The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite
began surveying the sky in December 2019, with the aim of producing all-sky X-ray source …

Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant
substructure. We present new, highly sensitive radio continuum observations of Abell 3266 …

Context. Scaling relations link the physical properties of clusters at cosmic scales. They are
used to probe the evolution of large-scale structure, estimate observables of clusters, and …

Many relaxed cool-core clusters host diffuse radio emission on scales of hundreds of
kiloparsecs: mini-haloes. However, the mechanism responsible for generating them, as well …

The discovery of diffuse radio emission in galaxy clusters proved the existence of energetic
cosmic-ray electrons and cosmic magnetic fields on Mpc-scales in the Universe …

Context. SMACS J0723. 3− 7327 is the first galaxy cluster lens observed by James Webb
Space Telescope (JWST). Based on its early release observation data, several groups have …

Context. Dynamical motions in the intra-cluster medium (ICM) can imprint distinctive features
on X-ray images that map the thermal bremsstrahlung emission from galaxy clusters, such …

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 …

Low-frequency radio observations show an increasing number of radio galaxies located in
galaxy clusters that display peculiar morphologies and spectral profiles. This is the result of …

Context. Galaxy clusters are the most massive bound objects in the recent history of the
universe; the number density of galaxy clusters as a function of mass and redshift is a …