and D.Tuyenbayev and N.Uchikata and T.Uchiyama and A.Ueda and T.Uehara and K.Ueno and G.Ueshima and F.Uraguchi and T.Ushiba and M. Putten and H.Vocca and J.Wang and T.Washimi and C.Wu and H.Wu and S.Wu and W.-R.Xu and T.Yamada and K.Yamamoto and T.Yamamoto and K.Yamashita and R.Yamazaki and Y.Yang and K.Yokogawa and J.Yokoyama and T.Yokozawa and T.Yoshioka and H.Yuzurihara and S.Zeidler and M.Zhan and H.Zhang and Y.zhao and Z.-H.Zhu},
  journal={arXiv: General Relativity and Quantum Cosmology},
  year={2020}
}
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… Expand
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