activity
19972021
most citedA very energetic supernova associated with the gamma-ray burst of 29 March 2003

1.5k citations · 18.4k across the 231 of their papers we have counts for

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55 papers · 1 filter

astro-ph.HE2021★ 21 cited

GRB 140102A: Insight into Prompt Spectral Evolution and Early Optical Afterglow Emission

Rahul Gupta, S. R. Oates, S. B. Pandey +38

We present and perform a detailed analysis of multi-wavelength observations of \thisgrb, an optical bright GRB with an observed reverse shock (RS) signature. Observations of this G…

astro-ph.HE2019★ 9 cited

Multiwavelength observations of GRB 140629A. A long burst with an achromatic jet break in the optical and X-ray afterglow

Y. -D. Hu, S. R. Oates, V. M. Lipunov +31

We investigate the long GRB140629A through multiwavelength observations, which cover optical, infrared and X-rays between 40s and 3yr after the burst, to derive the properties of t…

astro-ph.HE2019★ 1 cited

Outflows from GRB hosts are ubiquitous: Kinematics of z<0.3 GRB-SN hosts resolved with FLAMES

C. C. Thöne, L. Izzo, H. Flores +12

The hosts of long duration gamma-ray bursts are predominantly starburst galaxies at subsolar metallicity. At redshifts z<1, this implies that most of them are low-mass galaxies sim…

astro-ph.HE2019★ 31 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.HE2018★ 30 cited

The luminous host galaxy, faint supernova and rapid afterglow rebrightening of GRB 100418A

A. de Ugarte Postigo, C. C. Thoene, K. Bensch +35

Long gamma-ray bursts give us the chance to study both their extreme physics and the star-forming galaxies in which they form. GRB 100418A, at a z = 0.6239, had a bright optical an…

astro-ph.HE2017★ 7 cited

Colour variations in the GRB 120327A afterglow

A. Melandri, S. Covino, E. Zaninoni +42

We present a comprehensive temporal and spectral analysis of the long Swift GRB 120327A afterglow data to investigate the possible causes of the observed early time colour variatio…

astro-ph.HE2016★ 10 cited

A decade of GRB follow-up by BOOTES in Spain (2003-2013)

Martin Jelínek, Alberto J. Castro-Tirado, Ronan Cunniffe +20

This article covers ten years of GRB follow-ups by the Spanish BOOTES stations: 71 follow-ups providing 23 detections. Follow-ups by BOOTES-1B from 2005 to 2008 were given in the p…

astro-ph.HE2016★ 21 cited

GRB 110715A: The peculiar multiwavelength evolution of the first afterglow detected by ALMA

R. Sánchez-Ramírez, P. J. Hancock, G. Jóhannesson +35

We present the extensive follow-up campaign on the afterglow of GRB 110715A at 17 different wavelengths, from X-ray to radio bands, starting 81 seconds after the burst and extendin…

astro-ph.HE2016★ 101 cited

An achromatic break in the afterglow of the short GRB 140903A: evidence for a narrow jet

E. Troja, T. Sakamoto, S. B. Cenko +17

We report the results of our observing campaign on GRB140903A, a nearby (z=0.351) short duration (T90~0.3 s) gamma-ray burst discovered by Swift. We monitored the X-ray afterglow w…

astro-ph.HE2015★ 38 cited

The optical identifcation of events with poorly defined locations: The case of the Fermi GBM GRB140801A

V. M. Lipunov, J. Gorosabel, M. V. Pruzhinskaya +50

We report the early discovery of the optical afterglow of gamma-ray burst (GRB) 140801A in the 137 deg 3- error-box of the Fermi Gamma-ray Burst Monitor (GBM). MASTER is the…

astro-ph.HE2015★ 32 cited

The central engine of GRB 130831A and the energy breakdown of a relativistic explosion

M. De Pasquale, S. R. Oates, J. L. Racusin +37

Gamma-ray bursts (GRBs) are the most luminous explosions in the universe, yet the nature and physical properties of their energy sources are far from understood. Very important clu…

astro-ph.HE2015★ 22 cited

Limits on optical polarization during the prompt phase of GRB 140430A

D. Kopac, C. G. Mundell, J. Japelj +17

Gamma-ray burst GRB 140430A was detected by the Swift satellite and observed promptly with the imaging polarimeter RINGO3 mounted on the Liverpool Telescope, with observations begi…

astro-ph.HE2015★ 17 cited

Exploring the canonical behaviour of long gamma-ray bursts using an intrinsic multi-wavelength afterglow correlation

S. R. Oates, J. L. Racusin, M. De Pasquale +6

In this paper we further investigate the relationship, reported by Oates et al., 2012, between the optical/UV afterglow luminosity (measured at restframe 200s) and average afterglo…

astro-ph.HE2015★ 17 cited

Early optical follow-up of the nearby active star DG CVn during its 2014 superflare

M. D. Caballero-Garcia, V. Simon, M. Jelinek +20

DG CVn is a binary system in which one of the components is an M type dwarf ultra fast rotator, only three of which are known in the solar neighborhood. Observations of DG CVn by t…

astro-ph.HE2015★ 39 cited

GRB 140606B / iPTF14bfu: Detection of shock-breakout emission from a cosmological gamma-ray burst?

Z. Cano, A. de Ugarte Postigo, D. Perley +13

We present optical and near-infrared photometry of GRB~140606B (), and optical photometry and spectroscopy of its associated supernova (SN). The results of our modelling i…

astro-ph.HE2015★ 35 cited

The high-redshift gamma-ray burst GRB140515A

A. Melandri, M. G. Bernardini, P. D'Avanzo +22

High-redshift gamma-ray bursts have several advantages for the study of the distant universe, providing unique information about the structure and properties of the galaxies in whi…

astro-ph.HE2015★ 104 cited

Diversity in extinction laws of Type Ia supernovae measured between and

R. Amanullah, J. Johansson, A. Goobar +36

We present ultraviolet (UV) observations of six nearby Type~Ia supernovae (SNe~Ia) obtained with the Hubble Space Telescope, three of which were also observed in the near-IR (NIR)…

astro-ph.HE2014★ 105 cited

Circular polarization in the optical afterglow of GRB 121024A

K. Wiersema, S. Covino, K. Toma +37

Gamma-ray bursts (GRBs) are most probably powered by collimated relativistic outflows (jets) from accreting black holes at cosmological distances. Bright afterglows are produced wh…

astro-ph.HE2014★ 11 cited

Another short-burst host galaxy with an optically obscured high star formation rate: The case of GRB 071227

A. Nicuesa Guelbenzu, S. Klose, M. J. Michalowski +9

We report on radio continuum observations of the host galaxy of the short gamma-ray burst 071227 (z=0.381) with the Australia Telescope Compact Array (ATCA). We detect the galaxy i…

astro-ph.HE2014★ 17 cited

GRB 051008: A long, spectrally-hard dust-obscured GRB in a Lyman-Break Galaxy at z ~ 2.8

A. A. Volnova, A. S. Pozanenko, J. Gorosabel +17

We present observations of the dark Gamma-Ray Burst GRB 051008 provided by Swift/BAT, Swift/XRT, Konus-WIND, INTEGRAL/SPI-ACS in the high-energy domain and the Shajn, Swift/UVOT, T…

astro-ph.HE2014★ 41 cited

A Trio of GRB-SNe: GRB 120729A, GRB 130215A / SN 2013ez and GRB 130831A / SN 2013fu

Z. Cano, A. de Ugarte Postigo, A. Pozanenko +62

We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A / SN 2013ez and GRB 130831A / SN 2013fu. In the case…

astro-ph.HE2014★ 13 cited

Broad band polarimetric follow-up of Type IIP SN 2012aw

Brajesh Kumar, S. B. Pandey, C. Eswaraiah +1

We present the results based on R-band polarimetric follow-up observations of the nearby (~10 Mpc) Type II-plateau SN 2012aw. Starting from ~10 days after the SN explosion, these p…

astro-ph.HE2014★ 47 cited

The host of the SN-less GRB 060505 in high resolution

C. C. Thöne, L. Christensen, J. X. Prochaska +5

The spiral host galaxy of GRB 060505 at z=0.089 was the site of a puzzling long duration burst without an accompanying supernova. Studies of the burst environment by Thöne et al. (…

astro-ph.HE2014★ 12 cited

The dark nature of GRB 130528A and its host galaxy

S. Jeong, A. J. Castro-Tirado, M. Bremer +18

We study the dark nature of GRB 130528A through multi-wavelength observations and conclude that the main reason for the optical darkness is local extinction inside of the host gala…