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- Direct and slitless images with perfect WCSs
- catalog information (coordinates, magnitudes ...)
- Exposure times?
- Noise model? Or components of the noise model (gain, exptime, read noise, subtracted background)?
- Or is this already in an uncertainty array?
- Detector signatures already removed (e.g. CALWEBB_DETECTOR1)
- Identification of the pixels in the direct image corresponding to "the source" (e.g. from a segmentation map)
- Identification of any pixels in the direct image corresponding to contaminating sources
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