activity
20142019
most citedA Comprehensive Radio View of the Extremely Bright Gamma-Ray Burst 130427A

83 citations · 339 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE201942 cited

An HI absorption distance to the black hole candidate X-ray binary MAXI J1535-571

Jaiverdhan Chauhan, James C. A. Miller-Jones, Gemma E. Anderson +10

With the Australian Square Kilometre Array Pathfinder (ASKAP) we monitored the black hole candidate X-ray binary MAXI J1535--571 over seven epochs from 21 September to 2 October 20…

astro-ph.HE201647 cited

The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations

G. E. Anderson, A. Horesh, K. P. Mooley +12

We present a radio light curve of supernova (SN) 2014C taken with the Arcminute Microkelvin Imager (AMI) Large Array at 15.7 GHz. Optical observations presented by Milisavljevic et…

astro-ph.HE201624 cited

Disk-Jet quenching of the Galactic Black Hole Swift J1753.5-0127

A. P. Rushton, A. W. Shaw, R. P. Fender +8

We report on radio and X-ray monitoring observations of the BHC Swift J1753.5-0127 taken over a ~10 year period. Presented are daily radio observations at 15 GHz with the AMI-LA an…

astro-ph.HE201555 cited

The Needle in the 100 deg2 Haystack: Uncovering Afterglows of Fermi GRBs with the Palomar Transient Factory

Leo P. Singer, Mansi M. Kasliwal, S. Bradley Cenko +32

The Fermi Gamma-ray Space Telescope has greatly expanded the number and energy window of observations of gamma-ray bursts (GRBs). However, the coarse localizations of tens to a hun…

astro-ph.HE201429 cited

A prompt radio transient associated with a gamma-ray superflare from the young M dwarf binary DG CVn

R. P. Fender, G. E. Anderson, R. Osten +4

On 2014 April 23, the Swift satellite detected a gamma-ray superflare from the nearby star system DG CVn. This system comprises a M-dwarf binary with extreme properties: it is very…

astro-ph.HE201483 cited

A Comprehensive Radio View of the Extremely Bright Gamma-Ray Burst 130427A

A. J. van der Horst, Z. Paragi, A. G. de Bruyn +11

GRB 130427A was extremely bright as a result of occurring at low redshift whilst the energetics were more typical of high-redshift gamma-ray bursts (GRBs). We collected well-sample…