Changeset 798 for trunk/ICRC_01
- Timestamp:
- 05/17/01 08:06:03 (24 years ago)
- Location:
- trunk/ICRC_01
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- 1 added
- 1 edited
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trunk/ICRC_01/mccontrib.tex
r783 r798 13 13 \author[1]{O. Blanch} 14 14 \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} 20 19 \correspondence{H. Kornmayer (h.kornmayer@web.de)} 21 20 … … 181 180 the arrival time into account we get the response 182 181 of the trigger and FADC system for that pixel (see 183 also figure \ref{fig_star light}).182 also figure \ref{fig_starresp}). 184 183 This is done for all pixels in the camera. 185 184 … … 207 206 % 208 207 208 \subsection{starlight simulation} 209 210 Due to the big mirror surface the light from the stars around 211 the position of an expected gamma ray source is contributing to 212 the noise in the camera. We developed a program that allows use 213 to simulate the star light together with the generated shower. 214 This program takes all stars in the field of view of the camera 215 around chosen sky region. The light of these stars is track up to 216 the camera taking the frequency of the light into account. 217 After simulating the response of the photo cathode, we 218 get the number of emitted photo electrons per pixel and 219 time. 220 These number is used to generate a noise signal for all the pixels. 221 In figure \ref{fig_starresp} the response of the trigger and the 222 FADC system can be seen for one pixel with a star of 223 magnitude $m = 7$. 224 These stars are typical, because there will 225 be 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 % 242 243 209 244 210 245 \section{Results} … … 224 259 \end{acknowledgements} 225 260 226 \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 % 231 267 232 268 \begin{thebibliography}{99}
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