Page History

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• Retire aXe
• Retire aXeSIM
• Leverage the JWST infrastructure
  • just crds, gwcs and asdf?
• Enable common "Grismconf" infrastructure for:
  • pyLINEAR
  • grizli
  • EM2D, and Nor's other modules
  • JWST pipeline
  • (WFIRST)
• Ensure that users can do all the flavors of geometric transformations (and can understand them)
• Make sure calibration (files) are consistent with the approach to geometry
• Support the following HST modes:
  • WFC3/IR
  • ACS
  • WFC3/UVIZUVIS?
• Compatible with JWST pipeline outputs of WFSS modes (NIRISS and NIRCam)

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• Direct and slitless images with perfect WCSs
• catalog information
• 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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