activity
20182026
most citedThe intraday variations of polarization vector direction in radio source S5 0716+714

17 citations · 76 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.EP2026★ 5 cited

A comprehensive study of comet 67P/Churyumov-Gerasimenko in the 2021/2022 apparition. II. Colorimetry, polarimetry, modeling

Vera Rosenbush, Oleksandra Ivanova, Johannes Markkanen +5

This paper presents the second part of our multi-technique observational study of comet 67P during its 2021-2022 apparition. While the first paper focused on photometry and spectro…

astro-ph.GA2026

Here Be SDRAGNs - Spiral Galaxies Hosting Large Double Radio Sources

Jean Tate, William C. Keel, Michael O'Keeffe +16

We present a sample of large double radio sources hosted by spiral galaxies (Spiral Double Radio Active Galactic Nuclei, SDRAGNs). Candidates were selected during Radio Galaxy Zoo,…

astro-ph.EP2025★ 5 cited

A comprehensive study of comet 67P/Churyumov-Gerasimenko in the 2021/2022 apparition. I. Photometry, spectroscopy, morphology

V. Rosenbush, V. Kleshchonok, O. Ivanova +6

We present observations of comet 67P/Churyumov-Gerasimenko during its 2021/22 apparition, aiming to investigate its dust and gas environment and compare the results with those obta…

astro-ph.HE2024

A Two-Week Monitoring Campaign on Mrk 421

W. Peter Maksym, Ioannis Liodakis, M. Lynne Saade +153

X-ray polarization is a unique new probe of the particle acceleration in astrophysical jets made possible through the Imaging X-ray Polarimetry Explorer. Here we report on the firs…

astro-ph.HE2024★ 5 cited

Testing particle acceleration in blazar jets with continuous high-cadence optical polarization observations

Ioannis Liodakis, Sebastian Kiehlmann, Alan P. Marscher +44

Variability can be the pathway to understanding the physical processes in astrophysical jets, however, the high-cadence observations required to test particle acceleration models a…

astro-ph.HE2023

Optical circular polarization of blazar S4 0954+65 during high linear polarized states

I. Liodakis, E. Shablovinskaya, D. Blinov +17

Optical circular polarization observations can directly test the particle composition in black holes jets. Here we report on the first observations of the BL Lac type object S4 095…

astro-ph.EP2023★ 10 cited

Long-lasting activity of asteroid (248370) 2005 QN 173

Oleksandra Ivanova, Javier Licandro, Fernando Moreno +8

We present the results of observations of asteroid (248370) QN obtained during July 2021 - January 2022 with three telescopes. Our analysis revealed the presence of the dus…

astro-ph.GA2023

Intraday variations of polarization vector in blazars: a key to the optical jet structure?

Elena Shablovinskaya, Eugene Malygin, Dmitry Oparin

This report presents the results of optical polarimetric observations carried out with 6-m and 1-m telescopes at SAO RAS. The study of the blazar S5 0716+714 radiation showed the p…

astro-ph.HE2023★ 2 cited

Probing AGN with spectropolarimetry: accretion disk and SMBH parameters

M. Yu. Piotrovich, E. S. Shablovinskaya, E. A. Malygin +2

The interaction of a supermassive black hole with the matter of an accretion disk in the presence of a magnetic field is the key mechanism of energy release in active galactic nucl…

astro-ph.IM2023★ 12 cited

Astronomical Camera Based on a CCD261-84 Detector with Increased Sensitivity in the Near-Infrared

Irina Afanasieva, Valery Murzin, Valery Ardilanov +5

Herein, we describe the design, implementation and operation principles of an astronomical camera system, based on a large-format CCD261-84 detector with an extremely thick 200 mkm…

astro-ph.GA2023★ 3 cited

Polarimetric Reverberation Mapping in Medium-Band Filters

Elena Shablovinskaya, Luka Č. Popović, Roman Uklein +8

Earlier, we suggested the "reload" concept of the polarimetric reverberation mapping of active galactic nuclei (AGN), proposed for the first time more than 10 years ago. We have su…

astro-ph.HE2023★ 6 cited

Chromatic optical polarization of BL Lac: while faint and bright

Elena Shablovinskaya, Eugene Malygin, Dmitry Oparin

Due to the first results on astrophysical X-ray polarization provided by \textit{IXPE} observatory, the interest in wavelength-dependent synchrotron polarization of BL Lac type obj…

astro-ph.HE2022★ 2 cited

Determination of the Physical Parameters of AGNs in Seyfert 1 Galaxies LEDA 3095839 and VII Zw 244 Based on Spectropolarimetric Observations

Elena Shablovinskaya, Mikhail Piotrovich, Eugene Malygin +2

Here we present the detailed investigation of AGNs in two Seyfert 1 galaxies, LEDA 3095839 and VII Zw 244. Both of them were observed within the photometric reverberation mapping p…

astro-ph.GA2020★ 2 cited

Intraday variability of the polarization vector in AGN S5 0716+714

E. Shablovinskaya, V. Afanasiev

The bright radio source S5 0716+714, which is usually classified as a BL Lac object, is one of the most intensively studied blazar. S5 0716+714 demonstrates extremely peculiar prop…

astro-ph.IM2019★ 1 cited

Medium-band photometric reverberation mapping of AGNs at . Techniques and sample

Eugene Malygin, Roman Uklein, Elena Shablovinskaya +2

The most popular method of the broad-line region size estimation in active galactic nuclei (AGN) is the reverberation mapping based on measuring the time delay between the continuu…

astro-ph.GA2019★ 6 cited

Photometric reverberation mapping of AGNs at 0.1 < z < 0.8: I. Observational technique

Roman Uklein, Eugene Malygin, Elena Shablovinskaya +2

The improvement of the calibration relation for determining the size of the broad-line region from the observed optical luminosity of active galactic nuclei (AGN) is a necessary ta…

astro-ph.GA2018★ 17 cited

The intraday variations of polarization vector direction in radio source S5 0716+714

E. S. Shablovinskaya, V. L. Afanasiev

The bright radio source S5 0716+714, that is usually classified as BL Lac object, is one of the most intensively studied. S5 0716+714 demonstrates extremely peculiar properties suc…