Broadband radio circular polarization spectrum of the relativistic jet in PKS B2126-158
S. P. O'Sullivan, N. M. McClure-Griffiths, I. J. Feain, B. M., Gaensler, R. J. Sault

TL;DR
This study presents the most detailed circular polarization spectrum of an AGN jet, revealing a strong frequency dependence and a clear anti-correlation with linear polarization, indicating internal Faraday conversion as the primary CP generation mechanism.
Contribution
It provides the first robust measurement of the circular polarization spectrum of an AGN jet and establishes a direct relation between linear and circular polarization, supporting internal Faraday conversion.
Findings
Circular polarization increases with frequency up to 6.5 GHz
A turnover occurs between 6.5 and 8 GHz where CP decreases rapidly
Strong anti-correlation between linear and circular polarization
Abstract
We present full-Stokes radio polarization observations of the quasar PKS B2126-158 (z=3.268) from 1 to 10 GHz using the Australia Telescope Compact Array. The source has large fractional circular polarization, m_c \equiv |V|/I, detected at high significance across the entire band (from 15 to 90\sigma per 128 MHz sub-band). This allows us to construct the most robust circular polarization (CP) spectrum of an AGN jet to date. We find m_c \propto \nu^{+0.60\pm0.03} from 1.5 to 6.5 GHz, with a peak of m_c ~ 1% before the spectrum turns over somewhere between 6.5 and 8 GHz, above which m_c \propto \nu^{-3.0\pm0.4}. The fractional linear polarization (p) varies from <~0.2% to ~1% across our frequency range and is strongly anti-correlated with the fractional CP, with a best-fit power law giving m_c \propto p^{-0.24\pm0.03}. This is the first clear relation between the observed linear and…
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