activity
20082021
most citedVW LMi: tightest quadruple system known. Light-time effect and possible secular changes of orbits

32 citations · 78 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR202114 cited

Automatic classification of eclipsing binary stars using deep learning methods

Michal Čokina, Viera Maslej-Krešňáková, Peter Butka +1

In the last couple of decades, tremendous progress has been achieved in developing robotic telescopes and, as a result, sky surveys (both terrestrial and space) have become the sou…

astro-ph.HE2021

Optical Variability Correlated with X-ray Spectral Transition in the Black-Hole Transient ASASSN-18ey = MAXI J1820+070

Keito Niijima, Mariko Kimura, Yasuyuki Wakamatsu +49

How a black hole accretes matter and how this process is regulated are fundamental but unsolved questions in astrophysics. In transient black-hole binaries, a lot of mass stored in…

astro-ph.IM202119 cited

ELISa: A new tool for fast modelling of eclipsing binaries

Michal Čokina, Miroslav Fedurco, Štefan Parimucha

We present a new, fast, and easy to use tool for modelling light and radial velocity curves of close eclipsing binaries with built-in methods for solving an inverse problem. The ma…

astro-ph.SR201913 cited

Pulsational properties of ten new slowly pulsating B stars

M. Fedurco, E. Paunzen, S. Hümmerich +2

We collected a sample of ten hitherto unidentified SPB stars with the aim of describing their pulsational properties and identifying pulsational modes. Photometric time series data…

astro-ph200832 cited

VW LMi: tightest quadruple system known. Light-time effect and possible secular changes of orbits

T. Pribulla, D. Baludansky, P. Dubovsky +4

Tightest known quadruple systems VW LMi consists of contact eclipsing binary with P_12 = 0.477551 days and detached binary with P_34 = 7.93063 days revolving in rather tight, 355.0…