deletions | additions       diff --git a/floydsauto.tex b/floydsauto.tex  index 4fc4e53..b659c56 100644  --- a/floydsauto.tex  +++ b/floydsauto.tex 
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\usepackage{listings}  \section{FLOYDS Data Products}  Here we describe the data products available to the end user that are available in a tar file. \textbf{floydsauto} is the executable used to perform the   \emph{automatic reductions} at LCOGT headquarters.  
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standard star was observed the same night, a tar file of automatic  reductions for the standard frames will also be produced. The tar file  for standard prereduced frames will all start with "STD", e.g.:  \begin{small}  \begin{verbatim} \begin{lstlisting}  LCO2013A-003_fts_20130727_56503.tar.gz  STD_fts_20130727_56503.tar.gz  \end{verbatim}  \end{small} \end{lstlisting}  Each tar file will contain the following files:  \begin{small}  \begin{verbatim} \begin{lstlisting}  ESO323G077_offset_fts_20130727_red_2.0_56505_1.fits (Trimmed raw red part of the science frame)  ESO323G077_offset_fts_20130727_blue_2.0_56505_1.fits (Trimmed raw blue part of the science frame)  arc_ESO323G077_fts_20130727_red_2.0_56505_1.fits (Trimmed raw red part of the arc frame) 
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ttflatESO323G077_offset_fts_20130727_blue_2.0_56505_1.fits (rectified blue part of the flat frame)  ttflatESO323G077_offset_fts_20130727_red_2.0_56505_1.fits (rectified red part of the flat frame)  nttESO323G077_offset_fts_20130727_red_2.0_56505_1.fits (flat-field corrected red part of the science frame) ttESO323G077_offset_fts_20130727_blue_2.0_56505_1_2df.fits (2D flux calibrated blue frame)  ttESO323G077_offset_fts_20130727_red_2.0_56505_1_2df.fits (2D flux calibrated red frame)  nttESO323G077_offset_fts_20130727_red_2.0_56505_1_2df.fits (2D flat-field corrected, flux calibrated red frame)  nttESO323G077_offset_fts_20130727_merge_2.0_56505_1_2df_ex.fits (fast reduction 1D spectrum)  \end{verbatim}  \end{small} \end{lstlisting}  In summary, the extension ``\emph{2df}" "\emph{2df}"  indicates a flux calibrated spectrum, the prefix ``\emph{tt}" "\emph{tt}"  indicates that the frame has been geometrically \emph{transformed} along x- and y-axes, ``\emph{n}" "\emph{n}"  indicates that the frame has been flat field corrected. The typical  science name is composed (in order) of object name, telescope,  observation date, ``blue" "blue"  or ``red" "red"  (indicating second or first order), slit width, and MJD date when the reduction was performed.  Note that the user may reextract the spectrum from the blue and 
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summary pdf file is shown in Fig. \ref{fig:summer}.   Filenames are of the form:  \begin{small}  \begin{verbatim} \begin{lstlisting}  LCO2013A-003_fts_20130727_56503.tar  LCO2013A-003_fts_20130727_56503.pdf  \end{verbatim}  \end{small} \end{lstlisting}