Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Kazunari Masumoto"'
Autor:
Masaru Suzuki, Daichi Furusawa, Takumi Toyoshima, Kazunari Masumoto, Kyoichi Mori, Sho Owada, Yuichi Tsumaki, Ryota Murakami
Publikováno v:
Journal of Robotics and Mechatronics. 33:475-483
The biologging approach of attaching a logger to the body of an animal provides information that cannot be obtained by conventional direct visual observation. Marine zoologists have used this technique for observing sperm whales preying on giant squi
Autor:
Katsura Matsumoto, Tansel Ak, Miho Kawabata, Tomohito Ohshima, Hide Akazawa, Ömer Ayyıldız, R. Ishioka, Önder Orakoğlu, Chikako Nakata, Hasan Esenoğlu, Turker Ozkan, Emre Bektöre, Tolga Guver, Linda Schmidtobreick, Metin Altan, Kazunari Masumoto, Makoto Uemura, Antonio Bianchini, Taichi Kato, Takafumi Hori
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 489:1451-1462
The cataclysmic variable SDSS J214354.59+124457.8 (hereafter SDSS J214354) was observed photometrically on sixty one nights between 2012 July 28 and 2019 May 26. The long term variation of this object shows changes between two phases; a dwarf nova ty
Publikováno v:
The Proceedings of JSME annual Conference on Robotics and Mechatronics (Robomec). 2022:2A1-C05
Autor:
Masaru SUZUKI, Kazunari MASUMOTO, Hiroto NAKAGAWA, Kouta ABE, Hiroyuki NISHIMORI, Yuichi TSUMAKI, Kyoichi MORI, Koki TSUJII
Publikováno v:
The Proceedings of JSME annual Conference on Robotics and Mechatronics (Robomec). 2022:2A2-A09
Autor:
Takashi Hattori, Ken'ichi Nomoto, Tatsuya Nakaoka, Naoto Kojiguchi, Hiroshi Akitaya, Michitoshi Yoshida, Keiich Maeda, Takahiro Ui, Katsura Matsumoto, Daiki Fukushima, Yuki Moritani, Kazunari Masumoto, Koji S. Kawabata, Yuka Kanda, Makoto Uemura, Masayuki Yamanaka, Katsutoshi Takaki, Nozomu Tominaga, Ryosuke Itoh, Miho Kawabata, Chien-Hsiu Lee, Koji Takata
Publikováno v:
Publications of the Astronomical Society of Japan. 70
We present optical and near-infrared observations of the nearby Type Iax supernova (SN) 2014dt from 14 to 410 days after the maximum light. The velocities of the iron absorption lines in the early phase indicated that SN 2014dt showed slower expansio
Autor:
Masaru SUZUKI, Kazunari MASUMOTO, Hayato MUROFUSHI, Hiroto NAKAGAWA, Ryoko OZAKI, Sho OWADA, Yuichi TSUMAKI, Kyoichi MORI, Koki TSUJII
Publikováno v:
The Proceedings of JSME annual Conference on Robotics and Mechatronics (Robomec). 2021:2P1-M08
Autor:
Daisaku Nogami, Aleksei A. Sosnovskij, Franz-Josef Hambsch, Taichi Kato, Nikolai Pit, Arto Oksanen, Seiichiro Kiyota, Alex Baklanov, Kazuki Maeda, Kiyoshi Kasai, Lewis M. Cook, Yuki Sugiura, Risa Matsuda, Tomohito Ohshima, Naoto Kojiguchi, Kirill A. Antonyuk, Katsura Matsumoto, Nao Takeda, Daiki Fukushima, Gianluca Masi, Pavol A. Dubovsky, Aleksandr Sklyanov, Julia V. Babina, Yutaka Maeda, Hiroshi Itoh, Elena P. Pavlenko, Akira Imada, Shawn Dvorak, Rudolf Novak, Colin Littlefield, Kazunari Masumoto, Keisuke Isogai, Oksana I. Antonyuk, Miho Kawabata
We report on two superoutbursts of the AM CVn-type object CR Boo in 2014 April--March and 2015 May--June. A precursor outburst acompanied both of these superoutbursts. During the rising branch of the main superoutburst in 2014, we detected growing su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::363d37e3570514b9d4897c160df96d35
http://arxiv.org/abs/1605.05408
http://arxiv.org/abs/1605.05408
Autor:
Makoto Watanabe, Yumiko Oasa, Hiroshi Akitaya, Hideyuki Izumiura, Mizuki Isogai, Katsura Matsumoto, Tomoki Morokuma, Michitoshi Yoshida, Jun Takahashi, Ryo Miyanoshita, Keiichi Maeda, Hidekazu Hanayama, Koji S. Kawabata, Takahiro Nagayama, Kazunari Masumoto, Takahiro Ui, Ryosuke Itoh, Toshihiro Omodaka, Makoto Uemura, Issei Ueno, Nozomu Tominaga, Masayuki Yamanaka, Yoshihiko Saito, Masaomi Tanaka, Katsutoshi Takaki, Akira Arai, Rikako Ono, Daisaku Nogami, Tatsuya Nakaoka, Nobuharu Ukita, Takashi Nagao, Kazuhiro Sekiguchi, Miho Kawabata, Daisuke Kuroda, Ryo Noguchi, Kenshi Yanagisawa, Satoshi Honda
Publikováno v:
Publications of the Astronomical Society of Japan. 68(Number 5)
We present extensively dense observations of the super-Chandrasekhar supernova (SC SN) candidate SN 2012dn from $-11$ to $+140$ days after the date of its $B$-band maximum in the optical and near-infrared (NIR) wavelengths conducted through the OISTE
Autor:
Kazunari Masumoto, Megumi Takenaka, Hiroki Kinoshita, Enrique de Miguel, Pavol A. Dubovsky, Shizuo Kaneko, George Sjoberg, Vitaly Neustroev, Kazuyoshi Imamura, Kazuhiko Shiokawa, Aleksandr Sklyanov, D. Denisenko, Arto Oksanen, V. Krushevska, Aleksei A. Sosnovskij, Joseph Ulowetz, Noritoshi Otani, Steve Rau, Seiichiro Kiyota, J. L. Prieto, William N. Goff, Hidehiko Akazawa, Risa Matsuda, Peter Starr, Katsura Matsumoto, Ludwig Logie, Kevin B. Paxson, P. Golysheva, Roger D. Pickard, Nikolaj V. Pit, Sakiko Ishibashi, Rod Stubbings, Rudolf Novak, Michael Richmond, Hiroyuki Maehara, Franky Dubois, Kenji Hirosawa, Hideo Nishimura, Patrick Schmeer, Masaru Mukai, Tomohito Ohshima, Lewis M. Cook, Richard Sabo, Naoto Kojiguchi, Sergey Yu. Shugarov, Robert J. Modic, Kazuki Maeda, Javier Ruiz, Kirill A. Antonyuk, Tonny Vanmunster, Eddy Muyllaert, Daiki Fukushima, Franz-Josef Hambsch, Etienne Morelle, Natalia Katysheva, Berto Monard, Greg Bolt, Kiyoshi Kasai, Drahomir Chochol, Krzysztof Z. Stanek, Nick James, Jeremy Shears, Gianluca Masi, Maksim V. Andreev, Julia V. Babina, Raul Michel, Tamás Tordai, Yutaka Maeda, Minako Ogi, Jyunya Mikami, Christopher S. Kochanek, Masayuki Moriyama, Elena P. Pavlenko, Kenji Tanabe, William Stein, Igor Kudzej, Tim Crawford, Sergey Zharikov, Oksana I. Antonyuk, Benjamin J. Shappee, Keisuke Isogai, Hiroshi Itoh, Irina Voloshina, Denis Buczynski, Ian Miller, Stella Kafka, Colin Littlefield, Shawn Dvorak, Taichi Kato, A. A. Henden, Miho Kawabata, Seiji Ueda
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
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arXiv:1507.05610v1.-- et al.
Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 102 SU UMa-type dwarf novae, observed mainly during the 2014-2015 season, and characterized these obj
Continuing the project described by Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for 102 SU UMa-type dwarf novae, observed mainly during the 2014-2015 season, and characterized these obj
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95a9f8b3a390f729d41f4f05b9527d83
http://arxiv.org/abs/1507.05610
http://arxiv.org/abs/1507.05610
Autor:
Y. Kanda, Osamu Hashimoto, Yuki Moritani, Akihiko Fukui, Masayuki Yamanaka, Hisashi Miyamoto, Y. Ohashi, Katsutoshi Takaki, K. Yanagisawa, Takahiro Ui, Tatsuya Nakaoka, Akira Arai, Takuya Yamashita, Ken'ichi Nomoto, T. Ohsugi, Tatsuya Harao, Daisaku Nogami, Miho Kawabata, Hitoshi Sato, Michitoshi Yoshida, K. Kawaguchi, Nao Suzuki, Nobuyuki Kawai, Yasushi Fukazawa, K. Sakimoto, Shingo Chiyonobu, Issei Ueno, Kazunari Masumoto, Keiichi Maeda, Hidehiko Nakaya, Mahito Sasada, Makoto Uemura, Masaomi Tanaka, Ryosuke Itoh, Koji Mori, Hideyuki Izumiura, T. Urano, Hiroshi Akitaya, Osamu Nagae, Hiroyuki Tanaka, Koji S. Kawabata, T. Komatsu, Daisuke Kuroda, Satoshi Honda, Koji Takata, Katsura Matsumoto, Risako Matsui, Nana Ebisuda, Asami Nakashima
We presented optical and near-infrared multi-band linear polarimetry of the highly reddened Type Ia SN~2014J appeared in M82. SN~2014J exhibits large polarization at shorter wavelengths, e.g., $4.8$\% in $B$ band, and the polarization decreases rapid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8bb45c9be90409a2cd112f289591e960
http://arxiv.org/abs/1407.0452
http://arxiv.org/abs/1407.0452