1 | \section{Proposed Observation Strategies}
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2 |
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3 | First of all let's consider how many observations are we going to do.\\
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4 |
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5 | A rough estimation of the time consume due to GRB observation comes out
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6 | from the claimed GRB observation by SWIFT, of about 150-200 GRBs/year, and
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7 | the results on the studies on the MAGIC duty-cycle made by
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8 | Nicola Galante \cite{GALANTE} and Satoko Mizobuchi \cite{SATOKO}.
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9 | Considering a MAGIC duty-cycle of about 10\% and a tollerance of 5 hours
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10 | to point the GRB, we should be able to point about 1-2 GRB/month.
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11 | Such duty-cycle studies, made before MAGIC started its observations,
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12 | are reliable as long as weather constraints that were considered
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13 | (~maximum wind's speed of 10 m/s, maximum humidity of 80\% and
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14 | darkness at astronomical horizon~) revealed similar to the real ones that
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15 | are affecting MAGIC's observation time. In this duty-cycle study
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16 | also full moon night are considered usefull (~just requiring
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17 | a minimum angular distance of the GRB from the moon of 30$^\circ$~),
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18 | while 3-4 nights per month are actually skipped because of full moon,
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19 | but this reduction of the real duty-cycle is about compensated
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20 | by the tollerance of 5 hours for considering the alert
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21 | (~5 hours more before the beginning of the night usefull
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22 | for getting GRB's alerts are equivalent to an increase
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23 | of the duty-cycle of about 6 days per month~). Actually
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24 | observation's interruptions due to technical tasks are
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25 | not considered here. \\
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26 |
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27 | All this discussion tells us that, excluding from our
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28 | considerations interruptions of the observing time due to
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29 | technical tasks, MAGIC should employ 1-2 nights per month
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30 | in GRB observations. This means that we must do as much
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31 | as possible to observe them EVERY time that a usefull
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32 | alert occours.
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33 |
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34 | \subsection{What to do with the AMC ? }
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35 |
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36 | \ldots {\bf MARKUS G. } \ldots
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37 |
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38 | \subsection{What to do with moon shine ? }
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39 |
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40 | The telescope's slewing in case of a GRB alert will be done
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41 | without closing the camera lids, so that the camera could be
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42 | flashed by the moon during such movement. In principle
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43 | a fast moon-flash shouldn't damage the PMTs, but the behaviour
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44 | of the camera and of the Camera Control {\it guagua} must
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45 | be tested. Otherway, if such test concludes that it is not safe
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46 | at all to get even a short flash from the moon, the possibility
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47 | to implement a new feature into the Steering System wich
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48 | follow a different path while selwing must be considered.
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49 |
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50 |
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51 | \subsection{Calibration }
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52 |
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53 | \ldots {\bf MARKUS gAUG} \ldots
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54 |
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55 |
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56 | \subsection{In case of follow-up: Next steps}
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57 |
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58 | Analysis during day:
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59 | \par
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60 | If some significance is seen, observe the same position next night to get some OFF-data.
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61 |
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62 |
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