MeerKAT's large number (64) of 13.5 m diameter antennas, spanning 8 km with a densely
packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity …

We present the data and initial results from the first pilot survey of the Evolutionary Map of
the Universe (EMU), observed at 944 MHz with the Australian Square Kilometre Array …

Context. Inferences about dark matter, dark energy, and the missing baryons all depend on
the accuracy of our model of large-scale structure evolution. In particular, with cosmological …

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 …

We report the discovery of J0624–6948, a low-surface brightness radio ring, lying between
the Galactic Plane and the large magellanic cloud (LMC). It was first detected at 888 MHz …

Giant radio sources (GRSs) defined to be> 0.7 Mpc are the largest single objects in the
Universe and can be associated with both galaxies (GRGs) and quasars (GRQs). They are …

Context. The LOw Frequency ARray (LOFAR) is the only radio telescope that is presently
capable of high-sensitivity, high-resolution (ie< 1 mJy beam− 1 and< 15 ″) observations at …

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. Many massive galaxies launch jets from the accretion disk of their central black
hole, but only∼ 10 3 instances are known in which the associated outflows form giant radio …

Context. Giant radio galaxies (GRGs, or colloquially 'giants') are the Universe's largest
structures generated by individual galaxies. They comprise synchrotron-radiating active …