Index: /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex
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--- /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex	(revision 6814)
+++ /trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex	(revision 6815)
@@ -83,11 +83,11 @@
 %% Summary %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
 \begin{abstract}
-We ask for observations of Gamma-Ray Bursts (GRBs) for the next six months of year 2005.
-Therefore we present a detailed strategy for the observation of GRBs.
-X-Ray Flashes (XRFs) and Soft Gamma Repeaters (SGR)
-are also included in our proposal, given their similarities to GRB phenomena.
-All observations will be mainly triggered by \sw.
+We ask for observations of Gamma-Ray Bursts (GRBs) for the next six months of the year 2005.
+We present a detailed strategy for the observation of GRBs, X-Ray Flashes (XRFs) and 
+Soft Gamma Repeaters (SGR)
+(which are included in our proposal, given their similarities to GRB phenomena).
+The observations will be mainly triggered by \sw.
 In addition, the \he and \ig satellites can contribute a small number of alerts.
-The \sw collaboration expects a total alert rate of about 15 per months --
+The \sw collaboration expects a total alert rate of about 15 per month --
 although with big uncertainties -- out of which 1--2 should be
 observable by \ma due to our