From b31eb6af4ede08736e9f8cb03868fb888b2c9959 Mon Sep 17 00:00:00 2001 From: Shannon Osborne Date: Wed, 17 Jun 2020 13:17:24 -0700 Subject: [PATCH] update naming --- README.rst | 6 +++--- docs/index.rst | 2 +- docs/intro.rst | 2 +- 3 files changed, 5 insertions(+), 5 deletions(-) diff --git a/README.rst b/README.rst index 3b1b4b25..c81a482b 100644 --- a/README.rst +++ b/README.rst @@ -1,5 +1,5 @@ -WebbPSF: Simulated Point Spread Functions for JWST and Roman -============================================================= +WebbPSF: Simulated Point Spread Functions for the James Webb and Nancy Grace Roman Space Telescopes +=================================================================================================== .. image:: docs/readme_fig.png @@ -22,7 +22,7 @@ flagship infrared space telescope. WebbPSF can simulate images for any of the four science instruments plus the fine guidance sensor, including both direct imaging and coronagraphic modes. -WebbPSF also supports simulating PSFs for the upcoming Nancy Grace Roman Telescope (formerly WFIRST), +WebbPSF also supports simulating PSFs for the upcoming Nancy Grace Roman Space Telescope (formerly WFIRST), including its Wide Field Instrument and a preliminary version of the Coronagraph Instrument. Developed by Marshall Perrin, Joseph Long, Neil Zimmerman, Robel Geda, Shannon diff --git a/docs/index.rst b/docs/index.rst index 5c432132..268110d3 100644 --- a/docs/index.rst +++ b/docs/index.rst @@ -1,7 +1,7 @@ Documentation for WebbPSF =============================== -WebbPSF is a Python package that computes simulated point spread functions (PSFs) for NASA's James Webb Space Telescope (JWST) and Nancy Grace Roman Telescope (formerly WFIRST). WebbPSF 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 *not* a full optical model of JWST, but rather a tool for transforming optical path difference (OPD) maps, created with some other tool, into the resulting PSFs as observed with JWST's or WFIRST's instruments. +WebbPSF 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 (formerly WFIRST). WebbPSF 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 *not* a full optical model of JWST, but rather a tool for transforming optical path difference (OPD) maps, created with some other tool, into the resulting PSFs as observed with JWST's or WFIRST's instruments. .. figure:: ./fig_instrument_comparison.png :scale: 45 % diff --git a/docs/intro.rst b/docs/intro.rst index 57cd8eca..3b9e223b 100644 --- a/docs/intro.rst +++ b/docs/intro.rst @@ -3,7 +3,7 @@ Introduction **What this software does:** -* Uses OPD maps precomputed by detailed optical simulations of JWST and the Nancy Grace Roman Telescope (formerly WFIRST), and in the case of JWST +* Uses OPD maps precomputed by detailed optical simulations of JWST and the Nancy Grace Roman Space Telescope (formerly WFIRST), and in the case of JWST based on instrument and telescope flight hardware cryo-vacuum test results. * For JWST, computes PSF images with requested properties for any of JWST's instruments. Supports imaging, coronagraphy, and most spectrographic modes with all of JWST's instruments. IFUs are yet to come. * For WFIRST, computes PSFs with the Wide Field Imager, based on recent GSFC optical models, including field- and wavelength-dependent aberrations.