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        "author": "Miguel de Val-Borro",
        "author_email": "miguel.deval@gmail.com",
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        "classifiers": [
            "Development Status :: 3 - Alpha",
            "Intended Audience :: Developers",
            "Intended Audience :: Science/Research",
            "License :: OSI Approved :: MIT License",
            "Programming Language :: Python",
            "Programming Language :: Python :: 2",
            "Programming Language :: Python :: 2.7",
            "Programming Language :: Python :: 3",
            "Programming Language :: Python :: 3.4",
            "Programming Language :: Python :: 3.5",
            "Programming Language :: Python :: 3.6"
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        "description": "===============================\nCINE: Comet INfrared Excitation\n===============================\n\n\n``cine`` is a command-line tool for calculating infrared pumping efficiencies.\nAt large nucleocentric distances, one of the main mechanisms for molecular\nexcitation in comets is the fluorescence by the solar radiation followed by\nradiative decay to the ground vibrational state.  This code calculates the\neffective pumping rates for rotational levels in the ground vibrational state\nscaled by the heliocentric distance of the comet.  These coefficients are\nuseful for modeling rotational emission lines observed in cometary spectra at\nsub-millimeter wavelengths.\n\nCode releases are available on `PyPI <https://pypi.python.org/pypi/cine>`_, and\ndevelopment happens in the `github project page\n<https://github.com/migueldvb/cine>`_.\n\n\nInstallation\n------------\n\ncine can be installed using `pip <https://pypi.python.org/pypi/pip>`_:\n\n.. code-block:: bash\n\n    $ pip install cine\n\nor by cloning the github repository:\n\n.. code-block:: bash\n\n    $ # If you have a github account:\n    $ git clone git@github.com:migueldvb/cine.git\n    $ # If you do not:\n    $ git clone https://github.com/migueldvb/cine.git\n    $ cd cine\n    $ python setup.py install\n    $ # Or if you do not have root privileges:\n    $ python setup.py install --user\n\nWhen the package is installed using either method, the ``cine`` script will be\ncopied to a directory in the PATH environment variable and will be available\nfor general use.\n\nRequirements\n------------\n\nThe code requires the standard scientific Python packages (`numpy\n<http://www.numpy.org/>`_, `scipy <https://www.scipy.org/>`_, and `pandas\n<http://pandas.pydata.org/>`_) and astropy's affiliated package `astroquery\n<https://github.com/astropy/astroquery>`_.  to access the HITRAN and Lamda\ndatabases. Running the tests requires `nose\n<https://pypi.python.org/pypi/nose>`_.\n\n\nExample\n-------\n\n``cine`` is a command-line tool that is included in the package to generate\npumping rates for several molecules. For example, to obtain the effective\npumping rates between the seven lowest rotational levels in the ground\nvibrational state of HDO you can run the following command once ``CINE`` has\nbeen installed:\n\n.. code-block:: bash\n\n    $ cine --mol HDO --nlevels 7\n\nThis should create a file named ``G_HDO.dat`` which contains the pumping rates\nG :subscript:`ij` in units of s :superscript:`-1` between the rotational levels\ni and j shown in the first two columns. Note that the levels use zero-based\nindexing.\n\n.. code-block:: bash\n\n    0 3 2.568872e-05\n    0 4 2.570305e-05\n    0 5 1.552757e-05\n    1 2 6.253229e-05\n    1 6 2.987896e-05\n    2 1 6.196215e-05\n    2 6 4.410062e-05\n    3 0 7.547422e-05\n    3 4 3.103947e-05\n    3 5 5.048423e-05\n    4 0 1.253741e-04\n    4 3 5.128064e-05\n    4 5 4.679292e-05\n    5 0 7.481781e-05\n    5 3 8.287649e-05\n    5 4 4.643613e-05\n    6 1 4.820172e-05\n    6 2 7.201329e-05\n\nTo include more levels in the calculation, change the ``-n/-nlevels`` command-line\noption to a larger value.  cine has a ``-h/--help`` argument that presents an\nusage explanation describing each optional argument.\n\nThese coefficients are useful for deriving molecular production rates from cometary\nlines observed at sub-millimeter wavelengths combined with a code that\nsolves the radiative transfer equations such as `LIME\n<https://github.com/lime-rt/lime>`_.\n\n\nDownloading HITRAN data\n-----------------------\n\nTo download the molecular data cine uses the ``astroquery.hitran`` and\n``astroquery.lamda`` tools.  Set the ``LAMDA_DATA`` and ``HITRAN_DATA``\nenvironment variables (otherwise, the default\n``~/.astropy/cache/astroquery/Lamda``  and\n``~/.astropy/cache/astroquery/hitran`` will be used),\n\n\nTests\n-----\n\nIf ``nose`` is installed the tests can be run from the root of the repository as:\n\n.. code-block:: bash\n\n    $ python setup.py test\n\n\nContributing\n------------\n\nAny questions or bug reports can be raised in github's `issue tracker\n<https://github.com/migueldvb/cine/issues>`_ or `pull requests\n<https://github.com/migueldvb/cine/pulls>`_.\n\n\nProject Status\n--------------\n\n.. image:: https://travis-ci.org/migueldvb/cine.svg?branch=master\n    :target: https://travis-ci.org/migueldvb/cine?branch=master\n\n.. image:: https://coveralls.io/repos/github/migueldvb/cine/badge.svg?branch=master\n    :target: https://coveralls.io/github/migueldvb/cine?branch=master\n\n\nLicense\n-------\n\nCopyright 2017 Miguel de Val-Borro\n\n``CINE`` is free software made available under the MIT License.\nFor details see the LICENSE file.\n",
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