====== TARDIS ======
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TARDIS is a tool that creates synthetic observations (spectra) for exploding stars (supernovae).
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.. _tardiscredits:
Credits & Publication Policies
|DOI_BADGE|
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
_ 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, |CITATION|}. 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.
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 _
to the Acknowledgement.
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\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} }
.. |CITATION| replace:: kerzendorf_2026_23631067
.. |DOI_BADGE| image:: https://img.shields.io/badge/DOI-10.5281/zenodo.3631067-blue :target: https://doi.org/10.5281/zenodo.3631067
.. code-block:: bibtex
@software{kerzendorf_2026_23631067, author = {Kerzendorf, Wolfgang and Sim, Stuart and Vogl, Christian and Williamson, Marc and Pássaro, Ezequiel and Flörs, Andreas and Camacho, Yssa and Jančauskas, Vytautas and Harpole, Alice and Nöbauer, Ulrich and Lietzau, Stefan and Mishin, Mikhail and Tsamis, Fotis and Boyle, Aoife and Shingles, Luke and Gupta, Vaibhav and Desai, Karan and Klauser, Michael and Beaujean, Frederik and Suban-Loewen, Adam and Heringer, Epson and Barna, Barnabás and Gautam, Gaurav and Arya, Atharva and Shields, Joshua and Smith, Isaac and Cawley, Kevin and Singhal, Jaladh and Fullard, Andrew and Barbosa, Talytha and Yu, Jenny and O'Brien, Jack and Sondhi, Dhruv and Shields, Josh and Patel, Maryam and Varanasi, Kaushik and Rathi, Shikha and Chitchyan, Sona and Gillanders, James and Marie Lynn, Haille and McClellan, Connor and Gupta, Sumit and Savel, Arjun and Singh, Shreyas and Shah, Swayam and Eweis, Youssef and Reinecke, Martin and Holas, Alexander and Visser, Erin and Bylund, Tomas and Bentil, Laud and Black, William and Kumar, Asish and Dutta, Anirban and Saraf, Shreyans and Groneck, Ryan and Lu, Jing and Eguren, Jordi and Bartnik, Matthew and Kumar, Ansh and Srivastava, Sarthak and Varma Buddaraju, Rohith and Magee, Mark and Alam, Arib and Daksh, Ayushi and Kambham, Satwik and Livneh, Ran and Powers, Cecelia and Roldan, Israel and Bhakar, Jayant and Dadu, Aaryan and Rao, Rishmita and Rajagopalan, Srinath and Mishra, Sashank and Nitish, P and Reichenbach, John and Actions, GitHub and Jain, Rinkle and Gupta, Harshul and Singh, Sourav and Brar, Antreev and Chaumal, Aarya and Matsumura, Yuki and Gangbhoj, Riddhi and Sofiatti, Caroline and Kunisetty, Saanvi and Patidar, Abhishek and Kowalski, Nathan and Talegaonkar, Chinmay and Selsing, Jonatan and Gupta, Angel and Perkins, Haille and Aggarwal, Yash and L. Lim, P. and Patra, Nilesh and Buchner, Johannes and Volodin, Dmitry and Vieira, Nicholas and Diddige, Harshitha and Bhandari, Jhalak and Sarafina, Nance and Yap, Kevin and Nagadevi, Kona and Martinez, Laureano and Truong, Le and Zingale, Michael and Sandler, Morgan and Zaheer, Musabbiha and Lemoine, Thom and Wahi, Ujjwal and Watson, Clyde and Gupta, Suyash and Jaiswal, Abhayraj and Kumar, Aman and Nayak U, Ashwin and Kumar, Atul and Dasgupta, Debajyoti and PATIDAR, ABHISHEK and Chen, Nutan and Singh Rathore, Parikshit and Patel, Pratik and Prasad, Rohit and Gajanan Nalbalwar, Rudraksh and Sharma, Sampark and Venkat, Shashank and Prasad, Shilpi}, title = {tardis-sn/tardis: TARDIS v2026.10.25}, month = oct, year = 2026, publisher = {Zenodo}, version = {release-2026.10.25}, doi = {10.5281/zenodo.23631067}, url = {https://doi.org/10.5281/zenodo.23631067}, }
* License *
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This project is Copyright (c) TARDIS Collaboration and licensed under
the terms of the BSD 3-Clause license. This package is based upon
the Astropy package template _
which is licensed under the BSD 3-clause license. See the licenses folder for
more information.