The supernova–gamma-ray burst connection

SE Woosley, JS Bloom - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
Observations show that at least some gamma-ray bursts (GRBs) happen simultaneously
with core-collapse supernovae (SNe), thus linking by a common thread nature's two …

Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe

SR Furlanetto, SP Oh, FH Briggs - Physics reports, 2006 - Elsevier
Observations of the high-redshift Universe with the 21cm hyperfine line of neutral hydrogen
promise to open an entirely new window onto the early phases of cosmic structure formation …

X-Shooting ULLYSES: Massive stars at low metallicity-I. Project description

JS Vink, A Mehner, PA Crowther, A Fullerton… - Astronomy & …, 2023 - aanda.org
Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts,
and gravitational wave events involving spectacular black hole mergers indicate that the low …

Long γ-ray bursts and core-collapse supernovae have different environments

AS Fruchter, AJ Levan, L Strolger, PM Vreeswijk… - Nature, 2006 - nature.com
When massive stars exhaust their fuel, they collapse and often produce the extraordinarily
bright explosions known as core-collapse supernovae. On occasion, this stellar collapse …

Gamma-Ray Bursts in the Swift Era

N Gehrels, E Ramirez-Ruiz… - Annual Review of …, 2009 - annualreviews.org
With its rapid-response capability and multiwavelength complement of instruments, the Swift
satellite has transformed our physical understanding of γ-ray bursts (GRBs). Providing high …

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 afterglows of Swift-era gamma-ray bursts. I. Comparing pre-Swift and Swift-era long/soft (type II) GRB optical afterglows

DA Kann, S Klose, B Zhang, D Malesani… - The Astrophysical …, 2010 - iopscience.iop.org
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 2009 September, for a total of 76 …

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 …

Implications for Cosmic Reionization from the Optical Afterglow Spectrum of the Gamma-Ray Burst 050904 at z = 6.3

T Totani, N Kawai, G Kosugi, K Aoki… - Publications of the …, 2006 - academic.oup.com
The gamma-ray burst (GRB) 050904 at provides the first opportunity to probe the
intergalactic medium (IGM) by GRBs at the epoch of reionization. Here, we present a …

Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II–Data Release 7

P Noterdaeme, P Petitjean, C Ledoux… - Astronomy & …, 2009 - aanda.org
We present the results of a search for damped Lyman-α (DLA) systems in the Sloan Digital
Sky Survey II (SDSS), Data Release 7. We use a fully automatic procedure to identify DLAs …