activity
20092024
most citedSurvey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

194 citations · 711 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2024★ 7 cited

Diffraction modelling of a 2023 March 5 stellar occultation by subkilometer-sized asteroid (98943) 2001 CC21

Ko Arimatsu, Fumi Yoshida, Tsutomu Hayamizu +31

We present an analysis of a stellar occultation event caused by a near-Earth asteroid (98943) 2001 CC21, an upcoming flyby target in the Hayabusa2 extended mission, on March 5, 202…

astro-ph.EP2019★ 3 cited

Shape and Rotational Motion Models for Tumbling and Monolithic Asteroid 2012 :High Time Resolution Lightcurve with the Tomo-e Gozen Camera

Seitaro Urakawa, Ryou Ohsawa, Shigeyuki Sako +13

We present visible and near-infrared observations of a near-Earth object (NEO), 2012 . The NEO 2012 approached close to the Earth at a distance of ab…

astro-ph.SR2016★ 34 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VIII: The Eighth Year (2015-2016)

Taichi Kato, Franz-Josef Hambsch, Berto Monard +75

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 128 SU UMa-type dwarf novae observed mainly during the 2015-2016…

astro-ph.SR2015★ 51 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VII: The Seventh Year (2014-2015)

Taichi Kato, Franz-Josef Hambsch, Pavol A. Dubovsky +89

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly during the 2014-2015…

astro-ph.SR2014★ 50 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VI: The Sixth Year (2013-2014)

Taichi Kato, Pavol A. Dubovsky, Igor Kudzej +83

Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv:0905.1757), we collected times of superhump maxima for 56 SU UMa-type dwarf novae mainly observed durin…

astro-ph.SR2014★ 22 cited

Study of Negative and Positive Superhumps in ER Ursae Majoris

Tomohito Ohshima, Taichi Kato, Elena Pavlenko +45

We carried out the photometric observations of the SU UMa-type dwarf nova ER UMa during 2011 and 2012, which showed the existence of persistent negative superhumps even during the…

astro-ph.SR2013★ 54 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. V: The Fifth Year (2012-2013)

Taichi Kato, Franz-Josef Hambsch, Hiroyuki Maehara +84

Continuing the project described by Kato et al. (2009a, arXiv:0905.1757), we collected times of superhump maxima for SU UMa-type dwarf novae mainly observed during the 2012-2013 se…

astro-ph.SR2012★ 4 cited

Low-Resolution Spectroscopy of the Recurrent Nova T Pyxidis at its Early Stage of 2011 Outburst

Kazuyoshi Imamura, Kenji Tanabe

We present our observational results of the recurrent nova T Pyxidis at its early stage of 2011 outburst, using a low-resolution spectrograph () attached to a 28cm tel…

astro-ph.SR2012★ 79 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IV: The Fourth Year (2011-2012)

Taichi Kato, Franz-Josef Hambsch, Hiroyuki Maehara +85

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we studied 86 SU UMa-type dwarf novae. We confirmed the general trends such as the relation between period…

astro-ph.SR2012★ 29 cited

Discovery of Negative Superhumps during a Superoutburst of January 2011 in ER Ursae Majoris

Tomohito Ohshima, Taichi Kato, Elena P. Pavlenko +19

We report on a discovery of "negative" superhumps during the 2011 January superoutburst of ER UMa. During the superoutburst which started on 2011 January 16, we detected negative s…

astro-ph.SR2012★ 12 cited

Observational Report on the Classical Nova KT Eridani

Kazuyoshi Imamura, Kenji Tanabe

A report on the spectroscopic and multi-color photometric observations of high galactic latitude classical nova KT Eridani (Nova Eridani 2009) is presented. After 12.2 days from ma…

astro-ph.SR2012

Spectroscopy and Multi-color Photometry of U Scorpii at the Earliest Stage of 2010 Outburst

Kazuyoshi Imamura, Kenji Tanabe

We have performed our spectroscopic and multi-color photometric observations of the recurrent nova U Scorpii at the earliest stage of the 2010 outburst. 0.37 days after the discove…

astro-ph.SR2011★ 59 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. III: The Third Year (2010--2011)

Taichi Kato, Hiroyuki Maehara, Ian Miller +75

Continuing the project described by Kato et al. (2009, PASJ 61, S395, arXiv:0905.1757), we collected times of superhump maxima for 51 SU UMa-type dwarf novae mainly observed during…

astro-ph.SR2010★ 101 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. II: The Second Year (2009-2010)

Taichi Kato, Hiroyuki Maehara, Makoto Uemura +56

As an extension of the project in Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 61 SU UMa-type dwarf novae mainly observed during the 2009-2010 se…

astro-ph.SR2010★ 12 cited

Early Spectroscopy of the 2010 Outburst of U Scorpii

Masayuki Yamanaka, Makoto Uemura, Koji S. Kawabata +15

We present early spectroscopy of the recurrent nova U~Sco during the outburst in 2010. We successfully obtained time-series spectra at 0.37--0.44~d, where d…

astro-ph.SR2009★ 194 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

Taichi Kato, Akira Imada, Makoto Uemura +60

We systematically surveyed period variations of superhumps in SU UMa-type dwarf novae based on newly obtained data and past publications. In many systems, the evolution of superhum…