I've constructed the collection LATISS/calib/DM-32209 at NCSA. This contains bias, dark, defects, and flats for empty~empty , RG610~empty, SDSSg~empty, and FELH0600~empty. It's a CHAINED collection, so it also contains the camera as well. Processing from raw should need nothing more than -i LATISS/raw/all,LATISS/calib/DM-32209 as the input collections (along with any necessary skymaps).
Verification found a small number of NOISE test failures (flat-corrected image has excessive noise in some amplifiers relative to Poissonian expectation), but these generally fell either on C04 and C11 (which have known defects that aren't fully included in the defect masks) or on C05 and C06 (where there are strong dust spot signatures).
Marking this ticket as Done, and will open a new ticket if updated calibrations are needed.
Improvement
I've constructed the collection LATISS/calib/
DM-32209at NCSA. This contains bias, dark, defects, and flats for empty~empty , RG610~empty, SDSSg~empty, and FELH0600~empty. It's a CHAINED collection, so it also contains the camera as well. Processing from raw should need nothing more than -i LATISS/raw/all,LATISS/calib/DM-32209as the input collections (along with any necessary skymaps).Verification found a small number of NOISE test failures (flat-corrected image has excessive noise in some amplifiers relative to Poissonian expectation), but these generally fell either on C04 and C11 (which have known defects that aren't fully included in the defect masks) or on C05 and C06 (where there are strong dust spot signatures).
Marking this ticket as Done, and will open a new ticket if updated calibrations are needed.