Index: /trunk/MagicSoft/GRB-Proposal/Introduction.tex
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--- /trunk/MagicSoft/GRB-Proposal/Introduction.tex	(revision 6274)
+++ /trunk/MagicSoft/GRB-Proposal/Introduction.tex	(revision 6275)
@@ -19,9 +19,10 @@
 \par
 
-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
+In many publications, the possibility has been explored that more energetic $\gamma$-rays come along with the
+(low-energy) GRB. Proton-synchrotron emission~\cite{TOTANI} have been suggested
 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 high energy (HE) $\gamma$-emission from accelerated protons in the forward-shock has been predicted in~\cite{LI}.
+Long-term high energy (HE) $\gamma$-emission from accelerated protons in the 
+forward-shock has been predicted in~\cite{LI}.
 This model predicts GeV inverse Compton emission even one day after the burst.
 Even considering pure electron-synchrotron radiation, measurable GeV-emission for a significant 
@@ -106,5 +107,3 @@
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