[x] I have described the purpose of the suggested change, specifying what I need the enhancement to accomplish, i.e. what problem it solves.
[x] I have included any relevant links, screenshots, environment information, and data relevant to implementing the requested feature, as well as pseudocode for how I want to access the new functionality.
[x] If I have ideas for how the new feature could be implemented, I have provided explanations and/or pseudocode and/or task lists for the steps.
The code would need to take the E(B-V) value for every source as an additional input. It would then apply reddening to each template during the fit of each object.
It may be interesting to implement SED dependent galactic reddening as in Galametz 2017
https://www.aanda.org/articles/aa/pdf/2017/02/aa29333-16.pdf
This has been implemented in Phosphorous so might be possible without significant development effort.
https://anaconda.org/astrorama/phosphoros
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