FACT - The first Cherenkov telescope using a G-APD camera for TeV gamma-ray astronomy
dc.contributor.author | Anderhub, H. | |
dc.contributor.author | Backes, M. | |
dc.contributor.author | Biland, A. | |
dc.contributor.author | Boller, A. | |
dc.contributor.author | Braun, I. | |
dc.contributor.author | Bretz, T. | |
dc.contributor.author | Commichau, S. | |
dc.contributor.author | Commichau, V. | |
dc.contributor.author | Domke, M. | |
dc.contributor.author | Dorner, D. | |
dc.contributor.author | Gendotti, A. | |
dc.contributor.author | Grimm, O. | |
dc.contributor.author | Hildebrand, D. | |
dc.contributor.author | Horisberger, U. | |
dc.contributor.author | Köhne, J.-H. | |
dc.contributor.author | Krähenbühl, T. | |
dc.contributor.author | Kranich, D. | |
dc.contributor.author | Krumm, B. | |
dc.contributor.author | Lorenz, E. | |
dc.contributor.author | Lustermann, W. | |
dc.contributor.author | Mannheim, K. | |
dc.contributor.author | Neise, D. | |
dc.contributor.author | Pauss, F. | |
dc.contributor.author | Renker, D. | |
dc.contributor.author | Rhode, W. | |
dc.contributor.author | Ribordy, M. | |
dc.contributor.author | Rissi, M. | |
dc.contributor.author | Röser, U. | |
dc.contributor.author | Stark, L. S. | |
dc.contributor.author | Stucki, J.-P. | |
dc.contributor.author | Tibolla, O. | |
dc.contributor.author | Viertel, G. | |
dc.contributor.author | Vogler, P. | |
dc.contributor.author | von Gunten, H. | |
dc.contributor.author | Warda, K. | |
dc.contributor.author | Weitzela, Q. | |
dc.date.accessioned | 2012-03-05T15:55:54Z | |
dc.date.available | 2012-03-05T15:55:54Z | |
dc.date.issued | 2011-01-01 | |
dc.description.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 AGIS and CTA. In this article, we present the basic design of such a camera as well as some important details. | en |
dc.identifier.uri | http://hdl.handle.net/2003/29371 | |
dc.identifier.uri | http://dx.doi.org/10.17877/DE290R-4294 | |
dc.identifier.url | http://dx.doi.org/10.1016/j.nima.2010.10.081 | |
dc.language.iso | en | de |
dc.publisher | Elsevier | |
dc.relation.ispartofseries | Nuclear Instruments and Methods in Physics Research A ; Volume 639, Issue 1 | en |
dc.subject | Cherenkov telescope | en |
dc.subject | Geiger-mode avalanche photodiode (G-APD) | en |
dc.subject | ground-based gamma-ray astronomy | en |
dc.subject | instrumentation | en |
dc.subject.ddc | 004 | |
dc.title | FACT - The first Cherenkov telescope using a G-APD camera for TeV gamma-ray astronomy | en |
dc.type | Text | de |
dc.type.publicationtype | article | de |
dcterms.accessRights | open access |