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%%%  Kopyleft (K) 2000 J C Gonzalez
%%%  Max-Planck-Institut fuer Physik, 
%%%  Foehringer Ring 6, 80805 Muenchen, Germany
%%%  E-mail: gonzalez@mppmu.mpg.de
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\documentclass[12pt]{article}

\usepackage{magic-tdas}
\usepackage{xspace}
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\newcommand{\ig}{INTEGRAL\xspace}
\newcommand{\sw}{SWIFT\xspace}
\newcommand{\eg}{EGRET\xspace}
\newcommand{\ba}{BATSE\xspace}
\newcommand{\ma}{MAGIC\xspace}
\newcommand{\ip}{IPN\xspace}
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\begin{document}

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\title{Proposal for the Observation of Gamma-Ray Bursts with the MAGIC Telescope \\
     {\it \Large DRAFT 1.0 }}
\author{  N. Galante\\ \texttt{<nicola.galante@pd.infn.it>}\\
  M. Garczarczyk\\ \texttt{<garcz@mppmu.mpg.de>}\\
  M. Gaug\\ \texttt{<markus@ifae.es>} \\
  S. Mizobuchi\\ \texttt{<satoko@icrr.u-tokyo.ac.jp>} 
}
  
\date{January, 2005\\}
\TDAScode{MAGIC-TDAS 05-??\\ 0312??/NGalante}
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\begin{abstract}
We give a detailed plan for the observation of Gamma Ray Bursts for the year
2005. All observations will be triggered mainly by alerts of the satellites \he, \ig   
and above all \sw. we expect an alert rate of a total of about 
\par
\ldots HOW MANY??? \ldots
\par
per year out of which only about 
\par
\ldots HOW MANY??? \ldots
\par
will be followed by a position. 
We give a detailed description of the observation procedures in La Palma and 
propose to review the situation in half a year from now.
\end{abstract}

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\newpage

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\include{Introduction}
\include{Alerts}
\include{Monitor}
\include{Strategies}
\include{Timing}
\include{Requirements}
%------------------------------------------------------------



\section{Calibration and Tests}

{\ldots \it \bf Crab data at different axis-offsets to calibrate off-axis sensitivity  \ldots \\}

%%% BIBLIOGRAPHY %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

%%>>>> Use the following if you are using BibTeX for bibliography
%\theBibliography

%%>>>> Or the following if you include here by hand your 
%%>>>> bibliographic entries
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\bibitem{HETE} 
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\end{thebibliography}

\end{document}
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