activity
20152021
most citedThe X-ray counterpart to the gravitational wave event GW 170817

888 citations · 1.2k across the 8 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE202132 cited

DDOTI Observations of Gravitational-Wave Sources Discovered in O3

R. L. Becerra, S. Dichiara, A. M. Watson +8

We present optical follow-up observations with the DDOTI telescope of gravitational-wave events detected during the Advanced LIGO and Advanced Virgo O3 observing run. DDOTI is capa…

astro-ph.HE2020

A search for optical and near-infrared counterparts of the compact binary merger GW190814

A. L. Thakur, S. Dichiara, E. Troja +29

We report on our observing campaign of the compact binary merger GW190814, detected by the Advanced LIGO and Advanced Virgo detectors on August 14th, 2019. This signal has the best…

astro-ph.HE201919 cited

GRB 180620A: Evidence for late-time energy injection

Rosa L. Becerra, Fabio De Colle, Alan M. Watson +11

The early optical emission of gamma-ray bursts gives an opportunity to understand the central engine and first stages of these events. About 30\% of GRBs present flares whose origi…

astro-ph.HE201931 cited

A multi-wavelength analysis of a collection of short-duration GRBs observed between 2012-2015

S. B. Pandey, Y. Hu, A. J. Castro-Tirado +71

We investigate the prompt emission and the afterglow properties of short duration gamma-ray burst (sGRB) 130603B and another eight sGRB events during 2012-2015, observed by several…

astro-ph.HE201919 cited

Late Central Engine Activity in GRB 180205A

R. L. Becerra, A. M. Watson, N. Fraija +16

We present optical photometry of the afterglow of the long GRB 180205A with the COATLI telescope from 217 seconds to about 5 days after the {\itshape Swift}/BAT trigger. We analyse…

astro-ph.HE2018

Evidence for a Bright-Edged Jet in the Optical/NIR Afterglow of GRB 160625B

Robert Strausbaugh, Nathaniel Butler, William H. Lee +2

Using deep and high-cadence gamma-ray burst (GRB) afterglow data from RATIR, we observe a sharp and achromatic light curve break 12.6 days after the GRB, accompanied by an approxim…