The Ultraluminous GRB 110918A

@article{Frederiks2013TheUG,
  title={The Ultraluminous GRB 110918A},
  author={Dmitry D. Frederiks and Kevin Hurley and Dmitry S. Svinkin and Valentin D. Pal'shin and Vanessa Mangano and S. R. Oates and Rafail L. Aptekar and Sergey Golenetskii and E. P. Mazets and Philipp Oleynik and Anastasia Tsvetkova and Mikhail Ulanov and A. V. Kokomov and Thomas L. Cline and David N. Burrows and H A Krimm and Claudio Pagani and B. Sbarufatti and Michael H. Siegel and Igor G. Mitrofanov and Dmitriy Golovin and Maxim L. Litvak and Anton B. Sanin and William V. Boynton and Chuck Fellows and Keith Harshman and Heather L. Enos and Richard D. Starr and A. von Kienlin and Arne Rau and Xinxin Zhang and Jeffrey Goldstein},
  journal={The Astrophysical Journal},
  year={2013},
  volume={779},
  pages={151}
}
GRB 110918A is the brightest long gamma-ray burst (GRB) detected by Konus-WIND during its almost 19 yr of continuous observations and the most luminous GRB ever observed since the beginning of the cosmological era in 1997. We report on the final Interplanetary Network localization of this event and its detailed multiwavelength study with a number of space-based instruments. The prompt emission is characterized by a typical duration, a moderate peak energy of the time-integrated spectrum, and… 
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References

SHOWING 1-10 OF 80 REFERENCES
GRB 091024A AND THE NATURE OF ULTRA-LONG GAMMA-RAY BURSTS
We present a broadband study of gamma-ray burst (GRB) 091024A within the context of other ultra-long-duration GRBs. An unusually long burst detected by Konus-Wind (KW), Swift, and Fermi, GRB 091024A
Multiwavelength Observations of GRB 110731A: GeV Emission from Onset to Afterglow
We report on the multiwavelength observations of the bright, long gamma-ray burst GRB 110731A, by the Fermi and Swift observatories, and by the MOA and GROND optical telescopes. The analysis of the
The redshift and afterglow of the extremely energetic gamma-ray burst GRB 080916C
Context. The detection of GeV photons from gamma-ray bursts (GRBs) has important consequences for the interpretation and modelling of these most-energetic cosmological explosions. The full
THE AFTERGLOW OF GRB 130427A FROM 1 TO 10(16) GHz
We present multiwavelength observations of the afterglow of GRB 130427A, the brightest (in total fluence) gamma-ray burst (GRB) of the past 29 yr. Optical spectroscopy from Gemini-North reveals the
A Giant Flare from a Soft Gamma Repeater in the Andromeda Galaxy (M31)
The light curve, energy spectra, energetics, and IPN localization of an exceedingly intense, short-duration, hard-spectrum burst, GRB 070201, obtained from Konus-Wind, INTEGRAL (SPI-ACS), and
The low-extinction afterglow in the solar-metallicity host galaxy of γ-ray burst 110918A
Galaxies selected through long γ-ray bursts (GRBs) could be of fundamental importance when mapping the star formation history out to the highest redshifts. Before using them as efficient tools in the
Dust Sublimation by Gamma-ray Bursts and Its Implications
The prompt optical flash recently detected accompanying GRB 990123 suggests that, for at least some γ-ray bursts (GRBs), γ-ray emission is accompanied by prompt optical-UV emission with luminosity
BEAMING IN GAMMA-RAY BURSTS: EVIDENCE FOR A STANDARD ENERGY RESERVOIR
We present a comprehensive sample of all gamma-ray burst (GRB) afterglows with known distances, and we derive their conical opening angles based on observed broadband breaks in their light curves.
Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
We present the main results of a study of spectral and energetics properties of twelve gamma-ray bursts (GRBs) with redshift estimates. All GRBs in our sample were detected by BeppoSAX in a broad
Jet Breaks and Energetics of Swift Gamma-Ray Burst X-Ray Afterglows
We present a systematic temporal and spectral study of all Swift-X-ray Telescope observations of gamma-ray burst (GRB) afterglows discovered between 2005 January and 2007 December. After constructing
...
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3
4
5
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