- Timestamp:
- 02/18/05 10:20:15 (20 years ago)
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trunk/MagicSoft/TDAS-Extractor/Criteria.tex
r6580 r6583 16 16 such. If the background resolution is bad, the signal threshold goes up and vice versa. 17 17 18 Also an accurate determination of the signal arrival time may help to distinguish between signal and background. The signal arrival times vary smoothly from pixel to pixel while the background noise is randomly distributed in time. 18 Also an accurate determination of the signal arrival time may help to distinguish between signal and background. The signal arrival times vary smoothly from pixel to pixel while the background noise is randomly distributed in time. Therefore it must be insured that the reconstructed arrival time corresponds to the same reconstructed pulse as the reconstructed charge. 19 19 20 20 \par … … 76 76 observed sources. 77 77 78 78 79 \subsection{Low Gain Extraction} 79 80 … … 90 91 pulses are due to the large signals with a big impact on the image parameters, especially the size parameter. 91 92 93 92 94 \subsection{Stability} 93 95 96 The signal extraction algorithms has to stabelly reconstruct the charge for different types of pules with different intrinsic shapes and backgrounds: 94 97 98 \begin{itemize} 99 \item{cosmics signals from gammas, hadrons and muons} 100 \item{calibration pulses from different LED color pulsers} 101 \item{pulse generator pulses in the pulpo setup} 102 \end{itemize} 95 103 96 97 98 \subsection{Treatment of Calibration Pulses} 99 104 An important point is the difference between the pulse shapes of the calibration and Cherenkov signals. It has to be ensured that the calibration factor between the reconstructed charge in FADC counts and photo electrons for calibration events can be applied to Cherenkov signals. 100 105 101 106 … … 106 111 107 112 108 \ ldots {\textit Some comments by Hendrik ...}113 \subsection{CPU Requirements} 109 114 110 \subsection{CPU Requirements} 111 \ldots {\textit The needed CPU time for each extractor} 115 Depending on the reconstruction algorithm the signal reconstruction can take a significant amount of CPU time. Especially the more sophisticated signal extractors which search for the position of the Cherenkov signals in the recorded FADC time slices and perform a fit to these samples can be time consuming. 116 117 Thus for an online-analysis a different extraction algorithm might be chosen than for the final most accurate reconstruction of the signals offline. 112 118 113 119 114 120 115 121 122 \subsection{Treatment of Calibration Pulses} 123 124 116 125 \subsection{Pulpo Pulses} 126 117 127 \subsection{Cosmics Data?} 118 128 The results of this subsection are based on the following runs taken
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