Clusters of galaxies have been found to host Mpc-scale diffuse, non-thermal radio emission
in the form of central radio halos and peripheral relics. Turbulence and shock-related …

Radio relics are typically found to be arc-like regions of synchrotron emission in the outskirts
of merging galaxy clusters, bowing out from the cluster center. In most cases they show …

We present deep XMM-Newton, Karl G. Jansky Very Large Array, and upgraded Giant
Metrewave Radio Telescope observations of Abell 746, a cluster that hosts a plethora of …

Diffuse radio sources known as radio relics are direct tracers of shocks in the outskirts of
merging galaxy clusters. PSZ2 G200. 95–28.16, a low-mass merging cluster (M …

The morphology and the characteristic scale of polarized structures provide crucial insights
into the mechanisms that drive turbulence and maintain magnetic fields in magneto-ionic …

Observations of Faraday rotation and synchrotron emission in galaxy clusters imply large-
scale magnetic fields with $\mu\mathrm {G} $ strengths possibly extending back to $ z= 4 …

Diffuse radio sources known as radio relics are direct tracers of shocks in the outskirts of
merging galaxy clusters. PSZ2 G200. 95-28.16, a low-mass merging cluster ($\textrm {M} …

Non-thermal emission from relativistic electrons gives insight into the strength and
morphology of intra-cluster magnetic fields, as well as providing powerful tracers of structure …

Radio relics are diffuse, synchrotron, radio sources located at the outskirts of merging galaxy
clusters, characterized by elongated arc-like shapes, with sizes ranging between 0.5 to …