The ingestion and pre-processing activities include a number of steps that are
necessary for any further processing of the data.
The ingestion phase in particular converts the data as received by the DPC
into a data format that is designed and optimized for the photometric processing.
This requires matching information contained in different tables using the available
cross-match information. Trivial unit conversions are also applied in this stage.
Bias correction and computation of predicted positions are important modules in
the pre-processing stage.
Bias correction for the SM and AF observations is taken
care within the IDT pre-processing (see Section 2.3.5).
Only and observations need to be corrected for bias in PhotPipe. This
is done using the same algorithm and software as the one used in IDU.
Predicted positions of sources at the time of observation are required
for the calibration of flux loss and of the geometry of the BP/RP instruments.
The computation of predicted positions at the desired accuracy requires the
availability of astrophysical coordinates for all sources at a higher accuracy
than what is normally available from ground.
For Cycle 02, these were computed from the results of the AGIS processing.