Ignore:
Timestamp:
05/17/01 08:06:03 (23 years ago)
Author:
harald
Message:
The version of 17.5.2001. Introduction in the first draft.
File:
1 edited

Legend:

Unmodified
Added
Removed
  • trunk/ICRC_01/mccontrib.tex

    r783 r798  
    1313\author[1]{O. Blanch}
    1414\affil[1]{IFAE, Barcelona, Spain}
    15 \author[2]{H. Kornmayer}
    16 \affil[2]{Max-Planck-Institut f\"ur Physik, M\"unchen, Germany}
    17 \author[3]{J.C. Gonzalez}
    18 \affil[3]{Universidad Complutense Madrid, Spain}
    19 
     15\author[2]{J.C.  Gonzalez}
     16\affil[2]{Universidad Complutense Madrid, Spain}
     17\author[3]{H. Kornmayer}
     18\affil[3]{Max-Planck-Institut f\"ur Physik, M\"unchen, Germany}
    2019\correspondence{H. Kornmayer (h.kornmayer@web.de)}
    2120
     
    181180the arrival time into account we get the response
    182181of the trigger and FADC system for that pixel (see
    183 also figure \ref{fig_starlight}).
     182also figure \ref{fig_starresp}).
    184183This is done for all pixels in the camera.
    185184
     
    207206%
    208207
     208\subsection{starlight simulation}
     209
     210Due to the big mirror surface the light from the stars around
     211the position of an expected gamma ray source is contributing to
     212the noise in the camera. We developed a program that allows use
     213to simulate the star light together with the generated shower.
     214This program takes all stars in the field of view of the camera
     215around chosen sky region. The light of these stars is track up to
     216the camera taking the frequency of the light into account.
     217After simulating the response of the photo cathode, we
     218get the number of emitted photo electrons per pixel and
     219time.
     220These number is used to generate a noise signal for all the pixels.
     221In figure \ref{fig_starresp} the response of the trigger and the
     222FADC system can be seen for one pixel with a star of
     223magnitude $m = 7$.
     224These stars are typical, because there will
     225be always one $7^m$ star in the trigger area of the camera.
     226%
     227%
     228%
     229\begin{figure}[h]
     230 \vspace*{2.0mm} % just in case for shifting the figure slightly down
     231 \includegraphics[width=8.3cm]{signal.eps} % .eps for Latex,
     232                                            % pdfLatex allows .pdf, .jpg, .png and .tif
     233 \caption{The response of a pixel due to a star with magnitude
     234 $m=7$ in the field of view. On the left plot the response of the
     235 trigger system is plotted while on the right plot the content in the
     236 FADC system is shown.}
     237 \label{fig_starresp}
     238\end{figure}
     239%
     240%
     241%
     242
     243
    209244
    210245\section{Results}
     
    224259\end{acknowledgements}
    225260
    226 \appendix
    227 
    228 \section{Appendix section 1}
    229 
    230 Text in appendix.
     261%\appendix
     262%
     263%\section{Appendix section 1}
     264%
     265%Text in appendix.
     266%
    231267
    232268\begin{thebibliography}{99}
Note: See TracChangeset for help on using the changeset viewer.