Taichi Kato   Franz-Josef Hambsch   Hiroyuki Maehara   Gianluca Masi   Francesca Nocentini   Pavol A. Dubovsky   Igor Kudzej   Kazuyoshi Imamura   Minako Ogi   Kenji Tanabe   Hidehiko Akazawa   Thomas Krajci   Ian Miller   Enrique De Miguel   Arne Henden   Ryo Noguchi   Takehiro Ishibashi   Rikako Ono   Miho Kawabata   Hiroshi Kobayashi   Daisuke Sakai   Hirochika Nishino   Hisami Furukawa   Kazunari Masumoto   Katsura Matsumoto   Colin Littlefield   Tomohito Ohshima   Chikako Nakata   Satoshi Honda   Kenzo Kinugasa   Osamu Hashimoto   William Stein   Roger D. Pickard   Seiichiro Kiyota   Elena P. Pavlenko   Oksana I. Antonyuk   Aleksei V. Baklanov   Kirill Antonyuk   Denis Samsonov   Nikolaj Pit   Aleksei Sosnovskij   Arto Oksanen   Caisey Harlingten   Jenni Tyyskä   Berto Monard   Sergey Yu. Shugarov   Drahomir Chochol   Kiyoshi Kasai   Yutaka Maeda   Kenji Hirosawa   Hiroshi Itoh   Richard Sabo   Joseph Ulowetz   Etienne Morelle   Raul Michel   Genaro Suarez   Nick James   Shawn Dvorak   Irina B. Voloshina   Michael Richmond   Bart Staels   David Boyd   Maksim V. Andreev   Nikolai Parakhin   Natalia Katysheva   Atsushi Miyashita   Kazuhiro Nakajima   Greg Bolt   Stefano Padovan   Peter Nelson   Donn R. Starkey   Denis Buczynski   Peter Starr   William N. Goff   Denis Denisenko   Christopher S. Kochanek   Benjamin Shappee   Krzysztof Z. Stanek   Jose L. Prieto   Koh-Ichi Itagaki   Shizuo Kaneko   Rod Stubbings   Eddy Muyllaert   Jeremy Shears   Patrick Schmeer   Gary Poyner   Miguel Rodriguez-Marco   
Publications of the Astronomical Society of Japan 66(2) 2014年4月 [査読有り]
Continuing the project described in Kato et al. (2009, PASJ, 61, S395), we collected times of superhump maxima for SU UMa-type dwarf novae mainly observed during the 2012-2013 season. We found three objects (V444 Peg, CSS J203937, and MASTER J2126...
Publications of the Astronomical Society of Japan 66(4) 2014年 [査読有り]
We carried out photometric observations of the SUUMa-type dwarf nova ERUMa during 2011 and 2012, which showed the existence of persistent negative superhumps even during the superoutburst. We performed a two-dimensional period analysis of its ligh...
UPb ages of detrital zircons and white mica KAr ages are obtained from two psammitic schists from the western and eastern units of the Sanbagawa Metamorphic Belt located in the SakumaTenryu area. The detrital zircons in the sample from the western...