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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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astro-ph2008★ 29 cited

Simultaneous polarization monitoring of supernovae SN2008D/XT080109 and SN2007uy: isolating geometry from dust

J. Gorosabel, A. de Ugarte Postigo, A. J. Castro-Tirado +16

The possible existence of a continuum encompassing the diversity of explosive stellar deaths,ranging from ordinary SNe to relativistic hypernovae associated with long duration GRBs…

astro-ph2008★ 2 cited

Detection of the high z GRB 080913 and its implications on progenitors and energy extraction mechanisms

D. Perez-Ramirez, A. de Ugarte Postigo, J. Gorosabel +15

Aims: We present multiwavelength observations of one of the most distant gamma-ray bursts detected so far, GRB 080913. Based on these observations, we consider whether it could be…

astro-ph2008★ 42 cited

Optical and infrared flares from a transient Galactic soft gamma-ray repeater

A. J. Castro-Tirado, A. de Ugarte Postigo, J. Gorosabel +33

Soft gamma-ray repeaters (SGRs) are a rare type of gamma-ray transient sources that are ocasionally detected as bursts in the high-energy sky. They are thought to be produced by ma…

astro-ph2008★ 3 cited

The stellar-wind envelope around the supernova XRF/GRB060218/SN2006aj massive progenitor star

E. Sonbas, A. S. Moskvitin, T. A. Fatkhullin +8

In BTA spectra of the supernova SN2006aj, identified with the X-ray flash (XRF) and gamma-ray burst XRF/GRB060218/SN2006aj, we detected details interpreted as hydrogen lines, which…

astro-ph2008★ 72 cited

Early spectroscopic identification of SN 2008D

D. Malesani, J. P. U. Fynbo, J. Hjorth +27

SN 2008D was discovered while following up an unusually bright X-ray transient in the nearby spiral galaxy NGC 2770. We present early optical spectra (obtained 1.75 days after the…

astro-ph2008★ 45 cited

GRB 060605: multi-wavelength analysis of the first GRB observed using integral field spectroscopy

Patrizia Ferrero, Sylvio Klose, David Alexander Kann +16

The long and relatively faint gamma-ray burst GRB 060605 detected by \emph{Swift}/BAT lasted about 20 sec. Its afterglow could be observed with \emph{Swift}/XRT for nearly 1 day, w…

astro-ph2008★ 278 cited

The Afterglows of Swift-era Gamma-Ray Bursts II.: Type I GRB versus Type II GRB Optical Afterglows

D. A. Kann, S. Klose, B. Zhang +21

We use a large sample of GRB afterglow and prompt-emission data (adding further GRB afterglow observations in this work) to compare the optical afterglows (or the lack thereof) of…

astro-ph2008★ 45 cited

The extreme, red afterglow of GRB 060923A: Distance or dust?

N. R. Tanvir, A. J. Levan, E. Rol +16

Gamma-ray bursts are powerful probes of the early universe, but locating and identifying very distant GRBs remains challenging. We report here the discovery of the K-band afterglow…

astro-ph2008★ 68 cited

GRB 070306: A Highly Extinguished Afterglow

A. O. Jaunsen, E. Rol, D. J. Watson +12

We report on the highly extinguished afterglow of GRB 070306 and the properties of the host galaxy. An optical afterglow was not detected at the location of the burst, but in near-…

astro-ph2008★ 62 cited

On the distribution of stellar masses in gamma-ray burst host galaxies

J. M. Castro Cerón, M. J. Michałowski, J. Hjorth +6

We analyse Spitzer images of 30 long-duration gamma-ray burst (GRB) host galaxies. We estimate their total stellar masses (M*) based on the rest-frame K-band luminosities (L_Krest)…

astro-ph2007★ 354 cited

The Afterglows of Swift-era Gamma-Ray Bursts. I. Comparing pre-Swift and Swift era Long/Soft (Type II) GRB Optical Afterglows

D. A. Kann, S. Klose, B. Zhang +73

We have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to September 2009, for a total of 76…

astro-ph2007★ 59 cited

The dark nature of GRB 051022 and its host galaxy

A. J. Castro-Tirado, M. Bremer, S. McBreen +17

We present multiwavelength (X-ray/optical/near-infrared/millimetre) observations of GRB 051022 between 2.5 hours and ~1.15 yr after the event. It is the most intense gamma-ray burs…

astro-ph2007★ 32 cited

GRB 070311: a direct link between the prompt emission and the afterglow

C. Guidorzi, S. D. Vergani, S. Sazonov +30

We present prompt gamma-ray, early NIR/optical, late optical and X-ray observations of the peculiar GRB 070311 discovered by INTEGRAL, in order to gain clues on the mechanisms resp…

astro-ph2007★ 40 cited

The host of GRB 060206: kinematics of a distant galaxy

Christina C. Thoene, Klaas Wiersema, Cedric Ledoux +13

We present early (starting 1.6h after the burst) WHT/ISIS optical spectroscopy of the afterglow of the gamma-ray burst GRB 060206 detecting a range of metal absorption lines and th…

astro-ph2007★ 32 cited

GRB 060206 and the quandary of achromatic breaks in afterglow light curves

P. A. Curran, A. J. van der Horst, R. A. M. J. Wijers +20

Gamma-ray burst afterglow observations in the Swift era have a perceived lack of achromatic jet breaks compared to the BeppoSAX era. We present our multi-wavelength analysis of GRB…

astro-ph2007★ 26 cited

Spectroscopy and multiband photometry of the afterglow of intermediate duration gamma-ray burst 040924 and its host galaxy

K. Wiersema, A. J. van der Horst, D. A. Kann +19

We present optical photometry and spectroscopy of the afterglow and host galaxy of gamma-ray burst 040924. This GRB had a rather short duration of T90 ~2.4s, and a well sampled opt…

astro-ph2007★ 39 cited

On the nature of the short duration GRB 050906

A. J. Levan, N. R. Tanvir, P. Jakobsson +12

We present deep optical and infrared observations of the short duration GRB 050906. Although no X-ray or optical/IR afterglow was discovered to deep limits, the error circle of the…

astro-ph2007★ 61 cited

A case of mistaken identity? GRB 060912A and the nature of the long -- short GRB divide

A. J. Levan, P. Jakobsson, C. Hurkett +13

We investigate the origin of the GRB 060912A, which has observational properties that make its classification as either a long or short burst ambiguous. Short duration GRBs (SGRBs)…

astro-ph2007★ 2 cited

Gamma-ray burst host galaxies and the link to star-formation

J. P. U. Fynbo, J. Hjorth, D. Malesani +5

We briefly review the current status of the study of long-duration gamma-ray burst (GRB) host galaxies. GRB host galaxies are mainly interesting to study for two reasons: 1) they m…

astro-ph2007★ 126 cited

Spatially resolved properties of the GRB 060505 host: implications for the nature of the progenitor

Christina C. Thoene, Johan P. U. Fynbo, Goeran Oestlin +12

GRB 060505 was the first well-observed nearby possible long-duration GRB that had no associated supernova. Here we present spatially resolved spectra of the host galaxy of GRB 0605…

astro-ph2007★ 50 cited

The nature of the X-Ray Flash of August 24 2005

J. Sollerman, J. P. U. Fynbo, J. Gorosabel +23

We present comprehensive photometric R-band observations of the fading optical afterglow of the X-Ray Flash XRF050824, from 11 minutes to 104 days after the burst. The R-band light…

astro-ph2006★ 36 cited

Extensive multiband study of the X-ray rich GRB 050408. A likely off-axis event with an intense energy injection

A de Ugarte Postigo, T. A. Fatkhullin, G. Johannesson +40

Aims. Understand the shape and implications of the multiband light curve of GRB 050408, an X-ray rich (XRR) burst. Methods. We present a multiband optical light curve, covering the…

astro-ph2006★ 61 cited

Star formation rates and stellar masses in z ~ 1 gamma ray burst hosts

J. M. Castro Cerón, M. J. Michałowski, J. Hjorth +3

We analyse 4.5, 8 and 24 um band Spitzer images of six gamma ray burst host galaxies at redshifts close to 1. We constrain their star formation rates (SFR) based on the entire avai…

astro-ph2006

Fundamental Properties of GRB-Selected Galaxies: A Swift/VLT Legacy Survey

P. Jakobsson, J. Hjorth, J. P. U. Fynbo +2

We present the motivation, aims and preliminary result from the Swift/VLT legacy survey on gamma-ray burst host galaxies. This survey will produce a homogeneous and well-understood…