Y
Yoshio Saito
Researcher at Nihon University
Publications - 144
Citations - 2510
Yoshio Saito is an academic researcher from Nihon University. The author has contributed to research in topics: Fluorescence & Thymine. The author has an hindex of 26, co-authored 142 publications receiving 2403 citations. Previous affiliations of Yoshio Saito include University of Western Ontario & Centre national de la recherche scientifique.
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Journal ArticleDOI
Palladium-assisted routes to nucleosides.
Journal ArticleDOI
Stable Operation of a 300-m Laser Interferometer with Sufficient Sensitivity to Detect Gravitational-Wave Events within Our Galaxy
Masaki Ando,Koji Arai,Ryutaro Takahashi,Gerhard Heinzel,Seiji Kawamura,Daisuke Tatsumi,Nobuyuki Kanda,Hideyuki Tagoshi,Akito Araya,Hideki Asada,Youich Aso,M. A. Barton,Masa Katsu Fujimoto,Mitsuhiro Fukushima,Toshifumi Futamase,Kazuhiro Hayama,Gen'ichi Horikoshi,Hideki Ishizuka,Norihiko Kamikubota,Keita Kawabe,Nobuki Kawashima,Yoshinori Kobayashi,Yasufumi Kojima,Kazuhiro Kondo,Yoshihide Kozai,Kazuaki Kuroda,Namio Matsuda,Norikatsu Mio,Kazuyuki Miura,Osamu Miyakawa,Shoken M. Miyama,Shinji Miyoki,Shigenori Moriwaki,Mitsuru Musha,Shigeo Nagano,Ken'ichi Nakagawa,Takashi Nakamura,Ken-ichi Nakao,Kenji Numata,Yujiro Ogawa,M. Ohashi,Naoko Ohishi,Satoshi Okutomi,K. Oohara,Shigemi Otsuka,Yoshio Saito,Misao Sasaki,Shuichi Sato,Atsushi Sekiya,Masaru Shibata,Kentaro Somiya,Toshikazu Suzuki,Akiteru Takamori,Takahiro Tanaka,Shinsuke Taniguchi,Souichi Telada,Kuniharu Tochikubo,Takayuki Tomaru,Kimio Tsubono,Nobuhiro Tsuda,Takashi Uchiyama,Akitoshi Ueda,Ken-ichi Ueda,Koichi Waseda,Yuko Watanabe,Hiromi Yakura,Kazuhiro Yamamoto,Toshitaka Yamazaki +67 more
TL;DR: TAMA300, an interferometric gravitational-wave detector with 300-m baseline length, has been developed and operated with sufficient sensitivity to detect gravitational- wave events within the authors' galaxy and sufficient stability for observations.
Journal ArticleDOI
Design of base-discriminating fluorescent nucleosides
TL;DR: A new concept in the design of base-discriminating fluorescent (BDF) nucleosides that can clearly distinguish the type of base opposite the BDF base by a fluorescence change is demonstrated.
Journal ArticleDOI
Large-scale cryogenic gravitational wave telescope
Kazuaki Kuroda,M. Ohashi,Shinji Miyoki,Daisuke Tatsumi,Shuichi Sato,Hideki Ishizuka,Masa Katsu Fujimoto,Seiji Kawamura,Ryutaro Takahashi,Toshitaka Yamazaki,Koji Arai,Mitsuhiro Fukushima,Koichi Waseda,Souichi Telada,Akitoshi Ueda,Takakazu Shintomi,Akira Yamamoto,Toshikazu Suzuki,Yoshio Saito,Tomiyoshi Haruyama,Nobuaki Sato,Kimio Tsubono,Keita Kawabe,Masaki Ando,Ken-ichi Ueda,Hitoki Yoneda,Mitsuru Musha,Norikatsu Mio,Shigenori Moriwaki,Akito Araya,Nobuyuki Kanda,Michael E. Tobar +31 more
TL;DR: The Large-scale Cryogenic Gravitational wave Telescope (LCGT) project as mentioned in this paper was proposed to improve the sensitivity of the existing gravitational wave projects by ten times by using a higher power laser.
Journal ArticleDOI
First search for gravitational waves from inspiraling compact binaries using TAMA300 data
Hideyuki Tagoshi,Nobuyuki Kanda,Takahiro Tanaka,Daisuke Tatsumi,Souichi Telada,Masaki Ando,Koji Arai,A. Araya,Hideki Asada,M. A. Barton,Masa Katsu Fujimoto,M. Fukushima,Toshifumi Futamase,Gerhard Heinzel,Ge N.Ichi Horikoshi,Hideki Ishizuka,Norihiko Kamikubota,Keita Kawabe,Seiji Kawamura,Nobuki Kawashima,Yasufumi Kojima,Yoshihide Kozai,Kazuaki Kuroda,Namio Matsuda,Sumihiro Matsumura,Satoshi Miki,Norikatsu Mio,Osamu Miyakawa,Shoken M. Miyama,Shinji Miyoki,Eiichi Mizuno,Shigenori Moriwaki,Mitsuru Musha,Shigeo Nagano,Ke N.Ichi Nakagawa,Takashi Nakamura,Ken-ichi Nakao,Kenji Numata,Yujiro Ogawa,M. Ohashi,N. Ohishi,Akira Okutomi,K. Oohara,Shigemi Otsuka,Yoshio Saito,Misao Sasaki,Shuichi Sato,Atsushi Sekiya,Masaru Shibata,Kazumichi Shirakata,Kentaro Somiya,Toshikazu Suzuki,Ryutaro Takahashi,A. Takamori,Shinsuke Taniguchi,Kuniharu Tochikubo,Takayuki Tomaru,Kimio Tsubono,Nobuhiro Tsuda,Takashi Uchiyama,Akitoshi Ueda,Ken-ichi Ueda,Kozo Ueda,Koichi Waseda,Yuko Watanabe,Hiromi Yakura,Kazuhiro Yamamoto,T. Yamazaki +67 more
TL;DR: In this article, the authors analyzed 6 hours of data from the TAMA300 detector by matched filtering, searching for gravitational waves from inspiraling compact binaries and obtained an upper limit of 0.59/hour (C.L.=90%) on the event rate of inspirals of compact binaries with mass between 0.3M and 10M/solar and with signal-to-noise ratio greater than 7.2.