tardis-sn/tardis — TARDIS - Temperature And Radiative Diffusion In Supernovae

Description and use

TARDIS (Temperature And Radiative Diffusion In Supernovae) is an open‑source Python framework for simulating the radiative transfer and spectral formation in expanding supernova ejecta. It provides a modular, Monte‑Carlo based toolkit that lets researchers generate synthetic spectra, explore parameter spaces, and compare model predictions with observational data. The project is community‑driven, well‑documented, and integrates with common astrophysical libraries for easy extensibility.

Problem

tardis-sn/tardis may be useful when its README and activity match a concrete workflow.

Outcome

Early or unclear: treat as research material until maintenance, releases, docs, and issue activity are verified.

Evidence

TARDIS - Temperature And Radiative Diffusion In Supernovae

Source