TARDIS is a tool that creates synthetic observations (spectra) for exploding stars (supernovae).
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.
If you use this code for any publications or presentations please acknowledge it. Please cite Kerzendorf & Sim 2014 in the text
Please add this paragraph to the Acknowledgement:
This research made use of \textsc{Tardis}, a community-developed software
package for spectral synthesis in supernovae
\citep{2014MNRAS.440..387K, kerzendorf_wolfgang_2019_2590539}.
The development of \textsc{Tardis} received support from the
Google Summer of Code initiative
and from ESA's Summer of Code in Space program. \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 you also add this citation to acknowledgement Spectral modeling of type II supernovae. I. Dilution factors:
\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_2020_3893940,
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
Barbosa, Talytha and
Patel, Maryam and
Varanasi, Kaushik and
Eweis, Youssef and
Reinecke, Martin and
Bylund, Tomas and
Bentil, Laud and
Eguren, Jordi and
Livneh, Ran and
Singhal, Jaladh and
O'Brien, Jack and
Rajagopalan, Srinath and
Jain, Rinkle and
Reichenbach, John and
Mishra, Sashank and
Singh, Sourav and
Sofiatti, Caroline and
Selsing, Jonatan and
Kowalski, Nathan and
Savel, Arjun and
Talegaonkar, Chinmay and
Patel, Pratik and
Patra, Nilesh and
Nayak, Ashwin and
Kumar, Atul and
Sarafina, Nance and
Gillanders, James and
Sharma, Sampark and
Wahi, Ujjwal and
Dasgupta, Debajyoti and
Magee, Mark and
Yap, Kevin and
Gupta, Suyash},
title = {tardis-sn/tardis: TARDIS v3.0.dev3459},
month = jun,
year = 2020,
publisher = {Zenodo},
version = {v3.0.dev3459},
doi = {10.5281/zenodo.3893940},
url = {https://doi.org/10.5281/zenodo.3893940}
}