4.7 Article

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

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 457, Issue 2, Pages 2252-2262

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw158

Keywords

polarization; galaxies: active; galaxies: jets; galaxies: nuclei

Funding

  1. 'RoboPol' project under the 'Aristeia' Action of the 'Operational Programme Education and Lifelong Learning'
  2. European Social Fund (ESF) and Greek National Resources
  3. European Comission Seventh Framework Programme (FP7) [PCIG10-GA-2011-304001, PIRSES-GA-2012-31578]
  4. NASA [NNX11A043G, AST-1109911]
  5. Polish National Science Centre [2011/01/B/ST9/04618]
  6. St. Petersburg University research grant [6.38.335.2015]
  7. European Commission Seventh Framework Programme (FP7) through the Marie Curie Career Integration [PCIG-GA-2011-293531]
  8. NASA Headquarters under the NASA Earth and Space Science Fellowship Program [NNX14AQ07]
  9. Academy of Finland project [267324]
  10. International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne
  11. Academy of Finland (AKA) [267324] Funding Source: Academy of Finland (AKA)

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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 realized in nature.

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