source: branches/start/Dwarf/Documents/Agreement/agreement.tex

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1\documentclass[a4paper]{newletter}
2%\usepackage{german}
3
4\name{Tuorla Observatory,\\Dr.\ Leo Takalo}
5\street{V\"{a}is\"{a}l\"{a}ntie 20}
6\city{21500 Piikki\"o}
7\email{takalo@utu.fi}
8%\tel{Tel: (0551) 39-50\,50}
9
10\place{Tuorla}
11%\date{25. April 2000}
12
13\begin{document}
14\begin{letter}{Universit\"{a}t Dortmund\\Prof.\ Dr. Wolfgang Rhode\\Otto-Hahn-Stra\ss e 4\\44227 Dortmund\\Saksa}
15
16\opening{Agreement}
17
18Dear Prof.\ Dr.\ Dr.\ Rhode, dear Prof.\ Dr.\ Mannheim,
19
20we plan to use the proposed air-Cherenkov telescope prototype system
21DWARF on the MAGIC/ORM site on La Palma for the continuous monitoring
22of strong blazars. Whenever possible, the monitoring effort at VHE
23gamma rays will be complemented at optical and radio wavelengths using
24the KVA optical telescope operated by the Tuorla group and the
25Mets\"{a}hovi Radio Observatory. The ultimate goal of this program is
26to obtain long-term lightcurves of strong blazars to determine their
27flux variation power spectrum across a broad wavelength range. Thereby
28we expect to achieve a major progress in understanding the mechanism
29behind the variable non-thermal emission. The data rights of the
30different telescope facilities remain proprietary to the operating
31responsibles, but we intend to publish the results of joint campaigns
32together on the basis of a consensus decision.
33
34\vspace{0.5cm}
35
36\closing{Signature}
37
38\end{letter}
39\end{document}
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