source: trunk/MagicSoft/TDAS-Extractor/MAGIC_signal_reco.tex@ 5232

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1\documentclass[12pt]{article}
2\usepackage{magic-tdas}
3
4
5\usepackage[latin1]{inputenc}
6
7\usepackage{amsmath}
8\usepackage{amssymb}
9
10\usepackage{amsthm}
11
12\usepackage{graphicx}
13
14\usepackage{citesort}
15\usepackage{url}
16
17\setlength{\parindent}{0cm}
18
19\sloppy
20
21
22\renewcommand{\baselinestretch}{1.0}
23\renewcommand{\arraystretch}{1.0}
24
25
26
27\begin{document}
28
29
30
31%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
32%% Please, for the formatting just include here the standard
33%% elements: title, author, date, plus TDAScode
34%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
35\title{Comparison of Signal Reconstruction Algorithms for the MAGIC Telescope}
36\author{H. Bartko, O. Blanch, M. Gaug, F. Goebel, A. Moralejo, A. Robert, \\
37T. Schweizer, M. Shayduk, N. Sidro, W. Wittek}
38\date{Month dd, 2004\\}
39\TDAScode{MAGIC-TDAS 04-xx\\ 04mmdd}
40%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
41
42%% title %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
43\maketitle
44
45%% abstract %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
46\begin{abstract}
47Presently MAGIC uses a 300~MHz FADC system to sample the Cherenkov signals.
48In this note different algorithms to reconstruct the signal from the read out samples
49are described and compared. Criteria for comparison are defined and used to judge the
50different extractors applied to calibration signals, cosmics and pedestals. At the end,
51a best extractor is proposed. The question
52of pedestal calculation for the different extractors is adressed.
53\end{abstract}
54
55%% contents %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
56\thetableofcontents
57
58\newpage
59
60%% body %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
61
62%------------------------------------------------------------
63
64
65
66\section{Introduction}
67
68\begin{itemize}
69\item{Short description of the MAGIC read-out system}
70\end{itemize}
71
72\section{Pulse Shape Reconstruction}
73
74\begin{itemize}
75\item{Algorithm: overlay many events}
76\item{Differences cosmics / calibration}
77\item{Implementation / parameterization in the MC.
78\newline
79\newline
80\ldots {\it MAYBE, we should create MC calibration pulses for the subsequent studies }
81\newline
82\newline}
83\end{itemize}
84
85\section{Signal Reconstruction Algorithms}
86
87\ldots {\it In this section, the extractors are described, especially w.r.t. which free parameters are left to play,
88how they subtract the pedestal, how they compare between calibration and cosmics pulses and how an
89extraction in case of a pure pedestal event takes place. }
90\newline
91\newline
92{\it Missing coding:
93\begin{itemize}
94\item Implementing the AB-flag for all extractors \ldots Markus
95\item Implementing a low-gain extraction based on the high-gain information \ldots Arnau
96\item Joining the Sliding Window and Highest Integral extractor into one \ldots Markus
97\item Real fit to the expected pulse shape \ldots Hendrik, Wolfgang ???
98\end{itemize}
99}
100
101
102\subsection{Pure signal extractors}
103\subsubsection{Fixed Window}
104\subsubsection{Fixed Window Peak Search}
105\subsubsection{Fixed Window with integrated spline}
106
107\subsection{Pure time extractors}
108\subsubsection{Highest Integral}
109
110\subsection{Combined extractors}
111\subsubsection{Sliding Window with Highest Integral}
112\subsubsection{Digital Filter}
113\subsubsection{(Fast) Spline with Amplitude extraction}
114\subsubsection{Real fit to the expected pulse shape \newline
115\newline
116}
117
118%References: \cite{OF77} \cite{OF94}.
119
120\section{Criteria for an optimal pedestal extraction}
121
122\ldots {\it In this section, the distinction is made between:
123\begin{itemize}
124\item Defining the pedestal RMS as contribution
125to the extracted signal fluctuations (later used in the calibration)
126\item Defining the Pedestal Mean and RMS as the result of distributions obtained by
127applying the extractor to pedestal runs (yielding biases and modified widths).
128\item Deriving the correct probability for background fluctuations based on the extracted signal height.
129 ( including biases and modified widths).
130\end{itemize}
131\ldots Florian + ???
132\newline
133\newline
134}
135\section{Criteria for the Optimal Signal Extraction}
136
137\subsection{Resolution (amplitude and time)}
138\ldots {\it In this section, the jitter to exactly identical input pulses is measured, for times, amplitudes,
139high-gain and low-gain pulses
140\begin{itemize}
141\item Jitter to pulpo pulses \ldots Hendrik
142\item Jitter to pedestals (of different intensity) \ldots Hendrik
143\item Comparing MC signal with and w/o noise of different intensity \ldots Nuria
144\item Comparing the low-gain to high-gain ratio for different intensities \ldots Markus
145\item Derive the time jitter to calibration pulses \ldots Maxim ???
146\end{itemize}
147}
148
149\subsection{Bias}
150\ldots {\it In this section, the bias of the extractor for low and high intensities is defined and measured
151\begin{itemize}
152\item Bias to pedestals (of different intensity) \ldots Hendrik
153\item Comparing MC signal with and w/o noise of different intensity \ldots Nuria
154\end{itemize}
155}
156
157\subsection{Signal to Noise}
158\ldots {\it In this section, the signal to noise of an extractor is determined, for times and amplitudes
159\newline \ldots Maxim ???, Thomas ???
160}
161
162\subsection{Stability}
163\ldots {\it In this section, the stability of an extractor to slightly varying pulse shapes is examined.
164\begin{itemize}
165\item Stability w.r.t. different weights files \ldots Hendrik
166\item Outliers in time and amplitude extractions \ldots ???
167\item Stability of conversion factors from the calibration \ldots Markus
168\item Stability w.r.t. the calibration secondary pulses \ldots Hendrik ???
169\end{itemize}
170}
171
172\subsection{Linearity}
173\ldots {\it In this section, the Nuria plots are examined \newline \ldots Nuria
174
175\subsection{Treatment of calibration pulses}
176\ldots {\it In this section, the question of the different pulse shapes between calibration pulses, its
177secondary pulses, possible secondary pulses from hadronic showers and the typical Cherenkov
178pulses are extracted by the different extractors and typical dependencies examined, like the
179Razmik plot, the number of photo-electrons with number of slices, comparisons between different colours, etc.
180\newline \ldots Hendrik??? , Markus??? + ????}
181
182\subsection{Low gain extraction}
183\ldots {\it In this section, the stability of the low-gain extraction w.r.t. the high-gain extraction is
184examined. Useful plots are still to be defined.
185\newline \ldots Arnau ????}
186
187\subsection{Applicability for different sampling speeds / no pulse shaping.}
188\ldots {\it In this section, some comments of Hendrik will be made}
189
190\subsection{CPU requirements}
191\ldots {\it In this section, the needed CPU time is measured for each extractor independently
192\newline \ldots ALL (after all)}
193
194%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
195
196\section{Performance}
197\ldots {\it This section will be written after the previous one}
198
199\subsection{Calibration}
200\subsection{Pulpo Pulses}
201\subsection{MC Data}
202\subsection{Cosmics Data?}
203\subsection{Pedestals}
204
205\section{Discussion}
206\ldots {\it This section will discuss the best signal extractor \newline \ldots Thomas ???, Florian }
207
208\section{Conclusions}
209\ldots {\it This section will propose the best signal extractor.}
210
211%------------------------------------------------------------------------------
212
213
214\bibliography{bibfile}
215\bibliographystyle{bibstyle}
216
217
218\end{document}
219
220
221
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