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With this command the user can delete and undelete the astrometric
standards used for the transformation, and optionally displays
(slowly) the residuals. Input is the MIDAS table with the coordinates
of the standard stars.
After having displayed the residuals, the programs ask for the
identification of a star to be deleted/restored. This must be
the sequence Number in the MIDAS table and NOT the identifier
of the star. To finish the editing session type 0.
Petra Nass
1999-06-15