Zobrazeno 1 - 10
of 61
pro vyhledávání: '"OHNISHI, Kouji"'
Autor:
Hayakawa, Hisashi, Ebihara, Yusuke, Mishev, Alexander, Koldobskiy, Sergey, Kusano, Kanya, Bechet, Sabrina, Yashiro, Seiji, Iwai, Kazumasa, Shinbori, Atsuki, Mursula, Kalevi, Miyake, Fusa, Shiota, Daikou, Silveira, Marcos V. D., Stuart, Robert, Oliveira, Denny M., Akiyama, Sachiko, Ohnishi, Kouji, Ledvina, Vincent, Miyoshi, Yoshizumi
Publikováno v:
The Astrophysical Journal, 2024
In May 2024, the scientific community observed intense solar eruptions that resulted in a great geomagnetic storm and auroral extension, highlighting the need to document and quantify these events. This study mainly focuses on their quantification. T
Externí odkaz:
http://arxiv.org/abs/2407.07665
Akademický článek
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Autor:
Koshimoto, Naoki, Shvartzvald, Yossi, Bennett, David, Penny, Matthew, Hundertmark, Markus, Bond, Ian A., Zang, Weicheng, Henderson, Calen, Suzuki, Daisuke, Rattenbury, Nicholas J., Sumi, Takahiro, Abe, Fumio, Asakura, Yuichiro, Bhattacharya, Aparna, Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Li, M. C. A., Ling, C., Masuda, Kimiaki, Matsubara, Y., Matsuo, Taro, Muraki, Yasushi, Nagakane, Masayuki, Ohnishi, Kouji, Ranc, C., Saito, To., Sharan, A., Shibai, Hiroshi, Sullivan, Denis, Tristram, P., Yonehara, A., Gelino, Christopher, Beichman, Charles, Beaulieu, Jean-Philippe, Marquette, J. -B., Batista, Virginie, Friedmann, M., Hallakoun, N., Kaspi, Shai, Maoz, Dani, Bryden, G., Novati, Sebastiano Calchi, Howell, Steve, Wang, T., Mao, Shude, Fouque, Pascal, Korhonen, Heidi, Jorgensen, Uffe, Street, Rachel, Tsapras, Yiannis, Dominik, Martin, Kerins, Eamonn, Cassan, Arnaud, Snodgrass, Colin, Bachelet, Etienne, Bozza, Valerio, Bramich, D. M.
We report the discovery of a microlensing planet --- MOA-2016-BLG-227Lb --- with a large planet/host mass ratio of $q \simeq 9 \times 10^{-3}$. This event was located near the $K2$ Campaign 9 field that was observed by a large number of telescopes. A
Externí odkaz:
http://arxiv.org/abs/1704.01724
Autor:
Nagakane, Masayuki, Sumi, Takahiro, Koshimoto, Naoki, Bennett, David P., Bond, Ian A., Rattenbury, Nicholas J., Suzuki, Daisuke, Abe, Fumio, Asakura, Yuichiro, Barry, Richard K., Bhattacharya, Aparna, Donachie, M., Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Li, M. C. A., Ling, C. H., Masuda, Kimiaki, Matsubara, Y., Matsuo, Taro, Muraki, Yasushi, Ohnishi, Kouji, Ranc, C., Saito, To., Sharan, A., Shibai, Hiroshi, Sullivan, Denis J., Tristram, P. J., Yamada, Touko, Yonehara, A.
We report the discovery of a super-Earth mass planet in the microlensing event MOA-2012-BLG-505. This event has the second shortest event timescale of $t_{\rm E}=10 \pm 1$ days where the observed data show evidence of planetary companion. Our 15 minu
Externí odkaz:
http://arxiv.org/abs/1703.10769
Autor:
Fukui, Akihiko, Narita, Norio, Tristram, Paul J., Sumi, Takahiro, Abe, Fumio, Itow, Yoshitaka, Sullivan, Denis J., Bond, Ian A., Hirano, Teruyuki, Tamura, Motohide, Bennett, David P., Furusawa, Kei, Hayashi, Fumiya, Hearnshaw, John B., Hosaka, Shun, Kamiya, Koki, Kobara, Shuhei, Korpela, Aarno, Kilmartin, Pam M., Lin, Wei, Ling, Cho Hong, Makita, Shota, Masuda, Kimiaki, Matsubara, Yutaka, Miyake, Noriyuki, Muraki, Yasushi, Nagaya, Maiko, Nishimoto, Kenta, Ohnishi, Kouji, Omori, Kengo, Perrott, Yvette, Rattenbury, Nicholas, Saito, Toshiharu, Skuljan, Ljiljana, Suzuki, Daisuke, Sweatman, Winston L., Wada, Kohei
We have observed 7 new transits of the `hot Jupiter' WASP-5b using a 61 cm telescope located in New Zealand, in order to search for transit timing variations (TTVs) which can be induced by additional bodies existing in the system. When combined with
Externí odkaz:
http://arxiv.org/abs/1009.5769
Publikováno v:
In Bioorganic & Medicinal Chemistry 15 January 2019 27(2):425-435
We have measured the radiant of the Leonids meteor storm in November 2001 by using new observational and analysis techniques. The radiant was measured as the intersections of lines which were detected and extrapolated from images obtained at a single
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210627
Autor:
Yanagisawa, Masahisa, Ohnishi, Kouji, Takamura, Yuzaburo, Masuda, Hiroshi, Sakai, Yoshihito, Ida, Miyoshi, Adachi, Makoto, Ishida, Masayuki
Publikováno v:
In Icarus 2006 182(2):489-495
Autor:
OHNISHI, Kouji
Publikováno v:
長野工業高等専門学校紀要 = Memoirs of Nagano National College of Technology. 38:79-86
McNaught and Asher (2001) predicted the precise positions of radiant points due to the 4-rev (1866 yr.) and 9-rev (1699 yr) dust trails of the Leonids. To establish the dust trail theory and to measure the flux and magnitude distribution of very fain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::b59422be9828c9f21e1be7900ff05eb5
http://id.nii.ac.jp/1051/00000107/
http://id.nii.ac.jp/1051/00000107/
Publikováno v:
長野工業高等専門学校紀要 = Memoirs of Nagano National College of Technology. 38:87-94
McNaught and Asher (2001) predicted the Leonids Meteor Storm in 2001 due to the 4-rev (1866 yr.) and 9-rev (1699 yr) dust trails of the Leonids. To measure the flux and magnitude distribution of very faint meteors, we performed deep imaging telescopi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::013b442f5034ab6147674f488142e84b
http://id.nii.ac.jp/1051/00000108/
http://id.nii.ac.jp/1051/00000108/