Index: /trunk/ICRC_01/mccontrib.tex
===================================================================
--- /trunk/ICRC_01/mccontrib.tex	(revision 824)
+++ /trunk/ICRC_01/mccontrib.tex	(revision 825)
@@ -17,5 +17,4 @@
 \author[3]{H. Kornmayer}
 \affil[3]{Max-Planck-Institut f\"ur Physik, M\"unchen, Germany}
-\author[]{the MAGIC collaboration}
 
 \correspondence{O.Blanch blanch@ifae.es), H. Kornmayer (h.kornmayer@web.de)}
@@ -34,12 +33,12 @@
 
 \begin{abstract}
-For the understanding of a large Cherenkov telescope a detailed 
+For understanding the performance of the MAGIC telescope a detailed 
 simulation of air showers and of the detector response are
-unavoidable. Such a simulation must take into account the development
-of air showers in the atmosphere, the reflectivity of the mirrors, 
+indispensable. Such a simulation must take into account the development
+of the air showers in the atmosphere, the reflectivity of the mirrors, 
 the response of photo detectors 
 and the influence of both the light of night sky and the light of  
 bright stars. 
-A detailed study will be presented. 
+A detailed study is presented. 
 \end{abstract}