First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA
Creators: name: KAGRA Collaboration
name: Akutsu, T.
name: Ando, M.
name: Arai, K.
name: Arai, Y.
name: Araki, S.
name: Araya, A.
name: Aritomi, N.
name: Asada, H.
name: Aso, Y.
name: Atsuta, S.
name: Awai, K.
name: Bae, S.
name: Baiotti, L.
name: Barton, M. A.
name: Cannon, K.
name: Capocasa, E.
name: Chen, C-S.
name: Chiu, T-W.
name: Cho, K.
name: Chu, Y-K.
name: Craig, K.
name: Creus, W.
name: Doi, K.
name: Eda, K.
name: Enomoto, Y.
name: Flaminio, R.
name: Fujii, Y.
name: Fujimoto, M. -K.
name: Fukunaga, M.
name: Fukushima, M.
name: Furuhata, T.
name: Hagiwara, A.
name: Haino, S.
name: Hasegawa, K.
name: Hashino, K.
name: Hayama, K.
name: Hirobayashi, S.
name: Hirose, E.
name: Hsieh, B. H.
name: Huang, C-Z.
name: Ikenoue, B.
name: Inoue, Y.
name: Ioka, K.
name: Itoh, Y.
name: Izumi, K.
name: Kaji, T.
name: Kajita, T.
name: Kakizaki, M.
name: Kamiizumi, M.
name: Kanbara, S.
name: Kanda, N.
name: Kanemura, S.
name: Kaneyama, M.
name: Kang, G.
name: Kasuya, J.
name: Kataoka, Y.
name: Kawai, N.
name: Kawamura, S.
name: Kawasaki, T.
name: Kim, C.
name: Kim, J.
name: Kim, J. C.
name: Kim, W. S.
name: Kim, Y. -M.
name: Kimura, N.
name: Kinugawa, T.
name: Kirii, S.
name: Kitaoka, Y.
name: Kitazawa, H.
name: Kojima, Y.
name: Kokeyama, K.
name: Komori, K.
name: Kong, A. K. H.
name: Kotake, K.
name: Kozu, R.
name: Kumar, R.
name: Kuo, H-S.
name: Kuroyanagi, S.
name: Lee, H. K.
name: Lee, H. M.
name: Lee, H. W.
name: Leonardi, M.
name: Lin, C-Y.
name: Lin, F-L.
name: Liu, G. C.
name: Liu, Y.
name: Majorana, E.
name: Mano, S.
name: Marchio, M.
name: Matsui, T.
name: Matsushima, F.
name: Michimura, Y.
name: Mio, N.
name: Miyakawa, O.
name: Miyamoto, A.
name: Miyamoto, T.
name: Miyo, K.
name: Miyoki, S.
name: Morii, W.
name: Morisaki, S.
name: Moriwaki, Y.
name: Morozumi, T.
name: Murakami, I.
name: Musha, M.
name: Nagano, K.
name: Nagano, S.
name: Nakamura, K.
name: Nakamura, T.
name: Nakano, H.
name: Nakano, M.
name: Nakao, K.
name: Namai, Y.
name: Narikawa, T.
name: Naticchioni, L.
name: Quynh, L. Nguyen
name: Ni, W. -T.
name: Nishizawa, A.
name: Obuchi, Y.
name: Ochi, T.
name: Oh, J. J.
name: Oh, S. H.
name: Ohashi, M.
name: Ohishi, N.
name: Ohkawa, M.
name: Okutomi, K.
name: Ono, K.
name: Oohara, K.
name: Ooi, C. P.
name: Pan, S-S.
name: Park, J.
name: Arellano, F. E. Peña
name: Pinto, I.
name: Sago, N.
name: Saijo, M.
name: Saito, Y.
name: Saitou, S.
name: Sakai, K.
name: Sakai, Y.
name: Sakai, Y.
name: Sasai, M.
name: Sasaki, M.
name: Sasaki, Y.
name: Sato, N.
name: Sato, S.
name: Sato, T.
name: Sekiguchi, Y.
name: Seto, N.
name: Shibata, M.
name: Shimoda, T.
name: Shinkai, H.
name: Shishido, T.
name: Shoda, A.
name: Somiya, K.
name: Son, E. J.
name: Suemasa, A.
name: Suzuki, T.
name: Suzuki, T.
name: Tagoshi, H.
name: Tahara, H.
name: Takahashi, H.
name: Takahashi, R.
name: Takamori, A.
name: Takeda, H.
name: Tanaka, H.
name: Tanaka, K.
name: Tanaka, T.
name: Tanioka, S.
name: Martin, E. N. Tapia San
name: Tatsumi, D.
name: Terashima, S.
name: Tomaru, T.
name: Tomura, T.
name: Travasso, F.
name: Tsubono, K.
name: Tsuchida, S.
name: Uchikata, N.
name: Uchiyama, T.
name: Ueda, A.
name: Uehara, T.
name: Ueki, S.
name: Ueno, K.
name: Uraguchi, F.
name: Ushiba, T.
name: van Putten, M. H. P. M.
name: Vocca, H.
name: Wada, S.
name: Wakamatsu, T.
name: Watanabe, Y.
name: Xu, W-R.
name: Yamada, T.
name: Yamamoto, A.
name: Yamamoto, K.
name: Yamamoto, K.
name: Yamamoto, S.
name: Yamamoto, T.
name: Yokogawa, K.
name: Yokoyama, J.
name: Yokozawa, T.
name: Yoon, T. H.
name: Yoshioka, T.
name: Yuzurihara, H.
name: Zeidler, S.
name: Zhu, Z. -H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: KAGRA is a second-generation interferometric gravitational-wave detector with 3-km arms constructed at Kamioka, Gifu in Japan. It is now in its final installation phase, which we call bKAGRA (baseline KAGRA), with scientific observations expected to begin in late 2019. One of the advantages of KAGRA is its underground location of at least 200 m below the ground surface, which brings small seismic motion at low frequencies and high stability of the detector. Another advantage is that it cools down the sapphire test mass mirrors to cryogenic temperatures to reduce thermal noise. In April-May 2018, we have operated a 3-km Michelson interferometer with a cryogenic test mass for 10 days, which was the first time that km-scale interferometer was operated at cryogenic temperatures. In this article, we report the results of this "bKAGRA Phase 1" operation. We have demonstrated the feasibility of 3-km interferometer alignment and control with cryogenic mirrors.
description: 23 pages, 11 figures