Reduce an ACSIS science observation, without baselining
This recipe is suitable for ACSIS using either the RxA3, RxA3m or HARP backends.
A spatial/spectral cube whose filename is of the form gaYYYYMMDD_N, where YYYYMMDD is the UT date, and N is the group number. This is the coadded group file.
Spatial/spectral cubes whose filenames are of the form aYYYYMMDD_M, where YYYYMMDD is the UT date, and M is the observation number. These are created in case the data are not marked as good and so are reduced individually at CADC.
log.efficiency, only if the object is a planet for which this is allowed (URANUS, MARS or JUPITER).