Monitoring of high energy X-ray sources with the BeppoSAX GRBM

被引：0
|
作者：
Guidorzi, C [1 ]
Amati, L
Feroci, M
Costa, E
Frontera, F
Dal Fiume, D
Orlandini, M
机构：
[1] Univ Ferrara, Dipartmento Fis, I-44100 Ferrara, Italy
[2] CNR, Ist Astrofis Spaziale, Rome, Italy
[3] CNR, ITeSRE, I-40126 Bologna, Italy
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 69卷 / 1-3期
关键词：
D O I：
10.1016/S0920-5632(98)00309-0
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
The Gamma-Ray Burst Monitor (GRBM) aboard the BeppoSAX satellite has already shown good capabilities in the detection of Gamma-Ray Bursts (GRB). We have also tested its performance as monitor of the hard X-ray flux from strong celestial sources, using the Earth Occultation Technique. A verification of the on-ground calibrations of the instrument was performed deriving the flux of the Crab Nebula. In this paper we report results on Crab anti light curves of other sources detected.
引用
收藏
页码：664 / 667
页数：4
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