Index: /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex
===================================================================
--- /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex	(revision 6223)
+++ /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex	(revision 6224)
@@ -133,5 +133,6 @@
 \bibitem{WAXMAN} Cosmological Gamma-Ray Bursts and the Highest Energy Cosmics Rays, 
 Waxman E., Phys. Rev. Lett. 75, 386, 1995.
-\bibitem{BOETTCHER} Boettcher M, Dermer C.D., Astrophys. J. 499 L131, 1998.
+\bibitem{BOETTCHER} High-energy Gamma-Rays from Ultra-high-energy Protons in Gamma-Ray Bursts, 
+Boettcher M, Dermer C.D., Astrophys. J. 499 L131, 1998.
 \bibitem{MESZAROS93} Meszaros P., Rees M., Astrophys. J. 418 L59, 1993.
 \bibitem{CHIANG} Chiang J., Dermer C.D., Astrophys. J. 512 699, 1999.
Index: /trunk/MagicSoft/GRB-Proposal/Introduction.tex
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--- /trunk/MagicSoft/GRB-Proposal/Introduction.tex	(revision 6223)
+++ /trunk/MagicSoft/GRB-Proposal/Introduction.tex	(revision 6224)
@@ -21,5 +21,5 @@
 In many publications, the possibility that more energetic $\gamma$-rays come along with the
 (low-energy) GRB, have been explored. Proton-synchrotron emission~\cite{TOTANI} have been suggested
-as well as photon-pion production~\cite{WAXMAN,BAHCALL,BOETTCHER} and inverse-Compton scattering
+as well as photon-pion production~\cite{WAXMAN,BOETTCHER} and inverse-Compton scattering
 in the burst environment~\cite{MESZAROS93,CHIANG,PILLA,ZHANG2,BELOBORODOV}.
 Long-term HE $\gamma$-emission from accelerated protons in the forward-shock has been predicted in~\cite{LI}. 
@@ -74,5 +74,6 @@
 Alternatively, an increase of the baryon load within the fireball itself or low efficiency shocks could 
 produce XRFs.
-If there is a connection between XRFs and GRBs, they should originate at rather low redshifts (z $<$ 0.6).\\
+If there is a connection between XRFs and GRBs, 
+they should originate at rather low redshifts (z $<$ 0.6).\\
 
 Gamma-ray satellites react in the same way to XRFs and GRBs.