- Timestamp:
- 02/21/05 20:46:53 (20 years ago)
- Location:
- trunk/MagicSoft/TDAS-Extractor
- Files:
-
- 2 edited
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trunk/MagicSoft/TDAS-Extractor/MAGIC_signal_reco.tex
r6651 r6657 36 36 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% 37 37 \title{Comparison of Signal Reconstruction Algorithms for the MAGIC Telescope} 38 \author{H. Bartko, M. Gaug, F. Goebel, A. Moralejo, 39 M. Shayduk, N. Sidro, W. Wittek}40 \date{February 2 8$^{\mathrm{th}}$, 2005\\}41 \TDAScode{MAGIC-TDAS 05-xx\\ 05022 8}38 \author{H. Bartko, M. Gaug, F. Goebel, A. Moralejo,\\ 39 Th. Schweizer, M. Shayduk, N. Sidro, W. Wittek} 40 \date{February 21$^{\mathrm{st}}$, 2005\\} 41 \TDAScode{MAGIC-TDAS 05-xx\\ 050221} 42 42 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% 43 43 … … 52 52 are described and compared. Criteria for comparison are defined and used to judge the 53 53 different extractors applied to calibration signals, cosmics and pedestals. At the end, 54 a digital filter fitting the signal over four FADC slices is proposed as the best extractor. 55 The question of pedestal calculation for the different extractors is adressed. The digital filter 56 is used to extract and fit single photo-electron pulses from the night sky background. 54 extractors are recommended for the most conservative and the most advanced and demanding analyses. 55 It is shown that the digital filter 56 can be used to extract and fit single photo-electron pulses from the night sky background. 57 The achievable time resolution can be parameterized to be: 58 \begin{equation} 59 \Delta T_{\mathrm{cosmics}} \approx \sqrt{\frac{(2\,\mathrm{ns})^2}{<Q>/{\mathrm{phe}}} 60 + \frac{(4.5\,\mathrm{ns})^2}{<Q>^2/{\mathrm{phe^2}}} + (0.2\,\mathrm{ns})^2} . \nonumber 61 \label{eq:time:fitprediction} 62 \end{equation} 63 For galactic backgrounds an image cleaning threshold as low as 5~photo-electrons can be achieved 64 for rejecting 99.7\% of noise. 57 65 \end{abstract} 58 66 -
trunk/MagicSoft/TDAS-Extractor/Results.tex
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