activity
20172026
most cited154 MHz detection of faint, polarized flares from UV Ceti

50 citations · 174 across the 6 of their papers we have counts for

collaborators
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7 papers · 1 filter

astro-ph.HE2026

The second Arcminute Microkelvin Imager - Large Array Gamma-ray burst radio afterglow catalog

L. Rhodes, D. Ibrahim, N. Sqalli +13

Radio observations of gamma-ray burst afterglows provide insight in to the different emitting regions within the jet, its hydrodynamics and burst environment. In this paper, we pre…

astro-ph.HE2020

Measuring the distance to the black hole candidate X-ray binary MAXI J1348-630 using HI absorption

J. Chauhan, J. C. A. Miller-Jones, W. Raja +11

We present HI absorption spectra of the black hole candidate X-ray binary (XRB) MAXI J1348-630 using the Australian Square Kilometre Array Pathfinder (ASKAP) and MeerKAT. The ASKAP…

astro-ph.HE201922 cited

A detailed radio study of the energetic, nearby and puzzling GRB 171010A

J. S. Bright, A. Horesh, A. J. van der Horst +7

We present the results of an intensive multi-epoch radio frequency campaign on the energetic and nearby GRB 171010A with the Karl G. Janksy Very Large Array and Arcminute Microkelv…

astro-ph.HE2018

A newly discovered double-double candidate microquasar in NGC 300

R. Urquhart, R. Soria, M. W. Pakull +7

We present the discovery of a powerful candidate microquasar in NGC 300, associated with the S 10 optical nebula (previously classified as a supernova remnant). Chandra images show…

astro-ph.HE2018

LOFAR 150-MHz observations of SS 433 and W 50

J. W. Broderick, R. P. Fender, J. C. A. Miller-Jones +28

We present LOFAR high-band data over the frequency range 115-189 MHz for the X-ray binary SS 433, obtained in an observing campaign from 2013 February - 2014 May. Our results inclu…

astro-ph.HE201832 cited

Multiband counterparts of two eclipsing ultraluminous X-ray sources in M 51

R. Urquhart, R. Soria, H. M. Johnston +5

We present the discovery and interpretation of ionized nebulae around two ultraluminous X-ray sources in M 51; both sources share the rare property of showing X-ray eclipses by the…