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.{{cite journal |last1=Kerzendorf |first1=Wolfgang E. |last2=Sim |first2=Stuart A. |title=TARDIS: Temperature And Radiative Diffusion In Supernovae |journal=Astrophysics Source Code Library |date=1 February 2014 |pages=ascl:1402.018 |bibcode=2014ascl.soft02018K |url=https://ui.adsabs.harvard.edu/abs/2014ascl.soft02018K/abstract |access-date=14 January 2024}}{{cite journal |last1=Kerzendorf |first1=W. E. |last2=Sim |first2=S. A. |title=A spectral synthesis code for rapid modelling of supernovae |journal=Monthly Notices of the Royal Astronomical Society |date=1 April 2014 |volume=440 |issue=1 |pages=387–404 |doi=10.1093/mnras/stu055 |doi-access=free |url=https://academic.oup.com/mnras/article/440/1/387/1079501 |access-date=14 January 2024|arxiv=1401.5469 }}{{cite journal |last1=Harvey |first1=L |last2=Maguire |first2=K |last3=Magee |first3=M R |last4=Bulla |first4=M |last5=Dhawan |first5=S |last6=Schulze |first6=S |last7=Sollerman |first7=J |last8=Deckers |first8=M |last9=Dimitriadis |first9=G |last10=Reusch |first10=S |last11=Smith |first11=M |last12=Terwel |first12=J |last13=Coughlin |first13=M W |last14=Masci |first14=F |last15=Purdum |first15=J |last16=Reedy |first16=A |last17=Robert |first17=E |last18=Wold |first18=A |title=Early-time spectroscopic modelling of the transitional Type Ia Supernova 2021rhu with tardis |journal=Monthly Notices of the Royal Astronomical Society |date=2 May 2023 |volume=522 |issue=3 |pages=4444–4467 |doi=10.1093/mnras/stad1226 |doi-access=free |display-authors=1|arxiv=2304.10129 }}{{cite journal |last1=Vogl |first1=C. |last2=Kerzendorf |first2=W. E. |last3=Sim |first3=S. A. |last4=Noebauer |first4=U. M. |last5=Lietzau |first5=S. |last6=Hillebrandt |first6=W. |title=Spectral modeling of type II supernovae: II. A machine-learning approach to quantitative spectroscopic analysis |journal=Astronomy & Astrophysics |date=January 2020 |volume=633 |doi=10.1051/0004-6361/201936137 |arxiv=1911.04444 |bibcode=2020A&A...633A..88V |url=https://www.aanda.org/articles/aa/pdf/2020/01/aa36137-19.pdf |access-date=14 January 2024}}{{cite journal |last1=Kwok |first1=Lindsey A. |last2=Williamson |first2=Marc |last3=Jha |first3=Saurabh W. |last4=Modjaz |first4=Maryam |last5=Camacho-Neves |first5=Yssavo |last6=Foley |first6=Ryan J. |last7=Garnavich |first7=Peter |last8=Maeda |first8=Keiichi |last9=Milisavljevic |first9=Dan |last10=Pandya |first10=Viraj |last11=Dai |first11=Mi |last12=McCully |first12=Curtis |last13=Pritchard |first13=Tyler |last14=Singhal |first14=Jaladh |title=Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type Ic Supernova 2014ad |journal=The Astrophysical Journal |date=1 September 2022 |volume=937 |issue=1 |pages=40 |doi=10.3847/1538-4357/ac8989 |doi-access=free |arxiv=2204.03716 |bibcode=2022ApJ...937...40K |display-authors=1}}{{cite journal |last1=Williamson |first1=Marc |last2=Kerzendorf |first2=Wolfgang |last3=Modjaz |first3=Maryam |title=Modeling Type Ic Supernovae with tardis: Hidden Helium in SN 1994I? |journal=The Astrophysical Journal |date=1 February 2021 |volume=908 |issue=2 |pages=150 |doi=10.3847/1538-4357/abd244|doi-access=free |arxiv=2010.10528 |bibcode=2021ApJ...908..150W }}{{cite journal |last1=Kerzendorf |first1=Wolfgang E. |last2=Vogl |first2=Christian |last3=Buchner |first3=Johannes |last4=Contardo |first4=Gabriella |last5=Williamson |first5=Marc |last6=van der Smagt |first6=Patrick |title=Dalek: A Deep Learning Emulator for TARDIS |journal=The Astrophysical Journal Letters |date=1 April 2021 |volume=910 |issue=2 |pages=L23 |doi=10.3847/2041-8213/abeb1b|doi-access=free |arxiv=2007.01868 |bibcode=2021ApJ...910L..23K }}