Two recent discoveries, namely PSR J0901− 4046 and GLEAM-X J162759. 5− 523504.3
(hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic …

The Australian SKA Pathfinder (ASKAP) is being used to undertake a campaign to rapidly
survey the sky in three frequency bands across its operational spectral range. The first pass …

Motivated by the recent detection of ultralong-period radio transients, we investigate new
models of coherent radio emission via low-altitude electron–positron pair production in …

We present the results of a radio transient and polarization survey towards the Galactic
Centre, conducted as part of the Australian Square Kilometre Array Pathfinder Variables and …

ABSTRACT The Deeper, Wider, Faster (DWF) program coordinates observations with
telescopes across the electromagnetic spectrum, searching for transients on time-scales of …

The newest generation of radio telescopes is able to survey large areas with high sensitivity
and cadence, producing data volumes that require new methods to better understand the …

The Galactic center (GC) presents one of the highest stellar densities in our Galaxy, making
its surroundings an environment potentially rich in radio transients, such as pulsars and …

We report on the detection of MKT J174641. 0− 321404, a new radio transient found in
untargeted searches of wide-field MeerKAT radio images centred on the black hole X-ray …

The population of radio-loud stars has to date been studied primarily through either targeted
observations of a small number of highly active stars or wide-field, single-epoch surveys that …

The Doppler shift of a radio signal is caused by the relative motion between the transmitter
and receiver. The change in frequency of the signal over time is called the drift rate. In the …