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

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1\documentclass[a4paper]{newletter}
2%\usepackage{german}
3
4\institute{Mets\"{a}hovi Radio Observatory}
5\name{Dr.\ Merja Tornikoski}
6\street{Mets\"{a}hovintie 114}
7\city{FIN-02540 Kylm\"{a}l\"{a}}
8\email{merja.tornikoski@hut.fi}
9%\tel{Tel: (0551) 39-50\,50}
10
11\place{Kylm\"{a}l\"{a}}
12%\date{25. April 2000}
13
14\begin{document}
15\begin{letter}{Universit\"{a}t Dortmund\\Prof.\ Dr. Wolfgang Rhode\\Otto-Hahn-Stra\ss e 4\\44227 Dortmund\\Saksa}
16
17\opening{Agreement}
18
19Dear Prof.\ Dr.\ Dr.\ Rhode, dear Prof.\ Dr.\ Mannheim,
20
21we plan to use the proposed air-Cherenkov telescope prototype system
22DWARF on the MAGIC/ORM site on La Palma for the continuous monitoring
23of strong blazars. Whenever possible, the monitoring effort at VHE
24gamma rays will be complemented at optical and radio wavelengths using
25the KVA optical telescope operated by the Tuorla group and the
26Mets\"{a}hovi Radio Observatory. The ultimate goal of this program is
27to obtain long-term lightcurves of strong blazars to determine their
28flux variation power spectrum across a broad wavelength range. Thereby
29we expect to achieve a major progress in understanding the mechanism
30behind the variable non-thermal emission. The data rights of the
31different telescope facilities remain proprietary to the operating
32responsibles, but we intend to publish the results of joint campaigns
33together on the basis of a consensus decision.
34
35\vspace{0.5cm}
36
37\closing{Signature}
38
39\end{letter}
40\end{document}
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