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For astronomical applications, conversion from other data formats can be
done through FITS format. The FITS image must reside on disk.
Disk FITS conversion can be a non-trivial task is the input FITS file
has a complex structure. Several tools are thus available
- FITS_GILDAS (FITS to GILDAS) and GILDAS_FITS (GILDAS to FITS) Tasks
can process simple FITS files
- VECTORFITS FitsFile.fits FROM|TO GildasImage.gdf
provide a command line equivalent to the above tasks. Since FITS keywords are not fully normalized, although a standard subset is recommended, this command supports keyword redefinition. If you
receive a tape with source name coded as SOURCE (instead of OBJECT), all you need to do is to define a SIC symbol named SOURCE with translation OBJECT. This is done simply by typing the
command
SIC\SYMBOL SOURCE OBJECT
This trick does not work with the FITS_GILDAS task.
- SICDEFINE FITS Var FitsFile is similar to DEFINE IMAGE, and will create
a SIC structure which will copy the FITS file content. The LET command can be then used to copy (part of) this structure into an Image variable if needed, and thus convert to the image format.
It only works on existing FITS file however, and cannot be used to create a FITS file from
a SIC structure.
- SICDEFINE IMAGE will automatically attempt to convert a FITS file into
the Gildas equivalent, using the same method as FITS_GILDAS. This will work transparently
on simple FITS images (with no FITS XTENSION).
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Gildas manager
2014-07-01