Milagro search for VHE emission from GRBs in the Swift era

被引：0
|
作者：
Parkinson, P. M. Saz [1 ]
机构：
[1] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
来源：
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS | 2006年 / 121卷 / 12期
关键词：
D O I：
10.1393/ncb/i2007-10301-3
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Since its launch, in late 2004, Swift has been locating Gamma-Ray Bursts (GRBs) at a rate of similar to 100 per year. Very high energy (VHE) emission (> 100 GeV) is predicted by several models. Here, we present the results of a search for VHE emission from the most recent GRBs to fall within the Milagro field of view.
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页码：1573 / 1575
页数：3
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