ready for 1.2.1 doc update

.github/workflows/ci_workflows.yml

@@ -58,7 +58,7 @@ jobs:
 
     - name: Get WebbPSF Data
       run: | # Get WebbPSF data files (just a subset of the full dataset!) and set up environment variable
-           wget https://stsci.box.com/shared/static/ykkvequ9cbble6qg88ldhjoep4m9ey6x.gz -O /tmp/minimal-webbpsf-data.tar.gz
+           wget https://stsci.box.com/shared/static/0ojjfg3cieqdpd18vl1bjnpe63r82dx8.gz -O /tmp/minimal-webbpsf-data.tar.gz
            tar -xzvf /tmp/minimal-webbpsf-data.tar.gz
            echo "WEBBPSF_PATH=${{github.workspace}}/webbpsf-data" >> $GITHUB_ENV
 

docs/installation.rst

@@ -69,8 +69,8 @@ Installing the Required Data Files
 
 Files containing such information as the JWST pupil shape, instrument throughputs, and aperture positions are distributed separately from WebbPSF. To run WebbPSF, you must download these files and tell WebbPSF where to find them using the ``WEBBPSF_PATH`` environment variable.
 
-1. Download the following file:  `webbpsf-data-1.2.0.tar.gz <https://stsci.box.com/shared/static/34g3slaq4jidgccqj25qqo80tlk6tubl.gz>`_  [approx. 70 MB]
-2. Untar ``webbpsf-data-1.2.0.tar.gz`` into a directory of your choosing.
+1. Download the following file:  `webbpsf-data-1.2.1.tar.gz <https://stsci.box.com/shared/static/qxpiaxsjwo15ml6m4pkhtk36c9jgj70k.gz>`_  [approx. 70 MB]
+2. Untar ``webbpsf-data-1.2.1.tar.gz`` into a directory of your choosing.
 3. Set the environment variable ``WEBBPSF_PATH`` to point to that directory. e.g. ::
 
    export WEBBPSF_PATH=$HOME/data/webbpsf-data

docs/relnotes.rst

@@ -27,13 +27,17 @@ See https://github.com/spacetelescope/webbpsf/issues for currently open issues a
 Version History and Change Log
 -------------------------------
 
+Version 1.2.1
+=============
+Minor documentation updates
+
 Version 1.2.0
 =============
 We are pleased to announce the release of the latest version of WebbPSF version 1.2.0, now available on PyPi and GitHub. This release comes with new features and improvements including but not limited to:
 
 1. The addition of detector effects for JWST simulations. H2RG detector effects are included in two flavors, a simple ad hoc Gaussian convolution to model charge diffusion effects and a set of convolution kernels to model interpixel capacitance (IPC) and post-pixel coupling effects. We have found that these effects greatly improve the agreement between observations and simulations. See `JWST Detector Effects for more details. <https://webbpsf.readthedocs.io/en/latest/jwst_detector_effects.html>`_
 
-2. A new utility function for simulating matching PSFs to science data. See `Matching PSF sims to in-flight JWST data <https://webbpsf.readthedocs.io/en/latest/jwst_matching_psfs_to_data.html>`_. 
+2. A new utility function for simulating matching PSFs to science data. See `Matching PSF sims to in-flight JWST data <https://webbpsf.readthedocs.io/en/latest/jwst_matching_psfs_to_data.html>`_.
 
 3. Implement geometric distortion for Roman using the Roman SIAF.