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[ascl:2207.024] pymcfost: Python interface to the MCFOST 3D radiative transfer code

pymcfost provides an interface to and can be used to visualize results from the 3D radiative transfer code MCFOST (ascl:2207.023). pymcfost can set up continuum and line models, read a single model or library of models, plot basic quantities such as density structures and temperature maps, and plot observables, including SEDs, polarization maps, visibilities, and channels maps (with spatial and spectral convolution). It can also convert units (e.g. W.m-2 to Jy or brightness temperature), and it provides an interface to the ALMA CASA simulator (ascl:1107.013).

Code site:
https://github.com/cpinte/pymcfost
Used in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.493L.143N https://ui.adsabs.harvard.edu/abs/2022arXiv220309528P
Bibcode:
2022ascl.soft07024P

Views: 1202

ascl:2207.024
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