Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/56494
Citations | ||
Scopus | Web of Science® | Altmetric |
---|---|---|
?
|
?
|
Type: | Journal article |
Title: | HESS observations of the prompt and afterglow phases of GRB 060602B |
Author: | Aharonian, F. Akhperjanian, A. Barres de Almaida, U. Bazer-Bachi, A. Behera, B. Beilicke, M. Benbow, W. Bernlohr, K. Boisson, C. Borrel, V. Braun, I. Brion, E. Brucker, J. Buhler, R. Bulik, T. Busching, I. Boutelier, T. Carrigan, S. Chadwick, P. Chaves, R. et al. |
Citation: | The Astrophysical Journal: an international review of astronomy and astronomical physics, 2009; 690(2):1068-1073 |
Publisher: | Univ Chicago Press |
Issue Date: | 2009 |
ISSN: | 0004-637X 1538-4357 |
Statement of Responsibility: | F. Aharonian... G. Rowell... et al. |
Abstract: | 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) γ-ray range ( 100 GeV). On 2006 June 2, the Swift Burst Alert Telescope (BAT) registered an unusually soft γ-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 γ-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 × 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. |
Keywords: | gamma rays: bursts gamma rays: observations |
DOI: | 10.1088/0004-637X/690/2/1068 |
Published version: | http://dx.doi.org/10.1088/0004-637x/690/2/1068 |
Appears in Collections: | Aurora harvest 5 Physics publications |
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.