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Originally reported by: **Britton Smith (Bitbucket: [brittonsmith](https://bitbucket.org/brittonsmith), GitHub: [brittonsmith](https://github.com/brittonsmith))**
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Hello! I'm trying to run BEAGLE v0.10.5 on some mock catalogue objects using the HST+NIRCam filters in our deep survey configuration, and the program seems to be hanging up after MultiNest generates t…
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I have a general question regarding how I can set parameters as dependent in the .param files. For example, nebular_Z is marked as "dependent" in the example parameter files and it seems that it exac…
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Can be separated by dwarf/giants -- need to ensure we have a comparable scale for dwarfs and giants.
(Seen by plotting [Fe/H] vs Kordopatis metallicity, colored by logg)
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I have two issues. I was trying to add the MIRI filters to the BEAGLE filter list, and first, I found that _add_filters_ will spit out a segmentation fault if the filterfrm.res file is too long. So I …
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Originally reported by: **Nathan Goldbaum (Bitbucket: [ngoldbaum](https://bitbucket.org/ngoldbaum), GitHub: [ngoldbaum](https://github.com/ngoldbaum))**
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I ju…
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The widest spectral template coverage is for [Fe/H] = 0 (or close to zero), so it makes sense for this to be the starting value.
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I would like to include Ha and Hb in some fits (for now just Ha) and have attempted to do so in the additional files in the attached
.zip. When running `fit_3dhst_spec.param` I acquire the same erro…
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to wit, that the thing only seems to work at low metallicity. That's important!
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Currently the `get_metals` function in `get_met_ages_values` takes the metallicity value of the file from the name of the file.
It would be simpler if the metallicity would be read from the informati…