Covino 2009 地面Cerenkov 望远镜如何与Fermi配合

主要内容:


精彩摘抄:


文章信息:

· Find Similar Abstracts (with default settings below)

· arXiv e-print (arXiv:0901.1589)

· References in the Article

·

· Translate This Page

Title:		Gamma-ray burst observations with new generation imaging atmospheric Cerenkov Telescopes in the FERMI era
Authors:		Covino, S.; Garczarczyk, M.; Galante, N.; Gaug, M.; Antonelli, A.; Bastieri, D.; Campana, S.; Longo, F.; Scapin, V.
Publication:		eprint arXiv:0901.1589
Publication Date:		01/2009
Origin:		ARXIV
Keywords:		Astrophysics
Comment:		9 pages, two figures. Proceeding for the 6th "Science with the New Generation of High Energy Gamma-Ray Experiments" workshop
Bibliographic Code:		2009arXiv0901.1589C

Abstract

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.

---

Bibtex entry for this abstract Preferred format for this abstract (see Preferences)