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THE MAGNETIC FIELD AND POLARIZATION PROPERTIES OF RADIO GALAXIES IN DIFFERENT ACCRETION STATES
We use the integrated polarized radio emission at 1.4 GHz () from a large sample of active galactic nuclei (AGN; 796 sources at redshifts ) to study the large-scale magnetic field properties of radio galaxies in relation to the host galaxy accretion state. We find a fundamental difference in between …