activity
20192026
most citedThe Rapid ASKAP Continuum Survey I: Design and First Results

287 citations · 1.2k across the 44 of their papers we have counts for

collaborators

46 papers

astro-ph.SR2026

Coherent radio bursts, polarity reversal, and quiescent emission from the M4V dwarf WW PsA

Jackson Mitchell-Bolton, Laura Driessen, Tara Murphy +6

Coherent radio emission from magnetically active M dwarfs is largely observed in two varieties: stochastic solar-like bursts and beamed, rotationally modulated emission including a…

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.SR2026

Radio Properties of RS Canum Venaticorum Variables in VLASS and RACS

Suhasini S. Rao, Gregory R. Sivakoff, Craig O. Heinke +6

We performed a systematic search for radio emission from RS Canum Venaticorum (RS CVn) binaries, selected from the International Variable Star Index (VSX) catalog, in the Very Larg…

astro-ph.SR2026

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir

Barnali Das, Hayley Bignall, Andrew Zic +6

CU Vir, a magnetic hot star, is the first discovered Main-sequence Radio Pulse emitter (MRP) characterized by its ability to produce periodic radio pulses via electron cyclotron ma…

astro-ph.IM2026

VASTER: The ASKAP real-time fast-imaging pipeline -- overview and discovery of two long period transients

Yuanming Wang, Dougal Dobie, Tara Murphy +22

Recent developments in widefield radio telescopes have enabled searches of a new region of parameter space in the time domain: timescales of seconds to minutes, that have been over…

astro-ph.SR2026

The Variability of Radio Stars

Laura N. Driessen, Alex Andersson, Joseph R. Callingham +6

Stellar radio emission is highly variable with stellar flares lasting from milliseconds to hours. For some stars, their flares or bursts can repeat once every couple of hours, whil…

astro-ph.HE2026

The X-ray emission of the long-period transient and accreting cataclysmic variable ASKAP J174508.9-505149

M. Imbrogno, M. Veresvarska, Y. L. Wang +8

Long-period transients (LPTs) challenge our knowledge of the mechanism producing radio periodic pulsations in compact objects. Some LPTs have been associated with systems hosting a…

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.GA2026

One sightline, many systems: a FLASH discovery of HI towards scintillating quasar PKS 0405-385

E. F. Kerrison, H. Yoon, E. M. Sadler +15

We report the discovery of an intervening 21\,cm absorption line at z = 0.882 towards the z = 1.284 quasar PKS 0405-385, identified in the First Large Absorption Survey in HI (FLAS…

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.CO2026

The ASKAP Variables and Slow Transients (VAST) Extragalactic Survey - Data Release 1

Iris de Ruiter, Dougal Dobie, Tara Murphy +13

The Variables and Slow Transients (VAST) Survey on the Australian SKA Pathfinder (ASKAP) is designed to systematically explore the dynamic radio sky, detecting sources that vary on…

astro-ph.HE2026★ 2 cited

ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH?

Ashna Gulati, Tara Murphy, David L. Kaplan +24

We report the discovery of a slowly evolving, extragalactic radio transient, ASKAP J005512.2--255834 (hereafter ASKAP J0055-2558), identified using the Australian SKA Pathfinder in…

astro-ph.HE2025

Searching for Long-Period Radio Transients in ASKAP EMU Data with 10-Second Imaging

Yu Wing Joshua Lee, Yuanming Wang, Manisha Caleb +10

Long-period radio transients (LPTs) are a recently identified phenomenon that challenge our current understanding of compact objects and coherent radio emission mechanisms. These o…

astro-ph.HE2025

Sensitive Constraints on Coherent Radio Emission from Five Isolated White Dwarfs

Lei Zhang, Alexander Wolszczan, Joshua Pritchard +8

Coherent, periodic radio emission from pulsars has been widely interpreted as evidence of neutron stars as strongly magnetized compact objects. In recent years, radio pulses have a…

astro-ph.HE2025

ASKAP J144834-685644: a newly discovered long period radio transient detected from radio to X-rays

Akash Anumarlapudi, David L. Kaplan, Nanda Rea +13

Long-period radio transients (LPTs) are an emerging group of radio transients that show periodic polarized radio bursts with periods varying from a few minutes to a few hours. Fewe…

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.HE2024★ 20 cited

Detection of X-ray Emission from a Bright Long-Period Radio Transient

Ziteng Wang, Nanda Rea, Tong Bao +46

Recently, a class of long-period radio transients (LPTs) has been discovered, exhibiting emission on timescales thousands of times longer than radio pulsars. Several models had bee…

astro-ph.HE2024★ 60 cited

An emission state switching radio transient with a 54 minute period

M. Caleb, E. Lenc, D. L. Kaplan +19

Long-period radio transients are an emerging class of extreme astrophysical events of which only three are known. These objects emit highly polarised, coherent pulses of typically…

astro-ph.HE2024

Radio afterglows from tidal disruption events: An unbiased sample from ASKAP RACS

Akash Anumarlapudi, Dougal Dobie, David L. Kaplan +23

Late-time ( year) radio follow-up of optically-discovered tidal disruption events (TDEs) is increasingly resulting in detections at radio wavelengths, and there is growing ev…

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…