# The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at $z =$ 0.1343

@article{Fong2016TheAA,
title={The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at \$z =\$ 0.1343},
author={Wen-fai Fong and Raffaella Margutti and Ryan Chornock and Edo Berger and Benjamin. J. Shappee and Andrew J. Levan and Nial R. Tanvir and Nathan Smith and Peter A. Milne and Tanmoy Laskar and Derek B. Fox and Ragnhild Lunnan and Peter K. Blanchard and Jens Hjorth and Klaas Wiersema and A. van der Horst and Dennis Zaritsky},
journal={The Astrophysical Journal},
year={2016},
volume={833},
pages={151}
}
• Published 30 August 2016
• Physics, Geology
• The Astrophysical Journal
NASA through Einstein Postdoctoral Fellowship [PF4-150121]; James Arthur Fellowship at NYU; NASA Swift grant [NNX16AB04G]; NSF [AST-1411763]; NASA ADA [NNX15AE50G]; NASA through Hubble Fellowship - Space Telescope Science Institute [HST-HF-51348.001]; NASA [NAS 5-26555]; [14A-344]; [13830]

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## References

SHOWING 1-10 OF 108 REFERENCES
GRB 060218/SN 2006aj: A Gamma-Ray Burst and Prompt Supernova at z = 0.0335
• Physics
• 2006
We report the imaging and spectroscopic localization of GRB 060218 to a low-metallicity dwarf starburst galaxy at z = 0.03345 ± 0.00006. In addition to making it the second nearest gamma-ray burst
A Putative Early-Type Host Galaxy for GRB 060502B: Implications for the Progenitors of Short-Duration Hard-Spectrum Bursts
• Physics
• 2007
Starting with the first detection of an afterglow from a short-duration hard-spectrum γ-ray burst (SHB) by Swift last year, a growing body of evidence has suggested that SHBs are associated with an
The Afterglow, Energetics, and Host Galaxy of the Short-Hard Gamma-Ray Burst 051221a
• Physics
• 2006
We present detailed optical, X-ray, and radio observations of the bright afterglow of the short gamma-ray burst 051221a obtained with Gemini, Swift XRT, and the Very Large Array, as well as optical
GRB 060505: A Possible Short-Duration Gamma-Ray Burst in a Star-forming Region at a Redshift of 0.09
• Physics
• 2007
On 2006 May 5, a 4 s duration, low-energy, ~1049 erg, gamma-ray burst (GRB) was observed, spatially associated with a z = 0.0894 galaxy. Here we report the discovery of the GRB optical afterglow and
GRB 090426: the environment of a rest-frame 0.35-s gamma-ray burst at a redshift of 2.609
• Physics
• 2010
We present the discovery of an absorption-line redshift of z = 2.609 for GRB 090426, establishing the first firm lower limit to a redshift for a gamma-ray burst (GRB) with an observed duration of 90
The afterglow of GRB 050709 and the nature of the short-hard γ-ray bursts
• Physics
Nature
• 2005
The final chapter in the long-standing mystery of the γ-ray bursts (GRBs) centres on the origin of the short-hard class of bursts, which are suspected on theoretical grounds to result from the
The afterglow and elliptical host galaxy of the short γ-ray burst GRB 050724
• Physics
Nature
• 2005
Despite a rich phenomenology, γ-ray bursts (GRBs) are divided into two classes based on their duration and spectral hardness—the long-soft and the short-hard bursts. The discovery of afterglow
GRB 120521C at z ~ 6 and the Properties of High-redshift γ-Ray Bursts
• Physics
• 2013
We present optical, near-infrared, and radio observations of the afterglow of GRB 120521C. By modeling the multi-wavelength data set, we derive a photometric redshift of z ≈ 6.0, which we confirm
A Short GRB "No-Host'' Problem? Investigating Large Progenitor Offsets for Short GRBs with Optical Afterglows
[abridged] We investigate the afterglow properties and large-scale environments of several short-duration gamma-ray bursts (GRBs) with sub-arcsecond optical afterglow positions but no bright
SHORT GRB 130603B: DISCOVERY OF A JET BREAK IN THE OPTICAL AND RADIO AFTERGLOWS, AND A MYSTERIOUS LATE-TIME X-RAY EXCESS
• Physics
• 2013
We present radio, optical/NIR, and X-ray observations of the afterglow of the short-duration Swift and Konus-Wind GRB 130603B, and uncover a break in the radio and optical bands at ≈0.5 day after the