Compact steep-spectrum (CSS) and peaked-spectrum (PS) radio sources are compact,
powerful radio sources. The multi-frequency observational properties and current theories …

Radio observations of tidal disruption events (TDEs) probe material ejected by the disruption
of stars by supermassive black holes (SMBHs), uniquely tracing the formation and evolution …

The radio-emitting neutron star population encompasses objects with spin periods ranging
from milliseconds to tens of seconds. As they age and spin more slowly, their radio emission …

The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic
surveys. It has a large field of view and is sensitive to large-scale and compact emission. It …

The inner∼ 200 pc region of the Galaxy contains a 4 million M⊙ supermassive black hole
(SMBH), significant quantities of molecular gas, and star formation and cosmic-ray energy …

The Rapid ASKAP Continuum Survey (RACS) is the first large sky survey using the
Australian Square Kilometre Array Pathfinder (ASKAP), covering the sky south of+ 41$^\circ …

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 …

ABSTRACT MIGHTEE is a galaxy evolution survey using simultaneous radio continuum,
spectropolarimetry, and spectral line observations from the South African MeerKAT …

Over the past decade, several works have used the ratio between total (rest 8− 1000 μm)
infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (q IR), often referred to …

We present the HI emission project within the MIGHTEE survey, currently being carried out
with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind …