Document WebbPSF as pre 2.0.0

spacetelescope · Dec 17, 2024 · e9f8a0a · e9f8a0a
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diff --git a/docs/index.rst b/docs/index.rst
@@ -1,6 +1,7 @@
 Documentation for STPSF
 ===============================
 
+**(Formerly WebbPSF, for versions < 2.0)**
 STPSF is a Python package that computes simulated point spread functions (PSFs) for NASA's James Webb Space Telescope (JWST) and Nancy Grace Roman Space Telescope. STPSF transforms models of telescope and instrument optical state into PSFs, taking into account detector pixel scales, rotations, filter profiles, and point source spectra. It is rather a tool for transforming optical path difference (OPD) maps, created with observatory systems engineering models, into the resulting PSFs as observed with JWST's or Roman's instruments.
 
 .. figure:: ./fig_instrument_comparison.png

diff --git a/docs/relnotes.rst b/docs/relnotes.rst
@@ -23,6 +23,12 @@ See https://github.com/spacetelescope/stpsf/issues for currently open issues and
 Version History and Change Log
 -------------------------------
 
+Version 2.0.0
+=============
+*2024 December*
+Ready for Production Release
+All versions before 1.5.1 were part of the WebbPSF repository
+
 Version 1.5.2
 =============
 *2024 December*