Zobrazeno 1 - 10
of 108
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
Akademický článek
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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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::b5a9cdcebf2e7112891ba16ece9e7983
http://id.nii.ac.jp/1707/00028354/
http://id.nii.ac.jp/1707/00028354/
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
Publikováno v:
Publications of the Astronomical Society of Japan; Apr2017, Vol. 69 Issue 2, p1-10, 10p
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6d0749e73ac90ede961bafb4351f945
https://doi.org/10.1117/12.2055676
https://doi.org/10.1117/12.2055676
Publikováno v:
Publications of the Astronomical Society of Japan; Jun2016, Vol. 68 Issue supp1, pS14-1-S14-8, 8p