Changeset 5598

Timestamp:

12/14/04 22:35:58 (20 years ago)

Author:

hbartko

Message:

*** empty log message ***

Location:

trunk/MagicSoft/TDAS-Extractor

Files:

• Algorithms.tex (modified) (1 diff)
• Changelog (modified) (1 diff)
• Reconstruction.tex (modified) (1 diff)
• noise_autocorr_AB_36038_TDAS.eps (added)
• w_amp_MC_input_TDAS.eps (added)
• w_time_MC_input_TDAS.eps (added)

trunk/MagicSoft/TDAS-Extractor/Algorithms.tex

@@ -289 +289 @@
 %\end{equation}
 
+\begin{figure}[h!]
+\begin{center}
+\includegraphics[totalheight=7cm]{noise_autocorr_AB_36038_TDAS.eps}
+\end{center}
+\caption[Noise autocorrelation.]{Noise autocorrelation matrix for open camera including the noise due to night sky background fluctuations.} \label{fig:noise_autocorr_AB_36038_TDAS}
+\end{figure}
+
+\begin{figure}[h!]
+\begin{center}
+\includegraphics[totalheight=7cm]{w_time_MC_input_TDAS.eps}
+\end{center}
+\caption[Time weights.]{Time weights.} \label{fig:w_time_MC_input_TDAS}
+\end{figure}
+
+\begin{figure}[h!]
+\begin{center}
+\includegraphics[totalheight=7cm]{w_amp_MC_input_TDAS.eps}
+\end{center}
+\caption[Amplitude weights.]{Amplitude weights.} \label{fig:w_amp_MC_input_TDAS}
+\end{figure}
+
 
 

trunk/MagicSoft/TDAS-Extractor/Changelog

@@ -23 +23 @@
   * Introduction.tex: wrote some introduction, including
                       new figure Magic_readout_scheme1.eps
-  * Reconstruction.tes: wrote something about the pulse reconstruction
+  * Reconstruction.tex: wrote something about the pulse reconstruction
                         new figures: pulpo_shape_high_low_TDAS.eps
                                      pulpo_shape_high_low_MC_TDAS.eps
                                      shape_green_UV_data_TDAS.eps 
+  * Algorithms.tex:included new figures:w_time_MC_input_TDAS.eps
+                                        w_amp_MC_input_TDAS.eps                
+                                        noise_autocorr_AB_36038_TDAS.eps
   * bibfile.bib: included two more references about optical link and
                  PMTs

trunk/MagicSoft/TDAS-Extractor/Reconstruction.tex

@@ -26 +26 @@
 \end{figure}
 
-Figure \ref{fig:shape_green_high} shows the normalized average reconstructed pulse shape for green and UV calibration LED pulses \cite{MAGIC-calibration} as well as the normalized average reconstructed pulse shape for cosmics events. The pulses shape has a FWHM of about 6.5 ns and a significant tail.
+Figure \ref{fig:shape_green_high} shows the normalized average reconstructed pulse shape for green and UV calibration LED pulses \cite{MAGIC-calibration} as well as the normalized average reconstructed pulse shape for cosmics events. The pulse shape of the UV calibration pulses is quite similar to the reconstructed pulse shape for cosmics events, both have a FWHM of about 6.5 ns. As air showers due to hadronic cosmic rays trigger the telescope much more frequently than gamma showers the reconstructed pulse shape of the cosmics events corresponds mainly to hadron induced showers. The pulse shape due to electromagnetic air showers might be slightly different. The pulse shape for green calibration LED pulses is wider and has a pronounced tail.
+
+
+% The pulses shape has a FWHM of about 6.5 ns and a significant tail.