activity
20102016
most citedTime-correlation between the radio and gamma-ray activity in blazars and the production site of the gamma-ray emission

161 citations · 410 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2016126 cited

RoboPol: The optical polarization of gamma-ray--loud and gamma-ray--quiet blazars

E. Angelakis, T. Hovatta, D. Blinov +25

We present average R-band optopolarimetric data, as well as variability parameters, from the first and second RoboPol observing season. We investigate whether gamma- ray--loud and…

astro-ph.HE201662 cited

RoboPol: Do optical polarization rotations occur in all blazars?

D. Blinov, V. Pavlidou, I. Papadakis +23

We present a new set of optical polarization plane rotations in blazars, observed during the third year of operation of RoboPol. The entire set of rotation events discovered during…

astro-ph.GA201533 cited

C-Band All-Sky Survey: A First Look at the Galaxy

M. O. Irfan, C. Dickinson, R. D. Davies +18

We present an analysis of the diffuse emission at 5 GHz in the first quadrant of the Galactic plane using two months of preliminary intensity data taken with the C-Band All Sky Sur…

astro-ph.HE2014

The connection between the 15 GHz radio and gamma-ray emission in blazars

W. Max-Moerbeck, J. L. Richards, T. Hovatta +5

Since mid-2007 we have carried out a dedicated long-term monitoring programme at 15 GHz using the Owens Valley Radio Observatory 40 meter telescope. One of the main goals of this p…

astro-ph.IM20143 cited

Astronomical Receiver Modelling Using Scattering Matrices

O. G. King, Michael E. Jones, C. Copley +6

Proper modelling of astronomical receivers is vital: it describes the systematic errors in the raw data, guides the receiver design process, and assists data calibration. In this p…

astro-ph.HE201421 cited

Early-time polarized optical light curve of GRB 131030A

O. G. King, D. Blinov, D. Giannios +23

We report the polarized optical light curve of a gamma-ray burst afterglow obtained using the RoboPol instrument. Observations began 655 seconds after the initial burst of gamma-ra…