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eso-midas-doc-13SEPpl1.2-3.mga5.i586.rpm

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<H2><A NAME="SECTION00661000000000000000">&#160;</A>
 <A NAME="ccd:loading-telescope-instrument-specifications">&#160;</A>
<BR>
Loading the Telescope and Instrument Specifications
</H2>
  For reducing data from ESO instrumentation it is assumed that the 
  FITS headers conform the standards set by the document ``ESO Archive, 
  Data Interface Requirements''. In particular, the ESO specific 
  parameters are stored in a special set of FITS keywords (the ESO 
  hierarchical keywords). Using this standard, while reading in 
  the data FITS keywords are stored in well defined MIDAS descriptors 
  of the MIDAS frames.

<P>
As an example, in the ESO case the exposure type is stored in the ESO 
  hierarchical FITS keyword `HIERARCH ESO GEN EXPO TYPE'. The ESO-MIDAS 
  FITS reader converts that keyword into the MIDAS descriptor _EGE_TYPE. 
  Among the valid exposure types are (according the ESO Archive document): 
  <TT>bias</TT>, <TT>ff</TT>, <TT>ff-dome</TT>, <TT>ff-screen</TT>, <TT>ff-sky</TT>, 
  <TT>dk</TT>, <TT>sci</TT>. Therefore, when the CCD context is started or after 
  executing the command <TT>INIT/CCD</TT> links are created between the frame 
  descriptors and the corresponding CCD keyword. With these links the 
  CCD package knows which exposure types are used and which frame descriptor 
  contains the exposure type. 

<P>
To fill the CCD keywords with these descriptor names a separate procedure 
  is used: <TT>eso_descr.prg</TT>. A copy of this procedure is put in
  your working directory.
  If you need to change one or more descriptor names (<I>e.g.</I> the 
  descriptor name of the exposure time), make the modification(s) 
  and run the modified procedure, using <TT>@@ eso_descr</TT>. 

<P>
The CCD package has been developed to reduce CCD data coming from ESO's 
  telescopes on La Silla. However, some flexibility has been built-in to 
  enable the reduction of data coming from non-ESO telescope/instrument 
  combinations, cases in which the telescope and instrument parameters 
  are different. To fill the CCD keywords with the telescope and instrument
  setup parameters, like name of the telescope, CCD used, read-out noise, 
  frame size, etc. the command <TT>LOAD/CCD</TT> can be used. This command reads 
  these parameters for the MIDAS table <TT>eso_specs.tbl</TT> that, in case 
  it is not present in your working directory, will be created. At 
  initialization of the CCD context a copy of this table is put in the user's
  directory. In case non-ESO observing facilities have been used, or you want
  to modify or append the table with your own setup parameters, you can use
  the standard table commands <I>e.g.</I> <TT>EDIT/TABLE</TT>.

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