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Timestamp:
03/04/05 14:09:19 (20 years ago)
Author:
gaug
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*** empty log message ***
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  • trunk/MagicSoft/TDAS-Extractor/MAGIC_signal_reco.tex

    r6658 r6744  
    5555It is shown that the digital filter
    5656can be used to extract and fit single photo-electron pulses from the night sky background.
    57 The achievable time resolution can be parameterized to be:
    58 \begin{equation}
    59 \Delta T_{\mathrm{cosmics}} \approx \sqrt{\frac{(2\,\mathrm{ns})^2}{<Q>/{\mathrm{phe}}}
    60 + \frac{(4.5\,\mathrm{ns})^2}{<Q>^2/{\mathrm{phe^2}}} + (0.2\,\mathrm{ns})^2} . \nonumber
    61 \label{eq:time:fitprediction}
    62 \end{equation}
     57The achievable time resolution has been derived as a function of the incident number of
     58photo-electrons.
     59%\begin{equation}
     60%\Delta T_{\mathrm{cosmics}} \approx \sqrt{\frac{(2\,\mathrm{ns})^2}{<Q>/{\mathrm{phe}}}
     61%+ \frac{(4.5\,\mathrm{ns})^2}{<Q>^2/{\mathrm{phe^2}}} + (0.2\,\mathrm{ns})^2} . \nonumber
     62%\label{eq:time:fitprediction}
     63%\end{equation}
    6364For galactic backgrounds an image cleaning threshold as low as 5~photo-electrons can be achieved
    6465without using the timing information and for rejecting 99.7\% of noise.
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