Signal Reconstruction for the MAGIC Telescope
arXiv:astro-ph/0612385 · doi:10.1016/j.nima.2008.06.043
Abstract
Until April 2007 the MAGIC telescope used a 300 MSamples/s FADC system to sample the shaped PMT signals produced by the captured Cherenkov photons of air showers. Different algorithms to reconstruct the signal from the read-out samples (extractors) have been implemented and are described and compared. Criteria based on the obtained charge and time resolution/bias are defined and used to judge the different extractors, by applying them to calibration, cosmic and pedestal signals. The achievable charge and time resolution have been derived as functions of the incident number of photo-electrons.
Accepted for publication in NIM A
References in corpus (7)
- Variable VHE gamma-ray emission from Markarian 501
- The First VERITAS Telescope
- VHE Gamma-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC telescope
- Discovery of VHE gamma-ray emission from 1ES1218+30.4
- Tagging single muons and other long-flying relativistic charged particles by ultra-fast timing in air Cherenkov telescopes
- Study of the performance and capability of the new ultra-fast 2 GSample/s FADC data acquisition system of the MAGIC telescope
- Analysis of Flash ADC Data With VERITAS
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