output
20082023
most citedSurvey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

194 citations

16 papers

astro-ph.SR2023★ 1 cited

The 2022 active state of the AM CVn star NSV 1440

Taichi Kato, Rod Stubbings

We found an active state lasting for ~200 d in the AM CVn star NSV 1440 in 2022. During this state, the object reached a magnitude of 16.5, 2.0-2.5 mag above quiescence, and showed…

astro-ph.SR2019★ 16 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. X: The Tenth Year (2017)

Taichi Kato, Keisuke Isogai, Yasuyuki Wakamatsu +67

Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv/0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly duri…

astro-ph.SR2019★ 2 cited

CS Indi: SU UMa-Type Dwarf Nova with Long Precursor Outburst

Taichi Kato, Franz-Josef Hambsch, Berto Monard +3

We observed the 2018 November outburst of CS Ind and confirmed that it was a genuine superoutburst with a very long [0.12471(1) d in average] superhump period. The superoutburst wa…

astro-ph.SR2017★ 34 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IX: The Ninth Year (2016-2017)

Taichi Kato, Keisuke Isogai, Franz-Josef Hambsch +76

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016--201…

astro-ph.SR2017

Observation of a Deep Visual "Eclipse" in the WC9-Type Wolf-Rayet Star, WR 76

Rod Stubbings, Peredur Williams

The WC9-Type Wolf-Rayet star WR 76 is one of the most prolific dust makers identified from its infrared emission. WR 76 experienced a deep fading eclipse in 2016. The ~3.1 magnitud…

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…