Changeset 6179 for trunk/MagicSoft/GRB-Proposal/Introduction.tex

Timestamp:

02/01/05 17:20:21 (20 years ago)

Author:

garcz

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• trunk/MagicSoft/GRB-Proposal/Introduction.tex (modified) (2 diffs)

trunk/MagicSoft/GRB-Proposal/Introduction.tex

@@ -15 +15 @@
 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 +35 @@
 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