activity
20182021
most citedNew changing look case in NGC 1566

89 citations · 171 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2021

Multi-Wavelength Monitoring and Reverberation Mapping of a Changing Look Event in the Seyfert Galaxy NGC 3516

V. L. Oknyansky, M. S. Brotherton, S. S. Tsygankov +26

We present the results of photometric and spectroscopic monitoring campaigns of the changing look AGN NGC 3516 carried out in 2018 to 2020 covering the wavelength range from the X-…

astro-ph.GA202027 cited

The post-maximum behaviour of the changing-look Seyfert galaxy NGC 1566

V. L. Oknyansky, H. Winkler, S. S. Tsygankov +6

We present results of the long-term multi-wavelength study of optical, UV and X-ray variability of the nearby changing-look (CL) Seyfert NGC 1566 observed with the Swift Observator…

astro-ph.GA202031 cited

A flare in the optical spotted in the changing-look Seyfert NGC 3516

D. Ilic, V. Oknyansky, L. C. Popovic +14

We present observations from the short-term intensive optical campaign (from Sep2019 to Jan2020) of the changing-look Seyfert NGC 3516. This active galactic nucleus is known to hav…

astro-ph.GA2020

Variability and the size-luminosity relation of the intermediate mass AGN in NGC 4395

Hojin Cho, Jong-Hak Woo, Edmund Hodges-Kluck +31

We present the variability study of the lowest-luminosity Seyfert 1 galaxy NGC 4395 based on the photometric monitoring campaigns in 2017 and 2018. Using 22 ground-based and space…

astro-ph.GA20198 cited

The Relative Wavelength Independence of IR Time Lags in NGC4151 During the Years 2010-2015

V. L. Oknyansky, V. I. Shenavrin, N. V. Metlova +1

We present results of a study of the correlation between the infrared (JHKL) and optical(B) fluxes of the nucleus of the Seyfert galaxy NGC 4151 for the years 2010 - 2015 using our…

astro-ph.SR201916 cited

Supernova 2018aoq and a distance to Seyfert galaxy NGC 4151

D. Yu. Tsvetkov, P. V. Baklanov, M. Sh. Potashov +9

We present optical photometric observations of SN 2018aoq from 2 to 100 days after explosion, and 7 spectra at epochs from 11 to 71 days. The light curves and spectra are typical f…