most citedThe emission of interpulses by a 6.45-hour period coherent radio transient

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astro-ph.HE2026

Radio Monitoring of Classical Novae using the ASKAP Variable and Slow Transients Survey

Aishani Majumder, David L. Kaplan, Laura N. Driessen +3

We present a search for radio emission from classical novae at 887.5 MHz using data from the Australian SKA Pathfinder Variable And Slow Transient (VAST) survey. We cross-matched 4…

astro-ph.HE2026

Year-timescale changes in AGN radio luminosity as seen by the ASKAP Variables and Slow Transients Survey

Chloe Klare, Charlotte Ward, Dougal Dobie +6

A few dozen previously radio-quiet active galactic nuclei (AGN) have been observed to transition to radio-loud at 1-3 GHz frequencies over timescales of more than a decade, and thi…

astro-ph.HE2026★ 3 cited

Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary

Kovi Rose, Joshua Pritchard, Tara Murphy +26

Long period radio transients (LPTs) are coherent bursts of polarised radio emission that repeat periodically on timescales of minutes to hours. Little is known about the physical o…

astro-ph.HE2026

A sample of short-lived Galactic radio transients from ASKAP VAST

Akash Anumarlapudi, David L. Kaplan, Natasha Hurley Walker +6

Galactic radio transients (GRTs) are mysterious short-lived (~days to months) radio transients that are quiet at all other wavelengths. Until now, roughly half a dozen such sources…

astro-ph.HE2026

Discovery of a 36-minute long-period transient ASKAP J142431.2-612611

Joshua Pritchard, Tara Murphy, Dougal Dobie +13

We report the discovery of a new long-period radio transient, ASKAP J142431.2-612611, with a 36 minute period, identified in the Australian SKA Pathfinder Evolutionary Map of the U…

astro-ph.HE2025★ 34 cited

The emission of interpulses by a 6.45-hour period coherent radio transient

Y. W. J. Lee, M. Caleb, Tara Murphy +29

Long-period radio transients are a novel class of astronomical objects characterised by prolonged periods ranging from 18 minutes to 54 minutes. They exhibit highly polarised, cohe…