主要内容:
several, hours after the onset. High energy
精彩摘抄:
文章信息:
-
- · Full Printable Article (PDF/Postscript)
- · arXiv e-print (arXiv:0810.3639)
- · References in the Article
- · Also-Read Articles (Reads History)
- ·
- · Translate This Page
Title: |
| GRB observations with HESS |
Authors: |
| Tam, P. H.; Wagner, S. J.; Pühlhofer, G.; the HESS Collaboration |
Publication: |
| eprint arXiv:0810.3639 |
Publication Date: |
| 10/2008 |
Origin: |
| ARXIV |
Keywords: |
| Astrophysics |
Comment: |
| Proceeding of "Swift and GRBs: Unveiling the Relativistic Universe", held in Venice, 5-9 June 2006; Il Nuovo Cimento B, vol. 121 (2006), Issue 12, p.1595-1596; doi:10.1393/ncb/i2007-10322-x |
Bibliographic Code: |
| 2008arXiv0810.3639T |
Abstract
H.E.S.S. (High Energy Stereoscopic System), which is designed to detect TeV gamma-rays, is a system of four Imaging Atmospheric Cherenkov Telescopes situated in Namibia. The system has been shown to be very successful in detecting and observing galactic and extra-galactic TeV sources. In order to explore the highest energy end of GRB spectra, a GRB observing program has been established in the H.E.S.S. collaboration. Here we introduce our GRB observing program and report on its current status.
没有评论:
发表评论