<commit_before>PAHFIT
======

.. image:: https://readthedocs.org/projects/pypahfit/badge/?version=latest
   :target: http://pypahfit.readthedocs.io/en/latest/?badge=latest
   :alt: Documentation Status

.. image:: https://travis-ci.org/PAHFIT/pypahfit.svg?branch=master
   :target: https://travis-ci.org/PAHFIT/pypahfit
   :alt: CI Testing Status

.. image:: https://ci.appveyor.com/api/projects/status/3wi0ibux1yabc1dj/branch/master?svg=true
   :target: https://ci.appveyor.com/project/KarlGordon/pahfit/branch/master
   :alt: Windows CI Testing Status

.. image:: https://coveralls.io/repos/github/PAHFIT/pypahfit/badge.svg?branch=master
	   :target: https://coveralls.io/github/PAHFIT/pypahfit?branch=master

.. image:: http://img.shields.io/badge/powered%20by-AstroPy-orange.svg?style=flat
    :target: http://www.astropy.org
    :alt: Powered by Astropy Badge

``PAHFIT`` is a decomposition model and tool for astronomical infrared spectra, focusing on dust and gas emission features from the interstellar medium (see `<NAME>., <NAME>., et al., 2007, ApJ, 656, 770 <http://tir.astro.utoledo.edu/jdsmith/research/pahfit.php>`_).

This package provides an updated python implementation of ``PAHFIT``.  While the original versions of ``PAHFIT`` (``v1.x``) were written in IDL and focused mainly on Spitzer/IRS spectroscopic observations, the newer python-based versions (``>=v2.0``) will expand instrument coverage to other existing (e.g., AKARI) and planned (e.g., JWST) facilities, and will offer a more flexible modeling framework suitable for modeling a wider range of astrophysical sources.

Based on and inspired by the IDL code ``PAHFIT`` by <NAME> and <NAME>.

This package is potentially an affiliated package of `AstroPy`_.

Documentation
-------------

Hosted by readthedocs: <http://pypahfit.readthedocs.io/en/latest/>

In Development!
---------------

This code is currently in active development.
Contributions welcome (see below).

Contributors
------------
* <NAME>
* <NAME>
* <NAME>
* <NAME>
* <NAME>
* <NAME>
<commit_msg>Adding in language grade badge<commit_after>PAHFIT
======

.. image:: https://readthedocs.org/projects/pypahfit/badge/?version=latest
   :target: http://pypahfit.readthedocs.io/en/latest/?badge=latest
   :alt: Documentation Status

.. image:: https://travis-ci.org/PAHFIT/pypahfit.svg?branch=master
   :target: https://travis-ci.org/PAHFIT/pypahfit
   :alt: CI Testing Status

.. image:: https://ci.appveyor.com/api/projects/status/3wi0ibux1yabc1dj/branch/master?svg=true
   :target: https://ci.appveyor.com/project/KarlGordon/pahfit/branch/master
   :alt: Windows CI Testing Status

.. image:: https://coveralls.io/repos/github/PAHFIT/pypahfit/badge.svg?branch=master
	   :target: https://coveralls.io/github/PAHFIT/pypahfit?branch=master

.. image:: http://img.shields.io/badge/powered%20by-AstroPy-orange.svg?style=flat
    :target: http://www.astropy.org
    :alt: Powered by Astropy Badge

..image:: https://img.shields.io/lgtm/grade/python/g/PAHFIT/pahfit.svg?logo=lgtm&logoWidth=18
    :target: https://lgtm.com/projects/g/PAHFIT/pahfit/context:python
    :alt: Language grade

``PAHFIT`` is a decomposition model and tool for astronomical infrared spectra, focusing on dust and gas emission features from the interstellar medium (see `<NAME>., <NAME>., et al., 2007, ApJ, 656, 770 <http://tir.astro.utoledo.edu/jdsmith/research/pahfit.php>`_).

This package provides an updated python implementation of ``PAHFIT``.  While the original versions of ``PAHFIT`` (``v1.x``) were written in IDL and focused mainly on Spitzer/IRS spectroscopic observations, the newer python-based versions (``>=v2.0``) will expand instrument coverage to other existing (e.g., AKARI) and planned (e.g., JWST) facilities, and will offer a more flexible modeling framework suitable for modeling a wider range of astrophysical sources.

Based on and inspired by the IDL code ``PAHFIT`` by JD Smith and <NAME>.

This package is potentially an affiliated package of `AstroPy`_.

Documentation
-------------

Hosted by readthedocs: <http://pypahfit.readthedocs.io/en/latest/>

In Development!
---------------

This code is currently in active development.
Contributions welcome (see below).

Contributors
------------
* <NAME>
* <NAME>
* <NAME>
* <NAME>
* <NAME>
* <NAME>

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