activity
20122025
most citedThe structure and emission model of the relativistic jet in the quasar 3C 279 inferred from radio to high-energy gamma-ray observations in 2008-2010

194 citations · 1.2k across the 25 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.HE2021

Constraints on magnetic field and particle content in blazar jets through optical circular polarization

I. Liodakis, D. Blinov, S. B. Potter +1

Polarization offers a unique view in the physical processes of astrophysical jets. We report on optical circular polarization observations of two famous blazars, namely 3C 279 and…

astro-ph.CO2021★ 23 cited

SMILE: Search for MIlli-LEnses

C. Casadio, D. Blinov, A. C. S. Readhead +17

Dark Matter (DM) halos with masses below , which would help to discriminate between DM models, may be detected through their gravitational effect on distant…

astro-ph.HE2021★ 18 cited

Repeated pattern of gamma-ray flares in the lightcurve of the blazar 3C 279

D. Blinov, S. G. Jorstad, V. M. Larionov +10

The optical polarization plane of some blazars occasionally exhibits smooth hundred degree long rotations. Multiple theoretical models have been proposed to explain the nature of s…

astro-ph.HE2021★ 19 cited

The Time-Dependent Distribution of Optical Polarization Angle Changes in Blazars

S. Kiehlmann, D. Blinov, I. Liodakis +17

At optical wavelengths, blazar Electric Vector Position Angle (EVPA) rotations linked with gamma-ray activity have been the subject of intense interest and systematic investigation…

astro-ph.IM2021★ 9 cited

WALOP-South: A Four Camera One Shot Imaging Polarimeter for PASIPHAE Survey. Paper I -- Optical Design

Siddharth Maharana, John A. Kypriotakis, A. N. Ramaprakash +17

The WALOP-South instrument will be mounted on the 1 m SAAO telescope in South Africa as part of the PASIPHAE program to carry out a linear imaging polarization survey of the Galact…

astro-ph.HE2021★ 4 cited

Parameters of the type-IIP supernova SN 2012aw

A. A. Nikiforova, P. V. Baklanov, S. I. Blinnikov +7

We present the results the photometric observations of the Type IIP supernova SN 2012aw obtained for the time interval from 7 till 371 days after the explosion. Using the previousl…