BEAST¶
The Bayesian Extinction and Stellar Tool (BEAST) fits the ultraviolet to near-infrared photometric SEDs of stars to extract stellar and dust extinction parameters. The stellar parameters are age (t), mass (M), metallicity (M), and distance (d). The dust extinction parameters are dust column (Av), average grain size (Rv), and mixing between type A and B extinction curves (fA).
The full details of the BEAST are provide by Gordon et al. (2016, ApJ, 826, 104). <http://adsabs.harvard.edu/abs/2016ApJ…826..104G>
User Documentation¶
Developer Documentation¶
Reporting Issues¶
If you have found a bug in beast
please report it by creating a
new issue on the beast
GitHub issue tracker.
Please include an example that demonstrates the issue sufficiently so that the developers can reproduce and fix the problem. You may also be asked to provide information about your operating system and a full Python stack trace. The developers will walk you through obtaining a stack trace if it is necessary.
Contributing¶
Like the Astropy project, beast
is made both by and for its
users. We accept contributions at all levels, spanning the gamut from
fixing a typo in the documentation to developing a major new feature.
We welcome contributors who will abide by the Python Software
Foundation Code of Conduct.
beast
follows the same workflow and coding guidelines as
Astropy. The following pages will help you get started with
contributing fixes, code, or documentation (no git or GitHub
experience necessary):
- How to make a code contribution
- Coding Guidelines
- Try the development version
- Developer Documentation
For the complete list of contributors please see the beast contributors page on Github.