1. FACT—The first Cherenkov telescope using a G-APD camera for TeV gamma-ray astronomy
- Author
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Q. Weitzel, Oliver Grimm, Karl Mannheim, M. Domke, K. Warda, Felicitas Pauss, T. Krähenbühl, E. Lorenz, Dieter Renker, D. Neise, Adrian Biland, S. Commichau, D. Hildebrand, Patrick Vogler, Thomas Bretz, U. Horisberger, V. Commichau, Ilana M. Braun, Ulf Roser, H. von Gunten, L. S. Stark, B. Krumm, J.-H. Köhne, Daniel Kranich, Wolfgang Rhode, A. Boller, M. Rissi, A. Gendotti, Werner Lustermann, J.-P. Stucki, O. Tibolla, G. Viertel, Daniela Dorner, M. Ribordy, H. Anderhub, and Michael Backes
- Subjects
Physics ,Nuclear and High Energy Physics ,business.industry ,Cherenkov detector ,Astronomy ,IACT ,Gamma-ray astronomy ,Avalanche photodiode ,Cherenkov Telescope Array ,law.invention ,Telescope ,Crab Nebula ,Optics ,law ,business ,Instrumentation ,Cherenkov radiation - Abstract
Geiger-mode Avalanche Photodiodes (G-APD) bear the potential to significantly improve the sensitivity of Imaging Air Cherenkov Telescopes (IACT). We are currently building the First G-APD Cherenkov Telescope (FACT) by refurbishing an old IACT with a mirror area of 9.5 square meters and are constructing a new, fine-pixelized camera using novel G-APDs. The main goal is to evaluate the performance of a complete system by observing very high energy gamma-rays from the Crab Nebula. This is an important field test to check the feasibility of G-APD-based cameras to replace at some time the PMT-based cameras of planned future IACTs like AGE and CTA. In this article, we present the basic design of such a camera as well as some important details. (C) 2010 Elsevier B.V. All rights reserved.
- Published
- 2011