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]
^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.
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]
^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.