H.E.S.S. 高能伽马射线观测
天体物理学
2007-05-23 v1
摘要
H.E.S.S.成像大气厄尔塞克望远镜阵列目前是能探测0.1-10 TeV能量范围内高能伽马射线观测最灵敏的仪器。在完整四望远镜阵列运行超过两年后，已发现许多银河系和外银河系高能伽马射线源。凭借其卓越的灵敏度和大视场角相机，H.E.S.S.特别适合进行星图测绘和对扩展源的详细研究。本稿演示了近期H.E.S.S.结果的精选汇报。
引用
@article{arxiv.astro-ph/0606486,
title = {Very High Energy Gamma-Ray Observations with H.E.S.S},
author = {Christopher van Eldik},
journal= {arXiv preprint arXiv:astro-ph/0606486},
year = {2007}
}
备注
8 pages, 4 figures, to appear in the proceedings of the 41st Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 11-18 March 2006