The influence of imaging camera characteristics on the measured parameters of Cerenkov flashes

被引：9

作者：

Kornienko, A. P. ^{[1
]}

Stepanian, A. A. ^{[1
]}

Zyskin, Yu. L. ^{[1
]}

机构：

[1] Crimean Astrophys Observ, Nauchnyi, Crimea, Ukraine

来源：

ASTROPARTICLE PHYSICS | 1993年 / 1卷 / 02期

关键词：

D O I：

10.1016/0927-6505(93)90025-9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Monte Carlo simulation of the detection of Cerenkov flashes using a multichannel image camera (MIC) of a VHE gamma telescope were carried out. It is shown that convential data processing techniques are not optimal. The flash dimension, location and orientation errors were estimated. The error budget of the influence of the limited field of view of the detector and the night sky emission is assessed. The optimal method of observational data processing of Cerenkov flashes obtained by MIC is proposed.

引用

页码：245 / 254

页数：10

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