A Strong Limit on the Very-high-energy Emission from GRB 150323A
- Univ. of Utah, Salt Lake City, UT (United States)
- Washington Univ., St. Louis, MO (United States)
- Harvard Smithsonian Ctr for Astophysics, Amado, Arizona (United States)
- Univ. of California, Los Angeles, CA (United States)
- Univ. of Potsdam (Germany)
- National Univ. of Ireland Galway (Ireland)
- Purdue Univ., West Lafayette, IN (United States)
On 2015 March 23, the Very Energetic Radiation Imaging Telescope Array System (VERITAS) responded to a Swift-Burst Alert Telescope (BAT) detection of a gamma-ray burst, with observations beginning 270 s after the onset of BAT emission, and only 135 s after the main BAT emission peak. No statistically significant signal is detected above 140 GeV. The VERITAS upper limit on the fluence in a 40-minute integration corresponds to about 1% of the prompt fluence. Our limit is particularly significant because the very-high-energy (VHE) observation started only ~2 minutes after the prompt emission peaked, and Fermi-Large Area Telescope observations of numerous other bursts have revealed that the high-energy emission is typically delayed relative to the prompt radiation and lasts significantly longer. Also, the proximity of GRB 150323A (z = 0.593) limits the attenuation by the extragalactic background light to ~50% at 100–200 GeV. We conclude that GRB 150323A had an intrinsically very weak high-energy afterglow, or that the GeV spectrum had a turnover below ~100 GeV. If the GRB exploded into the stellar wind of a massive progenitor, the VHE non-detection constrains the wind density parameter to be A ≳ 3 × 1011 g cm-1, consistent with a standard Wolf–Rayet progenitor. Alternatively, the VHE emission from the blast wave would be weak in a very tenuous medium such as the interstellar medium, which therefore cannot be ruled out as the environment of GRB 150323A.
- Research Organization:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Organization:
- USDOE
- Contributing Organization:
- VERITAS Collaboration
- OSTI ID:
- 1544054
- Journal Information:
- The Astrophysical Journal (Online), Vol. 857, Issue 1; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
Teraelectronvolt emission from the γ-ray burst GRB 190114C
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text | January 2019 |
Synchrotron Self-Compton as a Likely Mechanism of Photons beyond the Synchrotron Limit in GRB 190114C
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journal | October 2019 |
Teraelectronvolt emission from the γ-ray burst GRB 190114C
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journal | November 2019 |
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