1 | \documentclass[12pt]{article}
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2 | \usepackage{magic-tdas}
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5 | \usepackage[latin1]{inputenc}
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7 | \usepackage{amsmath}
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8 | \usepackage{amssymb}
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10 | \usepackage{amsthm}
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12 | \usepackage{graphicx}
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14 | \usepackage{citesort}
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15 | \usepackage{url}
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16 |
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17 | \setlength{\parindent}{0cm}
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18 |
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19 | \sloppy
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22 | \renewcommand{\baselinestretch}{1.0}
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23 | \renewcommand{\arraystretch}{1.0}
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24 |
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25 |
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26 |
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27 | \begin{document}
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28 |
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29 |
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30 |
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31 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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32 | %% Please, for the formatting just include here the standard
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33 | %% elements: title, author, date, plus TDAScode
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34 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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35 | \title{Comparison of Signal Reconstruction Algorithms for the MAGIC Telescope}
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36 | \author{H. Bartko, O. Blanch, M. Gaug, F. Goebel, A. Moralejo, A. Robert, \\
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37 | T. Schweizer, M. Shayduk, N. Sidro, W. Wittek}
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38 | \date{Month dd, 2004\\}
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39 | \TDAScode{MAGIC-TDAS 04-xx\\ 04mmdd}
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40 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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41 |
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42 | %% title %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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43 | \maketitle
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44 |
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45 | %% abstract %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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46 | \begin{abstract}
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47 | Presently MAGIC uses a 300~MHz FADC system to sample the Cherenkov signals.
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48 | In this note different algorithms to reconstruct the signal from the read out samples
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49 | are described and compared. Criteria for comparison are defined and used to judge the
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50 | different extractors applied to calibration signals, cosmics and pedestals. At the end,
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51 | a best extractor is proposed. The question
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52 | of pedestal calculation for the different extractors is adressed.
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53 | \end{abstract}
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54 |
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55 | %% contents %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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56 | \thetableofcontents
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57 |
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58 | \newpage
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59 |
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60 | %% body %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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61 |
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62 | %------------------------------------------------------------
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63 |
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64 |
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65 |
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66 | \section{Introduction}
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67 |
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68 | \begin{itemize}
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69 | \item{Short description of the MAGIC read-out system}
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70 | \end{itemize}
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71 |
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72 | \section{Pulse Shape Reconstruction}
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73 |
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74 | \begin{itemize}
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75 | \item{Algorithm: overlay many events}
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76 | \item{Differences cosmics / calibration}
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77 | \item{Implementation / parameterization in the MC.
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78 | \newline
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79 | \newline
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80 | \ldots {\it MAYBE, we should create MC calibration pulses for the subsequent studies }
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81 | \newline
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82 | \newline}
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83 | \end{itemize}
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84 |
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85 | \section{Signal Reconstruction Algorithms}
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86 |
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87 | \ldots {\it In this section, the extractors are described, especially w.r.t. which free parameters are left to play,
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88 | how they subtract the pedestal, how they compare between calibration and cosmics pulses and how an
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89 | extraction in case of a pure pedestal event takes place. }
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90 | \newline
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91 | \newline
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92 | {\it Missing coding:
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93 | \begin{itemize}
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94 | \item Implementing the AB-flag for all extractors \ldots Markus
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95 | \item Implementing a low-gain extraction based on the high-gain information \ldots Arnau
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96 | \item Joining the Sliding Window and Highest Integral extractor into one \ldots Markus
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97 | \item Real fit to the expected pulse shape \ldots Hendrik, Wolfgang ???
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98 | \end{itemize}
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99 | }
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100 |
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101 |
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102 | \subsection{Pure signal extractors}
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103 | \subsubsection{Fixed Window}
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104 | \subsubsection{Fixed Window Peak Search}
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105 | \subsubsection{Fixed Window with integrated spline}
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106 |
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107 | \subsection{Pure time extractors}
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108 | \subsubsection{Highest Integral}
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109 |
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110 | \subsection{Combined extractors}
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111 | \subsubsection{Sliding Window with Highest Integral}
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112 | \subsubsection{Digital Filter}
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113 | \subsubsection{(Fast) Spline with Amplitude extraction}
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114 | \subsubsection{Real fit to the expected pulse shape \newline
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115 | \newline
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116 | }
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117 |
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118 | %References: \cite{OF77} \cite{OF94}.
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119 |
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120 | \section{Criteria for an optimal pedestal extraction}
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121 |
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122 | \ldots {\it In this section, the distinction is made between:
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123 | \begin{itemize}
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124 | \item Defining the pedestal RMS as contribution
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125 | to the extracted signal fluctuations (later used in the calibration)
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126 | \item Defining the Pedestal Mean and RMS as the result of distributions obtained by
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127 | applying the extractor to pedestal runs (yielding biases and modified widths).
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128 | \item Deriving the correct probability for background fluctuations based on the extracted signal height.
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129 | ( including biases and modified widths).
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130 | \end{itemize}
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131 | \ldots Florian + ???
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132 | \newline
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133 | \newline
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134 | }
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135 | \section{Criteria for the Optimal Signal Extraction}
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136 |
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137 | \subsection{Resolution (amplitude and time)}
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138 | \ldots {\it In this section, the jitter to exactly identical input pulses is measured, for times, amplitudes,
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139 | high-gain and low-gain pulses
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140 | \begin{itemize}
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141 | \item Jitter to pulpo pulses \ldots Hendrik
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142 | \item Jitter to pedestals (of different intensity) \ldots Hendrik
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143 | \item Comparing MC signal with and w/o noise of different intensity \ldots Nuria
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144 | \item Comparing the low-gain to high-gain ratio for different intensities \ldots Markus
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145 | \item Derive the time jitter to calibration pulses \ldots Maxim ???
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146 | \end{itemize}
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147 | }
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148 |
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149 | \subsection{Bias}
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150 | \ldots {\it In this section, the bias of the extractor for low and high intensities is defined and measured
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151 | \begin{itemize}
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152 | \item Bias to pedestals (of different intensity) \ldots Hendrik
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153 | \item Comparing MC signal with and w/o noise of different intensity \ldots Nuria
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154 | \end{itemize}
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155 | }
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156 |
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157 | \subsection{Signal to Noise}
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158 | \ldots {\it In this section, the signal to noise of an extractor is determined, for times and amplitudes
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159 | \newline \ldots Maxim ???, Thomas ???
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160 | }
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161 |
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162 | \subsection{Stability}
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163 | \ldots {\it In this section, the stability of an extractor to slightly varying pulse shapes is examined.
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164 | \begin{itemize}
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165 | \item Stability w.r.t. different weights files \ldots Hendrik
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166 | \item Outliers in time and amplitude extractions \ldots ???
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167 | \item Stability of conversion factors from the calibration \ldots Markus
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168 | \item Stability w.r.t. the calibration secondary pulses \ldots Hendrik ???
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169 | \end{itemize}
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170 | }
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171 |
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172 | \subsection{Linearity}
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173 | \ldots {\it In this section, the Nuria plots are examined \newline \ldots Nuria
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174 |
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175 | \subsection{Treatment of calibration pulses}
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176 | \ldots {\it In this section, the question of the different pulse shapes between calibration pulses, its
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177 | secondary pulses, possible secondary pulses from hadronic showers and the typical Cherenkov
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178 | pulses are extracted by the different extractors and typical dependencies examined, like the
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179 | Razmik plot, the number of photo-electrons with number of slices, comparisons between different colours, etc.
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180 | \newline \ldots Hendrik??? , Markus??? + ????}
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181 |
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182 | \subsection{Low gain extraction}
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183 | \ldots {\it In this section, the stability of the low-gain extraction w.r.t. the high-gain extraction is
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184 | examined. Useful plots are still to be defined.
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185 | \newline \ldots Arnau ????}
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186 |
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187 | \subsection{Applicability for different sampling speeds / no pulse shaping.}
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188 | \ldots {\it In this section, some comments of Hendrik will be made}
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189 |
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190 | \subsection{CPU requirements}
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191 | \ldots {\it In this section, the needed CPU time is measured for each extractor independently
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192 | \newline \ldots ALL (after all)}
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193 |
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194 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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195 |
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196 | \section{Performance}
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197 | \ldots {\it This section will be written after the previous one}
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198 |
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199 | \subsection{Calibration}
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200 | \subsection{Pulpo Pulses}
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201 | \subsection{MC Data}
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202 | \subsection{Cosmics Data?}
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203 | \subsection{Pedestals}
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204 |
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205 | \section{Discussion}
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206 | \ldots {\it This section will discuss the best signal extractor \newline \ldots Thomas ???, Florian }
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207 |
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208 | \section{Conclusions}
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209 | \ldots {\it This section will propose the best signal extractor.}
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210 |
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211 | %------------------------------------------------------------------------------
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212 |
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213 |
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214 | \bibliography{bibfile}
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215 | \bibliographystyle{bibstyle}
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216 |
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217 |
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218 | \end{document}
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219 |
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220 |
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221 |
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