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<H2><A NAME="SECTION00691000000000000000">&#160;</A>
 <A NAME="ccd:how-the-data-is-processed">&#160;</A>
<BR>
How the Data is Processed
</H2>
  Before any processing on the input frame is done, the <TT>REDUCE/CCD</TT> 
  command will first collect all resources needed for the calibration of the 
  science frame(s). These include the master calibration frames, the overscan 
  offset, and scaling parameters. So, at this point no operations are 
  done yet. This is done for efficiency reasons: all standard calibration 
  arithmetic on the input frame is done in one go. As an example, 
  suppose the science frame is supposed to be corrected for dark current
  and to be flat fielded. From the Association Table the command first
  identifies the names of the master dark and flat frames, and checks for
  their existence. If they are not present they will be created. 
  Next, the master dark and flat field will be checked on their 
  processing status. If they have not been processed yet, that will first be
  do by another (recursive) run of the <TT>REDUCE/CCD</TT> command. In this
  second run also the scaling factors (<I>i.e.</I> exposure times and 
  the mean of the flat field frame) will be determined.  

<P>
The standard calibration operation is done by a large <TT>COMPUTE/IMAGE</TT>
  with the following input:
  <BR><P></P>
<DIV ALIGN="CENTER">

<!-- MATH: \begin{equation}
out = (in-scan-biasfrm-darkscale*darkfrm) * flatscale/flatfrm
\end{equation} -->

<TABLE WIDTH="100%" ALIGN="CENTER">
<TR VALIGN="MIDDLE"><TD ALIGN="CENTER" NOWRAP>
<I>out</I> = (<I>in</I>-<I>scan</I>-<I>biasfrm</I>-<I>darkscale</I>*<I>darkfrm</I>) * <I>flatscale</I>/<I>flatfrm</I>
</TD>
<TD WIDTH=10 ALIGN="RIGHT">
(3.11)</TD></TR>
</TABLE>
</DIV>
<BR CLEAR="ALL"><P></P>
Here, <I>out</I> is the output frame, <I>in</I> is the input frame, <I>scan</I> is 
  the overscan bias value or frame, <I>biasfrm</I> is the master bias, 
  <I>darkfrm</I> and <I>darkscale</I> are the master dark frame and scaling factor, and 
  <I>flatfrm</I> and <I>flatscale</I> are the master flat field and the mean value of 
  the flat field. In the <TT>COMPUTE</TT> <I>biasfrm</I> and <I>darkfrm</I> can also be
  constants. 

<P>
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
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