The Magnetic Field and Polarization Properties of Radio Galaxies in Different Accretion States

Shane P. O'Sullivan, B. M. Gaensler, M. A. Lara-López +3

We use the integrated polarized radio emission at 1.4 GHz (${\Pi }_{1.4\mathrm{GHz}}$) from a large sample of AGN (796 sources at redshifts $z<0.7$) to study the large-scale magnetic field…