Index: trunk/MagicSoft/TDAS-Extractor/Criteria.tex
===================================================================
--- trunk/MagicSoft/TDAS-Extractor/Criteria.tex	(revision 6473)
+++ trunk/MagicSoft/TDAS-Extractor/Criteria.tex	(revision 6474)
@@ -17,4 +17,9 @@
 
 \subsection{Applicability for Different Sampling Speeds / No Pulse Shaping.}
+The current read-out system of the MAGIC telescope \cite{Magic-DAQ} with 300 MSamples/s is relatively slow compared to the fast pulses of about 2 ns FWHM of Cherenkov pulses. To acquire the pulse shape an artificial pulse shaping to about 6.5 ns FWHM is used. Thereby also more LONS is integrated that acts as noise. 
+
+For 2 ns FWHM fast pulses a 2 GSamples/s FADC provides at least 4 sampling points. This permits a reasonable reconstruction of the pulse shape. First prototype tests with fast digitization systems for MAGIC have been successfully conducted \cite{GSamlesFADC}. The signals have been reconstructed within the common MAGIC Mars software framework.
+
+
 \ldots {\textit Some comments by Hendrik ...}
 
Index: trunk/MagicSoft/TDAS-Extractor/Introduction.tex
===================================================================
--- trunk/MagicSoft/TDAS-Extractor/Introduction.tex	(revision 6473)
+++ trunk/MagicSoft/TDAS-Extractor/Introduction.tex	(revision 6474)
@@ -39,5 +39,5 @@
 resolution of 8 bit only, the signals are split into two branches with gains differing by a factor 10. 
 One branch is delayed by 55\,ns and then both branches are multiplexed and consecutively read-out by one FADC.
-Figure~\ref{fig:pulpo_shape_high} shows a typical average of identical input signals.
+Figure~\ref{fig:pulpo_shape_high} shows a typical average of identical input signals. A more detailed overview about the MAGIC read-out and DAQ system is given in \cite{Magic-DAQ}.
 % The maximum sustained trigger rate could be 1 kHz. The FADCs feature a FIFO memory which allows a significantly higher short-time rate.
 % Obviously by doing this, more LONS is integrated and thus the performance of the telescope on the analysis level is degraded. 
Index: trunk/MagicSoft/TDAS-Extractor/MAGIC_signal_reco.bbl
===================================================================
--- trunk/MagicSoft/TDAS-Extractor/MAGIC_signal_reco.bbl	(revision 6473)
+++ trunk/MagicSoft/TDAS-Extractor/MAGIC_signal_reco.bbl	(revision 6474)
@@ -12,4 +12,10 @@
   on optical fibers},
 \newblock Nucl. Instrum. Meth. {\bf A461} (2001) 517.
+
+\bibitem{Magic-DAQ}
+J.~Cortina et~al. (MAGIC Collab.),
+\newblock {\em The data acquisition of the MAGIC telescope},
+\newblock Prepared for International Symposium: The Universe Viewed in Gamma
+  Rays, Kashiwa, Chiba, Japan, 25-28 Sep 2002.
 
 \bibitem{MC-Camera}
@@ -38,4 +44,9 @@
 \newblock McGraw-Hill, 1977.
 
+\bibitem{GSamlesFADC}
+H.~Bartko et~al.,
+\newblock {\em TDAS 0501 Prototype Tests of a Multiplexed Fiber-Optic Ultra
+  Fast FADC Data Acquisition System for the MAGIC Telescope}, 2005.
+
 \bibitem{hardware-manual}
 M.~Gaug,
Index: trunk/MagicSoft/TDAS-Extractor/bibfile.bib
===================================================================
--- trunk/MagicSoft/TDAS-Extractor/bibfile.bib	(revision 6473)
+++ trunk/MagicSoft/TDAS-Extractor/bibfile.bib	(revision 6474)
@@ -1,2 +1,16 @@
+@manual{GSamlesFADC,
+     author    = "Bartko, H. and others",
+     title     = "TDAS 0501 Prototype Tests of a Multiplexed Fiber-Optic Ultra Fast FADC Data Acquisition System for the MAGIC Telescope",
+     year      = "2005"
+}
+
+@Article{Magic-DAQ,
+     author    = "Cortina, J. and others",
+ collaboration = "MAGIC",
+     title     = "The data acquisition of the MAGIC telescope",
+     note      = "Prepared for International Symposium: The Universe Viewed
+                  in Gamma Rays, Kashiwa, Chiba, Japan, 25-28 Sep 2002"
+}
+
 @manual{MC-Camera,
      author    = "Blanch,O. and Moralejo,A.",