activity
20112017
most citedSpectroscopic evidence for a low-mass black hole in SWIFT J1753.5-0127

55 citations · 148 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2017★ 7 cited

ASASSN-16eg: New candidate of long-period WZ Sge-type dwarf nova

Yasuyuki Wakamatsu, Keisuke Isogai, Mariko Kimura +19

We report on our photometric observations of the 2016 superoutburst of ASASSN-16eg. This object showed a WZ Sge-type superoutburst with prominent early superhumps with a period of…

astro-ph.SR2017★ 23 cited

The remarkable outburst of the highly evolved post-period-minimum dwarf nova SSS J122221.7-311525

V. V. Neustroev, T. R. Marsh, S. V. Zharikov +22

We report extensive 3-yr multiwavelength observations of the WZ Sge-type dwarf nova SSS J122221.7-311525 during its unusual double superoutburst, the following decline and in quies…

astro-ph.HE2016

Correlated X-ray and optical variability in intermediate polars during their outbursts

V. V. Neustroev, S. Tsygankov, V. Suleimanov +1

We present a study of the evolution of the optical and X-ray fluxes during outbursts of two short-period cataclysmic variables, the confirmed intermediate polar CC Scl and the inte…

astro-ph.SR2016★ 11 cited

Superoutburst of WZ Sge-type Dwarf Nova Below the Period Minimum: ASASSN-15po

Kosuke Namekata, Keisuke Isogai, Taichi Kato +38

We report on a superoutburst of a WZ Sge-type dwarf nova (DN), ASASSN-15po. The light curve showed the main superoutburst and multiple rebrightenings. In this outburst, we observed…

astro-ph.SR2016★ 10 cited

RZ Leonis Minoris Bridging between ER Ursae Majoris-Type Dwarf Nova and Novalike System

Taichi Kato, Ryoko Ishioka, Keisuke Isogai +64

We observed RZ LMi, which is renowned for the extremely (~19d) short supercycle and is a member of a small, unusual class of cataclysmic variables called ER UMa-type dwarf novae, i…

astro-ph.HE2014★ 55 cited

Spectroscopic evidence for a low-mass black hole in SWIFT J1753.5-0127

Vitaly Neustroev, Alexandra Veledina, Juri Poutanen +4

The black hole (BH) candidate SWIFT J1753.5-0127 has remained active since the onset of its 2005 outburst. Emission lines in the optical spectrum were observed at the very beginnin…

astro-ph.SR2013★ 8 cited

Steps towards a solution of the FS Aurigae puzzle. II. Confirmation of the intermediate polar status

V. V. Neustroev, G. H. Tovmassian, S. V. Zharikov +1

FS Aur is famous for a variety of uncommon and puzzling periodic photometric and spectroscopic variabilities. It was previously proposed that the precession of a fast-rotating magn…

astro-ph.SR2011★ 34 cited

Eclipses During the 2010 Eruption of the Recurrent Nova U Scorpii

Bradley E. Schaefer, Ashley Pagnotta, Aaron LaCluyze +34

The eruption of the recurrent nova U Scorpii on 28 January 2010 is now the all-time best observed nova event. We report 36,776 magnitudes throughout its 67 day eruption, for an ave…