activity
20152022
most citedMultiwavelength behaviour of the blazar 3C279: decade-long study from -ray to radio

51 citations · 199 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA20227 cited

Radio Variability and Broad-Band Spectra of Infrared Galaxies with and without OH Megamaser Emission

Yu. V. Sotnikova, T. V. Mufakharov, A. G. Mikhailov +7

We study the radio variability of galaxies with and without sources of hydroxyl (OH) megamaser radiation based on the continuum radio measurements conducted in 2019-2022 with the r…

astro-ph.GA20228 cited

Radio properties of the OH megamaser galaxy IIZw 096

Hong Wu, Zhongzu Wu, Yu. Sotnikova +9

Based on the two epochs EVN archive data from OH line observations of IIZw 096, we confirm that the high-resolution OH emission in this source mainly comes from two spots (OH1 and…

astro-ph.GA202131 cited

High-redshift quasars at -- I. Radio spectra

Yu. Sotnikova, A. Mikhailov, T. Mufakharov +7

We present the radio properties of optically selected quasars with . The complete sample consists of 102 quasars with a flux density level mJy in a declina…

astro-ph.HE20211 cited

The Baikal-GVD neutrino telescope: search for high-energy cascades

V. A. Allakhverdyan, A. D. Avrorin, A. V. Avrorin +63

Baikal-GVD is a neutrino telescope currently under construction in Lake Baikal. GVD is formed by multi-meganton subarrays (clusters). The design of Baikal-GVD allows one to search…

astro-ph.HE202011 cited

Flux-density measurements of the high-redshift blazar PSO J047.4478+27.2992 at 4.7 and 8.2 GHz with RATAN-600

T. Mufakharov, A. Mikhailov, Yu. Sotnikova +5

We report the first detection at 4.7 and 8.2 GHz with the RATAN-600 radio telescope of the source PSO J047.4478+27.2992, which has been announced as a blazar at z=6.1. The average…

astro-ph.HE20203 cited

Multi-wavelength observations of the BL Lac object Fermi J1544-0649: one year after its awakening

P. H. T. Tam, P. S. Pal, Y. D. Cui +15

We report observations of a transient source \fermi\ from radio to \grs. \fermi\ was discovered by the {\it Fermi-LAT} in May 2017. Follow-up {\it Swift-XRT} observations revealed…