Updated missing files

Author: ronnyerrmann

HiFLEx_UserManual.pdf

@@ -106,6 +106,7 @@ \section{Changelog (recently)}
 \subsection*{v1.3.6}
 \begin{itemize}\setlength\itemsep{0em}
   \item New parameter \verb|split_wavelength_solutions_at| to create wavelength solution when several chips are combined into one image.
+  \item Improved finding the shift of the ThAr lines to the wavelength solution.
 \end{itemize}
 
 \subsection*{v1.3.5}
@@ -1004,7 +1005,7 @@ \subsubsection{Getting the data}
 % HD 10180: G1V star with 7 planets: http://ui.adsabs.harvard.edu/abs/2011A%26A...528A.112L
 Search and download the data from \url{http://archive.eso.org/eso/eso_archive_main.html}. Check only 'HARPS/LaSilla'. For example data select night '2015 07 30' to find data of the asteroid Ceres, use '2004 07 12' and Program ID '072.C-0488(E)' for calibration data taken by the RV exoplanet search team, or use 2010 10 23/25 for HD\,10180 observation. Then download the data (save the download request script, cd to the folder, and run \verb|sh  downloadRequest<Number>script.sh|). The raw data (*.fits.Z) can be extracted with:
 
-\textbf{Extract both chips together (after identifting the order, a dummy order has to be added):}
+\textbf{Extract both chips together (after identifting the order, a dummy order has to be added, don't use background correction):}
 \begin{lstlisting}[style=base]
 gunzip *.fits.Z
 cat <<EOT > extract_single_chip.py
@@ -1141,11 +1142,11 @@ \subsubsection{HARPS data reduced by the ESO Phase 3 pipeline}
 Few problems occur when comparing the data of reduced with this pipeline and the data from the ESO Phase 3 pipeline:
 \begin{enumerate}\setlength\itemsep{0em}
   \item The bias correction can't be performed, as usually only one bias frame is available.
-  \item Overscan correction is not implemented in the pipeline.
+  \item Overscan correction is not implemented in HiFLEx.
   \item No cosmic ray removal is applied.
   \item Different flat fielding.
-  \item Traces have a fixed width, therefore the S/N of the extracted data might decrease slightly.
-  \item Only one CCD is processed at a time, which might decrease the precision of the wavelength solution.
+  %\item Traces have a fixed width, therefore the S/N of the extracted data might decrease slightly.
+  %\item Only one CCD is processed at a time, which might decrease the precision of the wavelength solution.
 \end{enumerate}
 
 \subsubsection{Analysing the reduced HARPS data with TERRA}