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 …

Galaxy clusters are useful cosmological probes and interesting astrophysical laboratories.
As the cluster samples continue to grow in size, a deeper understanding of the sample …

We report on the results of an image-based search for pulsar candidates toward the Galactic
bulge. We used mosaic images from the MeerKAT radio telescope that were taken as part of …

We present a multi-wavelength study of three new z∼ 5.6 quasi-stellar objects (QSOs)
identified from dedicated spectroscopic observations. The three sources were selected as …

The extragalactic γ-ray sky is dominated by relativistic jets aligned to the observer's line of
sight, ie, blazars. A few of their misaligned counterparts, eg, radio galaxies, are also …

The astrophysical γ-ray photons carry the signatures of the violent phenomena happening
on various astronomical scales in our Universe. This includes supernova remnants, pulsars …

The GLEAMing of the first supermassive black holes: III. Radio sources with ultra-faint host
galaxies Page 1 Publications of the Astronomical Society of Australia (2024), 41, e071, 21 pages …

Our data processing for SPICE-RACS-DR1 involved a two-stage process. First, image cubes
were produced using the ASKAPSOFT (Guzman et al., 2019) pipeline, and scripts that made …

The Gamma-ray detection from an astrophysical object indicates the presence of an extreme
environment where high-energy radiation is produced. With the continuous monitoring of the …

The broad-band radio spectral energy distribution (SED) of star-forming galaxies (SFGs)
contains a wealth of complex physics. We aim to determine the physical emission and loss …