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Timestamp:
05/31/01 11:31:39 (23 years ago)
Author:
harald
Message:
....
File:
1 edited

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  • trunk/ICRC_01/mccontrib.tex

    r824 r825  
    1717\author[3]{H. Kornmayer}
    1818\affil[3]{Max-Planck-Institut f\"ur Physik, M\"unchen, Germany}
    19 \author[]{the MAGIC collaboration}
    2019
    2120\correspondence{O.Blanch blanch@ifae.es), H. Kornmayer (h.kornmayer@web.de)}
     
    3433
    3534\begin{abstract}
    36 For the understanding of a large Cherenkov telescope a detailed
     35For understanding the performance of the MAGIC telescope a detailed
    3736simulation of air showers and of the detector response are
    38 unavoidable. Such a simulation must take into account the development
    39 of air showers in the atmosphere, the reflectivity of the mirrors,
     37indispensable. Such a simulation must take into account the development
     38of the air showers in the atmosphere, the reflectivity of the mirrors,
    4039the response of photo detectors
    4140and the influence of both the light of night sky and the light of 
    4241bright stars.
    43 A detailed study will be presented.
     42A detailed study is presented.
    4443\end{abstract}
    4544
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