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Timestamp:
02/21/05 13:04:14 (20 years ago)
Author:
hbartko
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  • trunk/MagicSoft/TDAS-Extractor/MonteCarlo.tex

    r6643 r6644  
    107107\end{figure}
    108108
     109\clearpage
     110
    109111%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
    110112
    111113\subsection{Measurement of the Biases \label{sec:mc:baises}}
    112114
     115We fitted the conversion factors obtained from the previous section in the constant region (above 10\,phe) and used
     116them to convert the extracted charge back to equivalent photo-electrons. After subtracting the simulated number of photo-electrons,
     117the bias (in units of photo-electrons) is obtained.
     118\par
     119Figure~\ref{fig:mc:ConversionvsNphe_FixW} through~\ref{fig:mc:ChargeRes_DFSpline} show the results for the tested extractors, with and
     120without added noise and for the high and low-gain regions separately.
     121\par
     122As expected, the fixed window extractor do not show any bias up to statistical precision. All sliding window extractor, however, do show
     123a bias. Usually, the bias vanishes for signals above 5--10~photo-electrons, except for the sliding windows with window sizes above
     1248~FADC slices. There, the bias only vanishes for signals above 20~photo-electrons. The size of the bias as well as the minimum signal
     125strength above which the bias vanishes are clearly correlated with the extraction window size. Therefore, smaller window sizes yield
     126smaller biases and extend their linear range further downwards. The best extractors have a negligible bias above about 5 photo-electrons.
     127This corresponds to the results found in section~\ref{sec:pedestals} where the lowest image cleaning threshold for extra-galactic
     128noise levels yielded about 5 photo-electrons as well.
     129\par
     130All integrating spline extractors and all sliding window extractors with extraction windows above or equal 6 FADC slices
     131 yield the comparably smallest biases. The rest results to be about a factor 1.5 higher. The spline and digital filter biases fall
     132down very steeply.
     133
     134
    113135\begin{figure}[htp]%%[t!]
    114136\centering
     
    120142  \vspace{\floatsep}
    121143  \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_FixW_WithNoise_LoGain.eps}
    122   \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_FixW_WithNoise_LoGain.eps}
    123144\caption[Bias Fixed Windows]{The measured bias (extracted charge divided by the conversion factor minus the number of photoelectrons)
    124145versus number of photoelectrons,
     
    159180\label{fig:mc:ConversionvsNphe_DFSpline}
    160181\end{figure}
     182
     183\clearpage
     184
     185%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
     186
     187\subsection{Measurement of the Resolutions \label{sec:mc:resolutions}}
    161188
    162189\begin{figure}[htp]
     
    208235\clearpage
    209236
     237%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%5
     238
    210239\subsection{Charge Signals with and without Simulated Noise \label{fig:mc:sec:mc:chargenoise}}
    211240
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