activity
20152026
most citedProbable detection of an eruptive filament from a superflare on a solar-type star

144 citations · 1.1k across the 67 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.SR2019★ 10 cited

IW And-Type State in IM Eridani

Taichi Kato, Yasuyuki Wakamatsu, Naoto Kojiguchi +20

IW And stars are a recently recognized group of dwarf novae which are characterized by a repeated sequence of brightening from a standstill-like phase with damping oscillations fol…

astro-ph.HE2019★ 21 cited

SN 2018hna: 1987A-like supernova with a signature of shock breakout

Avinash Singh, D. K. Sahu, G. C. Anupama +22

High cadence ultraviolet, optical and near-infrared photometric and low-resolution spectroscopic observations of the peculiar Type II supernova (SN) 2018hna are presented. The earl…

astro-ph.HE2019★ 28 cited

Type Ia SN 2019ein: New Insights into the Similarities and diversities among High-Velocity SNe Ia

Miho Kawabata, Keiichi Maeda, Masayuki Yamanaka +38

We present optical observations of type Ia supernova (SN) 2019ein, starting at 2 days after the estimated explosion date. The spectra and the light curves show that SN 2019ein belo…

astro-ph.SR2019★ 3 cited

ASASSN-18fk: A new WZ Sge-type dwarf nova with multiple rebrightenings and a new candidate for a superhumping intermediate polar

E. Pavlenko, K. Niijima, P. Mason +23

We present the result of a multi-longitude campaign on the photometric study of the dwarf nova ASASSN-18fk during its superoutburst in 2018. It was observed with 18 telescopes at 1…

astro-ph.SR2019★ 11 cited

NSV 1440: First WZ Sge-type Object in AM CVn stars and candidates

Keisuke Isogai, Taichi Kato, Berto Monard +5

In 2015 and 2017, the AM CVn candidate NSV 1440 showed superoutbursts having the characteristic features of WZ Sge-type dwarf novae (DNe). By analogy with hydrogen-rich cataclysmic…

astro-ph.SR2019★ 11 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…