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most citedSuperflares on Solar Type Stars Observed with Kepler I. Statistical Properties of Superflares

492 citations · 4.2k across the 103 of their papers we have counts for

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Showing 2009Show all

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astro-ph.SR2009

A Prediction of Supersoft X-Ray Phase of Classical Nova V5583 Sagittarii

Izumi Hachisu, Mariko Kato, Seiichiro Kiyota +1

We have observed the fast nova V5583 Sagittarii with five B, V, y, R_C, and I_C bands, and found that these multi-band light curves are almost identical with those of V382 Vel 1999…

astro-ph.SR2009★ 4 cited

Dwarf Novae in the Shortest Orbital Period Regime: I. A New Short Period Dwarf Nova, OT J055717+683226

Makoto Uemura, Akira Arai, Taichi Kato +20

We report the observation of a new dwarf nova, OT J055717+683226, during its first-ever recorded superoutburst in December 2006. Our observation shows that this object is an SU UMa…

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…

astro-ph.SR2009★ 8 cited

Photometry of Three Superoutbursts of the SU UMa-type Dwarf Nova, SW Ursae Majoris

Yuichi Soejima, Daisaku Nogami, Taichi Kato +16

We investigated the superhump evolution, analysing optical photometric observations of the 2000 February-March, the 2002 October-November, and the 2006 September superoutbursts of…

astro-ph.SR2009★ 1 cited

Rebrightening Phenomenon in Classical Novae

Taichi Kato, Kazuhiro Nakajima, Hiroyuki Maehara +1

Two classical novae V1493 Aql and V2362 Cyg were known to exhibit unprecedented large-amplitude rebrightening during the late stage of their evolution. We analyzed common propertie…

astro-ph.SR2009★ 25 cited

SDSS J080434.20+510349.2: Eclipsing WZ Sge-Type Dwarf Nova with Multiple Rebrightenings

Taichi Kato, Elena P. Pavlenko, Hiroyuki Maehara +8

We observed the 2006 superoutburst of SDSS J080434.20+510349.2 during its plateau phase, rebrightening phase, and post-superoutburst final decline. We found that this object is a g…