64 citations · 579 across the 38 of their papers we have counts for
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astro-ph.GA2018★ 3 cited
Multicomponent Power Density Spectra of Kepler AGNs, an instrumental artifact or a physical origin?
A. Dobrotka, P. Bezak, M. Revalski +1
We analysed the light curves of four active galactic nuclei (AGN) from the Kepler field, and find multicomponent power density spectra with characteristic frequencies that are surp…
astro-ph.SR2018★ 33 cited
Multiwavelength observations of V407 Lupi (ASASSN-16kt) --- a very fast nova erupting in an intermediate polar
E. Aydi, M. Orio, A. P. Beardmore +19
We present a detailed study of the 2016 eruption of nova V407 Lupi (ASASSN-16kt), including optical, near-infrared, X-ray, and ultraviolet data from SALT, SMARTS, SOAR, Chandra, Sw…
astro-ph.HE2018★ 17 cited
What we learn from the X-ray grating spectra of Nova SMC 2016
M. Orio, J. -U. Ness, A. Dobrotka +17
Nova SMC 2016 has been the most luminous nova known in the direction of the Magellanic Clouds. It turned into a very luminous supersoft X-ray source between day 16 and 28 after the…