Performance of the Stereoscopic System of the HEGRA Imaging Air ÿ

A. Konopelko,M. Hemberger,F. Aharonian,A. Daum,W. Hofmann,H. Krawczynski,A. G. Akhperjanian,J. A. Barrio,H. Bojahr,J. L. Contreras,J. Cortina,T. Deckers,S. Denninghoff,Julio Fernández,V. Fonseca,J. Gonzalez,V Haustein,G. Heinzelmann,G. Hermann,M. Heß,A. Heusler,H. Hohl,I. Holl,D. Horns,R. S. Kankanian,M. Kestel,J. Kettler,O. Kirstein,H. Kornmayer,D. Kranich,H. Lampeitl,A. Lindner,E. Lorenz,N. Magnussen,H. Meyer,R. Mirzoyan,A. Moralejo,L. Padilla,M. Panter,D. Petry,R. Plaga,A. Plyasheshnikov,J. Prahl,C. Prosch,G. Rauterberg,W. Rhode,V. Sahakian,M. Samorski,J. Sanchez,D. Schmele,F. Schroeder,W. Stamm,B. Wiebel-Sooth,C. A. Wiedner,M. Willmer,H. Wirth

Performance of the Stereoscopic System of the HEGRA Imaging Air ÿ

2008

). The telescope array, primarily designed for stereoscopic observations ofthe γ-radiation at energies above several hundred GeV [1] is formed by ﬁve identicalIACTs - one at the center, and four others at the corners of a 100 m by 100 m square area.The multi-mirror reﬂector of each system telescope has an area of 8.5m

Keywords:

Stereoscopy
Astronomy
Telescope
HEGRA
Physics
Optics
Astrophysics

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