1 | \documentclass[12pt]{article}
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2 | \usepackage{magic-tdas}
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3 |
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4 |
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5 | \usepackage[latin1]{inputenc}
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6 |
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7 | \usepackage{amsmath}
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8 | \usepackage{amssymb}
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9 |
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10 | \usepackage{amsthm}
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11 | \usepackage{color}
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12 |
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13 | \usepackage{graphicx}
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14 | \usepackage{caption2}
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15 |
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16 | %\usepackage{citesort}
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17 | \usepackage{url}
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18 | \usepackage{mdwlist}
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19 | \usepackage{lscape}
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20 |
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21 | \setlength{\parindent}{0cm}
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22 |
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23 | \sloppy
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24 |
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25 | \renewcommand{\captionfont}{\small\slshape}
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26 | \renewcommand{\baselinestretch}{1.0}
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27 | \renewcommand{\arraystretch}{1.0}
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28 |
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29 | \begin{document}
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30 |
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31 |
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32 |
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33 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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34 | %% Please, for the formatting just include here the standard
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35 | %% elements: title, author, date, plus TDAScode
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36 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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37 | \title{Comparison of Signal Reconstruction Algorithms for the MAGIC Telescope}
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38 | \author{H. Bartko, M. Gaug, A. Moralejo, \\
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39 | Th. Schweizer, M. Shayduk, N. Sidro, W. Wittek}
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40 | \date{February 28$^{\mathrm{th}}$, 2005\\}
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41 | \TDAScode{MAGIC-TDAS 05-xx\\ 050228}
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42 | %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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43 |
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44 | %% title %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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45 | \maketitle
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46 |
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47 | %% abstract %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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48 | \begin{abstract}
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49 | Presently, the MAGIC telescope uses a 300~MHz FADC system to sample the transmitted and shaped signals from
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50 | the captured Cherenkov light of air showers.
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51 | In this note. different algorithms to reconstruct the signal from the read out samples
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52 | are described and compared. Criteria for comparison are defined and used to judge the
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53 | different extractors applied to calibration signals, cosmics and pedestals. At the end,
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54 | a digital filter fitting the signal over four FADC slices is proposed as the best extractor.
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55 | The question of pedestal calculation for the different extractors is adressed. The digital filter
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56 | is used to extract and fit single photo-electron pulses from the night sky background.
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57 | \end{abstract}
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58 |
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59 | %% contents %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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60 | \newpage
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61 | \tableofcontents
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62 |
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63 | %% body %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
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64 | %\include{pedplots}
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65 | \include{Introduction}
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66 | \include{Reconstruction}
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67 | \include{Algorithms}
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68 | \include{Criteria}
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69 | \include{Pedestal}
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70 | \include{Calibration}
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71 | \include{Pulpo}
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72 | \include{MonteCarlo}
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73 | \include{Speed}
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74 | \include{Results}
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75 | \include{Conclusions}
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76 | %\include{pheplots}
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77 |
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78 | \bibliography{bibfile}
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79 | \bibliographystyle{bibstyle}
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80 |
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81 | \end{document}
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82 |
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83 |
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84 |
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