\section{Requirements to start full GRB observations}

In the previous sessions we described the status and tasks we still plan to do
in order to complete the GRB Alarm System.
Parallel to our system also the different subsystems of the MAGIC telescope have
to implement and test strategies for the GRB survay.

\par

We strongly push the responsibles of the drive-, camera-, amc- and central
control subsystemsto fullfill the criteria defined in~\cite{design}. We suggest
to make a one week shift wherethe experts meet together and test the GRB
stategies. In order to avoid good observation timewe suggest to make the shift
during the moon period. This shift should take place, in arrangementwith the
different subsystem responsibles, before april this year. The time limitation is
based onthe moment when SWIFT will start to work fully automaticly, sending
allerts in real time to the groundstations.
\par

We present a list of tasks that are very crucial for the GRB survay:

\par

\begin{itemize}
\item {\bf Fast slewing:}\

One of the most important issues is to implement and test the fast movements
of the telescope. Specially the communication between CC and Cosy has to be arranged for
the case of fast movements.

\item {\bf Use of look-up tables:}\

The use of look-up tables to correct the mirror focus during the movement to the GRB
coordinates is advantegous. In the alert situation it is a vaste of time if we would have to
close the camera lids and carry out the full laser adjustment (\~5~min) before starting the observation.
The reproducibility of the focus with the use of look-up tables has to be proven.
In order to use the time during the telescope movement for the focussing of the mirrors to the desired
telescope positon, the AMC needs the coordinates immediately. In this case it is necessary to change the protocol between the AMC and CC.

\item {\bf Behaviour of the camera during moon:}\

It has to be checked what happens when during the pointing to a GRB position the telescope move over the
moon. It is excluded by the GRB Alert System that a burst closer than 30$\deg$ to the moon will be pointed. However it is not prevented that during the movement of the telescope the moon will pass the FOV.
In this case the HV of the PMTs will be reduced automatically and will not increase fast enought for the
GRB observation.

\end{itemize}

\par

All this issues have to be checked during the suggested shift. The aim would be to send fake allerts to
the GRB Alarm System and proove the behaviour of all subsystems.


