| 1 | \section{Monte Carlo \label{sec:mc}}
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| 2 |
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| 3 | \subsection{Introduction \label{sec:mc:intro}}
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| 4 |
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| 5 | Many characteristics of the extractor can only be investigated with the use of Monte-Carlo simulations~\cite{MC-Camera}
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| 6 | of signal pulses and noise for the following reasons:
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| 7 |
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| 8 | \begin{itemize}
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| 9 | \item While in real conditions, the signal can only be obtained in a Poisson distribution, simulated pulses of a specific
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| 10 | number of photo-electrons can be generated.
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| 11 | \item The intrinsic arrival time spread can be chosen within the simulation.
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| 12 | \item The noise auto-correlation in the low-gain channel cannot be determined from data,
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| 13 | but instead has to be retrieved from Monte-Carlo studies.
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| 14 | \item The same pulse can be studied with and without added noise, where the noise level can be deliberately adjusted.
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| 15 | \item The photo-multiplier and optical link gain fluctuations can be tuned or switched off completely.
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| 16 | \end{itemize}
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| 17 |
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| 18 | Nevertheless, there are always systematic differences between the simulation and the real detector. In our case, especially the
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| 19 | following short-comings are of concern:
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| 20 |
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| 21 | \begin{itemize}
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| 22 | \item The low-gain pulse is not yet simulated with the correct pulse width, but instead the same pulse shape as the one of the
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| 23 | high-gain channel has been used.
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| 24 | \item The low-gain pulse starts to saturate at already about 200 photo-electrons while in reality,
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| 25 | this limit lies at more than 500 photo-electrons for an inner pixel. This is due to the wider low-gain pulse in real conditions.
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| 26 | \item The low-gain pulse is delayed by only 15 FADC slices in the Monte-Carlo simulations, while it arrives about 16.5 FADC slices
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| 27 | after the high-gain pulse in real conditions.
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| 28 | \item No switching noise due to the low-gain switch has been simulated.
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| 29 | \item The intrinsic transit time spread of the photo-multipliers has not been simulated.
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| 30 | \item The pulses have been simulated in steps of 0.2\,ns before digitization. There is thus an artificial numerical time resolution
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| 31 | limit of $0.2\,\mathrm{ns}/\sqrt{12} \approx 0.06\,\mathrm{ns}$.
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| 32 | \item The total dynamic range of the entire signal transmission chain was set to infinite, thus the detector has been simulated
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| 33 | to be completely linear.
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| 34 | \end{itemize}
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| 35 |
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| 36 | For the subsequent studies, the following settings have been used:
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| 37 |
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| 38 | \begin{itemize}
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| 39 | \item The gain fluctuations for signal pulses were switched off.
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| 40 | \item The gain fluctuations for the background noise of the light of night sky were instead fully simulated, i.e. very close to
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| 41 | real conditions.
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| 42 | \item The intrinsic arrival time spread of the photons was set to be 1\,ns, as expected for gamma showers.
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| 43 | \item The conversion of total integrated charge to photo-electrons was set to be 7.8~FADC~counts
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| 44 | per photo-electron, independent of the signal strength.
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| 45 | \item The trigger jitter was set to be uniformly distributed over 1~FADC slice only.
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| 46 | \item Only one inner pixel has been simulated.
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| 47 | \end{itemize}
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| 48 |
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| 49 | The last point had the consequence that the extractor {\textit {\bf MExtractFixedWindowPeakSearch}} could not be tested since
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| 50 | it was equivalent to the sliding window.
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| 51 | In the following, we used the Monte-Carlo to determine especially the following quantities for each of the tested extractors:
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| 52 |
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| 53 | \begin{itemize}
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| 54 | \item The charge resolution as a function of the input signal strength.
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| 55 | \item The charge extraction bias as a function of the input signal strength.
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| 56 | \item The time resolution as a function of the input signal strength.
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| 57 | \item The effect of adding or removing noise for the above quantities.
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| 58 | \end{itemize}
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| 59 |
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| 60 | \subsection{Conversion Factors \label{sec:mc:convfactors}}
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| 61 |
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| 62 | The following figures~\ref{fig:mc:ChargeDivNphe_FixW} through~\ref{fig:mc:ChargeDivNphe_DFSpline} show the conversion factors
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| 63 | between reconstructed charge and the number of input photo-electrons for each of the tested extractors, with and without added noise
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| 64 | and for the high-gain and low-gain channels, respectively. One can see that the conversion factors depend on the extraction window size and
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| 65 | that the addition of noise raises the conversion factors uniformly for all fixed window extractors in the high-gain channel,
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| 66 | while the sliding window extractors show a bias a low signal intensities.
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| 67 |
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| 68 | \begin{figure}[htp]%%[t!]
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| 69 | \centering
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| 70 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_FixW_NoNoise_HiGain.eps}
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| 71 | \vspace{\floatsep}
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| 72 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_FixW_WithNoise_HiGain.eps}
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| 73 | \vspace{\floatsep}
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| 74 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_FixW_NoNoise_LoGain.eps}
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| 75 | \vspace{\floatsep}
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| 76 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_FixW_WithNoise_LoGain.eps}
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| 77 | \caption[Charge per Number of photo-electrons Fixed Windows]{Extracted charge per photoelectron versus number of photoelectrons,
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| 78 | for fixed window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 79 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 80 | \label{fig:mc:ChargeDivNphe_FixW}
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| 81 | \end{figure}
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| 82 |
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| 83 | \begin{figure}[htp]
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| 84 | \centering
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| 85 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_SlidW_NoNoise_HiGain.eps}
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| 86 | \vspace{\floatsep}
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| 87 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_SlidW_WithNoise_HiGain.eps}
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| 88 | \vspace{\floatsep}
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| 89 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_SlidW_NoNoise_LoGain.eps}
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| 90 | \vspace{\floatsep}
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| 91 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_SlidW_WithNoise_LoGain.eps}
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| 92 | \caption[Charge per Number of photo-electrons Sliding Windows]{Extracted charge per photoelectron versus number of photoelectrons,
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| 93 | for sliding window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 94 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 95 | \label{fig:mc:ChargeDivNphe_SlidW}
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| 96 | \end{figure}
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| 97 |
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| 98 | \begin{figure}[htp]
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| 99 | \centering
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| 100 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_DFSpline_NoNoise_HiGain.eps}
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| 101 | \vspace{\floatsep}
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| 102 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_DFSpline_WithNoise_HiGain.eps}
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| 103 | \vspace{\floatsep}
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| 104 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_DFSpline_NoNoise_LoGain.eps}
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| 105 | \vspace{\floatsep}
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| 106 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeDivNphevsNphe_DFSpline_WithNoise_LoGain.eps}
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| 107 | \caption[Charge per Number of photo-electrons Spline and Digital Filter]{Extracted charge per photoelectron versus number of photoelectrons,
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| 108 | for spline and digital filter extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 109 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 110 | \label{fig:mc:ChargeDivNphe_DFSpline}
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| 111 | \end{figure}
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| 112 |
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| 113 | \clearpage
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| 114 |
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| 115 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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| 116 |
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| 117 | \subsection{Measurement of the Biases \label{sec:mc:baises}}
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| 118 |
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| 119 | We fitted the conversion factors obtained from the previous section in the constant region (above 10\,phe) and used
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| 120 | them to convert the extracted charge back to equivalent photo-electrons. After subtracting the simulated number of photo-electrons,
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| 121 | the bias (in units of photo-electrons) is obtained.
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| 122 | \par
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| 123 | Figure~\ref{fig:mc:ConversionvsNphe_FixW} through~\ref{fig:mc:ChargeRes_DFSpline} show the results for the tested extractors, with and
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| 124 | without added noise and for the high and low-gain regions separately.
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| 125 | \par
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| 126 | As expected, the fixed window extractor do not show any bias up to statistical precision. All sliding window extractor, however, do show
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| 127 | a bias. Usually, the bias vanishes for signals above 5--10~photo-electrons, except for the sliding windows with window sizes above
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| 128 | 8~FADC slices. There, the bias only vanishes for signals above 20~photo-electrons. The size of the bias as well as the minimum signal
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| 129 | strength above which the bias vanishes are clearly correlated with the extraction window size. Therefore, smaller window sizes yield
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| 130 | smaller biases and extend their linear range further downwards. The best extractors have a negligible bias above about 5 photo-electrons.
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| 131 | This corresponds to the results found in section~\ref{sec:pedestals} where the lowest image cleaning threshold for extra-galactic
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| 132 | noise levels yielded about 5 photo-electrons as well.
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| 133 | \par
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| 134 | All integrating spline extractors and all sliding window extractors with extraction windows above or equal 6 FADC slices
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| 135 | yield the comparably smallest biases. The rest results to be about a factor 1.5 higher. The spline and digital filter biases fall
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| 136 | down very steeply.
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| 137 |
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| 138 |
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| 139 | \begin{figure}[htp]%%[t!]
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| 140 | \centering
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| 141 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_FixW_NoNoise_HiGain.eps}
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| 142 | \vspace{\floatsep}
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| 143 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_FixW_WithNoise_HiGain.eps}
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| 144 | \vspace{\floatsep}
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| 145 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_FixW_NoNoise_LoGain.eps}
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| 146 | \vspace{\floatsep}
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| 147 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_FixW_WithNoise_LoGain.eps}
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| 148 | \caption[Bias Fixed Windows]{The measured bias (extracted charge divided by the conversion factor minus the number of photoelectrons)
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| 149 | versus number of photoelectrons,
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| 150 | for fixed window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 151 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 152 | \label{fig:mc:ConversionvsNphe_FixW}
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| 153 | \end{figure}
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| 154 |
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| 155 | \begin{figure}[htp]
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| 156 | \centering
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| 157 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_SlidW_NoNoise_HiGain.eps}
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| 158 | \vspace{\floatsep}
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| 159 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_SlidW_WithNoise_HiGain.eps}
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| 160 | \vspace{\floatsep}
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| 161 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_SlidW_NoNoise_LoGain.eps}
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| 162 | \vspace{\floatsep}
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| 163 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_SlidW_WithNoise_LoGain.eps}
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| 164 | \caption[Bias Sliding Windows]{The measured bias (extracted charge divided by the conversion factor minus the number of photoelectrons)
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| 165 | versus number of photoelectrons,
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| 166 | for sliding window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 167 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 168 | \label{fig:mc:ConversionvsNphe_SlidW}
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| 169 | \end{figure}
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| 170 |
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| 171 | \begin{figure}[htp]
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| 172 | \centering
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| 173 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_DFSpline_NoNoise_HiGain.eps}
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| 174 | \vspace{\floatsep}
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| 175 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_DFSpline_WithNoise_HiGain.eps}
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| 176 | \vspace{\floatsep}
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| 177 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_DFSpline_NoNoise_LoGain.eps}
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| 178 | \vspace{\floatsep}
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| 179 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ConversionvsNphe_DFSpline_WithNoise_LoGain.eps}
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| 180 | \caption[Bias Spline and Digital Filter]{The measured bias (extracted charge divided by the conversion factor minus the number of photoelectrons)
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| 181 | versus number of photoelectrons,
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| 182 | for spline and digital filter extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 183 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 184 | \label{fig:mc:ConversionvsNphe_DFSpline}
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| 185 | \end{figure}
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| 186 |
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| 187 | \clearpage
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| 188 |
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| 189 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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| 190 |
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| 191 | \subsection{Measurement of the Resolutions \label{sec:mc:resolutions}}
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| 192 |
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| 193 | In order to obtain the resolution of a given extractor, we calculated the RMS of the distribution:
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| 194 |
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| 195 | \begin{equation}
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| 196 | R_{\mathrm{MC}} \approx RMS(\widehat{Q}_{rec} - Q_{sim})
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| 197 | \end{equation}
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| 198 |
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| 199 | where $\widehat{Q}_{rec}$ is the reconstructed charge, calibrated to photo-electrons with the conversion factors obtained in
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| 200 | section~\ref{sec:mc:convfactors}.
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| 201 | \par
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| 202 | One can see that for small signals, small extraction windows yield better resolutions, but extractors which do not
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| 203 | entirely cover the whole pulse, show a clear dependency of the resolution with the signal strength. In the high-gain region,
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| 204 | this is valid for all fixed window extractors up to 6~FADC slices integration region, all sliding window extractors up to 4~FADC
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| 205 | slices and for all spline extractors and the digital filter. Among those extractors with a signal dependent resolution, the
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| 206 | digital filter with 6~FADC slices extraction window shows the smallest dependency, namely 80\% per 50 photo-electrons. This
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| 207 | finding is at first sight in contradiction with eq.~\ref{eq:of_noise} where the (theoretical) resolution depends only on the
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| 208 | noise intensity, but not on the signal strength. Here, the input light distribution of the simulated light pulse introduces the
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| 209 | amplitude dependency (the constancy is recovered for photon signals with no intrinsic input time spread). Here, the main
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| 210 | difference between the spline and digital filter extractors is found: At all intensities, but especially very low intensities, the
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| 211 | resolution of the digital filter is much better than the one for the spline.
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| 212 |
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| 213 | \begin{figure}[htp]
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| 214 | \centering
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| 215 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_FixW_NoNoise_HiGain.eps}
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| 216 | \vspace{\floatsep}
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| 217 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_FixW_WithNoise_HiGain.eps}
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| 218 | \vspace{\floatsep}
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| 219 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_FixW_NoNoise_LoGain.eps}
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| 220 | \vspace{\floatsep}
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| 221 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_FixW_WithNoise_LoGain.eps}
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| 222 | \caption[Charge Resolution Fixed Windows]{The measured resolution (RMS of extracted charge divided by the conversion factor minus the number of photoelectrons) versus number of photoelectrons,
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| 223 | for fixed window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 224 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 225 | \label{fig:mc:ChargeRes_FixW}
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| 226 | \end{figure}
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| 227 |
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| 228 | \begin{figure}[htp]
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| 229 | \centering
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| 230 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_SlidW_NoNoise_HiGain.eps}
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| 231 | \vspace{\floatsep}
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| 232 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_SlidW_WithNoise_HiGain.eps}
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| 233 | \vspace{\floatsep}
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| 234 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_SlidW_NoNoise_LoGain.eps}
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| 235 | \vspace{\floatsep}
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| 236 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_SlidW_WithNoise_LoGain.eps}
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| 237 | \caption[Charge Resolution Sliding Windows]{The measured resolution (RMS of extracted charge divided by the conversion factor minus the number of photoelectrons) versus number of photoelectrons,
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| 238 | for sliding window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 239 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 240 | \label{fig:mc:ChargeRes_SlidW}
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| 241 | \end{figure}
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| 242 |
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| 243 | \begin{figure}[htp]
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| 244 | \centering
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| 245 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_DFSpline_NoNoise_HiGain.eps}
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| 246 | \vspace{\floatsep}
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| 247 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_DFSpline_WithNoise_HiGain.eps}
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| 248 | \vspace{\floatsep}
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| 249 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_DFSpline_NoNoise_LoGain.eps}
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| 250 | \vspace{\floatsep}
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| 251 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_ChargeRes_DFSpline_WithNoise_LoGain.eps}
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| 252 | \caption[Charge Resolution Spline and Digital Filter]{The measured resolution
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| 253 | (RMS of extracted charge divided by the conversion factor minus the number of photoelectrons) versus number of photoelectrons,
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| 254 | for spline and digital filter extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 255 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 256 | \label{fig:mc:ChargeRes_DFSpline}
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| 257 | \end{figure}
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| 258 |
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| 259 | \clearpage
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| 260 |
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| 261 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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| 262 |
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| 263 | \subsection{Arrival Times \label{sec:mc:times}}
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| 264 |
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| 265 | Like in the case of the charge resolution, we calculated the RMS of the distribution of the deviation of the
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| 266 | reconstructed arrival time with respect to the simulated time:
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| 267 |
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| 268 | \begin{equation}
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| 269 | \Delta T_{\mathrm{MC}} \approx RMS(\widehat{T}_{rec} - T_{sim})
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| 270 | \end{equation}
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| 271 |
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| 272 | where $\widehat{T}_{rec}$ is the reconstructed arrival time and $T_{sim}$ the simulated one.
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| 273 | \par
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| 274 | Generally, the time resolutions $\Delta T_{\mathrm{MC}}$ are about a factor 1.5 better than those obtained
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| 275 | from the calibration (section~\ref{sec:cal:timeres}, figure~\ref{fig:time:dep}). This
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| 276 | is understandable since the Monte-Carlo pulses are smaller and
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| 277 | further the intrinsic time spread of the photo-multiplier has not been simulated. Moreover, no time resolution offset was
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| 278 | simulated, thus the reconstructed time resolutions follow about a $1/\sqrt{N_{\mathrm{phe}}}$\,--\,behaviour over the whole low-gain range.
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| 279 | The spline extractors level off in contradiction to what has been found with the calibration pulses.
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| 280 | \par
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| 281 | In figure~\ref{fig:mc:TimeRes_SlidW}, one can see nicely the effect of the addition of noise to the reconstructed time
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| 282 | resolution: While without noise all sliding window extractors with a window size of at least 4~FADC slices show the same time
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| 283 | resolution, with added noise, the resolution degrades with larger extraction window sizes. This can be understood by the fact that
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| 284 | an extractor covers the whole pulse if integrating at least 4~FADC slices and each additional slice can only be affected by the noise.
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| 285 |
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| 286 | \begin{figure}[htp]
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| 287 | \centering
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| 288 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_SlidW_NoNoise_HiGain.eps}
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| 289 | \vspace{\floatsep}
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| 290 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_SlidW_WithNoise_HiGain.eps}
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| 291 | \vspace{\floatsep}
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| 292 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_SlidW_NoNoise_LoGain.eps}
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| 293 | \vspace{\floatsep}
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| 294 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_SlidW_WithNoise_LoGain.eps}
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| 295 | \caption[Time Resolution Sliding Windows]{The measured time resolution (RMS of extracted time minus simulated time)
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| 296 | versus number of photoelectrons,
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| 297 | for sliding window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 298 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 299 | \label{fig:mc:TimeRes_SlidW}
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| 300 | \end{figure}
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| 301 |
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| 302 | \begin{figure}[htp]
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| 303 | \centering
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| 304 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_DFSpline_NoNoise_HiGain.eps}
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| 305 | \vspace{\floatsep}
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| 306 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_DFSpline_WithNoise_HiGain.eps}
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| 307 | \vspace{\floatsep}
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| 308 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_DFSpline_NoNoise_LoGain.eps}
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| 309 | \vspace{\floatsep}
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| 310 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_TimeRes_DFSpline_WithNoise_LoGain.eps}
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| 311 | \caption[Time Resolution Spline and Digital Filter]{The measured time resolution (RMS of extracted time minus simulated time)
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| 312 | versus number of photoelectrons,
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| 313 | for spline and digital filter window extractors in different window sizes. The top plots show the high-gain and the bottom ones
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| 314 | low-gain regions. Left: without noise, right: with simulated noise.}
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| 315 | \label{fig:mc:TimeRes_DFSpline}
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| 316 | \end{figure}
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| 317 |
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| 318 |
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| 319 | %%% Local Variables:
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| 320 | %%% mode: latex
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| 321 | %%% TeX-master: "MAGIC_signal_reco"
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| 322 | %%% TeX-master: "MAGIC_signal_reco"
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| 323 | %%% End:
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| 324 |
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| 325 |
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| 326 |
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| 327 |
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| 328 |
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| 329 |
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| 330 |
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| 331 |
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| 332 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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| 333 |
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| 334 | \clearpage
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| 335 |
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| 336 | \subsection{Charge Signals with and without Simulated Noise \label{fig:mc:sec:mc:chargenoise}}
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| 337 |
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| 338 |
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| 339 | \begin{figure}[htp]
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| 340 | \centering
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| 341 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_Bias_SlidW_HiGain.eps}
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| 342 | \vspace{\floatsep}
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| 343 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_Bias_FixW_HiGain.eps}
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| 344 | \vspace{\floatsep}
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| 345 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_Bias_DFSpline_HiGain.eps}
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| 346 | \caption[Bias due to noise high-gain]{Bias due to noise: Difference of extracted charge of same events, with and without simulated noise,
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| 347 | for different extractor methods in the high-gain region.}
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| 348 | \label{fig:mc:Bias_HiGain}
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| 349 | \end{figure}
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| 350 |
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| 351 | \begin{figure}[htp]
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| 352 | \centering
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| 353 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_Bias_SlidW_LoGain.eps}
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| 354 | \vspace{\floatsep}
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| 355 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_Bias_FixW_LoGain.eps}
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| 356 | \vspace{\floatsep}
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| 357 | \includegraphics[width=0.49\linewidth]{TimeAndChargePlots/TDAS_Bias_DFSpline_LoGain.eps}
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| 358 | \caption[Bias due to noise low-gain]{Bias due to noise: Difference of extracted charge of same events, with and without simulated noise,
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| 359 | for different extractor methods in the low-gain region.}
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| 360 | \label{fig:mc:Bias_LoGain}
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| 361 | \end{figure}
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