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| 001 | 187276 | ||
| 005 | 20250730144750.0 | ||
| 024 | 7 | _ | |a 10.1088/2041-8205/795/1/L3 |2 doi |
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| 024 | 7 | _ | |a arXiv:1410.5367 |2 arXiv |
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| 024 | 7 | _ | |a 10.3204/PUBDB-2014-03844 |2 datacite_doi |
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| 088 | 1 | _ | |a arXiv:1410.5367 |
| 088 | _ | _ | |a arXiv:1410.5367 |2 arXiv |
| 100 | 1 | _ | |a Aliu, E. |0 P:(DE-HGF)0 |b 0 |
| 245 | _ | _ | |a Constraints on very High Energy Emission from GRB 130427A |
| 260 | _ | _ | |a London |c 2014 |b Institute of Physics Publ. |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 500 | _ | _ | |a © The American Astronomical Society |
| 520 | _ | _ | |a Prompt emission from the very fluent and nearby (z = 0.34) gamma-ray burst GRB 130427A was detected by several orbiting telescopes and by ground-based, wide-field-of-view optical transient monitors. Apart from the intensity and proximity of this GRB, it is exceptional due to the extremely long-lived high-energy (100 MeV to 100 GeV) gamma-ray emission, which was detected by the Large Area Telescope on the Fermi Gamma-Ray Space Telescope for ~70 ks after the initial burst. The persistent, hard-spectrum, high-energy emission suggests that the highest-energy gamma rays may have been produced via synchrotron self-Compton processes though there is also evidence that the high-energy emission may instead be an extension of the synchrotron spectrum. VERITAS, a ground-based imaging atmospheric Cherenkov telescope array, began follow-up observations of GRB 130427A ~71 ks (~20 hr) after the onset of the burst. The GRB was not detected with VERITAS; however, the high elevation of the observations, coupled with the low redshift of the GRB, make VERITAS a very sensitive probe of the emission from GRB 130427A for E > 100 GeV. The non-detection and consequent upper limit derived place constraints on the synchrotron self-Compton model of high-energy gamma-ray emission from this burst. |
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| 700 | 1 | _ | |a Aune, T. |0 P:(DE-HGF)0 |b 1 |e Corresponding author |
| 700 | 1 | _ | |a Barnacka, A. |0 P:(DE-HGF)0 |b 2 |
| 700 | 1 | _ | |a Beilicke, M. |0 P:(DE-HGF)0 |b 3 |
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| 700 | 1 | _ | |a Buckley, J. H. |0 P:(DE-HGF)0 |b 7 |
| 700 | 1 | _ | |a Bugaev, V. |0 P:(DE-HGF)0 |b 8 |
| 700 | 1 | _ | |a Byrum, K. |0 P:(DE-HGF)0 |b 9 |
| 700 | 1 | _ | |a Cardenzana, J. V |0 P:(DE-HGF)0 |b 10 |
| 700 | 1 | _ | |a Cerruti, M. |0 P:(DE-HGF)0 |b 11 |
| 700 | 1 | _ | |a Chen, Xuhui |0 P:(DE-H253)PIP1018140 |b 12 |
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