| Name | webbpsf JSON |
| Version |
1.3.0
JSON |
| download |
| home_page | None |
| Summary | Creates simulated point spread functions for the James Webb Space Telescope |
| upload_time | 2024-05-28 14:31:48 |
| maintainer | None |
| docs_url | None |
| author | None |
| requires_python | >=3.10 |
| license | BSD 3-Clause License Copyright (c) 2010-2018, Space Telescope Science Institute, AURA All rights reserved. Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: * Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. * Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. * Neither the name of the copyright holder nor the names of its contributors may be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. |
| keywords |
|
| VCS |
 |
| bugtrack_url |
|
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astropy
ipython
matplotlib
numpy
photutils
poppy
pysiaf
scipy
synphot
astroquery
|
| Travis-CI |
No Travis.
|
| coveralls test coverage |
No coveralls.
|
WebbPSF: Simulated Point Spread Functions for the James Webb and Nancy Grace Roman Space Telescopes
===================================================================================================
.. image:: https://github.com/spacetelescope/webbpsf/blob/stable/docs/readme_fig.png?raw=true
.. image:: https://img.shields.io/pypi/v/webbpsf.svg
:target: https://pypi.python.org/pypi/webbpsf
:alt: Badge showing current released PyPI version
.. image:: https://github.com/spacetelescope/webbpsf/workflows/CI/badge.svg?branch=develop
:target: https://github.com/spacetelescope/webbpsf/actions
:alt: Github Actions CI Status
.. image:: https://codecov.io/gh/spacetelescope/webbpsf/branch/master/graph/badge.svg
:target: https://codecov.io/gh/spacetelescope/webbpsf
.. |Documentation Status| image:: https://img.shields.io/readthedocs/webbpsf/latest.svg?logo=read%20the%20docs&logoColor=white&label=Docs&version=latest
:target: https://webbpsf.readthedocs.io/en/latest/
:alt: Documentation Status
.. image:: https://img.shields.io/badge/ascl-1504.007-blue.svg?colorB=262255
:target: http://ascl.net/1504.007
WebbPSF produces simulated PSFs for the James Webb Space Telescope, NASA's
flagship infrared space telescope. WebbPSF can simulate images for any of the
four science instruments plus the fine guidance sensor, including both direct
imaging, coronagraphic, and spectroscopic modes.
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, Shannon Osborne, Robel Geda, Bradley Sappington, Marcio Meléndez,
Charles-Phillipe Lajoie, Jarron Leisenring, Neil Zimmerman, Keira Brooks,
Justin Otor, Trey Kulp, Lauren Chambers, Alden Jurling, and collaborators, 2010-2024.
Documentation can be found online at https://webbpsf.readthedocs.io
WebbPSF requires input data for its simulations, including optical path
difference (OPD) maps, filter transmission curves, and coronagraph Lyot mask
shapes. These data files are not included in this source distribution.
Please see the documentation to download the required data files.
Raw data
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"description": "WebbPSF: Simulated Point Spread Functions for the James Webb and Nancy Grace Roman Space Telescopes\n===================================================================================================\n\n.. image:: https://github.com/spacetelescope/webbpsf/blob/stable/docs/readme_fig.png?raw=true\n\n.. image:: https://img.shields.io/pypi/v/webbpsf.svg\n :target: https://pypi.python.org/pypi/webbpsf\n :alt: Badge showing current released PyPI version\n\n.. image:: https://github.com/spacetelescope/webbpsf/workflows/CI/badge.svg?branch=develop\n :target: https://github.com/spacetelescope/webbpsf/actions\n :alt: Github Actions CI Status\n\n.. image:: https://codecov.io/gh/spacetelescope/webbpsf/branch/master/graph/badge.svg\n :target: https://codecov.io/gh/spacetelescope/webbpsf\n\n.. |Documentation Status| image:: https://img.shields.io/readthedocs/webbpsf/latest.svg?logo=read%20the%20docs&logoColor=white&label=Docs&version=latest\n :target: https://webbpsf.readthedocs.io/en/latest/\n :alt: Documentation Status\n\n.. image:: https://img.shields.io/badge/ascl-1504.007-blue.svg?colorB=262255\n :target: http://ascl.net/1504.007\n\nWebbPSF produces simulated PSFs for the James Webb Space Telescope, NASA's\nflagship infrared space telescope. WebbPSF can simulate images for any of the\nfour science instruments plus the fine guidance sensor, including both direct\nimaging, coronagraphic, and spectroscopic modes.\n\nWebbPSF also supports simulating PSFs for the upcoming Nancy Grace Roman Space Telescope (formerly WFIRST),\nincluding its Wide Field Instrument and a preliminary version of the Coronagraph Instrument.\n\nDeveloped by Marshall Perrin, Joseph Long, Shannon Osborne, Robel Geda, Bradley Sappington, Marcio Mel\u00e9ndez, \nCharles-Phillipe Lajoie, Jarron Leisenring, Neil Zimmerman, Keira Brooks, \nJustin Otor, Trey Kulp, Lauren Chambers, Alden Jurling, and collaborators, 2010-2024.\n\nDocumentation can be found online at https://webbpsf.readthedocs.io\n\nWebbPSF requires input data for its simulations, including optical path\ndifference (OPD) maps, filter transmission curves, and coronagraph Lyot mask\nshapes. These data files are not included in this source distribution.\nPlease see the documentation to download the required data files.\n",
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