[HTML][HTML] Gamma-ray bursts and the fireball model

T Piran - Physics Reports, 1999 - Elsevier
Gamma-ray bursts (GRBs) have puzzled astronomers since their accidental discovery in the
late 1960s. The BATSE detector on the COMPTON-GRO satellite has been detecting one …

Gamma-ray burst afterglows

JV Paradijs, C Kouveliotou… - Annual review of …, 2000 - annualreviews.org
▪ Abstract The discovery of counterparts in X-ray and optical to radio wavelengths has
revolutionized the study of γ-ray bursts, until recently the most enigmatic of astrophysical …

An unusual supernova in the error box of the γ-ray burst of 25 April 1998

TJ Galama, PM Vreeswijk, J Van Paradijs… - nature, 1998 - nature.com
The discovery of afterglows associated with γ-ray bursts at X-ray, optical and radio
wavelengths and the measurement of the redshifts of some of these events, has established …

The observed offset distribution of gamma-ray bursts from their host galaxies: a robust clue to the nature of the progenitors

JS Bloom, SR Kulkarni… - The Astronomical Journal, 2002 - iopscience.iop.org
We present a comprehensive study to measure the locations of gamma-ray bursts (GRBs)
relative to their host galaxies. In total, we find the offsets of 20 long-duration GRBs from their …

Low-resolution spectroscopy of gamma-ray burst optical afterglows: biases in the Swift sample and characterization of the absorbers

JPU Fynbo, P Jakobsson, JX Prochaska… - The Astrophysical …, 2009 - iopscience.iop.org
We present a sample of 77 optical afterglows (OAs) of Swift detected gamma-ray bursts
(GRBs) for which spectroscopic follow-up observations have been secured. Our first …

GRB hosts through cosmic time-VLT/X-Shooter emission-line spectroscopy of 96 γ-ray-burst-selected galaxies at 0.1< z< 3.6

T Krühler, D Malesani, JPU Fynbo, OE Hartoog… - Astronomy & …, 2015 - aanda.org
We present data and initial results from VLT/X-Shooter emission-line spectroscopy of 96
galaxies selected by long γ-ray bursts (GRBs) at 0.1< z< 3.6, the largest sample of GRB host …

The nature of “dark” gamma-ray bursts

J Greiner, T Krühler, S Klose, P Afonso… - Astronomy & …, 2011 - aanda.org
Context. Thirteen years after the discovery of the first afterglows, the nature of dark gamma-
ray bursts (GRB) still eludes explanation: while each long-duration GRB typically has an X …

A population of massive, luminous galaxies hosting heavily dust-obscured gamma-ray bursts: implications for the use of GRBs as tracers of cosmic star formation

DA Perley, AJ Levan, NR Tanvir… - The Astrophysical …, 2013 - iopscience.iop.org
We present observations and analysis of the host galaxies of 23 heavily dust-obscured
gamma-ray bursts (GRBs) observed by the Swift satellite during the years 2005–2009 …

The Swift gamma-ray burst host galaxy legacy survey. I. Sample selection and redshift distribution

DA Perley, T Krühler, S Schulze… - The Astrophysical …, 2016 - iopscience.iop.org
ABSTRACT We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("
SHOALS"), a multi-observatory high-redshift galaxy survey targeting the largest unbiased …

The 2175 Å dust feature in a gamma-ray burst afterglow at redshift 2.45

T Krühler, AK Yoldaş, J Greiner… - The Astrophysical …, 2008 - iopscience.iop.org
We present optical and near-infrared photometry of the afterglow of the long gamma-ray
burst (GRB) 070802 at redshift 2.45 obtained with the ESO/MPI 2.2 m telescope equipped …