activity
20142023
most citedRepetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni

86 citations · 144 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20236 cited

2021 superoutburst of WZ Sge-type dwarf nova V627 Pegasi lacks an early superhump phase

Yusuke Tampo, Taichi Kato, Naoto Kojiguchi +27

Superoutbursts in WZ Sge-type dwarf novae (DNe) are characterized by both early superhumps and ordinary superhumps originating from the 2:1 and 3:1 resonances, respectively. Howeve…

astro-ph.HE201686 cited

Repetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni

Mariko Kimura, Keisuke Isogai, Taichi Kato +65

How black holes accrete surrounding matter is a fundamental, yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion…

astro-ph.SR201416 cited

OT J075418.7+381225 and OT J230425.8+062546: Promising Candidates for the Period Bouncer

Chikako Nakata, Taichi Kato, Daisaku Nogami +15

We report on photometric observations of two dwarf novae, OT J075418.7+381225 and OT J230425.8+062546, which underwent superoutburst in 2013 (OT J075418) and in 2011 (OT J230425).…

astro-ph.SR201419 cited

NY Serpentis: SU UMa-Type Nova in the Period Gap with Diversity of Normal Outbursts

Elena P. Pavlenko, Taichi Kato, Oksana I. Antonyuk +16

We present photometric study of NY Ser, an in-the-gap SU UMa-type nova, in 2002 and 2013. We determined the duration of the superoutburst and the mean superhump period to be 18 d a…

astro-ph.SR201417 cited

Superoutburst of SDSS J090221.35+381941.9: First Measurement of Mass Ratio in an AM CVn-Type Object using Growing Superhumps

Taichi Kato, Tomohito Ohshima, Denis Denisenko +36

We report on a superoutburst of the AM CVn-type object SDSS J090221.35+381941.9 [J0902; orbital period 0.03355(6) d] in 2014 March-April. The entire outburst consisted of a precurs…