Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..515..363c&link_type=abstract
GeV-TeV GAMMA RAY ASTROPHYSICS WORKSHOP: Towards a Major Atmospheric Cherenkov Detector VI. AIP Conference Proceedings, Volume
Astronomy and Astrophysics
Astrophysics
X- And Gamma-Ray Telescopes And Instrumentation
Scientific paper
The MAGIC Telescope will use FADCs to sample the camera pixel signals. This allows to analyze features of the Cherenkov time pulses with ~1 ns resolution and to minimize data taking deadtime and noise. Here we report on the first tests of a 300 MHz FADC 32-channel unit and on some special solutions for enlarging the signal's dynamical range. In the long run MAGIC will be provided with >1 GHz FADCs in order to profit from the full speed capabilities of the PMs in use [1 ns FWHM]. .
Cortina Jaun
Lorenz Eckart
MAGICT Collaboration
Mirzoyan Rafayel
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