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Release Notes

Version History and Change Log

Version 2.3

  • Added support for F213 filter
  • Allow users to specify psf_cache_location in addCatalogue function.
  • Updated WebbPSF version to be >= 1.3
  • Constrained numpy version < 2.0 given the conflict with Pandeia.
  • Updated documentation to reflect the fact STIPS creates L3 images.

Version 2.2.1

  • Fixed a bug on the version of STIPS in __init__.py
  • Updated WebbPSF version to be >= 1.1.1 instead of == 1.1.1
  • Updated synphot>=1.1.1 and stsynphot>=1.1.0 from forced to specific version.

Version 2.2.0

  • Added a functionality to allow for faster simulations of extended sources.
  • Fixed a bug related to the simulation of extended sources.
  • Fixed a bug related to the WCS.
  • Updated pandeia to version 3.1 and its corresponding reference files.
  • Changed the minimum required Python version to 3.10

Version 2.1.0

  • Updated the Flux PHOTFNU values to match Pandeia
  • Updated the background and noise estimates to use Pandeia
  • Updated webbpsf to version 1.1
  • Updated pandeia to version 2.0

Version 2.0.0

  • STIPS now uses an ePSF, and calculates source appearance on a per-source basis
  • Dropped support for python 2, and python <= 3.7
  • Dropped support for HST and JWST instruments
  • Dropped support for jbt background tool, as its results are JWST-specific
  • Updated pandeia to 1.7
  • Updated webbpsf to 1.0.0
  • Dropped astropy helpers code

Version 1.0.8

2020 May 22

STIPS Improvements

Version 1.0.7

2020 January 8

STIPS Improvements

General bug fixes and small changes

  • Updated astro_image.py to use a PC matrix rather than a CD matrix for the image WCS, which hopefully will result in astropy actually giving you a correctly formatted FITS WCS. [:pr:`46`, :user:`york-stsci`]
  • Adding WCS information to PSF files. PSF files will now have the following:
    • RA equal to the observation RA at which they were produced
    • DEC equal to the observation DEC at which they were produced
    • PA equal to the observation PA at which they were produced
    • CDELT keywords equal to the PIXELSCL keyword, but adjusted to degrees rather than arcsec.
    • [:pr:`47`, :user:`york-stsci`]