Input optics systems of the KAGRA detector during O3GK

Akutsu, T.; Ando, M.; Arai, K.; Arai, Y.; Araki, S.; Araya, A.; Aritomi, N.; Asada, H.; Aso, Y.; Bae, S.; Bae, Y.; Baiotti, L.; Bajpai, R.; Barton, M. A.; Cannon, K.; Cao, Z.; Capocasa, E.; Chan, M.; Chen, C.; Chen, K.; Chen, Y.; Chiang, C.-I.; Chu, H.; Chu, Y.-K.; Eguchi, S.; Enomoto, Y.; Flaminio, R.; Fujii, Y.; Fujikawa, Y.; Fukunaga, M.; Fukushima, M.; Furuhata, T.; Gao, D.; Ge, G.-G.; Ha, S.; Hagiwara, A.; Haino, S.; Han, W.-B.; Hasegawa, K.; Hattori, K.; Hayakawa, H.; Hayama, K.; Himemoto, Y.; Hiranuma, Y.; Hirata, N.; Hirose, E.; Hong, Z.; Hsieh, B.-H.; Huang, G.-Z.; Huang, H.-Y.; Huang, P.; Huang, Y.-C.; Huang, Y.-J.; Hui, D. C. Y.; Ide, S.; Ikenoue, B.; Imam, S.; Inayoshi, K.; Inoue, Y.; Ioka, K.; Ito, K.; Itoh, Y.; Izumi, K.; Jeon, C.; Jin, H.-B.; Jung, K.; Jung, P.; Kaihotsu, K.; Kajita, T.; Kakizaki, M.; Kamiizumi, M.; Kanbara, S.; Kanda, N.; Kang, G.; Kataoka, Y.; Kawaguchi, K.; Kawai, N.; Kawasaki, T.; Kim, C.; Kim, J.; Kim, J. C.; Kim, W. S.; Kim, Y.-M.; Kimura, N.; Kita, N.; Kitazawa, H.; Kojima, Y.; Kokeyama, K.; Komori, K.; Kong, A. K. H.; Kotake, K.; Kozakai, C.; Kozu, R.; Kumar, R.; Kume, J.; Kuo, C.; Kuo, H.-S.; Kuromiya, Y.; Kuroyanagi, S.; Kusayanagi, K.; Kwak, K.; Lee, H. K.; Lee, H. W.; Lee, R.; Leonardi, M.; Li, K. L.; Lin, L. C.-C.; Lin, C.-Y.; Lin, F.-K.; Lin, F.-L.; Lin, H. L.; Liu, G. C.; Luo, L.-W.; Majorana, E.; Marchio, M.; Michimura, Y.; Mio, N.; Miyakawa, O.; Miyamoto, A.; Miyazaki, Y.; Miyo, K.; Miyoki, S.; Mori, Y.; Morisaki, S.; Moriwaki, Y.; Nagano, K.; Nagano, S.; Nakamura, K.; Nakano, H.; Nakano, M.; Nakashima, R.; Nakayama, Y.; Narikawa, T.; Naticchioni, L.; Negishi, R.; Quynh, L. Nguyen; Ni, W.-T.; Nishizawa, A.; Nozaki, S.; Obuchi, Y.; Ogaki, W.; Oh, J. J.; Oh, K.; Oh, S. H.; Ohashi, M.; Ohishi, N.; Ohkawa, M.; Ohta, H.; Okutani, Y.; Okutomi, K.; Oohara, K.; Ooi, C.; Oshino, S.; Otabe, S.; Pan, K.-C.; Pang, H.; Parisi, A.; Park, J.; Arellano, F. E. Peña; Pinto, I.; Sago, N.; Saito, S.; Saito, Y.; Sakai, K.; Sakai, Y.; Sakuno, Y.; Sato, S.; Sato, T.; Sawada, T.; Sekiguchi, T.; Sekiguchi, Y.; Shao, L.; Shibagaki, S.; Shimizu, R.; Shimoda, T.; Shimode, K.; Shinkai, H.; Shishido, T.; Shoda, A.; Somiya, K.; Son, E. J.; Sotani, H.; Sugimoto, R.; Suresh, J.; Suzuki, T.; Tagoshi, H.; Takahashi, H.; Takahashi, R.; Takamori, A.; Takano, S.; Takeda, H.; Takeda, M.; Tanaka, H.; Tanaka, K.; Tanaka, T.; Tanioka, S.; Tapia San Martín, E. N.; Telada, S.; Tomaru, T.; Tomigami, Y.; Tomura, T.; Travasso, F.; Trozzo, L.; Tsang, T.; Tsao, J.-S.; Tsubono, K.; Tsuchida, S.; Tsutsui, T.; Tsuzuki, T.; Tuyenbayev, D.; Uchikata, N.; Uchiyama, T.; Ueda, A.; Uehara, T.; Ueno, K.; Ueshima, G.; Uraguchi, F.; Ushiba, T.; Putten, M. H. P. M.; Vocca, H.; Wang, J.; Washimi, T.; Wu, C.; Wu, H.; Wu, S.; Xu, W.-R.; Yamada, T.; Yamamoto, K.; Yamamoto, T.; Yamashita, K.; Yamazaki, R.; Yang, Y.; Yano, K.; Yokogawa, K.; Yokoyama, J.; Yokozawa, T.; Yoshioka, T.; Yuzurihara, H.; Zeidler, S.; Zhan, M.; Zhang, H.; Zhao, Y.; Zhu, Z.-H.; Goetz, R.; Heintze, M.; Liu, J.; Müller, C.; Savage, R. L.; Tanner, D. B.

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Akito Araya
Akutsu et al., 2022

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Oxford University Press, Progress of Theoretical and Experimental Physics, 2(2023), 2022

DOI: 10.1093/ptep/ptac166

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@article{Akutsu2022,
  abstract = {Abstract KAGRA, the underground and cryogenic gravitational-wave detector, was operated for its solo observation from February 25 to March 10, 2020, and its first joint observation with the GEO 600 detector from April 7 to April 21, 2020 (O3GK). This study presents an overview of the input optics systems of the KAGRA detector, which consist of various optical systems, such as a laser source, its intensity and frequency stabilization systems, modulators, a Faraday isolator, mode-matching telescopes, and a high-power beam dump. These optics were successfully delivered to the KAGRA interferometer and operated stably during the observations. The laser frequency noise was observed to limit the detector sensitivity above a few kilohertz, whereas the laser intensity did not significantly limit the detector sensitivity.},
  author = {Akutsu, T. and Ando, M. and Arai, K. and Arai, Y. and Araki, S. and Araya, A. and Aritomi, N. and Asada, H. and Aso, Y. and Bae, S. and Bae, Y. and Baiotti, L. and Bajpai, R. and Barton, M. A. and Cannon, K. and Cao, Z. and Capocasa, E. and Chan, M. and Chen, C. and Chen, K. and Chen, Y. and Chiang, C.-I. and Chu, H. and Chu, Y.-K. and Eguchi, S. and Enomoto, Y. and Flaminio, R. and Fujii, Y. and Fujikawa, Y. and Fukunaga, M. and Fukushima, M. and Furuhata, T. and Gao, D. and Ge, G.-G. and Ha, S. and Hagiwara, A. and Haino, S. and Han, W.-B. and Hasegawa, K. and Hattori, K. and Hayakawa, H. and Hayama, K. and Himemoto, Y. and Hiranuma, Y. and Hirata, N. and Hirose, E. and Hong, Z. and Hsieh, B.-H. and Huang, G.-Z. and Huang, H.-Y. and Huang, P. and Huang, Y.-C. and Huang, Y.-J. and Hui, D. C. Y. and Ide, S. and Ikenoue, B. and Imam, S. and Inayoshi, K. and Inoue, Y. and Ioka, K. and Ito, K. and Itoh, Y. and Izumi, K. and Jeon, C. and Jin, H.-B. and Jung, K. and Jung, P. and Kaihotsu, K. and Kajita, T. and Kakizaki, M. and Kamiizumi, M. and Kanbara, S. and Kanda, N. and Kang, G. and Kataoka, Y. and Kawaguchi, K. and Kawai, N. and Kawasaki, T. and Kim, C. and Kim, J. and Kim, J. C. and Kim, W. S. and Kim, Y.-M. and Kimura, N. and Kita, N. and Kitazawa, H. and Kojima, Y. and Kokeyama, K. and Komori, K. and Kong, A. K. H. and Kotake, K. and Kozakai, C. and Kozu, R. and Kumar, R. and Kume, J. and Kuo, C. and Kuo, H.-S. and Kuromiya, Y. and Kuroyanagi, S. and Kusayanagi, K. and Kwak, K. and Lee, H. K. and Lee, H. W. and Lee, R. and Leonardi, M. and Li, K. L. and Lin, L. C.-C. and Lin, C.-Y. and Lin, F.-K. and Lin, F.-L. and Lin, H. L. and Liu, G. C. and Luo, L.-W. and Majorana, E. and Marchio, M. and Michimura, Y. and Mio, N. and Miyakawa, O. and Miyamoto, A. and Miyazaki, Y. and Miyo, K. and Miyoki, S. and Mori, Y. and Morisaki, S. and Moriwaki, Y. and Nagano, K. and Nagano, S. and Nakamura, K. and Nakano, H. and Nakano, M. and Nakashima, R. and Nakayama, Y. and Narikawa, T. and Naticchioni, L. and Negishi, R. and Quynh, L. Nguyen and Ni, W.-T. and Nishizawa, A. and Nozaki, S. and Obuchi, Y. and Ogaki, W. and Oh, J. J. and Oh, K. and Oh, S. H. and Ohashi, M. and Ohishi, N. and Ohkawa, M. and Ohta, H. and Okutani, Y. and Okutomi, K. and Oohara, K. and Ooi, C. and Oshino, S. and Otabe, S. and Pan, K.-C. and Pang, H. and Parisi, A. and Park, J. and Arellano, F. E. Peña and Pinto, I. and Sago, N. and Saito, S. and Saito, Y. and Sakai, K. and Sakai, Y. and Sakuno, Y. and Sato, S. and Sato, T. and Sawada, T. and Sekiguchi, T. and Sekiguchi, Y. and Shao, L. and Shibagaki, S. and Shimizu, R. and Shimoda, T. and Shimode, K. and Shinkai, H. and Shishido, T. and Shoda, A. and Somiya, K. and Son, E. J. and Sotani, H. and Sugimoto, R. and Suresh, J. and Suzuki, T. and Tagoshi, H. and Takahashi, H. and Takahashi, R. and Takamori, A. and Takano, S. and Takeda, H. and Takeda, M. and Tanaka, H. and Tanaka, K. and Tanaka, T. and Tanioka, S. and Tapia San Martín, E. N. and Telada, S. and Tomaru, T. and Tomigami, Y. and Tomura, T. and Travasso, F. and Trozzo, L. and Tsang, T. and Tsao, J.-S. and Tsubono, K. and Tsuchida, S. and Tsutsui, T. and Tsuzuki, T. and Tuyenbayev, D. and Uchikata, N. and Uchiyama, T. and Ueda, A. and Uehara, T. and Ueno, K. and Ueshima, G. and Uraguchi, F. and Ushiba, T. and Putten, M. H. P. M. and Vocca, H. and Wang, J. and Washimi, T. and Wu, C. and Wu, H. and Wu, S. and Xu, W.-R. and Yamada, T. and Yamamoto, K. and Yamamoto, T. and Yamashita, K. and Yamazaki, R. and Yang, Y. and Yano, K. and Yokogawa, K. and Yokoyama, J. and Yokozawa, T. and Yoshioka, T. and Yuzurihara, H. and Zeidler, S. and Zhan, M. and Zhang, H. and Zhao, Y. and Zhu, Z.-H. and Goetz, R. and Heintze, M. and Liu, J. and Müller, C. and Savage, R. L. and Tanner, D. B.},
  doi = {10.1093/ptep/ptac166},
  journal = {Progress of Theoretical and Experimental Physics},
  month = {dec},
  title = {Input optics systems of the KAGRA detector during O3GK},
  url = {https://doi.org/10.1093/ptep/ptac166},
  volume = {2023},
  year = {2022}
}

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Input optics systems of the KAGRA detector during O3GK

Journal article published in 2022 by T. Akutsu

, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya

, N. Aritomi

, H. Asada

, Y. Aso

, S. Bae

, Y. Bae, L. Baiotti

, R. Bajpai

, M. A. Barton

, K. Cannon

and other authors. T. Akutsu

, M. Ando, K. Arai, Y. Arai, S. Araki, A. Araya

, N. Aritomi

, H. Asada

, Y. Aso

, S. Bae

, Y. Bae, L. Baiotti

, R. Bajpai

, M. A. Barton

, K. Cannon

, Z. Cao

, E. Capocasa

, M. Chan, C. Chen

, K. Chen, Y. Chen, C.-I. Chiang, H. Chu, Y.-K. Chu, S. Eguchi

, Y. Enomoto

, R. Flaminio, Y. Fujii, Y. Fujikawa, M. Fukunaga, M. Fukushima, T. Furuhata, D. Gao

, G.-G. Ge

, S. Ha, A. Hagiwara, S. Haino, W.-B. Han

, K. Hasegawa, K. Hattori, H. Hayakawa, K. Hayama, Y. Himemoto, Y. Hiranuma

, N. Hirata, E. Hirose, Z. Hong, B.-H. Hsieh, G.-Z. Huang, H.-Y. Huang

, P. Huang

, Y.-C. Huang

, Y.-J. Huang

, D. C. Y. Hui

, S. Ide, B. Ikenoue, S. Imam, K. Inayoshi

, Y. Inoue, K. Ioka, K. Ito, Y. Itoh

, K. Izumi, C. Jeon, H.-B. Jin

, K. Jung, P. Jung

, K. Kaihotsu, T. Kajita

, M. Kakizaki

, M. Kamiizumi

, S. Kanbara, N. Kanda

, G. Kang, Y. Kataoka, K. Kawaguchi

, N. Kawai, T. Kawasaki

, C. Kim

, J. Kim

, J. C. Kim, W. S. Kim, Y.-M. Kim

, N. Kimura, N. Kita, H. Kitazawa, Y. Kojima, K. Kokeyama

, K. Komori, A. K. H. Kong

, K. Kotake

, C. Kozakai

, R. Kozu, R. Kumar, J. Kume, C. Kuo, H.-S. Kuo, Y. Kuromiya, S. Kuroyanagi

, K. Kusayanagi, K. Kwak

, H. K. Lee

, H. W. Lee

, R. Lee

, M. Leonardi

, K. L. Li

, L. C.-C. Lin

, C.-Y. Lin

, F.-K. Lin, F.-L. Lin

, H. L. Lin

, G. C. Liu

, L.-W. Luo

, E. Majorana

, M. Marchio, Y. Michimura

, N. Mio, O. Miyakawa

, A. Miyamoto, Y. Miyazaki, K. Miyo

, S. Miyoki

, Y. Mori, S. Morisaki, Y. Moriwaki, K. Nagano

, S. Nagano

, K. Nakamura

, H. Nakano

, M. Nakano, R. Nakashima, Y. Nakayama, T. Narikawa, L. Naticchioni

, R. Negishi, L. Nguyen Quynh

, W.-T. Ni

, A. Nishizawa

, S. Nozaki, Y. Obuchi, W. Ogaki, J. J. Oh

, K. Oh

, S. H. Oh, M. Ohashi

, N. Ohishi, M. Ohkawa

, H. Ohta, Y. Okutani, K. Okutomi, K. Oohara

, C. Ooi, S. Oshino

, S. Otabe, K.-C. Pan

, H. Pang, A. Parisi

, J. Park

, F. E. Peña Arellano

, I. Pinto, N. Sago

, S. Saito, Y. Saito, K. Sakai, Y. Sakai, Y. Sakuno, S. Sato, T. Sato, T. Sawada

, T. Sekiguchi, Y. Sekiguchi

, L. Shao

, S. Shibagaki

, R. Shimizu, T. Shimoda, K. Shimode

, H. Shinkai

, T. Shishido, A. Shoda

, K. Somiya

, E. J. Son

, H. Sotani

, R. Sugimoto

, J. Suresh

, T. Suzuki, H. Tagoshi

, H. Takahashi

, R. Takahashi

, A. Takamori, S. Takano, H. Takeda

, M. Takeda, H. Tanaka, K. Tanaka, T. Tanaka, S. Tanioka

, E. N. Tapia San Martín, S. Telada, T. Tomaru

, Y. Tomigami, T. Tomura

, F. Travasso

, L. Trozzo

, T. Tsang

, J.-S. Tsao, K. Tsubono, S. Tsuchida, T. Tsutsui, T. Tsuzuki

, D. Tuyenbayev

, N. Uchikata

, T. Uchiyama

, A. Ueda, T. Uehara

, K. Ueno

, G. Ueshima, F. Uraguchi, T. Ushiba

, M. H. P. M. Putten, H. Vocca

, J. Wang

, T. Washimi

, C. Wu

, H. Wu, S. Wu, W.-R. Xu, T. Yamada, K. Yamamoto

, T. Yamamoto, K. Yamashita, R. Yamazaki, Y. Yang

, K. Yano, K. Yokogawa, J. Yokoyama

, T. Yokozawa, T. Yoshioka, H. Yuzurihara, S. Zeidler

, M. Zhan, H. Zhang, Y. Zhao

, Z.-H. Zhu

, R. Goetz, M. Heintze, J. Liu, C. Müller, R. L. Savage, D. B. Tanner

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Abstract

Abstract KAGRA, the underground and cryogenic gravitational-wave detector, was operated for its solo observation from February 25 to March 10, 2020, and its first joint observation with the GEO 600 detector from April 7 to April 21, 2020 (O3GK). This study presents an overview of the input optics systems of the KAGRA detector, which consist of various optical systems, such as a laser source, its intensity and frequency stabilization systems, modulators, a Faraday isolator, mode-matching telescopes, and a high-power beam dump. These optics were successfully delivered to the KAGRA interferometer and operated stably during the observations. The laser frequency noise was observed to limit the detector sensitivity above a few kilohertz, whereas the laser intensity did not significantly limit the detector sensitivity.

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Input optics systems of the KAGRA detector during O3GK

Abstract