tardis-sn/tardis
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.
Use in a workflow
tardis-sn/tardis may be useful when its README and activity match a concrete workflow.
Limitations and review notes
Early or unclear: treat as research material until maintenance, releases, docs, and issue activity are verified.
- Source: github
- Language: Python
- Record date: 2026-09-05T17:32:13.531Z