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 in the text and add the following paragraph to the Acknowledgement section:
This research made use of \textsc{tardis}, a community-developed software package for spectral synthesis in supernovae \citep{2014MNRAS.440..387K, kerzendorf_wolfgang_2021_5732521}. 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 to the Acknowledgement.
citep{2019A&A...621A..29V}
The following BibTeX entries are needed for the references:
@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}
}
@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}
}
@software{kerzendorf_wolfgang_2021_5732521,
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
Fullard, Andrew and
Cawley, Kevin and
Singhal, Jaladh and
Smith, Isaac and
Barbosa, Talytha and
Sondhi, Dhruv and
Patel, Maryam and
Varanasi, Kaushik and
Gillanders, James and
O'Brien, Jack and
Arya, Atharva and
Eweis, Youssef and
Reinecke, Martin and
Bylund, Tomas and
Bentil, Laud and
Savel, Arjun and
Yu, Jenny and
Eguren, Jordi and
Alam, Arib and
Magee, Mark and
Livneh, Ran and
Rajagopalan, Srinath and
Mishra, Sashank and
Floers, Andreas and
Reichenbach, John and
Jain, Rinkle and
Brar, Antreev and
Singh, Sourav and
Sofiatti, Caroline and
Talegaonkar, Chinmay and
Kowalski, Nathan and
Selsing, Jonatan and
Wahi, Ujjwal and
Sandler, Morgan and
Sarafina, Nance and
Patra, Nilesh and
Singh Rathore, Parikshit and
Patel, Pratik and
Sharma, Sampark and
Gupta, Suyash and
Volodin, Dmitry and
Aggarwal, Yash and
Dasgupta, Debajyoti and
Kolliboyina, Chaitanya and
Yap, Kevin and
Nayak U, Ashwin and
Kharkar, Atharwa and
Kumar, Atul},
title = {tardis-sn/tardis: TARDIS v2021.11.28},
month = nov,
year = 2021,
publisher = {Zenodo},
version = {release-2021.11.28},
doi = {10.5281/zenodo.5732521},
url = {https://doi.org/10.5281/zenodo.5732521}
}