Journal
ASTROPHYSICAL JOURNAL
Volume 690, Issue 2, Pages 1068-1073Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/690/2/1068
Keywords
gamma rays: bursts; gamma rays: observations
Categories
Funding
- German Ministry for Education and Research ( BMBF)
- Max Planck Society
- French Ministry for Research
- CNRS-IN2P3
- CNRSCharles University
- UK Science and Technology Facilities Council (STFC
- Polish Ministry of Science and Higher Education
- South African Department of Science and Technology
- National Research Foundation
- University of Namibia
- SFB [439]
- IMPRS-HD
- STFC [PP/E001319/1, ST/F002963/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/F002963/1, PP/E001319/1] Funding Source: researchfish
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We report on the first completely simultaneous observation of a gamma-ray burst (GRB) using an array of Imaging Atmospheric Cherenkov Telescopes, which is sensitive to photons in the very high energy (VHE) gamma-ray range (greater than or similar to 100 GeV). On 2006 June 2, the Swift Burst Alert Telescope (BAT) registered an unusually soft gamma-ray burst (GRB 060602B). The burst position was under observation using the High Energy Stereoscopic System (HESS) at the time the burst occurred. Data were taken before, during, and after the burst. A total of 5 hr of observations were obtained during the night of 2006 June 2-3, and five additional hours were obtained over the next three nights. No VHE gamma-ray signal was found during the period covered by the HESS observations. The 99% confidence level flux upper limit (> 1 TeV) for the prompt phase (9 s) of GRB 060602B is 2.9 x 10(-9) erg cm(-2) s(-1). Due to the very soft BAT spectrum of the burst compared with other Swift GRBs and its proximity to the Galactic center, the burst is likely associated with a Galactic X-ray burster, although the possibility of it being a cosmological GRB cannot be ruled out. We discuss the implications of our flux limits in the context of these two bursting scenarios.
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