Polarimetric Properties of Blazars Caught by the WEBT
Claudia M. Raiteri, Massimo Villata

TL;DR
This paper reviews the polarimetric properties of blazars observed by the WEBT, highlighting their variability and the insights gained into blazar emission mechanisms through extensive multi-wavelength and polarimetric monitoring.
Contribution
It provides a comprehensive review of WEBT's polarimetric observations of blazars, emphasizing the role of polarization variability in understanding blazar physics.
Findings
Strong variability in polarization degree and angle observed.
Evidence supporting a geometrical interpretation of blazar variability.
Enhanced understanding of blazar emission mechanisms through polarimetric data.
Abstract
Active galactic nuclei come in many varieties. A minority of them are radio-loud, and exhibit two opposite prominent plasma jets extending from the proximity of the supermassive black hole up to megaparsec distances. When one of the relativistic jets is oriented closely to the line of sight, its emission is Doppler beamed and these objects show extreme variability properties at all wavelengths. These are called "blazars". The unpredictable blazar variability, occurring on a continuous range of time-scales, from minutes to years, is most effectively investigated in a multi-wavelength context. Ground-based and space observations together contribute to give us a comprehensive picture of the blazar emission properties from the radio to the gamma-ray band. Moreover, in recent years, a lot of effort has been devoted to the observation and analysis of the blazar polarimetric radio and optical…
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