Changeset 6833

Timestamp:

03/16/05 14:54:59 (20 years ago)

Author:

hbartko

Message:

*** empty log message ***

File:

• trunk/MagicSoft/GC-Proposal/GC.tex (modified) (3 diffs)

trunk/MagicSoft/GC-Proposal/GC.tex

@@ -32 +32 @@
 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 +57 @@
 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 +184 @@
    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