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 …

Radio mini-haloes are poorly understood, moderately extended diffuse radio sources that
trace the presence of magnetic fields and relativistic electrons on scales of hundreds of …

The pre-merging system of galaxy clusters Abell 3391-Abell 3395 located at a mean redshift
of 0.053 has been observed at 1 GHz in an ASKAP/EMU Early Science observation as well …

Aims. We study the intra-cluster magnetic field in the poor galaxy cluster Abell 194 by
complementing radio data, at different frequencies, with data in the optical and X-ray bands …

The Taipan galaxy survey (hereafter simply 'Taipan') is a multi-object spectroscopic survey
starting in 2017 that will cover 2π steradians over the southern sky (δ≲ 10°,| b|≳ 10°), and …

We know that magnetic fields are pervasive across all scales in the Universe and over all of
cosmic time and yet our understanding of many of the properties of magnetic fields is still …

Next-generation radio interferometers, such as the Square Kilometre Array, will revolutionize
our understanding of the Universe through their unprecedented sensitivity and resolution …

One process affecting gas-rich cluster galaxies is ram pressure stripping (RPS), ie, the
removal of galactic gas through direct interaction with the intracluster medium (ICM) …

Faraday rotation measures (RMs) of extragalactic radio sources provide information on line-
of-sight magnetic fields, including contributions from our Galaxy, source environments, and …

We present a radio and X-ray analysis of the galaxy cluster SPT-CL J2032–5627.
Investigation of public data from the Australian Square Kilometre Array Pathfinder (ASKAP) …