Ultraluminous X-ray sources

P Kaaret, H Feng, TP Roberts - Annual Review of Astronomy …, 2017 - annualreviews.org
We review observations of ultraluminous X-ray sources (ULXs). X-ray spectroscopic and
timing studies of ULXs suggest a new accretion state distinct from those seen in Galactic …

The first cosmic structures and their effects

B Ciardi, A Ferrara - Space Science Reviews, 2005 - Springer
Despite much recent theoretical and observational progress in our knowledge of the early
universe, many fundamental questions remain only partially answered. Here, we review the …

Rotating massive main-sequence stars-i. grids of evolutionary models and isochrones

I Brott, SE de Mink, M Cantiello, N Langer… - Astronomy & …, 2011 - aanda.org
We present a dense grid of evolutionary tracks and isochrones of rotating massive main-
sequence stars. We provide three grids with different initial compositions tailored to compare …

The galaxy population hosting gamma-ray bursts

S Savaglio, K Glazebrook… - The Astrophysical …, 2009 - iopscience.iop.org
We present the most extensive and complete study of the properties for the largest sample
(46 objects) of gamma-ray burst (GRB) host galaxies. The redshift interval and the mean …

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 …

Formation of the first nuclear clusters and massive black holes at high redshift

B Devecchi, M Volonteri - The Astrophysical Journal, 2009 - iopscience.iop.org
We present a model for the formation of massive black holes (∼ 1000 M☉) due to stellar-
dynamical processes in the first stellar clusters formed at early cosmic times (z∼ 10–20) …

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 …

The optically unbiased gamma-ray burst host (TOUGH) survey. I. Survey design and catalogs

J Hjorth, D Malesani, P Jakobsson… - The Astrophysical …, 2012 - iopscience.iop.org
Long-duration gamma-ray bursts (GRBs) are powerful tracers of star-forming galaxies. We
have defined a homogeneous subsample of 69 Swift GRB-selected galaxies spanning a …

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 …