Observation of VHE Gamma Ray Sources with the MAGIC telescope
Observation of VHE Gamma Ray Sources with the MAGIC telescope
Observation of VHE Gamma Ray Sources with the MAGIC telescope
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The <strong>MAGIC</strong> <strong>telescope</strong><br />
• Largest Imaging Air<br />
Cherenkov Telescope<br />
for γ-ray astronomy<br />
(17 m mirror dish)<br />
Canary Island La Palma<br />
2200 m asl<br />
• low energy trigger<br />
threshold<br />
E γ<br />
= 50-60<br />
GeV<br />
• fast repositioning<br />
t R<br />
100 physicists, 18 institutes, 11 countries:<br />
Barcelona IFAE, Barcelona UAB, HU Berlin, Crimean Observatory, U.C. U<br />
Davis,<br />
U. Dortmund, U. Lodz, , UCM Madrid, INR Moscow, MPI München,<br />
INFN/ U. Padua, INFN/ U. Siena, S<strong>of</strong>ia, Tuorla Observatory,<br />
Yerevan Phys. Institute, INFN/ U. Udine, , U. Würzburg, , ETH ZürichZ<br />
P.Majumdar, 24 th August, IIA, India
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