TARDIS (software)

TARDIS, Temperature And Radiative Diffusion In Supernovae, is an open-source 1D Monte Carlo radiative-transfer spectral synthesis program used for numerical modelling and analysis of supernovae.^[1]^[2]^[3]^[4]^[5]^[6]^[7]

References

^ Kerzendorf, Wolfgang E.; Sim, Stuart A. (1 February 2014). "TARDIS: Temperature And Radiative Diffusion In Supernovae". Astrophysics Source Code Library: ascl:1402.018. Bibcode:2014ascl.soft02018K. Retrieved 14 January 2024.
^ Kerzendorf, W. E.; Sim, S. A. (1 April 2014). "A spectral synthesis code for rapid modelling of supernovae". Monthly Notices of the Royal Astronomical Society. 440 (1): 387–404. arXiv:1401.5469. doi:10.1093/mnras/stu055. Retrieved 14 January 2024.
^ Harvey, L; et al. (2 May 2023). "Early-time spectroscopic modelling of the transitional Type Ia Supernova 2021rhu with tardis". Monthly Notices of the Royal Astronomical Society. 522 (3): 4444–4467. arXiv:2304.10129. doi:10.1093/mnras/stad1226.
^ Vogl, C.; Kerzendorf, W. E.; Sim, S. A.; Noebauer, U. M.; Lietzau, S.; Hillebrandt, W. (January 2020). "Spectral modeling of type II supernovae: II. A machine-learning approach to quantitative spectroscopic analysis" (PDF). Astronomy & Astrophysics. 633. arXiv:1911.04444. Bibcode:2020A&A...633A..88V. doi:10.1051/0004-6361/201936137. Retrieved 14 January 2024.
^ Kwok, Lindsey A.; et al. (1 September 2022). "Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type Ic Supernova 2014ad". The Astrophysical Journal. 937 (1): 40. arXiv:2204.03716. Bibcode:2022ApJ...937...40K. doi:10.3847/1538-4357/ac8989.
^ Williamson, Marc; Kerzendorf, Wolfgang; Modjaz, Maryam (1 February 2021). "Modeling Type Ic Supernovae with tardis: Hidden Helium in SN 1994I?". The Astrophysical Journal. 908 (2): 150. arXiv:2010.10528. Bibcode:2021ApJ...908..150W. doi:10.3847/1538-4357/abd244.
^ Kerzendorf, Wolfgang E.; Vogl, Christian; Buchner, Johannes; Contardo, Gabriella; Williamson, Marc; van der Smagt, Patrick (1 April 2021). "Dalek: A Deep Learning Emulator for TARDIS". The Astrophysical Journal Letters. 910 (2): L23. arXiv:2007.01868. Bibcode:2021ApJ...910L..23K. doi:10.3847/2041-8213/abeb1b.

External links

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[1] Kerzendorf, Wolfgang E.; Sim, Stuart A. (1 February 2014). "TARDIS: Temperature And Radiative Diffusion In Supernovae". Astrophysics Source Code Library: ascl:1402.018. Bibcode:2014ascl.soft02018K. Retrieved 14 January 2024.

[2] Kerzendorf, W. E.; Sim, S. A. (1 April 2014). "A spectral synthesis code for rapid modelling of supernovae". Monthly Notices of the Royal Astronomical Society. 440 (1): 387–404. arXiv:1401.5469. doi:10.1093/mnras/stu055. Retrieved 14 January 2024.

[3] Harvey, L; et al. (2 May 2023). "Early-time spectroscopic modelling of the transitional Type Ia Supernova 2021rhu with tardis". Monthly Notices of the Royal Astronomical Society. 522 (3): 4444–4467. arXiv:2304.10129. doi:10.1093/mnras/stad1226.

[4] Vogl, C.; Kerzendorf, W. E.; Sim, S. A.; Noebauer, U. M.; Lietzau, S.; Hillebrandt, W. (January 2020). "Spectral modeling of type II supernovae: II. A machine-learning approach to quantitative spectroscopic analysis" (PDF). Astronomy & Astrophysics. 633. arXiv:1911.04444. Bibcode:2020A&A...633A..88V. doi:10.1051/0004-6361/201936137. Retrieved 14 January 2024.

[5] Kwok, Lindsey A.; et al. (1 September 2022). "Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type Ic Supernova 2014ad". The Astrophysical Journal. 937 (1): 40. arXiv:2204.03716. Bibcode:2022ApJ...937...40K. doi:10.3847/1538-4357/ac8989.

[6] Williamson, Marc; Kerzendorf, Wolfgang; Modjaz, Maryam (1 February 2021). "Modeling Type Ic Supernovae with tardis: Hidden Helium in SN 1994I?". The Astrophysical Journal. 908 (2): 150. arXiv:2010.10528. Bibcode:2021ApJ...908..150W. doi:10.3847/1538-4357/abd244.

[7] Kerzendorf, Wolfgang E.; Vogl, Christian; Buchner, Johannes; Contardo, Gabriella; Williamson, Marc; van der Smagt, Patrick (1 April 2021). "Dalek: A Deep Learning Emulator for TARDIS". The Astrophysical Journal Letters. 910 (2): L23. arXiv:2007.01868. Bibcode:2021ApJ...910L..23K. doi:10.3847/2041-8213/abeb1b.

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