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

492 citations · 4.8k across the 143 of their papers we have counts for

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astro-ph2008★ 11 cited

Photometric Studies of a WZ Sge-Type Dwarf Nova Candidate, ASAS160048-4846.2

Yuichi Soejima, Akira Imada, Daisaku Nogami +2

We report on our time-resolved CCD photometry during the 2005 June superoutburst of a WZ Sge-type dwarf nova candidate, ASAS 160048-4846.2. The ordinary superhumps underwent a comp…

astro-ph2008

Spectroscopic Observations of WZ Sge-type Dwarf Novae, GW Lib and V455 And in Superoutburst

D. Nogami, K. Hiroi, Y. Suzuki +13

We carried out intensive spectroscopic observations of two WZ Sge-type dwarf novae, GW Lib, and V455 And during their superoutbursts in 2007, at 6 observatories. The observations c…

astro-ph2008★ 9 cited

The 2006 November outburst of EG Aquarii: the SU UMa nature revealed

Akira Imada, Rod Stubbings, Taichi Kato +32

We report time-resolved CCD photometry of the cataclysmic variable EG Aquarii during the 2006 November outburst During the outburst, superhumps were unambiguously detected with a m…

astro-ph2008★ 8 cited

Photometric Studies of New Southern SU UMa-type dwarf novae, FL Triangulum Australe and CTCV J0549-4921

Akira Imada, Taichi Kato, L. A. G. Monard +4

We report time-resolved optical CCD photometry on newly discovered SU UMa-type dwarf novae, FL TrA and CTCV J0549-4921. During the 2006 August outburst, we detected superhumps with…

astro-ph2007★ 1 cited

Discovery of The New WZ Sge Star, SDSS J080434.20+510349.2

E. Pavlenko, S. Yu. Shugarov, N. A. Katysheva +13

We present the results of photometric observations of SDSS J080434.20+510349.2 in its low state and during an outburst and spectroscopy during the outburst. We found such peculiari…

astro-ph2007★ 24 cited

Discovery of a WZ Sge-Type Dwarf Nova, SDSS J102146.44+234926.3: Unprecedented Infrared Activity during a Rebrightening Phase

M. Uemura, A. Arai, T. Krajci +26

Several SU UMa-type dwarf novae, in particular, WZ Sge-type stars tend to exhibit rebrightenings after superoutbursts. The rebrightening phenomenon is problematic for the disk inst…