activity
20232026
most citedAn emission state switching radio transient with a 54 minute period

60 citations · 124 across the 28 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2025★ 3 cited

The Dawes Review 13: A New Look at The Dynamic Radio Sky

Tara Murphy, David L. Kaplan

Astronomical objects that change rapidly give us insight into extreme environments, allowing us to identify new phenomena, test fundamental physics, and probe the Universe on all s…

astro-ph.SR2025★ 2 cited

Discovery of Main-sequence Radio Pulse emitters from widefield sky surveys

Barnali Das, Matt E. Shultz, Joshua Pritchard +6

Magnetic AB stars are known to produce periodic radio pulses by the electron cyclotron maser emission (ECME) mechanism. Only 19 such stars, known as 'Main-sequence Radio Pulse emit…

astro-ph.SR2025

VAST-MeMeS: Characterising non-thermal radio emission from magnetic massive stars using the Australian SKA Pathfinder

Barnali Das, Laura N. Driessen, Matt E. Shultz +7

Magnetic massive stars are stars of spectral types O, B and A that harbour kG strength (mostly dipolar) surface magnetic fields. Their non-thermal radio emission has been de…

astro-ph.SR2024

A two-minute burst of highly polarised radio emission originating from low Galactic latitude

Dougal Dobie, Andrew Zic, Lucy S. Oswald +19

Several sources of repeating coherent bursts of radio emission with periods of many minutes have now been reported in the literature. These "ultra-long period" (ULP) sources have n…

astro-ph.SR2024★ 1 cited

The Sydney Radio Star Catalogue: properties of radio stars at megahertz to gigahertz frequencies

Laura N. Driessen, Joshua Pritchard, Tara Murphy +12

We present the Sydney Radio Star Catalogue, a new catalogue of stars detected at megahertz to gigahertz radio frequencies. It consists of 839 unique stars with 3,405 radio detectio…

astro-ph.SR2023

Multi-epoch sampling of the radio star population with the Australian SKA Pathfinder

Joshua Pritchard, Tara Murphy, George Heald +5

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 widefield, single-epoch surve…