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<H3><A NAME="SECTION00692200000000000000">
Bias, Dark and Flat Field Correction</A>
</H3>
   This part has already been discussed in 
   Section&nbsp;<A HREF="node42.html#ccd:preparing-your-calibration-frames">3.8</A>.
   Depending on the keywords <TT>SC_BSCOR</TT>, <TT>SC_DKCOR</TT>, and 
   <TT>SC_FFCOR</TT> the calibration procedure checks for the availability 
   of the master bias, dark, and flat field calibration frames. If they 
   can not be found they will be created using the input frames listed in the 
   Association Table, and according to the keyword setting for combining.

<P>
The next step after having obtained the calibration frames is to   
   process these frames. For example, after the flat is created/found 
   it will be checked for its processing status. If it has not been 
   processed any on-going calibration (<I>i.e.</I> of a science frame) will be 
   interrupted, and the flat field will be processed. After this has been 
   completed processing of the science frame will continue.

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