Changeset 5716


Ignore:
Timestamp:
01/07/05 13:04:32 (20 years ago)
Author:
gaug
Message:
*** empty log message ***
Location:
trunk/MagicSoft/TDAS-Extractor
Files:
4 edited

Legend:

Unmodified
Added
Removed

  • trunk/MagicSoft/TDAS-Extractor/Algorithms.tex

    r5709 r5716  
    1313}
    1414
    15 \subsection{Pure signal extractors}
     15\subsection{Pure Signal Extractors}
    1616
    1717The pure signal extractors have in common that they compute only the
    … …  
    3636As it does not correct for the clock-noise, only an even number of samples is allowed.
    3737
    38 \subsubsection{Fixed Window with global Peak Search}
     38\subsubsection{Fixed Window with Global Peak Search}
    3939
    4040This extractor is implemented in the MARS-class {\textit{MExtractFixedWindowPeakSearch}}.
    … …  
    5858\end{description}
    5959
    60 \subsubsection{Fixed Window with integrated cubic spline}
     60\subsubsection{Fixed Window with Integrated Cubic Spline}
    6161
    6262This extractor is implemented in the MARS-class {\textit{MExtractFixedWindowSpline}}.
    … …  
    6666As it does not correct for the clock-noise, only an odd number of samples is allowed.
    6767
    68 \subsection{Combined extractors}
     68\subsection{Combined Extractors}
    6969
    7070The combined extractors have in common that they compute the arrival time and
    … …  
    101101be chosen} \ldots
    102102
    103 \subsubsection{Sliding Window with amplitude-weighted time}
     103\subsubsection{Sliding Window with Amplitude-Weighted Time}
    104104
    105105This extractor is implemented in the MARS-class {\textit{MExtractTimeAndChargeSlidingWindow}}.
    … …  
    123123\end{description}
    124124
    125 \subsubsection{Cubic Spline with Sliding Window or Amplitude extraction}
     125\subsubsection{Cubic Spline with Sliding Window or Amplitude Extraction}
    126126
    127127This extractor is implemented in the MARS-class {\textit{MExtractTimeAndChargeSpline}}.
    … …  
    369369\end{description}
    370370
    371 \subsubsection{Real fit to the expected pulse shape }
     371\subsubsection{Real Fit to the Expected Pulse Shape }
    372372
    373373This extractor is not yet implemented as MARS-class...

  • trunk/MagicSoft/TDAS-Extractor/Changelog

    r5708 r5716  
    29292004/01/05: Markus Gaug
    3030  * Introduction.tex: Some changes in style
     31  * Algorithms.tex: Fixed section headers
     32  * Reconstruction.tex: text updated
    3133
    32342005/01/04: Hendrik Bartko

  • trunk/MagicSoft/TDAS-Extractor/Pedestal.tex

    r5698 r5716  
    1 \section{Criteria for an optimal pedestal extraction}
     1\section{Criteria for an Pptimal Pedestal Extraction}
    22
    33\ldots {\it In this section, the distinction is made between:
    … …  
    101101where $c$ is the photon/ADC conversion factor  $<ST>/<m_{pe}>$.
    102102
    103 \subsection{How to retrieve Bias $B$ and Error $R$}
     103\subsection{How to Retrieve Bias $B$ and Error $R$}
    104104
    105105$R$ is in general different from the pedestal RMS. It cannot be
    … …  
    130130\end{enumerate}
    131131
    132 \subsubsection{ \label{sec:determiner} Determine error $R$ by applying the signal extractor to a fixed window
    133 of pedestal events}
     132\subsubsection{ \label{sec:determiner} Determine Error $R$ by Applying the Signal Extractor to a Fixed Window
     133of Pedestal Events}
    134134
    135135By applying the signal extractor to a fixed window of pedestal events, we

  • trunk/MagicSoft/TDAS-Extractor/Reconstruction.tex

    r5707 r5716  
    3030
    3131Clearly visible are the high and the low gain pulses. The low gain
    32 pulse is attenuated by a factor of about 10 and delayed by about 50 ns with respect to the high gain pulse.
     32pulse is attenuated by a factor of about 10 and delayed by about 55\,ns with respect to the high gain pulse.
    3333
    34 Figures~\ref{fig:pulpo_shape_low} show the average normalized reconstructed pulse shapes for pulse generator pulses (pulpo setup) in the high and in the low gain, respectively. The input FWHM of the pulse generator pulses is about 2 ns. The FWHM of the average reconstructed high gain pulse shape is about 6.3 ns, while the FWHM of the average reconstructed low gain pulse shape is about 10 ns. The pulse broadening of the low gain pulses with respect to the high gain pulses is due to the electric 50 ns on board delay line of the MAGIC receiver boards. %   while the FWHM of the average reconstructed low gain pulse shape is
     34Figures~\ref{fig:pulpo_shape_low} shows the averaged normalized reconstructed pulse shapes for the ``pulpo''
     35pulses in the high and in the low gain, respectively. The input FWHM of the pulse generator pulses is
     36about 2\,ns. The FWHM of the average reconstructed high gain pulse shape is about 6.3\,ns, while the FWHM of
     37the average reconstructed low gain pulse shape is about 10\,ns. The pulse broadening of the low gain pulses
     38with respect to the high gain pulses is due to the limited dynamic range of the passive 55\,ns on board
     39delay line of the MAGIC receiver boards.
     40%   while the FWHM of the average reconstructed low gain pulse shape is
    3541% Due to the electric delay line for the low gain pules on the receiver board the low gain pulse is widened with respect to the high gain. It has a FWHM of about 10 ns.
    3642
    … …  
    8086%%% mode: latex
    8187%%% TeX-master: "MAGIC_signal_reco"
    82 %%% TeX-master: "MAGIC_signal_reco"
    8388%%% End:
Note: See TracChangeset for help on using the changeset viewer.