Changeset 6218 for trunk

Timestamp:

02/03/05 08:57:09 (20 years ago)

Author:

gaug

Message:

*** empty log message ***

File:

• trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex (modified) (3 diffs)

trunk/MagicSoft/GRB-Proposal/GRB_proposal_2005.tex

@@ -71 +71 @@
 \begin{abstract}
 We present a detailed strategy for the observation of Gamma Ray Bursts (GRBs) for the first
-half year of 2005. All observations will be mainly triggered by alerts from \sw. In addition
-\he and \ig satellites will contribute to the number of alerts.
-We expect an alert rate in total of about 15 per months where 1--2 should be observable due to our
-duty cycle. Because it is still unknown how many alerts \sw will deliver in total and its precise sky coverage,
-we cannot predict the alert frequency better than 100\% uncertainty. This leads to a expected observation time
-of 5$\pm$5 hours per month. This number includes already observation during the moon time.
+half year of 2005. 
+All observations will be mainly triggered by alerts from \sw. 
+In addition, the \he and \ig satellites can contribute a small number of alerts.
+The \sw collaboration expects a total alert rate of about 15 per months -- 
+although with big uncertainties -- out of which 1--2 should be observable due to our
+duty cycle. The overlap in sky converages between \sw and \ma seems to be favorable for \ma. 
+As it is still unknown how many alerts \sw will deliver exactly, and how its sky coverage matches 
+with the one of \ma,
+we cannot predict the alert frequency now to better than 100\% uncertainty. 
+This leads to an expected observation time
+of 5$\pm$5 hours per month. This number includes observation during moon-time.
 We give a detailed description of the observation procedures in La Palma and
-propose to review the situation in half a year from now.
+propose to spend one dedicated night to test the automatic alert procedure 
+with the subsystem experts. 
+We suggest to review the situation in half a year from now.
 \end{abstract}
 
@@ -132 +139 @@
 Zhang B., Meszaros P., Astrophys. J. 559, 110, 2001.
 \bibitem{BELOBORODOV} Optical and GeV-TeV Flashes from GRBs, Beloborodov A., ApJ, 618, L13, 2005.
+\bibitem{LI} Li Z., Dai G., Lu T., accepted for A\&A, astro-ph/0208435, 2002.
+\bibitem{ASAF2} Prompt GRB Spectra: Detailed Calculation and the Effect of Pair Production,
+Pe'er A., Waxman E., ApJ, 603, 448, 2004.
 \bibitem{EGRET} Hurley K. et al., Nature, 372, 652
 \bibitem{DINGUS1} Observations of the Highest Energy Gamma Rays from GRBs,
@@ -149 +159 @@
 \bibitem{GRAND} Sub-TeV Gammas in Coincidence with BATSE Gamma Ray Bursts,
 Poirier J, et al., Physical Review D, 67, 042001, 2003.
-\bibitem{ASAF2} Prompt GRB Spectra: Detailed Calculation and the Effect of Pair Production,
-Pe'er A., Waxman E., ApJ, 603, 448, 2004.
-\bibitem{LI} Li Z., Dai G., Lu T., accepted for A\&A, astro-ph/0208435, 2002.
 \bibitem{ICRC} The MAGIC Telescope and the Observation of GRBs,
 Galante N. et al., Proceedings of the 28$^{th}$ ICRC, Tsukuba, Japan, 2003.