.. _tardiscredits:

******************************
Credits & Publication Policies
******************************

We provide TARDIS as a free, open-source tool. If you are using it, please
adhere to a few policies and acknowledge the TARDIS Team.

Publication Policies
====================

If you use this code for any publications or presentations please acknowledge
it.  Please cite `Kerzendorf & Sim 2014
<http://adsabs.harvard.edu/abs/2014MNRAS.440..387K>`_  in the text and add the
following paragraph to the Acknowledgement section:

.. parsed-literal::

    This research made use of \\textsc{tardis}, a community-developed software package for spectral
    synthesis in supernovae \\citep{2014MNRAS.440..387K, |ZENODO|}. The
    development of \\textsc{tardis} received support from GitHub, the Google Summer of Code
    initiative, and from ESA's Summer of Code in Space program. \\textsc{tardis} is a fiscally
    sponsored project of NumFOCUS. \\textsc{tardis} makes extensive use of Astropy and Pyne.
If you use any of the full relativity treatments or use TARDIS for modelling
Type II supernovae, also add `Spectral modeling of type II supernovae. I. Dilution factors <https://ui.adsabs.harvard.edu/abs/2019A%26A...621A..29V>`_ 
to the Acknowledgement.

.. parsed-literal::

    \citep{2019A&A...621A..29V}

The following BibTeX entries are needed for the references:

.. code-block:: bibtex

    @ARTICLE{2014MNRAS.440..387K,
           author = {{Kerzendorf}, W.~E. and {Sim}, S.~A.},
            title = "{A spectral synthesis code for rapid modelling of supernovae}",
          journal = {\mnras},
    archivePrefix = "arXiv",
           eprint = {1401.5469},
     primaryClass = "astro-ph.SR",
         keywords = {radiative transfer, methods: numerical, supernovae: general},
             year = 2014,
            month = may,
           volume = 440,
            pages = {387-404},
              doi = {10.1093/mnras/stu055},
           adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.440..387K},
          adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

.. code-block:: bibtex

    @ARTICLE{2019A&A...621A..29V,
           author = {{Vogl}, C. and {Sim}, S.~A. and {Noebauer}, U.~M. and {Kerzendorf}, W.~E. and {Hillebrandt}, W.},
            title = "{Spectral modeling of type II supernovae. I. Dilution factors}",
          journal = {\aap},
         keywords = {radiative transfer, methods: numerical, stars: distances, supernovae: general, supernovae: individual: SN1999em, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics},
             year = "2019",
            month = "Jan",
           volume = {621},
              eid = {A29},
            pages = {A29},
              doi = {10.1051/0004-6361/201833701},
    archivePrefix = {arXiv},
           eprint = {1811.02543},
     primaryClass = {astro-ph.HE},
           adsurl = {https://ui.adsabs.harvard.edu/abs/2019A&A...621A..29V},
          adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

.. include:: ZENODO.rst