The setup coding for SCIENCE frames is INS.FILT1.NAME_DET.NDIT_DET.DIT
The current cascade is: SCI_PAW requires:
a dark imatching in NDIT and DIT
a twilight flat matching in filter and
a photometric standard star observations matching in filter
Science data with DPR.TYPE=OBJECT,EXTENDED (data mode = SCI_EXT), are handled by the
science recipe of the pipeline in a different manner.
The calibration plan of SCI_PAW and SCI_EXT is the same.
calChecker does not check completeness of calibrations used for calibrations.
