Index: trunk/MagicSoft/GC-Proposal/GC.tex
===================================================================
--- trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6781)
+++ trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6782)
@@ -118,5 +118,5 @@
  \hline
  (RA, dec), epoch J2000.0 & $(17^h45^m12^s,-29.01$ deg)
-\\ heliocentric distance  & $8\pm0.4$ kpc \cite{Eisenhauer2003, ApJ 597(2003)L121} 
+\\ heliocentric distance  & $8\pm0.4$ kpc \cite{Eisenhauer2003} 
 (1 deg = 140 pc)
 \\ mass of the black hole & $2\pm0.5 \cdot 10^6 M_{\odot}$ 
@@ -143,5 +143,5 @@
 is very large $~2.2 \cdot 10^{37} \mathrm{erg}/\mathrm{s}$, which is 
 equivalent to about 10 Crab pulsars. An independent analysis of the EGRET data 
-\cite{Hooper2002, A&A 335 (1998) 161} indicates a point source whose position is different from the GC at a confidence level beyond 99.9 \%.
+\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} 
 
 Up to now, the GC has been observed at 
Index: trunk/MagicSoft/GC-Proposal/bibbib.bib
===================================================================
--- trunk/MagicSoft/GC-Proposal/bibbib.bib	(revision 6781)
+++ trunk/MagicSoft/GC-Proposal/bibbib.bib	(revision 6782)
@@ -1,2 +1,25 @@
+@ARTICLE{Hooper2002,
+author = {Hooper},
+journal = "A\&A",
+volume = "335",
+year =  1998,
+pages = {161}
+}
+
+
+@ARTICLE{Eisenhauer2003,
+   author = {{Eisenhauer}, F. and {Sch{\" o}del}, R. and {Genzel}, R. and 
+	{Ott}, T. and {Tecza}, M. and {Abuter}, R. and {Eckart}, A. and 
+	{Alexander}, T.},
+    title = "{A Geometric Determination of the Distance to the Galactic Center}",
+  journal = "ApJ",
+     year = 2003,
+    month = nov,
+   volume = 597,
+    pages = {L121-L124},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ApJ...597L.121E&db_key=AST},
+  adsnote = {Provided by the NASA Astrophysics Data System}
+}
+
 @ARTICLE{Fatuzzo2003,
    author = {{Fatuzzo}, M. and {Melia}, F.},
