I am working in the Euclid Consortium’s External Surveys Organization Unit tasked with developing the software tools to “process” LSST data spanning the Euclid survey and convert the data into the Euclid format for further processing. In short, we use the Rubin Obs LSST Science Pipeline only up to the level of ‘CalibrateTask’ just to do the processing per visit. The calexp and src data products are then converted to the Euclid format for further processing.
We would like to know what pipetask(s) within the current/upcoming release of the LSST Science Pipeline correct for Bandpass Variations across the focal plane? I am wondering if such a task(s) would be performed across visits.
Many thanks in advance for any info you’re able to share.