Describe point source centroiding procedure existing in HDRL/CPL
Hi @buddel : @jpott and @verdoes just now contemplated requirements on the point source centroiding procedure for the AO PSF of stellar point sources in the science images and the PSFs produced by the pinholes in the Warm and Cold Astrometric Mask.
Could you point us two to ESO's (and/or your) description of the point source centroiding procedure that already exists in the High-level Data Reduction Library and/or Common Pipeline Library?
Then we can evaluate of that suffices MICADO's needs for distortion calibration or not.
Thanks, Gijs