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1.5.0 (2023-10-18)

  • Major updates to the readthedocs documentation, particularly for UVIS pipeline and new full-well saturation [#68, #83]
  • Updated some Python APIs for calwf3 component wrappers and explained parameters [#69, #71, #85]
  • Updated embedsub.py to ensure all input extensions are included in the output file [#70]
  • Reversed the use of column and row parameters when accessing image data and updated example for pstack [#73]
  • Modified how an image section is specified and reversed the use of column and row parameters for pstat [#75]
  • Dropped support for Python 3.8 [#79]

1.4.0 (2022-03-10)

  • fixed matplotlib plotting issue, added explicit draw and interaction plots
  • updates to package setup, removed support for TEAL interface [#63]
  • changes to documentation infrastructure and text [#64]
  • fixed bug in sub2full.py that required input file to be in pwd, now a file path can be supplied [#64]
  • removed 'version' argument (which corresponds to the command line -r flag) from calwf3 python interface [#64]
  • updates to module docstrings [#64]

1.3.5 (released)

  • Documentation-only updates corresponding to calwf3 3.4.1 release
  • travis sphinx install update for testing

1.3.4 (released)

  • bugfix for input string to calwf3 executables

1.3.3 (released)

This release incorporates documentations changes for CALWF3 which will increase from v3.3 to v3.4 with the installation of HSTDP 2016.2 in the Space Telescope Data processing system. Included are:

  • updated information on CTE correction for subarray images
  • updated information on Sink pixel detection for subarray images
  • updated interaction with the Jupyter notebook when interacting with the calwf3 executables
  • improved logging and error return information from the kernel

1.3.2 (released)

  • package reorganization
  • addition of output capture/logging to the calwf3 executables, help display text in jupyter notebook
  • moved the documentation to readthedocs and removed the local build, users will now be pointed to RTD from the display_help() function