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BEAST-Fitting
Bayesian Extinction And Stellar Tool
Add documentation explaining how filter libraries are created (being addressed by PR #757). Also, include version control so that the BEAST checks to make sure it's using the correct, up-to-date,...
Once we merge PR #757, we also need to update vega.hd5 file. I believe Vega fluxes in each filters were computed and stored using the old version of the filter...
This is a reminder for me to investigate the potential placement of input ASTs, specifically in the edge cases where the fractional coverage area is less the 50%. I originally...
Need to implement diagonal shapely boxes, as a response to Issue #704 in order to preserve the xy functionality of make_ast_xy_list.py.
The BEAST generates input AST files in a format tailored to dolphot, but with an extra line for the header which actually dolphot doesn't require. I think this should either...
Now that we have the Padova/Colibri models incorporated into the downloadable data #357 , we need some criteria for when to use the models for a given star. At the...
For folks interested in running the BEAST on specific locations of interest (SNRs, X-ray sources, AGB stars, etc.), it would be helpful to be able to tell the AST list...
Similar to the work already done for the 1D pPDFs. See PR #727.
I just learned that there is a good method we can try to generate input ASTs. The method is called 'Latin Hypercube sampling' (https://en.wikipedia.org/wiki/Latin_hypercube_sampling). I haven't looked into any details...