Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Ko, Ono"'
Autor:
Kubota, Megu, Tamagawa, Toru, Makishima, Kazuo, Nakano, Toshio, Iwakiri, Wataru, Sugizaki, Mutsumi, Ko, Ono
Publikováno v:
Publ. Astron. Soc. Japan (2019) 00 (0), 1-13
The typical accreting neutron star, Aquila X-1, was observed with Suzaku seven times in the decay phase of an outburst in 2007 September-October. Among them, the second to the fourth observations were performed 10 to 22 days after the outburst peak,
Externí odkaz:
http://arxiv.org/abs/1902.05225
Publikováno v:
同志社スポーツ健康科学 = Doshisha Journal of Health & Sports Science. 13:19-28
本研究では,プロ野球・Jリーグ・Bリーグ・オリンピックにおけるスポーツ観戦についての新聞記事を内容分析することにより,コロナ禍におけるスポーツ観戦スタイルの実態を明らか
Autor:
Toshio Nakano, Wataru Iwakiri, Megu Kubota, Toru Tamagawa, Mutsumi Sugizaki, Ko Ono, Kazuo Makishima
The typical accreting neutron star, Aquila X-1, was observed with Suzaku seven times in the decay phase of an outburst in 2007 September-October. Among them, the second to the fourth observations were performed 10 to 22 days after the outburst peak,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0330fca6602c71c0b196ac001cdb7c2
http://arxiv.org/abs/1902.05225
http://arxiv.org/abs/1902.05225
The neutron star Low-Mass X-ray Binary GS 1826-238 was observed with Suzaku on 2009 October 21, for a total exposure of 103 ksec. Except for the type I bursts, the source intensity was constant to within ~10%. Combining the Suzaku XIS, HXD-PIN and HX
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eda9f0b62d4a0b05657c880229536a22
The recurrent soft X-ray transient Aquila X-1 was observed with Suzaku for a gross duration of 79.9 ks, on 2011 October 21 when the object was in a rising phase of an outburst. During the observation, the source exhibited a clear spectral transition
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af4800c54fcdc6399e0d8036417cfabe
Autor:
Zhongli Zhang, Kazuhiro Nakazawa, Shinya Yamada, Soki Sakurai, Haiguang Xu, Kazuo Makishima, Ko Ono
Utilizing an archived Suzaku data acquired on 2007 December 25 for 46 ks, X-ray spectroscopic properties of the dipping and eclipsing low-mass X-ray binary EXO 0748$-$676 were studied. At an assumed distance of 7.1 kpc, the data gave a persistent una
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5131e6f66979ac5bba7c692fefeef1bd
Autor:
Toshio Nakano, G. Sato, Ikumi Edahiro, Tadayuki Takahashi, Ko Ono, Kouichi Hagino, Hiroaki Murakami, Kazuhiro Nakazawa, Soki Sakurai, Kunihiro Goto, Terukazu Nishida, Masanori Ohno, Motohide Kokubun, Daisuke Yonetoku, S. Torii, Hiromitsu Takahashi, Hirokazu Odaka, Shin'ya Tokuda, S. Furui, Jun Kataoka, Yasushi Fukazawa, Syogo Kobayashi, Yoichi Yatsu, Kazutaka Yamaoka, Hiroyasu Tajima, Shin Watanabe, Takeshi Nakamori, Takayuki Yuasa, Hideki Uchiyama, Kazuo Makishima, Makoto Sasano, R. Sato, Tatsuhiko Saito, Katsuma Miyake, T. Kawano
Publikováno v:
Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray.
The hard X-ray imager (HXI) and soft gamma-ray detector (SGD) onboard Astro-H observe astronomical objects with high sensitivity in the hard X-ray (5−80 keV) and soft gamma-ray (40−600 keV) energy bands. To achieve this high sensitivity, backgrou
Autor:
Hiromitsu Takahashi, Shinya Yamada, S. Torii, Ko Ono, Kazuo Makishima, Zhongli Zhang, Masaru Matsuoka, Hirofumi Noda, Soki Sakurai, Kazuhiro Nakazawa
The neutron-star Low-Mass X-ray Binary Aquila X-1 was observed by Suzaku for seven times, from 2007 September 28 to October 30. The observations successfully traced an outburst decay in which the source luminosity decreased almost monotonically from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e16111026a60e2ab9b1eda5954596914
http://arxiv.org/abs/1308.6091
http://arxiv.org/abs/1308.6091
Autor:
Hisanori Horiuchi, Takeshi Kimura Kimu, Toshihiro Tamura, Tomohisa Tada, Neiko Ozasa, Ko Ono, Satoshi Shizu, Toshikazu Jinnai, Junichi Tazaki
Publikováno v:
Journal of the American College of Cardiology. 55(10)
Publikováno v:
Publications of the Astronomical Society of Japan; Apr2017, Vol. 69 Issue 2, p1-10, 10p