Index: /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex
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--- /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex	(revision 6178)
+++ /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex	(revision 6179)
@@ -120,5 +120,7 @@
 Pilla R.P., Loeb A., ApJ, 494, L167, 1998.
 \bibitem{ZHANG1} High-Energy Spectral Components in Gamma-Ray Burst Afterglows,
-Zhang \& Meszaros, ApJ, 559, 110, 2001.
+Zhang B., Meszaros P., ApJ, 559, 110, 2001.
+\bibitem{RAZZAQUE} GeV and Higher Energy Photon Interactions in GRB Fireballs and Surroundings,
+Razzaque S., Meszaros P., Zhang B., ApJ, 613, 1072, 2004.
 \bibitem{TOTANI} Totani T., ApJ, 502, L13 (1998), 509 L81 (1998), 536, L23, 2000.
 \bibitem{WAXMAN} Waxman E., Phys. Rev. Lett. 75, 386, 1995.
@@ -131,5 +133,7 @@
 \bibitem{BELOBORODOV} Optical and GeV-TeV Flashes from GRBs, Beloborodov A., ApJ, 618, L13, 2005.
 \bibitem{EGRET} Hurley K. et al., Nature, 372, 652
-\bibitem{DINGUS} ESLAB29, Towards the Source of Gamma-Ray Bursts, Dingus, Ap\&SS, 231, 187, 1995.
+\bibitem{DINGUS1} Observations of the Highest Energy Gamma Rays from GRBs,
+Dingus B.L., AIP Conference Proceedings, 662, 240, 2003.
+\bibitem{DINGUS2} ESLAB29, Towards the Source of Gamma-Ray Bursts, Dingus, Ap\&SS, 231, 187, 1995.
 \bibitem{GONZALES} A GRB with high-energy Spectral Component Inconsistent with the Synchrotron Shock Model, Gonzales at al., Nature, 424, 749, 2003.
 \bibitem{AMENOMORI} Search for 10 TeV burst-like events coincident with the BATSE bursts
Index: /trunk/MagicSoft/GRB-Proposal/Introduction.tex
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--- /trunk/MagicSoft/GRB-Proposal/Introduction.tex	(revision 6178)
+++ /trunk/MagicSoft/GRB-Proposal/Introduction.tex	(revision 6179)
@@ -15,5 +15,5 @@
 Models based on both internal and external shocks predicts VHE fluence comparable to,
 or in certain situations stronger than, the keV-MeV radiation,
-with duration ranging from shorter than the keV-MeV burst to extended TeV afterglows~\cite{DERMER, PILLA, ZHANG1}.
+with duration ranging from shorter than the keV-MeV burst to extended TeV afterglows~\cite{DERMER, PILLA, ZHANG1, RAZZAQUE}.
 
 \par
@@ -35,6 +35,5 @@
 each indicating some excess over background but without stringent evidence.
 The only significant detection was performed by \eg which detected seven GRBs emitting high energy (HE)
-photons in the 100\,MeV to 18\,GeV range~\cite{EGRET}. The data shows no evidence of a HE cut-off
-in the GRB spectrum~\cite{DINGUS}. Recent results indicate that the spectrum of some GRBs contains a very hard, luminous, long-duration component~\cite{GONZALES}.
+photons in the 100\,MeV to 18\,GeV range~\cite{EGRET, DINGUS1}. The data shows no evidence of a HE cut-off in the GRB spectrum~\cite{DINGUS2}. Recent results indicate that the spectrum of some GRBs contains a very hard, luminous, long-duration component~\cite{GONZALES}.
 There have been results suggesting gamma rays beyond the GeV range from the TIBET air shower array
 in coincidence with BATSE bursts~\cite{AMENOMORI}, rapid follow-up observations by the