activity
20172024
most citedFirst Detection of Two Superoutbursts during Rebrightening Phase of a WZ Sge-type Dwarf Nova: TCP J21040470+4631129

16 citations · 31 across the 7 of their papers we have counts for

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8 papers · 1 filter

astro-ph.SR20222 cited

Analysis of the IW And star ASAS J071404+7004.3

Taichi Kato, Kiyoshi Kasai, Elena P. Pavlenko +14

We made a time-resolved photometric campaign of the bright cataclysmic variable ASAS J071404+7004.3 in 2020. Inight et al. (2022, arXiv/2109.14514) recently published time-resolved…

astro-ph.SR2021

Spectroscopic and Photometric Observations of Dwarf Nova Superoutbursts by the 3.8 m Telescope Seimei and the Variable Star Network

Yusuke Tampo, Keisuke Isogai, Naoto Kojiguchi +59

We present spectroscopic and photometric observations of 17 dwarf-nova superoutbursts obtained by KOOLS-IFU mounted on the 3.8 m telescope Seimei at Okayama Observatory of Kyoto Un…

astro-ph.SR202016 cited

First Detection of Two Superoutbursts during Rebrightening Phase of a WZ Sge-type Dwarf Nova: TCP J21040470+4631129

Yusuke Tampo, Kojiguchi Naoto, Keisuke Isogai +51

We report photometric and spectroscopic observations and analysis of the 2019 superoutburst of TCP J21040470+4631129. This object showed a 9-mag superoutburst with early superhumps…

astro-ph.SR20191 cited

Cool spots on the surface of the active giant PZ Mon

Yu. V. Pakhomov, V. I. Shenavrin, N. I. Bondar' +4

Based on the multiband (BVRIJHKL) photometric observations of the active red giant PZ Mon performed for the first time in the winter season of 2017-2018, we have determined the mai…

astro-ph.SR201911 cited

Discovery of Standstills in the SU UMa-Type Dwarf Nova NY Serpentis

Taichi Kato, Elena P. Pavlenko, Nikolaj V. Pit +40

We found that the SU UMa-type dwarf nova NY Ser in the period gap [orbital period 0.097558(6) d] showed standstills twice in 2018. This is the first clear demonstration of a stands…

astro-ph.SR2018

Asynchronous polar V1500 Cyg: orbital, spin and beat periods

E. P. Pavlenko, P. A. Mason, A. A. Sosnovskij +7

The bright Nova Cygni 1975 is a rare nova on a magnetic white dwarf (WD). Later it was found to be an asynchronous polar, now called V1500 Cyg. Our multisite photometric campaign o…