For a moving target, it is possible to permit the telescope to track at sidereal rate, and adjust the telescope offsets for the motion of a slowly moving target, i.e. one that stays within the field within an observation group. Registration uses the revised offsets and in the mosaic the stars trail while the object does not, and so can be seen and measured more easily.
At present the ephemeris is via a pre-prepared text file, given by
environment variable ORAC_EPHEMERIS, if defined, otherwise
$ORAC_DATA_OUT/target_ephemeris.dat. See one of the
moving-target recipes, say
MOVING_JITTER_SELF_FLAT, for
more details. Once the ephemeris is available as a web service, the
file could become merely a backup; this would automate the process and
so the observer would not have to prepare the file at altitude just
before the epoch of observation.
[_ADJUST_OFFSETS_TO_MOVING_TARGET_]
ORAC-DR -- imaging data reduction