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19982024
most citedGiant Radio Sources

153 citations · 2.1k across the 89 of their papers we have counts for

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20 papers · 1 filter

astro-ph2008

A radio and near-infrared mini-survey of the MGRO J2019+37 complex

J. M. Paredes, J. Marti, C. H. Ishwara-Chandra +9

MGRO J2019+37 is an unidentified source of very high energy gamma-rays originally reported by the MILAGRO collaboration as the brightest TeV source in the Cygnus region. Despite th…

astro-ph2008★ 38 cited

Deep low-frequency observations with the Giant Metrewave Radio Telescope: a search for relic radio emission

S. K. Sirothia, D. J. Saikia, C. H. Ishwara-Chandra +1

We present deep multifrequency observations using the Giant Metrewave Radio Telescope at 153, 244, 610 and 1260 MHz of a field centered on J0916+6348, to search for evidence of fos…

astro-ph2008★ 6 cited

Radio detections towards unidentified variable EGRET sources

J. M. Paredes, J. Marti, C. H. Ishwara-Chandra +6

Context. A considerable fraction of the gamma-ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been…

astro-ph2007

GRB 030329: three years of radio afterglow monitoring

A. J. van der Horst, A. Kamble, R. A. M. J. Wijers +7

Radio observations of gamma-ray burst (GRB) afterglows are essential for our understanding of the physics of relativistic blast waves, as they enable us to follow the evolution of…

astro-ph2007★ 7 cited

GRB 030329: 3 years of radio afterglow monitoring

A. J. van der Horst, A. Kamble, R. A. M. J. Wijers +7

Radio observations of gamma-ray burst (GRB) afterglows are essential for our understanding of the physics of relativistic blast waves, as they enable us to follow the evolution of…

astro-ph2007★ 81 cited

Detailed study of the GRB 030329 radio afterglow deep into the non-relativistic phase

A. J. van der Horst, A. Kamble, L. Resmi +8

We explore the physics behind one of the brightest radio afterglows ever, GRB 030329, at late times when the jet is non-relativistic. We determine the physical parameters of the bl…