Index: /trunk/MagicSoft/GC-Proposal/GC.tex
===================================================================
--- /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6832)
+++ /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6833)
@@ -32,5 +32,6 @@
 Key Programs: Galactic Center / Dark Matter
 }
-\author{H. Bartko, A. Biland, S. Commichau, P. Flix, S. Stark, W. Wittek}
+\author{H. Bartko, A. Biland, E. Bisesi, S. Commichau, P. Flix,\\
+ S. Stark, W. Wittek}
 \date{March 21, 2005\\}
 \TDAScode{}%MAGIC 05-xx\\ 04mmdd/HBartko
@@ -56,5 +57,5 @@
 the annihilation of SUSY-neutralino dark matter (DM) particles, other models 
 like Kaluza-Klein dark matter are not ruled out. Moreover, assuming a 
-universal DM density profile, the GC is expected to yield the largest DM flux 
+universal DM density profile, the GC is expected to yield the largest gamma flux from particle DM annihilation 
 amongst the favored candidates, due to its proximity.
 
@@ -183,4 +184,5 @@
    Hendrik Bartko      & MPI Munich    & hbartko@mppmu.mpg.de & data analysis, spectra, wobble mode
 \\ Adrian Biland       & ETH Zurich    & biland@particle.phys.ethz.ch & OFF pointing, Moon observations
+\\ Erica Bisesi	       & Univ. Udine   & bisesi@fisica.uniud.it & dark matter halo modelling, clumpness
 \\ Sebastian Commichau & ETH Zurich    & commichau@particle.phys.ethz.ch &
  data analysis, MC generation, spectra