Changeset 6286 for trunk/MagicSoft/TDAS-Extractor/Pedestal.tex
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- 02/07/05 20:31:22 (20 years ago)
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trunk/MagicSoft/TDAS-Extractor/Pedestal.tex
r5993 r6286 1 \section{ Criteria for an OptimalPedestal Extraction \label{sec:pedestals}}1 \section{Pedestal Extraction \label{sec:pedestals}} 2 2 3 3 \ldots {\it In this section, the distinction is made between: … … 23 23 (eq.~\ref{eq:autocorr}), 24 24 where the diagonal elements give what is usually denoted as the ``Pedestal RMS''. 25 26 25 \par 27 26 … … 63 62 For the normal image cleaning, knowledge of $B$ is sufficient and the 64 63 error $R$ should be known in order to calculate a correct background probability. 65 66 \par67 \ldots {\textit{\bf THOMAS SCHWEIZER ???}}68 64 \par 69 65 Also for the model analysis $B$ and $R$ are needed if one wants to keep small … … 131 127 \end{enumerate} 132 128 133 \subsubsection{ \label{sec:determiner} Determine $R$ by Applyingthe Signal Extractor to a Fixed Window129 \subsubsection{ \label{sec:determiner} Application of the Signal Extractor to a Fixed Window 134 130 of Pedestal Events} 135 131 136 132 By applying the signal extractor to a fixed window of pedestal events, we 137 determine dthe parameter $R$ for the case of no signal ($ST = 0$). In the case of133 determine the parameter $R$ for the case of no signal ($ST = 0$). In the case of 138 134 all extractors using a fixed window from the beginning (extractors nr. \#1 to \#22 139 in section~\ref{sec:algorithms}), the results are thus by construction the sameas calculating135 in section~\ref{sec:algorithms}), the results are thus the same by construction as calculating 140 136 the mean and the RMS of a same (fixed) number of FADC slices (the conventional ``Pedestal 141 137 Calculation''). 142 138 \par 139 In MARS, this possibility is implemented with a function-call to 140 {\textit{\bf MJPedestal::SetExtractionWithExtractorRndm()}}. 143 141 \par 144 142 In the case of the amplitude extracting spline (extractor nr. \#23), we placed the … … 155 153 \begin{enumerate} 156 154 \item Closed camera and no (Poissonian) fluctuation due to photons from the night sky background 157 \item The camera pointing to a 155 \item The camera pointing to an extra-galactic region with stars in the field of view 158 156 \item The camera illuminated by a continuous light source of high intensity causing much higher pedestal 159 157 fluctuations than in usual observation conditions. … … 199 197 \vspace{\floatsep} 200 198 \includegraphics[height=0.29\textheight]{MExtractTimeAndChargeDigitalFilter_Weights_cosmics_weights.dat_Range_00_18_02_14_Run_38995_Signal_Pixel200.eps} 201 \caption{MExtractTimeAndChargeDigitalFilter: Distribution of extracted "pedestals" from pedestal run with galactic star background for one channel.} 199 \caption{MExtractTimeAndChargeDigitalFilter: Distribution of extracted "pedestals" from pedestal run with 200 extra-galactic star background for one channel.} 202 201 \label{fig:df:distped:run38995} 203 202 \vspace{\floatsep} … … 217 216 \includegraphics[height=0.27\textheight]{MExtractTimeAndChargeDigitalFilter_Weights_cosmics_weights.dat_Range_01_14_02_14_Run_38995_RelMean.eps} 218 217 \caption{MExtractTimeAndChargeDigitalFilter: Difference in mean pedestal (per FADC slice) from pedestal 219 run with galactic star background (in photo-electrons)}218 run with extra-galactic star background (in photo-electrons)} 220 219 \label{fig:df:relmean:run38995} 221 220 \vspace{\floatsep} … … 239 238 \caption{MExtractTimeAndChargeDigitalFilter: Difference pedestal RMS (per FADC slice) with extraction algorithm 240 239 appied on a fixed window, and simply summing up the same number of FADC slices. 241 from pedestal run with galactic star background for inner (left)240 from pedestal run with extra-galactic star background for inner (left) 242 241 and outer (right) pixels. } 243 242 \label{fig:df:relrms:run38995} … … 261 260 \includegraphics[height=0.29\textheight]{MExtractTimeAndChargeSpline_Amplitude_Range_00_10_04_11_Run_38995_Signal_Pixel200.eps} 262 261 \caption{MExtractTimeAndChargeSpline with amplitude: Distribution of extracted "pedestals" from pedestal run 263 with galactic star background for one channel.}262 with extra-galactic star background for one channel.} 264 263 \label{fig:amp:distped:run38995} 265 264 \vspace{\floatsep} … … 281 280 \caption{MExtractTimeAndChargeSpline with amplitude: Difference in mean pedestal (per FADC slice) with extraction algorithm 282 281 appied on a fixed window, and simply summing up the same number of FADC slices 283 Pedestal run with galactic star background.}282 Pedestal run with extra-galactic star background.} 284 283 \label{fig:amp:relmean:run38995} 285 284 \vspace{\floatsep} … … 304 303 \caption{MExtractTimeAndChargeSpline with amplitude: Difference pedestal RMS (per FADC slice) with extraction 305 304 algorithm appied on a fixed window, and simply summing up the same number of FADC slices. 306 Pedestal run with galactic star background for inner (left)305 Pedestal run with extra-galactic star background for inner (left) 307 306 and outer (right) pixels.} 308 307 \label{fig:amp:relrms:run38995} … … 327 326 \includegraphics[height=0.27\textheight]{MExtractTimeAndChargeSpline_Rise-and-Fall-Time_0.5_1.5_Range_01_10_02_12_Run_38995_RelMean.eps} 328 327 \caption{MExtractTimeAndChargeSpline with integral over 2 slices: Difference in mean pedestal (per FADC slice) 329 Pedestal run with galactic star background.}328 Pedestal run with extra-galactic star background.} 330 329 \label{fig:int:relmean:run38995} 331 330 \vspace{\floatsep} … … 346 345 \includegraphics[height=0.25\textheight]{MExtractTimeAndChargeSpline_Rise-and-Fall-Time_0.5_1.5_Range_01_10_02_12_Run_38995_RMSDiff.eps} 347 346 \caption{MExtractTimeAndChargeSpline with integral over 2 slices: Difference pedestal RMS (per FADC slice) 348 from pedestal run with galactic star background for inner (left)347 from pedestal run with extra-galactic star background for inner (left) 349 348 and outer (right) pixels (in photo-electrons).} 350 349 \label{fig:amp:relrms:run38995} … … 358 357 359 358 359 \subsubsection{ \label{sec:determiner} Application of the Signal Extractor to a Sliding Window 360 of Pedestal Events} 361 362 By applying the signal extractor to a sliding window of pedestal events, we 363 determine the bias $B$ and the error $R$. 364 \par 365 In MARS, this possibility is implemented with a function-call to 366 {\textit{\bf MJPedestal::SetExtractionWithExtractor()}}. 367 368 \begin{figure}[htp] 369 \centering 370 \includegraphics[height=0.4\textheight]{SinglePheRatio-28-Run38995.eps} 371 \caption{MExtractTimeAndChargeDigitalFilter: Fit to the ratio of the area beneath the pedestal peak and 372 the single photo-electron(s) peak(s) with extraction algorithm 373 applied on a sliding window of different sizes. 374 A pedestal run with extra-galactic star background has been taken and one exemplary pixel (Nr. 100). 375 A rate of 0.07 phe/ns has been obtained.} 376 \label{fig:df:ratiofit:run38995} 377 \vspace{\floatsep} 378 \includegraphics[height=0.4\textheight]{SinglePheRatio-28-Run39258.eps} 379 \caption{MExtractTimeAndChargeDigitalFilter: Fit to the ratio of the area beneath the pedestal peak and 380 the single photo-electron(s) peak(s) with extraction algorithm 381 applied on a sliding window of different sizes. 382 A pedestal run with galactic star background has been taken and one exemplary pixel (Nr. 100). 383 A rate of 0.09 phe/ns has been obtained.} 384 \label{fig:df:ratiofit:run39258} 385 \end{figure} 386 387 360 388 361 389 %%% Local Variables: 362 390 %%% mode: latex 363 391 %%% TeX-master: "MAGIC_signal_reco" 364 %%% TeX-master: "MAGIC_signal_reco"365 %%% TeX-master: "MAGIC_signal_reco"366 %%% TeX-master: "MAGIC_signal_reco."367 %%% TeX-master: "MAGIC_signal_reco"368 %%% TeX-master: "Pedestal"369 %%% TeX-master: "MAGIC_signal_reco"370 %%% TeX-master: "MAGIC_signal_reco."371 %%% TeX-master: "MAGIC_signal_reco"372 392 %%% End:
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