RoboPol: first season rotations of optical polarization plane in blazars
- Univ. of Crete, Heraklion (Greece). Inst. for Plasma Physics, Dept. of Physics; St. Petersburg State Univ., St. Petersburg (Russia). Astronomical Inst.
- Univ. of Crete, Heraklion (Greece). Inst. for Plasma Physics, Dept. of Physics; Foundation for Research and Technology (Forth), Heraklion (Greece). Inst. of Electronic Structure and Laser (IESL)
- Max Planck Inst. for Radio Astronomy, Bonn (Germany)
- Univ. of Crete, Heraklion (Greece). Inst. for Plasma Physics, Dept. of Physics
- California Inst. of Technology (CalTech), Pasadena, CA (United States). Cahill Center for Astronomy and Astrophysics
- Max Planck Inst. for Radio Astronomy, Bonn (Germany)
- Inter-Univ. Centre for Astronomy and Astrophysics, Ganeshkhind (India)
- Nicolaus Copernicus Univ., Torun (Poland). Centre for Astronomy
- Aalto Univ., Metsahovi, (Finland). Metsahovi Radio Observatory
- Foundation for Research and Technology (Forth), Heraklion (Greece). Inst. of Electronic Structure and Laser (IESL); Univ. of Crete, Heraklion (Greece). Inst. for Plasma Physics, Dept. of Physics
Here, we present first results on polarization swings in optical emission of blazars obtained by RoboPol, a monitoring programme of an unbiased sample of gamma-ray bright blazars specially designed for effective detection of such events. A possible connection of polarization swing events with periods of high activity in gamma-rays is investigated using the data set obtained during the first season of operation. It was found that the brightest gamma-ray flares tend to be located closer in time to rotation events, which may be an indication of two separate mechanisms responsible for the rotations. Blazars with detected rotations during non-rotating periods have significantly larger amplitude and faster variations of polarization angle than blazars without rotations. Our simulations show that the full set of observed rotations is not a likely outcome (probability ≤1.5 × 10-2) of a random walk of the polarization vector simulated by a multicell model. Furthermore, it is highly unlikely (~5 × 10-5) that none of our rotations is physically connected with an increase in gamma-ray activity.
- Research Organization:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE; National Aeronautics and Space Administration (NASA); European Commission (EC); National Science Foundation (NSF); Polish National Science Centre (NCN)
- Grant/Contract Number:
- AC02-76SF00515; NNX11A043G; AST-1109911; NNX14AQ07H; 2011/01/B/ST9/04618; PCIG-GA-2011-293531
- OSTI ID:
- 1354926
- Journal Information:
- Monthly Notices of the Royal Astronomical Society, Vol. 453, Issue 2; ISSN 0035-8711
- Publisher:
- Royal Astronomical SocietyCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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