Metadata-Version: 2.1
Name: muse-psfr
Version: 1.0rc2
Summary: MUSE WFM-AO PSF reconstruction from SPARTA
Home-page: UNKNOWN
Author: Simon Conseil
Author-email: simon.conseil@univ-lyon1.fr
License: BSD 3-Clause License
Keywords: astronomy,astrophysics,science,muse,vlt
Platform: UNKNOWN
Classifier: Programming Language :: Python :: 3
Requires-Python: >=3.5
Requires-Dist: mpdaf
Requires-Dist: astropy
Requires-Dist: scipy
Requires-Dist: numpy
Requires-Dist: joblib
Provides-Extra: all
Requires-Dist: matplotlib ; extra == 'all'
Requires-Dist: colorama ; extra == 'all'
Provides-Extra: docs
Requires-Dist: numpydoc ; extra == 'docs'
Requires-Dist: sphinx-rtd-theme ; extra == 'docs'
Requires-Dist: sphinx-automodapi ; extra == 'docs'
Requires-Dist: sphinxcontrib-programoutput ; extra == 'docs'
Requires-Dist: matplotlib ; extra == 'docs'

MUSE-PSFR - PSF reconstruction for MUSE WFM-AO
==============================================

The *muse-psfr* code allows to reconstruct a PSF for the MUSE WFM-AO mode, using
telemetry data from SPARTA. See documentation for details.

The method will be presented in more details in a forthcoming publication ([Fusco et al. in prep.]).

.. image:: https://travis-ci.org/musevlt/muse-psfr.svg?branch=master
  :target: https://travis-ci.org/musevlt/muse-psfr

.. image:: https://codecov.io/gh/musevlt/muse-psfr/branch/master/graph/badge.svg
  :target: https://codecov.io/gh/musevlt/muse-psfr



