activity
20002024
most citedA new population of ultra-long duration gamma-ray bursts

293 citations · 1.1k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2024★ 1 cited

Rapid Response Mode observations of GRB 160203A: Looking for fine-structure line variability at z=3.52

G. Pugliese, A. Saccardi, V. D Elia +26

Gamma-ray bursts are the most energetic known explosions. Despite fading rapidly, they allow to measure redshift and important properties of their host-galaxies. We report the phot…

astro-ph.GA2014★ 83 cited

The warm, the excited, and the molecular gas: GRB 121024A shining through its star-forming galaxy

M. Friis, A. De Cia, T. Krühler +28

We present the first reported case of the simultaneous metallicity determination of a gamma-ray burst (GRB) host galaxy, from both afterglow absorption lines as well as strong emis…

astro-ph.HE2014★ 131 cited

GRB 120422A/SN 2012bz: Bridging the Gap between Low- And High-Luminosity GRBs

S. Schulze, D. Malesani, A. Cucchiara +62

At low redshift, a handful of gamma-ray bursts (GRBs) have been discovered with peak luminosities () substantially lower than the average…

astro-ph.CO2013★ 83 cited

The metallicity and dust content of a redshift 5 gamma-ray burst host galaxy

M. Sparre, O. E. Hartoog, T. Krühler +26

Observations of the afterglows of long gamma-ray bursts (GRBs) allow the study of star-forming galaxies across most of cosmic history. Here we present observations of GRB 111008A f…

astro-ph.CO2013★ 93 cited

Molecular Hydrogen in the Damped Lyman-alpha System towards GRB 120815A at z=2.36

T. Krühler, C. Ledoux, J. P. U. Fynbo +32

We present the discovery of molecular hydrogen (H_2), including the presence of vibrationally-excited H_2^* in the optical spectrum of the afterglow of GRB 120815A at z=2.36 obtain…

astro-ph.HE2013★ 293 cited

A new population of ultra-long duration gamma-ray bursts

A. J. Levan, N. R. Tanvir, R. L. C. Starling +38

We present comprehensive multiwavelength observations of three gamma-ray bursts (GRBs) with durations of several thousand seconds. We demonstrate that these events are extragalacti…

astro-ph.IM2012★ 26 cited

MOONS: a Multi-Object Optical and Near-infrared Spectrograph for the VLT

M. Cirasuolo, J. Afonso, R. Bender +77

MOONS is a new conceptual design for a Multi-Object Optical and Near-infrared Spectrograph for the Very Large Telescope (VLT), selected by ESO for a Phase A study. The baseline des…

astro-ph.HE2012★ 100 cited

GRB 100219A with X-shooter - abundances in a galaxy at z = 4.7

C. C. Thoene, J. P. U. Fynbo, P. Goldoni +24

Abundances of galaxies at redshifts z > 4 are difficult to obtain from damped Ly α (DLA) systems in the sightlines of quasars (QSOs) due to the Ly α forest blanketing and the low n…

astro-ph.HE2012★ 96 cited

SGR J1550-5418 bursts detected with the Fermi Gamma-ray Burst Monitor during its most prolific activity

A. J. van der Horst, C. Kouveliotou, N. M. Gorgone +32

We have performed detailed temporal and time-integrated spectral analysis of 286 bursts from SGR J1550-5418 detected with the Fermi Gamma-ray Burst Monitor (GBM) in January 2009, r…

astro-ph.HE2009★ 27 cited

GRB 090313: X-shooter's first shot at a GRB

A. de Ugarte Postigo, P. Goldoni, C. C. Thöne +26

Context. X-shooter is the first second-generation instrument to become operative at the ESO Very Large Telescope (VLT). It is a broad-band medium-resolution spectrograph designed w…

astro-ph2000★ 120 cited

VLT spectroscopy of GRB 990510 and GRB 990712; probing the faint and bright end of the GRB host galaxy population

P. M. Vreeswijk, A. Fruchter, L. Kaper +15

We present time-resolved optical spectroscopy of the afterglows of the gamma-ray bursts GRB 990510 and GRB 990712. Through the identification of several absorption lines in the fir…

astro-ph2000★ 65 cited

GRB990712: First Indication of Polarization Variability in a Gamma-ray Burst Afterglow

E. Rol, R. A. M. J. Wijers, P. M. Vreeswijk +9

We report the detection of significant polarization in the optical afterglow of GRB990712 on three instances 0.44, 0.70 and 1.45 days after the gamma-ray burst, with (P, theta) bei…