Index: /trunk/MagicSoft/GC-Proposal/Changelog
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--- /trunk/MagicSoft/GC-Proposal/Changelog	(revision 6863)
+++ /trunk/MagicSoft/GC-Proposal/Changelog	(revision 6864)
@@ -1,2 +1,5 @@
+2005/03/20 Hendrik
+* further corrections
+
 2005/03/20 Sebastian
 * Made some small corrections
Index: /trunk/MagicSoft/GC-Proposal/GC.tex
===================================================================
--- /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6863)
+++ /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6864)
@@ -140,5 +140,5 @@
 \cite{Hooper2002} indicates a point source whose position is different from the GC at a confidence level beyond 99.9 \%. %\cite{Hooper2002, A&A 335 (1998) 161} 
 
-At energies above 200 GeV, the GC has been observed by Veritas, Cangaroo and HESS, \cite{GC_whipple,
+At energies above 200 GeV, the GC has been observed by Veritas, Cangaroo and HESS \cite{GC_whipple,
 GC_cangaroo,GC_hess}. The spectra as measured by these experiments are displayed in Figure \ref{fig:GC_gamma_flux} while Figure \ref{fig:GC_source_location} shows the 
 different reconstructed positions of the GC source. Recently a second TeV