activity
20062017
most citedDiscovery of the Ultra-Bright Type II-L Supernova 2008es

141 citations · 1.1k across the 19 of their papers we have counts for

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12 papers · 1 filter

astro-ph.HE2014★ 87 cited

A Luminous, Fast Rising UV-Transient Discovered by ROTSE: a Tidal Disruption Event?

J. Vinko, F. Yuan, R. M. Quimby +6

We present follow-up observations of an optical transient (OT) discovered by ROTSE on Jan. 21, 2009. Photometric monitoring was carried out with ROTSE-IIIb in the optical and Swift…

astro-ph.HE2014★ 3 cited

The Optical Luminosity Function of Gamma-ray Bursts deduced from ROTSE-III Observations

X. H. Cui, X. F. Wu, J. J. Wei +16

We present the optical luminosity function (LF) of gamma-ray bursts (GRBs) estimated from a uniform sample of 58 GRBs from observations with the Robotic Optical Transient Search Ex…

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.HE2012★ 16 cited

The origin of the early time optical emission of Swift GRB 080310

O. M. Littlejohns, R. Willingale, P. T. O'Brien +28

We present broadband multi-wavelength observations of GRB 080310 at redshift z = 2.43. This burst was bright and long-lived, and unusual in having extensive optical and near IR fol…

astro-ph.HE2011★ 49 cited

Panchromatic observations of the textbook GRB 110205A: constraining physical mechanisms of prompt emission and afterglow

W. Zheng, R. F. Shen, T. Sakamoto +56

We present a comprehensive analysis of a bright, long duration (T90 ~ 257 s) GRB 110205A at redshift z= 2.22. The optical prompt emission was detected by Swift/UVOT, ROTSE-IIIb and…

astro-ph.HE2011★ 85 cited

Sn 2008in - bridging the gap between normal and faint supernovae of type IIP

Rupak Roy, Brijesh Kumar, Stefano Benetti +18

We present optical photometric and low-resolution spectroscopic observations of the Type II plateau supernova (SN) 2008in, which occurred in the outskirts of the nearly face-on spi…

astro-ph.HE2010★ 60 cited

The Swift/Fermi GRB 080928 from 1 eV to 150 keV

A. Rossi, S. Schulze, S. Klose +28

We present the results of a comprehensive study of the gamma-ray burst 080928 and of its afterglow. GRB 080928 was a long burst detected by Swift/BAT and Fermi/GBM. It is one of th…

astro-ph.HE2010★ 44 cited

GRB 090902B: afterglow observations and implications

S. B. Pandey, C. A. Swenson, D. A. Perley +30

The optical-infrared afterglow of the LAT-detected long duration burst, GRB 090902B, has been observed by several instruments. The earliest detection by ROTSE-IIIa occurred 80 minu…

astro-ph.HE2010★ 31 cited

GRB 081008: from burst to afterglow and the transition phase in between

F. Yuan, P. Schady, J. L. Racusin +30

We present a multi-wavelength study of GRB 081008, at redshift 1.967, by Swift, ROTSE-III and GROND. Compared to other Swift GRBs, GRB 081008 has a typical gamma-ray isotropic equi…

astro-ph.HE2009

Prompt optical observations of Fermi-LAT bursts and GRB 090902B

S. B. Pandey, Carl W. Akerlof, W. Zheng +1

Observations of high energy emission from gamma-ray bursts (GRBs) constrain the extreme physical conditions associated with these energetic cosmic explosions. The Large Area Telesc…

astro-ph.HE2009★ 56 cited

Multi-wavelength observations of the energetic GRB 080810: detailed mapping of the broadband spectral evolution

K. L. Page, R. Willingale, E. Bissaldi +31

GRB 080810 was one of the first bursts to trigger both Swift and the Fermi Gamma-ray Space Telescope. It was subsequently monitored over the X-ray and UV/optical bands by Swift, in…

astro-ph.HE2009★ 111 cited

Looking Into the Fireball: ROTSE-III and Swift Observations of Early GRB Afterglows

E. S. Rykoff, F. Aharonian, C. W. Akerlof +21

We report on a complete set of early optical afterglows of gamma-ray bursts (GRBs) obtained with the ROTSE-III telescope network from March 2005 through June 2007. This set is comp…