activity
20002023
most citedSwings between rotation and accretion power in a millisecond binary pulsar

460 citations · 2.5k across the 87 of their papers we have counts for

collaborators

88 papers

astro-ph.IM2023

Measuring photometric redshifts for high-redshift radio source surveys

Kieran J. Luken, Ray P. Norris, X. Rosalind Wang +3

With the advent of deep, all-sky radio surveys, the need for ancillary data to make the most of the new, high-quality radio data from surveys like the Evolutionary Map of the Unive…

astro-ph.SR2023★ 11 cited

A Study of Twelve Potential Merger Candidate Contact Binary Systems

Surjit S. Wadhwa, Bojan Arbutina, Nick F. H. Tothill +4

Photometric observations and analysis of twelve previously poorly studied contact binary systems is presented. All show total eclipses and have extremely low mass ratios ranging fr…

astro-ph.GA2023★ 21 cited

MeerKAT view of the Dancing Ghosts -- Peculiar Galaxy Pair PKS 2130-538 in Abell 3785

Velibor Velović, William D. Cotton, Miroslav D. Filipovi'c +3

We present MeerKAT L-band (886-1682 MHz) observations of the extended radio structure of the peculiar galaxy pair PKS 2130-538 known as the "Dancing Ghosts". The complex of bending…

astro-ph.HE2023★ 29 cited

Detection of extended gamma-ray emission around the Geminga pulsar with H.E.S.S

H. E. S. S. Collaboration, :, F. Aharonian +165

Geminga is an enigmatic radio-quiet gamma-ray pulsar located at a mere 250 pc distance from Earth. Extended very-high-energy gamma-ray emission around the pulsar was discovered by…

astro-ph.HE2022★ 13 cited

New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud

Luke M. Bozzetto, Miroslav D. Filipović, H. Sano +34

We present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). This new sample is…

astro-ph.SR2022★ 10 cited

Simplified Method for the Identification of Low Mass Ratio Contact Binary Systems that are Potential Red Nova Progenitors

Surjit S. Wadhwa, Ain Y. De Horta, Miroslav D. Filipovic +4

The study presents a simplified method to identify potential bright red nova progenitors based on the amplitude of the light curve and infrared (J-H) colour of a contact binary sys…