Y
Yasuhiro Kashiwagi
Researcher at Mitsubishi Electric
Publications - 11
Citations - 349
Yasuhiro Kashiwagi is an academic researcher from Mitsubishi Electric. The author has contributed to research in topics: Supernova & Neutron. The author has an hindex of 3, co-authored 3 publications receiving 325 citations.
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Journal ArticleDOI
Image Stabilization System for Hinode (Solar-B) Solar Optical Telescope
Toshifumi Shimizu,Shin Nagata,Saku Tsuneta,T. D. Tarbell,Christopher G. Edwards,R. A. Shine,C. Hoffmann,E. Thomas,S. Sour,R. Rehse,Osamu Ito,Yasuhiro Kashiwagi,Masaki Tabata,Kazuhide Kodeki,M. Nagase,K. Matsuzaki,K. Kobayashi,Kiyoshi Ichimoto,Yoshinori Suematsu +18 more
TL;DR: The Hinode Solar Optical Telescope (SOT) is the first space-borne visible-light telescope that enables us to observe magnetic field dynamics in the solar lower atmosphere with 0.2 -0.3 arcsec spatial resolution under extremely stable (seeing-free) conditions.
Proceedings ArticleDOI
Image stabilization system on SOLAR-B Solar Optical Telescope
Toshifumi Shimizu,Shin’ichi Nagata,Chris Edwards,Theodore D. Tarbell,Yasuhiro Kashiwagi,Kazuhide Kodeki,Osamu Ito,Hiroyuki Miyagawa,Masayuki Nagase,Syunsaku Inoue,Kazumasa Kaneko,Yasushi Sakamoto,Kiyoshi Ichimoto,Saku Tsuneta,Shiro Miki,Makoto Endo,Masaki Tabata,Toshitaka Nakaoji,K. Matsuzaki,Ken Kobayashi,Masashi Otsubo,Yoshinori Suematsu,Kazuyoshi Kumagai,Motokazu Noguchi,Tomonori Tamura,Masao Nakagiri +25 more
TL;DR: In this article, an image stabilization system is installed to the Solar Optical Telescope onboard SOLAR-B, which stabilizes images on the focal plane CCD detectors in the frequency range lower than about 20Hz.
Journal ArticleDOI
Development of a Correlation Tracker and a Tip-Tilt Mirror System for SOLAR-B
Kazuhide Kodeki,Yasuhiro Kashiwagi,Shiro Miki,Makoto Endoh,Osamu Itoh,Toshihumi Shimizu,Keiichi Matsuzaki,Shin’ichi Nagata,Kiyoshi Ichimoto,Saku Tsuneta +9 more
TL;DR: In this article, the authors proposed using the correlation tracker and tip-tilt mirror package (CTM), which stabilizes the sun observation image, and the mechanism and the control and determination methods of the control gain of CTM were described.
Journal ArticleDOI
Search for Cosmic-Ray Boosted Sub-GeV Dark Matter Using Recoil Protons at Super-Kamiokande.
T. Abe,Yoshinari Hayato,Katsuki Hiraide,K. Ieki,M. Ikeda,J. Kameda,Y. Kanemura,R. Kaneshima,Yasuhiro Kashiwagi,Y. Kataoka,S. Miki,S. Mine,M. Miura,Shigetaka Moriyama,Yuuki Nakano,Masayuki Nakahata,S. Nakayama,Yuto Noguchi,K. Okamoto,K. Sato,Hiroyuki Sekiya,Hisashi Shiba,Kazuhiro Shimizu,Masato Shiozawa,Y. Sonoda,Y. Suzuki,Atsushi Takeda,Y. Takemoto,A. Takenaka,H. Tanaka,S.Watanabe,T. Yano,S.R. Han,T. Kajita,Ko Okumura,Tsuguhiko Tashiro,Touichirou Tomiya,X. Wang,J. Xia,S. Yoshida,G. D. Megias,Pablo Fernandez,L. Labarga,N. Ospina,Bryan Zaldivar,B. W. Pointon,E. Kearns,J. L. Raaf,L. Wan,T. Wester,J. Bian,N. J. Griskevich,W. R. Kropp,S. Locke,M. B. Smy,H. W. Sobel,V. Takhistov,Adriana Kiczkowski Yankelevich,J. C. Hill,R. G. Park,Baran Bodur,Kate Scholberg,C. W. Walter,Lucy Bernard,A. Coffani,O. Drapier,Sonia El Hedri,A. Giampaolo,Th. A. Mueller,Pietro Paganini,B. Quilain,T. Ishizuka,T. Nakamura,J. S. Jang,John G. Learned,K. U. Choi,S. V. Cao,L. H. V. Anthony,D. Martin,Mark Scott,A. A. Sztuc,Y. Uchida,Vincenzo Berardi,M. G. Catanesi,E. Radicioni,N. F. Calabria,L. N. Machado,G. De Rosa,G. Collazuol,F. Iacob,M. Lamoureux,Marco Mattiazzi,L. Ludovici,M. Gonin,G. Pronost,Chie Fujisawa,Y. Maekawa,Y. Nishimura,M. Friend,Takehisa Hasegawa,T. Ishida,T. Kobayashi,M. Jakkapu,T. Matsubara,T. Nakadaira,Y. Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,T. Boschi,F. Di Lodovico,J Gao,A. Goldsack,Teppei Katori,J. Migenda,Mahdi Taani,S. Zsoldos,Y. Kotsar,H. Ozaki,A. Suzuki,Y. Takeuchi,C. Bronner,Ji Feng,T. Kikawa,M. Mori,Tsuyoshi Nakaya,R. A. Wendell,K. Yasutome,S. J. Jenkins,N. McCauley,P. Mehta,Ka Ming Tsui,Y. Fukuda,Yoshitaka Itow,Hiroaki Menjo,Kiyoaki Ninomiya,J. Lagoda,S. M. Lakshmi,Mangani Lal Mandal,P. Mijakowski,Yogeendra Prabhu,J. Zalipska,M. Jia,J. Jiang,C. K. Jung,M. J. Wilking,C. Yanagisawa,M. Harada,Hirokazu Ishino,S. Ito,Hussain Kitagawa,Yusuke Koshio,Fumitake Nakanishi,S. Sakai,G.D. Barr,D. Barrow,L. Cook,S. Samani,D. L. Wark,F. Nova,J. Yang,M. Malek,J. McElwee,O. Stone,M. Thiesse,L. F. Thompson,H. Okazawa,S. B. Kim,J. W. Seo,Intae Yu,A. K. Ichikawa,K. Nakamura,S. Tairafune,Kyoshi Nishijima,K. Iwamoto,K. Nakagiri,Y. Nakajima,Noriko Taniuchi,Masashi Yokoyama,K. Martens,P. de Perio,Mark R. Vagins,M. Kuze,S. Izumiyama,Michiaki Inomoto,M. Ishitsuka,Hiroshi Ito,Tatsushi Kinoshita,R. Matsumoto,Yuta Ommura,Noriko Shigeta,M. Shinoki,Takuo Suganuma,Kazunobu Yamauchi,J. F. Martin,T. Towstego,R. Akutsu,V. Gousy-Leblanc,M. Hartz,A. Konaka,N. W. Prouse,S. Chen,B D Xu,B Zhang,M. Posiadala-Zezula,David Hadley,M. Nicholson,M. O'Flaherty,B. Richards,A. Ali,B. Jamieson,Ll. Marti,A. Minamino,G. Pintaudi,S. Sano,S. Suzuki,Kenji Wada +216 more
TL;DR: In this paper , a search for cosmic-ray boosted dark matter with hadrons using directional information was conducted using the Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase).
Journal ArticleDOI
Searching for Supernova Bursts in Super-Kamiokande IV
T. Mori,K. Abe,Yoshinari Hayato,Katsuki Hiraide,K. Ieki,M. Ikeda,S.Imaizumi,J. Kameda,Y. Kanemura,R. Kaneshima,Yasuhiro Kashiwagi,Y. Kataoka,S. Miki,S. Mine,M. Miura,Shigetaka Moriyama,Y. Nagao,Masayuki Nakahata,Yuuki Nakano,S. Nakayama,Yuto Noguchi,T. Okada,K. Okamoto,A. Orii,K. Sato,Hiroyuki Sekiya,Hisashi Shiba,Kazuhiro Shimizu,Masato Shiozawa,Y. Sonoda,Y. Suzuki,Atsushi Takeda,Y. Takemoto,A. Takenaka,H. Tanaka,Touichirou Tomiya,S.Watanabe,T. Yano,S. Yoshida,S.R. Han,T. Kajita,Ko Okumura,Tsuguhiko Tashiro,X. Wang,J. Xia,G. D. Megias,D. Bravo-Berguño,Pablo Fernandez,L. Labarga,N. Ospina,Bryan Zaldivar,S. Zsoldos,B. W. Pointon,F. d. M. Blaszczyk,E. Kearns,J. L. Raaf,J. L. Stone,L. Wan,T. Wester,J. Bian,N. J. Griskevich,W. R. Kropp,S. Locke,M. B. Smy,H. W. Sobel,V. Takhistov,Yankelevich,J. C. Hill,J. Y. Kim,I. T. Lim,R. G. Park,Baran Bodur,Kate Scholberg,C. W. Walter,Lucy Bernard,A. Coffani,O. Drapier,Sonia El Hedri,A. Giampaolo,Th. A. Mueller,Pietro Paganini,B. Quilain,T. Ishizuka,T. Nakamura,J. S. Jang,John G. Learned,L. H. V. Anthony,D. Martin,Mark Scott,A. A. Sztuc,Y. Uchida,Vincenzo Berardi,M. G. Catanesi,E. Radicioni,N. F. Calabria,L. N. Machado,G. De Rosa,G. Collazuol,F. Iacob,M. Lamoureux,Marco Mattiazzi,L. Ludovici,M. Gonin,G. Pronost,Y. Maekawa,Y. Nishimura,Chie Fujisawa,M. Friend,Takehisa Hasegawa,T. Ishida,T. Kobayashi,M. Jakkapu,T. Matsubara,T. Nakadaira,Y. Oyama,K. Sakashita,T. Sekiguchi,Takuya Tsukamoto,H. Ozaki,Tomoo Shiozawa,A. Suzuki,Y. Takeuchi,Shoji Yamamoto,Y. Kotsar,Y. Ashida,C. Bronner,Ji Feng,Seiko Hirota,T. Kikawa,Tsuyoshi Nakaya,R. A. Wendell,K. Yasutome,N. McCauley,P. Mehta,Ka Ming Tsui,Y. Fukuda,Yoshitaka Itow,Hiroaki Menjo,K. Ninomiya,T. Niwa,M. Tsukada,J. Lagoda,S. M. Lakshmi,P. Mijakowski,J. Zalipska,Mangani Lal Mandal,Yogeendra Prabhu,J. Jiang,C. K. Jung,C. Vilela,M. J. Wilking,C. Yanagisawa,M. Jia,K. Hagiwara,M. Harada,T. Horai,Hirokazu Ishino,S. Ito,Hussain Kitagawa,Yusuke Koshio,W. Ma,Fumitake Nakanishi,N. Piplani,S. Sakai,G.D. Barr,D. Barrow,L. Cook,S. Samani,D. L. Wark,F. Nova,T. Boschi,J Gao,A. Goldsack,Teppei Katori,F. Di Lodovico,J. Migenda,Mahdi Taani,J. Yang,S. J. Jenkins,M. Malek,J. McElwee,O. Stone,M. Thiesse,L. F. Thompson,H. Okazawa,S. B. Kim,J. W. Seo,Intae Yu,Kaihei Nishijima,Masatoshi Koshiba,K. Nakagiri,Y. Nakajima,K. Iwamoto,Noriko Taniuchi,Masashi Yokoyama,K. Martens,P. de Perio,Mark R. Vagins,M. Kuze,S. Izumiyama,T. Yoshida,Michiaki Inomoto,M. Ishitsuka,Hiroshi Ito,Tatsushi Kinoshita,R. Matsumoto,K. Ohta,Yuta Ommura,Noriko Shigeta,M. Shinoki,Takuo Suganuma,Kazunobu Yamauchi,J. F. Martin,T. Towstego,R. Akutsu,V. Gousy-Leblanc,M. Hartz,A. Konaka,N. W. Prouse,S. Chen,B D Xu,B Zhang,M. Posiadala-Zezula,David Hadley,M. Nicholson,M.O. Flaherty,B. Richards,A. Ali,B. Jamieson,Jill Walker,Ll. Marti,A. Minamino,G. Pintaudi,R. Sasaki,S. Sano,S. Suzuki,Kenji Wada,S. V. Cao,A. K. Ichikawa,K. Nakamura,S. Tairafun +240 more
TL;DR: In this article , the authors focus on detecting more distant supernovae whose event rate may be too small to trigger in real time, but may be identified using an offline approach.