Index: /trunk/MagicSoft/GC-Proposal/Changelog
===================================================================
--- /trunk/MagicSoft/GC-Proposal/Changelog	(revision 6867)
+++ /trunk/MagicSoft/GC-Proposal/Changelog	(revision 6868)
@@ -1,2 +1,6 @@
+2005/03/21 Hendrik
+* GC.tex
+  added Mose and Villi as investigators
+
 2005/03/20 Hendrik
 * further corrections
Index: /trunk/MagicSoft/GC-Proposal/GC.tex
===================================================================
--- /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6867)
+++ /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6868)
@@ -33,5 +33,5 @@
 }
 \author{H. Bartko, A. Biland, E. Bisesi, S. Commichau, P. Flix,\\
- S. Stark, W. Wittek}
+M. Mariotti, V. Scalzotto, S. Stark, W. Wittek}
 \date{March 21, 2005\\}
 \TDAScode{}%MAGIC 05-xx\\ 04mmdd/HBartko
@@ -188,4 +188,6 @@
  data analysis, spectra, geomagnetic effects
 \\ Pepe Flix           & IFAE Barcelona& jflix@ifae.es & data analysis, disp, spectra, dark matter
+\\ Mose Mariotti       & INFN Padua   & mose.mariotti@pd.infn.it & disp, dark matter
+\\ Villi Scalzotto     & INFN Padua   & scalzotto@pd.infn.it & data analysis, disp
 \\ Sabrina Stark       & ETH Zurich    & lstark@particle.phys.ethz.ch  & data analysis, spectra
 \\ Wolfgang Wittek     & MPI Munich    & wittek@mppmu.mpg.de & padding, unfolding, disp
@@ -510,5 +512,5 @@
 The bigger circle in the center of Fig. \ref{fig:GC_starfield_OFF1}
 indicates the ON region around the GC. 
-An appropriate OFF region, with a sky field similar to that of the ON region,  would be the one marked by the bigger circle in the upper left part of Fig.\ref{fig:GC_starfield_OFF1} . Like the ON region, the OFF region is centered at the Galactic Plane and contains the bright star Sgr 3 (at (RA, dec) = $(17^h47^m34^s,\;-27^{\circ}49'51"$) ) in its outer part. The center of the OFF region has the coordinates GC$_{OFF}$ = (RA, dec) = $(17^h51^m12^s,\;-26^{\circ}52'00")$. The difference in RA between the GC and GC$_{OFF}$ corresponds is 6 minutes. Thus GC$_{OFF}$ culminates 6 minutes later than the GC.
+An appropriate OFF region, with a sky field similar to that of the ON region,  would be the one marked by the bigger circle in the upper left part of Fig.\ref{fig:GC_starfield_OFF1} . Like the ON region, the OFF region is centered at the Galactic Plane and contains the bright star Sgr 3 (at (RA, dec) = $(17^h47^m34^s,\;-27^{\circ}49'51"$) ) in its outer part. The center of the OFF region has the coordinates GC$_{\mathrm{OFF}}$ = (RA, dec) = $(17^h51^m12^s,\;-26^{\circ}52'00")$. The difference in RA between the GC and GC$_{\mathrm{OFF}}$ corresponds is 6 minutes. Thus GC$_{\mathrm{OFF}}$ culminates 6 minutes later than the GC.
 
 %In order to have the most appropriate OFF data we propose to