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[ascl:2012.025] Magritte: 3D radiative transfer library

Magritte performs 3D radiative transfer modeling; though focused on astrophysics and cosmology, the techniques can also be applied more generally. The code uses a deterministic ray-tracer with a formal solver that currently focuses on line radiative transfer. Magritte can either be used as a C++ library or as a Python package.

Code site:
https://github.com/Magritte-code/Magritte
Described in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.499.5194D https://ui.adsabs.harvard.edu/abs/2020MNRAS.492.1812D
Bibcode:
2020ascl.soft12025D

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ascl:2012.025
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