The DIRTY radiative tranfer/dust emission model for dusty astrophysical sources. DIRTY stands for "DustI Radiative Transfer, Yeah!" These pages specifically refer to DIRTYv2, the complete rewrite of the original DIRTY code to be more robust, flexible, and spiffy. DIRTY solves the radiative transfer problem in full 3D including non-equilibrium and equilibrium thermal dust emission.
See https://dirty-dustrt.readthedocs.io.
Please cite Gordon et al. (2001, ApJ, 551, 269), Misselt et al. (2001, ApJ, 551, 277), and Law et al. (2018, ApJS, 236, 32) if you find this code useful in your research.
No support implied. Support possible on a best effort basis. Interesting the developers in your science use has the most chance of success, but the developers are busy with many other projects.
Contributions should follow the astropy open-development model (even though this code is not in python).
Please open a new issue or new pull request for bugs, feedback, or new features you would like to see. If there is an issue you would like to work on, please leave a comment and we will be happy to assist. New contributions and contributors are very welcome!
New to github or open source projects? If you are unsure about where to start or haven't used github before, please feel free to contact @karllark. Want more information about how to make a contribution? Take a look at the astropy contributing and developer documentation.
Feedback and feature requests? Is there something missing you would like to see? Please open an issue or send an email to @karllark. DIRTY_dustrt follows the Astropy Code of Conduct and strives to provide a welcoming community to all of our users and contributors.
This project is Copyright (c) Karl Gordon, Karl Misselt, & Ka-Hei Law and licensed under the terms of the BSD 3-Clause license.