FERMI时代新一代成像大气切伦科夫望远镜的伽马射线暴观测
Gamma-ray burst observations with new generation imaging atmospheric Cerenkov Telescopes in the FERMI era
摘要：
在FERMI卫星发射并成功开始运行之后，与伽马射线暴的高能观测有关的议题得到了科学界的极大关注。毫无疑问，高能观测在限制发射过程和伽马射线暴的物理条件方面的诊断能力是相关的。我们简要地讨论了如何伽马射线暴观测与地面成像阵列切伦科夫望远镜，在GeV-TeV的范围内，可以竞争和合作的费米观测，在MeV-GeV的范围内，让研究人员获得更详细和完整的图片的提示和余辉阶段的伽马射线暴。
英文摘要：
After the launch and successful beginning of operations of the FERMI satellite, the topics related to high-energy observations of gamma-ray bursts have obtained a considerable attention by the scientific community. Undoubtedly, the diagnostic power of high-energy observations in constraining the emission processes and the physical conditions of gamma-ray burst is relevant. We briefly discuss how gamma-ray burst observations with ground-based imaging array Cerenkov telescopes, in the GeV-TeV range, can compete and cooperate with FERMI observations, in the MeV-GeV range, to allow researchers to obtain a more detailed and complete picture of the prompt and afterglow phases of gamma-ray bursts.
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