English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Radio emission in blazars -- the aligned subset of Active Galactic Nuclei(AGN) -- is produced by synchrotron electrons moving relativistically in theirjet's magnetic field. Under the assumption of some degree of uniformity of thefield, the emission can be highly polarized -- linearly and circularly. In theradio regime, the observed variability is in most of the cases attributed toflaring events undergoing opacity evolution, i.e. transitions from opticallythick to thin emission (or vice versa). These transistions have a specificsignature in the polarization parameter space (angle and magnitude) which canbe traced with high cadence polarization monitoring and provide us with aunique probe of the microphysics of the emitting region. Here we present thefull Stokes analysis of radio emission from blazars observed in the frameworkof the F-GAMMA program and discuss the case study of PKS\,1510$-$089 which hasshown a prominent polarization event around MJD 55900.

Multi-frequency linear and circular radio polarization monitoring of jet emission elements in $Fermi$ blazars