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The FADC readout of the MAGIC telescope

Authors: Juan Cortina; Eckart Lorenz; R. Mirzoyan;

The FADC readout of the MAGIC telescope

Abstract

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].

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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