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GRB 130427A is the brightest gamma-ray burst observed by any satellite in almost 30 years and one of the most thoroughly observed. I will present a summary of the worldwide campaign to monitor the afterglow of this event from GHz to TeV energies and from seconds to years after the explosio...
We present one of the best sampled early time light curves of a gamma-ray burst (GRB) at radio wavelengths. Using the Arcminute Mircrokelvin Imager (AMI) we observed GRB 130427A at the central frequency of 15.7 GHz between 0.36 and 59.32 days post-burst.
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et al. NuSTAR observations of GRB 130427A establish a single component synchrotron afterglow origin for the late optical to multi-GeV emission. Astrophys. J. Lett. 779, L1 (2013). ADS Google Scholar Amati, L. et al. Intrinsic spectra and energetics of BeppoSAX gamma-ray bursts with known...
Using the Arcminute Mircrokelvin Imager (AMI), we observed GRB 130427A at the central frequency of 15.7GHz between 0.36 and 59.32d post-burst. These results yield one of the earliest radio detections of a GRB and demonstrate a clear rise in flux less than one day after the γ-ray ...
We present one of the best sampled early time light curves of a gamma-ray burst (GRB) at radio wavelengths. Using the Arcminute Mircrokelvin Imager (AMI) we observed GRB 130427A at the central frequency of 15.7 GHz between 0.36 and 59.32 days post-burst. These results yield one of the ...
Fermi-LAT Observations of the Gamma-Ray Burst GRB 130427A The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide c... - 《Science》 被引量: 85发表: 0年 Fermi-LAT Observations of the Gamma-...
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 ... D Perley,S Cenko,A Corsi,... - 《Astrophysical Journal》 被引量: 57发表...
Probing the bright radio flare and afterglow of GRB 130427A with the Arcminute Microkelvin Imager. Mon. Not. R. Astron. Soc. 2014, 440, 2059–2065. [Google Scholar] [CrossRef] [Green Version] Singer, L.P.; Kasliwal, M.M.; Cenko, S.B.; Perley, D.A.; Anderson, G.E.; Anupam...