The second stage of the JWST calibration pipeline processes the uncalibrated slope images to calibrated slope images correcting for some detector/instrument/telescope effects in the process.
The second stage of the calibration pipeline takes as input uncalibrated slope images, corrects for some detector/instrument/telescope effects, and outputs calibrated slope images.
Stage 2 modules:
- CALWEBB_IMAGE2: All imaging data (including coronagraphy and AMI)
- CALWEBB_SPEC2: All spectroscopic data
Published July 11, 2017