Gamma-ray astrophysics with AGILE

被引：1
|
作者：
Tavani, M [1 ]
机构：
[1] Ist Astrofis Spaziale & Fis Spaziale, IASF, Sez Roma, I-00133 Rome, Italy
来源：
TEXAS IN TUSCANY | 2003年
关键词：
D O I：
10.1142/9789812704009_0017
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Gamma-ray astrophysics above 30 MeV will soon be revitalized by a new generation of high-energy detectors in space. We discuss here the AGILE Mission that will be dedicated to gamma-ray astrophysics above 30 MeV during the period 2005-2006. The main characteristics of AGILE are: (1) excellent imaging and monitoring capabilities both in the gamma-ray (30 MeV - 30 GeV) and hard X-ray (1040 keV) energy ranges (reaching an arcminute source positioning), (2) very good timing (improving by three orders of magnitude the instrumental deadtime for gamma-ray detection compared to previous instruments), and (3) excellent imaging and triggering capability for Gamma-Ray Bursts. The AGILE scientific program will emphasize a quick response to gamma-ray transients and multiwavelength studies of gamma-ray sources.
引用
收藏
页码：183 / 196
页数：14
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