Characteristics of the multi-telescope coincidence trigger of the HEGRA IACT system

被引:31
作者
Bulian, N
Daum, A
Hermann, G
Hess, M
Hofmann, W
Lampeitl, H
Puhlhofer, G
Kohler, C
Panter, M
Stein, M
Borst, G
Rauterberg, G
Samorski, M
Sauerland, C
Stamm, W
机构
[1] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany
[2] Univ Kiel, Inst Kernphys, D-24118 Kiel, Germany
关键词
D O I
10.1016/S0927-6505(98)00003-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The HEGRA-collaboration is operating a system of imaging atmospheric Cherenkov telescopes to search for sources of TeV-gamma-rays. Air showers are observed in stereoscopic mode with several telescopes simultaneously. To trigger the telescope system a versatile two-level trigger scheme has been implemented, which allows a significant reduction of the energy threshold with respect to single telescopes. The technical implementation of this trigger scheme and the performance of the trigger system are described. Results include the dependence of single- and multi-telescope trigger rates on the trigger thresholds, on the orientation of the telescopes, and on the type of the primary particle. (C) 1998 Elsevier Science B.V.
引用
收藏
页码:223 / 233
页数:11
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