Discovery of magnetised CGM at z ~ 1
Using radio observations of thousands of distant quasars, we probe magnetic fields in the circumgalactic medium (CGM) of galaxies from z~0.4 to z~2.4.
Using radio observations of thousands of distant quasars, we probe magnetic fields in the circumgalactic medium (CGM) of galaxies from z~0.4 to z~2.4.
DR3 RM Grid in equatorial coordinates.
Predicted polarized source counts for SKA-Low as a function of sensitivity.
Using POSSUM rotation measures, we probe the magnetised environment of the Shapley Supercluster core and compare observations with cosmological simulations.