From 445dc841c3f9406de7032094d4ba0bdd51edb632 Mon Sep 17 00:00:00 2001 From: Marshall Perrin Date: Fri, 3 May 2024 13:48:23 -0400 Subject: [PATCH] implement model for MIRI cruciform field dependence, and add radial term --- docs/relnotes.rst | 1 - webbpsf/constants.py | 2 +- 2 files changed, 1 insertion(+), 2 deletions(-) diff --git a/docs/relnotes.rst b/docs/relnotes.rst index 7e227a32..49191ad1 100644 --- a/docs/relnotes.rst +++ b/docs/relnotes.rst @@ -37,7 +37,6 @@ X. Improved support for NIRSpec and MIRI IFU PSF calculations, including additio X. Improved PSF models for MIRI imager, in particular including an empirical model for the field-dependent shifts of the cruciform artifact seen at short wavelengths. - Version 1.2.1 ============= Minor documentation updates diff --git a/webbpsf/constants.py b/webbpsf/constants.py index 27785ba5..4222b398 100644 --- a/webbpsf/constants.py +++ b/webbpsf/constants.py @@ -400,4 +400,4 @@ # See Gaspar et al. 2021 for illustrative figures. # This is a rough approximation of a detector-position-dependent phenomenon MIRI_CRUCIFORM_INNER_RADIUS_PIX = 12 -MIRI_CRUCIFORM_RADIAL_SCALEFACTOR = 0.005 # Brightness factor for the diffuse circular halo \ No newline at end of file +MIRI_CRUCIFORM_RADIAL_SCALEFACTOR = 0.005 # Brightness factor for the diffuse circular halo