Strong scientific motivation are pushing the second generation of ground base Cherenkov telescopes to lower as much as possible their energy threshold. MAGIC will be the biggest single telescope, in terms of collection area (250 m(2)), foreseen for the second-half of 2001. The large collection area, the new photodetector and the electronic design will allow the telescope to lower the energy threshold below 30 GeV. For this telescope a two-level pattern trigger is designed to work in severe high pixel rate. The MAGIC trigger architecture and its implementation is presented. (C) 2001 Elsevier Science B.V. All rights reserved
The MAGIC 17m diameter Cherenkov telescope will be upgraded with a second telescope with advanced ph...
The atmospheric Cherenkov telescope MAGIC for ground-based gamma-ray astronomy is operating since la...
The Magor Atmospheric Gamma-ray Imaging Cherenkov telescope (MAGIC) is at its commissioning phase an...
Strong scientific motivation are pushing the second generation of ground base Cherenkov telescopes t...
The MAGIC telescope aims at the detection of very low energy gamma rays (E > 30 GeV) through the ...
The Major Atmospheric Gamma-ray Imaging Cherenkov telescope (MAGIC) aims at the detection of very lo...
The MAGIC Telescope is now on its final commissioning phase and will become operational before the e...
The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope aims at the detection of very low energy...
The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope aims at the detection of very low energy...
The MAGIC Collaboration is building an imaging \u10cerenkov telescope at La Palma site (2200 m a.s.l...
MAGIC is a system of two 17 m diameter Imaging Atmospheric Cherenkov Telescopes (IACTs) for ground-b...
Abstract: MAGIC is a stereoscopic system of two 17 m diameter Imaging Air Cherenckov Telescopes (IAC...
A project to construct a 17 m diameter imaging air Cherenkov telescope, called the MAGIC Telescope, ...
The MAGIC telescopes have been designed primarily to reach the lowest possible energy threshold with...
Technical research and development for the MAGIC project started some eight years ago, with the clea...
The MAGIC 17m diameter Cherenkov telescope will be upgraded with a second telescope with advanced ph...
The atmospheric Cherenkov telescope MAGIC for ground-based gamma-ray astronomy is operating since la...
The Magor Atmospheric Gamma-ray Imaging Cherenkov telescope (MAGIC) is at its commissioning phase an...
Strong scientific motivation are pushing the second generation of ground base Cherenkov telescopes t...
The MAGIC telescope aims at the detection of very low energy gamma rays (E > 30 GeV) through the ...
The Major Atmospheric Gamma-ray Imaging Cherenkov telescope (MAGIC) aims at the detection of very lo...
The MAGIC Telescope is now on its final commissioning phase and will become operational before the e...
The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope aims at the detection of very low energy...
The Major Atmospheric Gamma-ray Imaging Cherenkov Telescope aims at the detection of very low energy...
The MAGIC Collaboration is building an imaging \u10cerenkov telescope at La Palma site (2200 m a.s.l...
MAGIC is a system of two 17 m diameter Imaging Atmospheric Cherenkov Telescopes (IACTs) for ground-b...
Abstract: MAGIC is a stereoscopic system of two 17 m diameter Imaging Air Cherenckov Telescopes (IAC...
A project to construct a 17 m diameter imaging air Cherenkov telescope, called the MAGIC Telescope, ...
The MAGIC telescopes have been designed primarily to reach the lowest possible energy threshold with...
Technical research and development for the MAGIC project started some eight years ago, with the clea...
The MAGIC 17m diameter Cherenkov telescope will be upgraded with a second telescope with advanced ph...
The atmospheric Cherenkov telescope MAGIC for ground-based gamma-ray astronomy is operating since la...
The Magor Atmospheric Gamma-ray Imaging Cherenkov telescope (MAGIC) is at its commissioning phase an...