FADC Pulse Reconstruction Using a Digital Filter for the MAGIC Telescope

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dc.creatorBartko, H.
dc.creatorGaug, M.
dc.creatorMoralejo, A.
dc.creatorSidro, N.
dc.date2005-06-20
dc.date.accessioned2026-07-07T02:18:01Z
dc.date.available2026-07-07T02:18:01Z
dc.descriptionPresently, the MAGIC telescope uses a 300 MHz FADC system to sample the transmitted and shaped signals from the captured Cherenkov light of air showers. We describe a method of Digital Filtering of the FADC samples to extract the charge and the arrival time of the signal: Since the pulse shape is dominated by the electronic pulse shaper, a numerical fit can be applied to the FADC samples taking the noise autocorrelation into account. The achievable performance of the digital filter is presented and compared to other signal reconstruction algorithms.
dc.descriptionto be published in the proceedings of the conference "Towards a Network of Atmospheric Cherenkov Detectors VII", 27-29 April 2005 - Ecole Polytechnique, Palaiseau, France
dc.identifierhttps://arxiv.org/abs/astro-ph/0506459
dc.identifierhttp://arxiv.org/abs/astro-ph/0506459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9333
dc.subjectAstrophysics
dc.titleFADC Pulse Reconstruction Using a Digital Filter for the MAGIC Telescope
dc.typetext

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