activity
20162021
most citedASASSN-18aan: An Eclipsing SU UMa-type Cataclysmic Variable with a 3.6-hour Orbital Period and a Late G-type Secondary Star

11 citations · 31 across the 4 of their papers we have counts for

collaborators

12 papers

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.SR20217 cited

Search for magnetic accretion in SW Sextantis systems

I. J. Lima, C. V. Rodrigues, C. E. Ferreira Lopes +9

SW Sextantis systems are nova-like cataclysmic variables that have unusual spectroscopic properties, which are thought to be caused by an accretion geometry having part of the mass…

astro-ph.SR202111 cited

ASASSN-18aan: An Eclipsing SU UMa-type Cataclysmic Variable with a 3.6-hour Orbital Period and a Late G-type Secondary Star

Yasuyuki Wakamatsu, John R. Thorstensen, Naoto Kojiguchi +41

We report photometric and spectroscopic observations of the eclipsing SU UMa-type dwarf nova ASASSN-18aan. We observed the 2018 superoutburst with 2.3 mag brightening and found the…

astro-ph.HE20208 cited

X-ray Spectra and Light Curves of Cooling Novae and a Nova-Like

Bangzheng Sun, Marina Orio, Andrej Dobrotka +3

We present X-ray observations of novae V2491 Cyg and KT Eri about 9 years post-outburst, of the dwarf nova and post-nova candidate EY Cyg, and of a VY Scl variable. The first three…

astro-ph.HE20205 cited

Modeling of 35-day superorbital cycle of and light curves of IMXB HZ Her/Her X-1

D. A. Kolesnikov, N. I. Shakura, K. A. Postnov +13

The X-ray binary Her X-1 consists of an accreting neutron star and the optical component HZ Her. The 35-day X-ray superorbital variability of this system is known since its discove…

astro-ph.SR2020

Multi-wavelength photometry during the 2018 superoutburst of the WZ Sge-type dwarf nova EG Cancri

Mariko Kimura, Keisuke Isogai, Taichi Kato +45

We report on the multi-wavelength photometry of the 2018 superoutburst in EG Cnc. We have detected stage A superhumps and long-lasting late-stage superhumps via the optical photome…