From dc1752ece277963f98fb96800a07c1dd8208612e Mon Sep 17 00:00:00 2001
From: Andreas Kopmann <andreas.kopmann@kit.edu>
Date: Tue, 31 Jul 2012 23:57:04 +0200
Subject: Initial version of the UFO camera users manual

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+% Appendix to the UFO camera user manual
+%
+
+\begin{appendix}
+
+\chapter{Camera characterization}
+\label{camera_char}
+
+Camera characterization is done in IEKP using tungsten X-ray tube, and ANKA detector lab, using visible light.
+Estimation of dark noise is given in \figurename~\ref{darknoise}. Camera setting for long integration time is setting the PGA value (analog gain) on address 102 to 0, which is a default value. For short integration time, PGA value is 3, which is a maximum one. Other sensor register values, unless otherwise stated, are recommended values.
+
+\begin{figure}[ht]
+\centering
+\includegraphics[width=0.70\textwidth]{images/camera_char1.png}
+\caption{\label{darknoise}The total dark noise vs. integration time at different camera settings}
+\end{figure}
+\begin{table}[h]
+\begin{center}
+{\begin{tabular}{|c|c|}
+\hline
+Parameters & Values \\ 
+\hline
+Quantum efficiency &  57.41 \% \\
+\hline
+Dark noise  $\sigma_{d}$ &  10 $e^{-}$\\
+\hline
+Dynamic range & 57.22 dB \\
+\hline
+Conversion factor	& 7.82 $e^{-}/{DN}$ \\
+\hline
+\end{tabular}}
+\caption{10 bit characterization of UFO camera}
+\label{char_10b}
+\end{center}
+\end{table}
+
+
+
+\end{appendix}
+
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