activity
20022023
most citedA Radio Counterpart to a Neutron Star Merger

543 citations · 6.4k across the 98 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.HE2013★ 18 cited

The optical rebrightening of GRB100814A: an interplay of forward and reverse shocks?

Massimiliano De Pasquale, N. P. M. Kuin, S. Oates +36

We present a wide dataset of gamma-ray, X-ray, UVOIR, and radio observations of the Swift GRB100814A. At the end of the slow decline phase of the X-ray and optical afterglow, this…

astro-ph.HE2013★ 24 cited

Electron Cooling in a Young Radio Supernova: SN 2012aw

Naveen Yadav, Alak Ray, Sayan Chakraborti +8

We present the radio observations and modeling of an optically bright Type II-P supernova (SN), SN 2012aw which exploded in the nearby galaxy Messier 95 (M95) at a distance of $10\…

astro-ph.HE2013★ 20 cited

Radio observations of GRB 100418a: Test of an energy injection model explaining long-lasting GRB afterglows

A. Moin, P. Chandra, J. C. A. Miller-Jones +6

We present the results of our radio observational campaign on GRB 100418a, for which we used the Australia Telescope Compact Array (ATCA), Very Large Array (VLA) and the Very Long…

astro-ph.HE2013★ 253 cited

A panchromatic view of the restless SN2009ip reveals the explosive ejection of a massive star envelope

R. Margutti, D. Milisavljevic, A. M. Soderberg +54

The 2012 explosion of SN2009ip raises questions about our understanding of the late stages of massive star evolution. Here we present a comprehensive study of SN2009ip during its r…

astro-ph.HE2013★ 140 cited

A Reverse Shock in GRB 130427A

T. Laskar, E. Berger, B. A. Zauderer +7

We present extensive radio and millimeter observations of the unusually bright GRB 130427A at z=0.340, spanning 0.67 to 12 days after the burst. Taken in conjunction with detailed…

astro-ph.HE2013★ 29 cited

The progenitor of SN 2011ja: Clues from circumstellar interaction

Sayan Chakraborti, Alak Ray, Randall Smith +7

Massive stars, possibly red supergiants, which retain extended hydrogen envelopes until core collapse, produce Type II Plateau (IIP) supernovae. The ejecta from these explosions sh…