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The `transitions` property of `BaseSpectralModel` in `spectral_models/base.py` seems to return a copy of the session linelist (see the bottom of http://docs.astropy.org/en/stable/table/modify_table.ht…
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@mdietze Marcos has told me that you are more familiar with the xml file procedure to set parameters for PFTs.
What I would like to do is take three existing PFTs (e,m,l tropical), make an exact copy …
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We need a common method to parse in line lists from binary/ASCII formats, and then export them in different formats (e.g., latex and/or formatted for MOOG if the Python-wrapped MOOG version isn't used…
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The Latex escapes a lot of common characters, so importing the BIBTEX files from content-resolver in most cases lead to Latex errors. The rules for escaping characters are very complicated.
At PANGAE…
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There are significant differences in the stellar atmospheres between old SMH and new SMHR. It causes differences in stellar parameters.
I took Anna's EW for HD122563 and put in the same stellar param…
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Hi,
I am using `scuff-neq` to compute the **Radiative heat transfer** between 1D SiO2 gratings in the paper [Radiative heat transfer between two dielectric nanogratings in the scattering approach](htt…
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Hello!
So, I'm trying to fit some CANDELS objects at z < 4, and the resulting fits, at least the best ln(likelihood) fits, are coming out pretty poor, as compared to the data.
As an example, we fi…
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The model density, temperature and abundance are stored in the grid structure. Therefore, the corresponding functions, `density()`, `temperature()` and `abundances()` are called only during the grid c…
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This is an area to discuss how we implement domains in Python. My first efforts on this have not been entirely successful and I think it is a good idea to try to summarize what we want to do and what…
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Hi,
I install `scuff-em-Overhaul201512`, trying to reproduce the example [Thermal radiation, heat transfer, and non-equilibrium Casimir forces between silicon dioxide spheres](http://homerreid.github.…