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Besides the standard product described in the previous sections, a number
of additional commands is implemented or will be considered and implemented
later. E.g. within MIDAS a command to remove cosmic rays already
exists. Hence, this command can be implemented in the standard CCD
pipeline procedure.
After the data have been calibrated, one might need to combine a number
of science frames into a combined frame. A tool for doing this should
correct for possible differences in sky background, exposure time,
positions, etc. In a previous version of the CCD context such a tool did
exist. We might consider porting this tool to the new CCD context.
Petra Nass
1999-06-15