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Timestamp:
02/18/05 10:20:15 (20 years ago)
Author:
hbartko
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*** empty log message ***
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  • trunk/MagicSoft/TDAS-Extractor/Criteria.tex

    r6580 r6583  
    1616such. If the background resolution is bad, the signal threshold goes up and vice versa.
    1717
    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.
     18Also 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.
    1919
    2020\par
     
    7676observed sources.
    7777
     78
    7879\subsection{Low Gain Extraction}
    7980
     
    9091pulses are due to the large signals with a big impact on the image parameters, especially the size parameter.
    9192
     93
    9294\subsection{Stability}
    9395
     96The signal extraction algorithms has to stabelly reconstruct the charge for different types of pules with different intrinsic shapes and backgrounds:
    9497
     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}
    95103
    96 
    97 
    98 \subsection{Treatment of Calibration Pulses}
    99 
     104An 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.
    100105
    101106
     
    106111
    107112
    108 \ldots {\textit Some comments by Hendrik ...}
     113\subsection{CPU Requirements}
    109114
    110 \subsection{CPU Requirements}
    111 \ldots {\textit The needed CPU time for each extractor}
     115Depending 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
     117Thus for an online-analysis a different extraction algorithm might be chosen than for the final most accurate reconstruction of the signals offline.
    112118
    113119
    114120
    115121
     122\subsection{Treatment of Calibration Pulses}
     123
     124
    116125\subsection{Pulpo Pulses}
     126
    117127\subsection{Cosmics Data?}
    118128The results of this subsection are based on the following runs taken
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