English

RoboPol: optical polarization-plane rotations and flaring activity in blazars

High Energy Astrophysical Phenomena 2016-02-17 v2

Abstract

We present measurements of rotations of the optical polarization of blazars during the second year of operation of RoboPol, a monitoring programme of an unbiased sample of gamma-ray bright blazars specially designed for effective detection of such events, and we analyse the large set of rotation events discovered in two years of observation. We investigate patterns of variability in the polarization parameters and total flux density during the rotation events and compare them to the behaviour in a non-rotating state. We have searched for possible correlations between average parameters of the polarization-plane rotations and average parameters of polarization, with the following results: (1) there is no statistical association of the rotations with contemporaneous optical flares; (2) the average fractional polarization during the rotations tends to be lower than that in a non-rotating state; (3) the average fractional polarization during rotations is correlated with the rotation rate of the polarization plane in the jet rest frame; (4) it is likely that distributions of amplitudes and durations of the rotations have physical upper bounds, so arbitrarily long rotations are not realised in nature.

Keywords

Cite

@article{arxiv.1601.03392,
  title  = {RoboPol: optical polarization-plane rotations and flaring activity in blazars},
  author = {D. Blinov and V. Pavlidou and I. E. Papadakis and T. Hovatta and T. J. Pearson and I. Liodakis and G. V. Panopoulou and E. Angelakis and M. Baloković and H. Das and P. Khodade and S. Kiehlmann and O. G. King and A. Kus and N. Kylafis and A. Mahabal and A. Marecki and D. Modi and I. Myserlis and E. Paleologou and I. Papamastorakis and B. Pazderska and E. Pazderski and C. Rajarshi and A. Ramaprakash and A. C. S. Readhead and P. Reig and K. Tassis and J. A. Zensus},
  journal= {arXiv preprint arXiv:1601.03392},
  year   = {2016}
}

Comments

12 pages, 12 figures, accepted to MNRAS

R2 v1 2026-06-22T12:28:59.886Z