- Timestamp:
- 05/31/01 11:31:39 (23 years ago)
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trunk/ICRC_01/mccontrib.tex
r824 r825 17 17 \author[3]{H. Kornmayer} 18 18 \affil[3]{Max-Planck-Institut f\"ur Physik, M\"unchen, Germany} 19 \author[]{the MAGIC collaboration}20 19 21 20 \correspondence{O.Blanch blanch@ifae.es), H. Kornmayer (h.kornmayer@web.de)} … … 34 33 35 34 \begin{abstract} 36 For the understanding of a large Cherenkovtelescope a detailed35 For understanding the performance of the MAGIC telescope a detailed 37 36 simulation of air showers and of the detector response are 38 unavoidable. Such a simulation must take into account the development39 of air showers in the atmosphere, the reflectivity of the mirrors,37 indispensable. Such a simulation must take into account the development 38 of the air showers in the atmosphere, the reflectivity of the mirrors, 40 39 the response of photo detectors 41 40 and the influence of both the light of night sky and the light of 42 41 bright stars. 43 A detailed study will bepresented.42 A detailed study is presented. 44 43 \end{abstract} 45 44
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