source: trunk/MagicSoft/GRB-Proposal/Strategies.tex@ 6091

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