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TARDIS - Temperature And Radiative Diffusion In Supernovae

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TARDIS

https://img.shields.io/badge/powered%20by-NumFOCUS-orange.svg?style=flat&colorA=E1523D&colorB=007D8A https://img.shields.io/static/v1?logo=visualstudiocode&label=&message=Open%20in%20Visual%20Studio%20Code&labelColor=2c2c32&color=007acc&logoColor=007acc

TARDIS is a tool that creates synthetic observations (spectra) for exploding stars (supernovae).

https://img.shields.io/endpoint?url=https://jsonbin.org/tardis-bot/tardis/badges/docstr-cov

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:

This research made use of \textsc{tardis}, a community-developed software package for spectral
synthesis in supernovae \citep{2014MNRAS.440..387K, kerzendorf_wolfgang_2023_8128141}. 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_2023_8128141,
  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
                  Smith, Isaac and
                  Cawley, Kevin and
                  Singhal, Jaladh and
                  Arya, Atharva and
                  Barbosa, Talytha and
                  Sondhi, Dhruv and
                  O'Brien, Jack and
                  Yu, Jenny and
                  Patel, Maryam and
                  Varanasi, Kaushik and
                  Gillanders, James and
                  Chitchyan, Sona and
                  Savel, Arjun and
                  Reinecke, Martin and
                  Eweis, Youssef and
                  Bylund, Tomas and
                  Bentil, Laud and
                  Black, William and
                  Eguren, Jordi and
                  Alam, Arib and
                  Bartnik, Matthew and
                  Magee, Mark and
                  Kumar, Ansh and
                  Varma Buddaraju, Rohith and
                  Shields, Joshua and
                  Livneh, Ran and
                  Kambham, Satwik and
                  Rajagopalan, Srinath and
                  Mishra, Sashank and
                  Rathi, Shikha and
                  Floers, Andreas and
                  Reichenbach, John and
                  Jain, Rinkle and
                  Holas, Alexander and
                  Singh, Sourav and
                  Chaumal, Aarya and
                  Singh, Shreyas and
                  Brar, Antreev and
                  Bhakar, Jayant and
                  Daksh, Ayushi and
                  Actions, GitHub and
                  Kowalski, Nathan and
                  Sofiatti, Caroline and
                  Kumar, Aman and
                  Talegaonkar, Chinmay and
                  Selsing, Jonatan and
                  Patidar, Abhishek and
                  Sharma, Sampark and
                  Zaheer, Musabbiha and
                  Patel, Pratik and
                  Singh Rathore, Parikshit and
                  Patra, Nilesh and
                  Sarafina, Nance and
                  Gupta, Harshul and
                  Sandler, Morgan and
                  Martinez, Laureano and
                  Yap, Kevin and
                  Prasad, Shilpi and
                  Venkat, Shashank and
                  Kumar, Atul and
                  Gupta, Suyash and
                  Lemoine, Thom and
                  Wahi, Ujjwal and
                  Aggarwal, Yash and
                  Matsumura, Yuki and
                  Volodin, Dmitry and
                  Dasgupta, Debajyoti and
                  PATIDAR, ABHISHEK and
                  Truong, Le and
                  Kharkar, Atharwa and
                  Nayak U, Ashwin and
                  Kolliboyina, Chaitanya},
  title        = {tardis-sn/tardis: TARDIS v2023.07.09},
  month        = jul,
  year         = 2023,
  publisher    = {Zenodo},
  version      = {release-2023.07.09},
  doi          = {10.5281/zenodo.8128141},
  url          = {https://doi.org/10.5281/zenodo.8128141}
}

License

https://img.shields.io/conda/l/conda-forge/tardis-sn http://img.shields.io/badge/powered%20by-AstroPy-orange.svg?style=flat

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.

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TARDIS - Temperature And Radiative Diffusion In Supernovae

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