DM-33959 has been bumped up the priority list for pipelines. We're expecting a fix to land in w15. DM-31855 is essentially a duplicate so this has been marked as 'won't fix. This would apply astrometric and and photometric calibrations to source parquet tables.
Would a second matching step need to run to make table of matched sources?
Prior issues with AuxTel photometric calibration issues now understood, a bug to the calibrated fluxes written to parquet tables was discovered and a fix is under development (see
DM-34019
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Getting issue details...STATUS
). For now, we can still calibrate fluxes using AFW tables and photoCalib object. Calibration is good but shows some systematics in scatter.
I need to generate/register a skymap for the different fields in order perform co-addition, is there a way to do this outside of repo/main to allow for experimentation?
butler register-skymap --config-file /path/to/file /path/to/repo (could experiment on rc2subset, example config in obs_lsst )
Are there any single-visit/detector level metrics are implemented now in Faro that are worth running on the afw tables we have already generated?
Keith Bechtol to make a ticket to better understand mapping of these camera and calibration products characterization efforts to verification documents and the focus of these efforts. Discuss with the SCLT
