Index: trunk/MagicSoft/GRB-Proposal/Strategies.tex
===================================================================
--- trunk/MagicSoft/GRB-Proposal/Strategies.tex	(revision 6164)
+++ trunk/MagicSoft/GRB-Proposal/Strategies.tex	(revision 6165)
@@ -25,6 +25,5 @@
 The duty-cycle in~\cite{NICOLA} will be increased by taking into account that \ma should also observe the afterglow emission of an burst that occured up to 5 hours before the start of the shift. Different GRB models predict delayed prompt GeV emission as well as acceleration of photons during the afterglows up to the threshold energy of \ma (for more details see chapter 5).
 
-The afterglow observation is equivalent to an increase of the duty-cycle of about 6 days per month.\\
-
+The afterglow observation is equivalent to an increase of the duty-cycle of about 6 days per month.
 
 \subsection{GRB observations in case of moon shine}
@@ -57,5 +56,5 @@
 \subsection{Active Mirror Control behaviour}
 
-To reduce the time before starting of the observation, the use of the look-up tables (LUTs) is necessary.
+To reduce the time before starting the observation, the use of the look-up tables (LUTs) is necessary.
 Once generated, the {\it AMC} will use the LUTs and automaticaly focus the panels for a given telescope position. The {\it CC} should send the burst coordinates to the {\it Drive} and the {\it AMC} software in the same time. In this way the panels could be focussed already during the telescope movement.
 
@@ -111,5 +110,5 @@
 
 \begin{itemize}
-\item In case of a repeated outbursts for a longer time period of direct observation
-\item In the other case for having Off-data at exactly the same sky location.
+\item In case of a repeated outbursts for a longer time period of direct observation.
+\item In the other case for having off-data at exactly the same sky location.
 \end{itemize}