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Halobacterium sp. GRB

Known as: Halobacterium GRB, Halobacterium sp. (strain GRB) 
National Institutes of Health

Papers overview

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2014
2014
A Trio of GRB-SNe : GRB 120729 A , GRB 130215 A / SN 2013 ez and GRB 130831 A / SN 2013 fu
We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A… 
Review
2014
Review
2014
THE FIRST GAMMA-RAY BURSTS IN THE UNIVERSE
Gamma-ray bursts (GRBs) are the ultimate cosmic lighthouses, capable of illuminating the universe at its earliest epochs. Could… 
2014
2014
GRB 130427A AND SN 2013cq: A MULTI-WAVELENGTH ANALYSIS OF AN INDUCED GRAVITATIONAL COLLAPSE EVENT
We performed a data analysis of the observations by the Swift, NuStar, and Fermi satellites in order to probe the induced… 
2014
2014
GRB 140515A at z=6.33: Constraints on the End of Reionization From a Gamma-ray Burst in a Low Hydrogen Column Density Environment
We present the discovery and subsequent spectroscopy with Gemini-North of the optical afterglow of the Swift gamma-ray burst (GRB… 
2014
2014
Light Curve Properties of Supernovae Associated With Gamma-ray Bursts
Little is known about the diversity in the light curves of GRB-SNe, including whether the light curve of SN 1998bw can be used as… 
2013
2013
GRB 110709B in the induced gravitational collapse paradigm
Context. Gamma-ray burst (GRB) 110709B is the first source for which Swift-BAT was triggered twice, with a time separation of ∼10… 
2011
2011
On the nature of GRB 050509b: a disguised short GRB
(shortened) Context: GRB GRB 050509b, detected by the \emph{Swift} satellite, is the first case where an X-ray afterglow has been… 
2010
2010
THE Ep–FLUX CORRELATION IN THE RISING AND DECAYING PHASES OF GAMMA-RAY BURST PULSES: EVIDENCE FOR VIEWING ANGLE EFFECT?
A time-resolved spectral analysis for a sample of 22 intense, broad gamma-ray burst (GRB) pulses from the Compton Gamma Ray… 
2004
2004
High-Energy Photon Emission in the Early Afterglow of GRBs
We consider the emission within the fireball model framework of very high energy, ~1 GeV to >1 TeV photons, on a minute timescale… 
Review
2002
Review
2002
Cosmological Microlensing Statistics: Variability Rates for Quasars and Gamma-Ray Burst Afterglows and Implications for Macrolensing Magnification Bias and Flux Ratios
The fraction of quasars and gamma-ray burst (GRB) afterglows that vary because of microlensing by the stellar populations of… 
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