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reported by: @CloudyLex
we should agree with this calculation
```
Title:
Modeling of continuous absorption of electromagnetic radiation in dense partially ionized plasmas
Authors:
Mihajlov, A.…
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https://github.com/Open-Astrophysics-Bookshelf/star_formation_notes/blob/fc6dac3a31fecec319fe129a72eeb73b1b483de6/chapters/chapter1.tex#L36
> The gas, in contrast, does not emit thermal radiation b…
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reported by: @CloudyLex
```
Title:
Influence of inelastic collisions with hydrogen atoms on the non-LTE modelling of Ca i and Ca ii lines in late-type stars
Authors:
Mashonkina, L.; Sitnova, T.; …
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A lot of *context* for this in #195, but this is a new issue to be more specific.
While a lot of the analysis functionality is meant to operate on spectral lines, currently `specutils` has no conce…
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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 moment we are not assuming any dust …
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This issue is for discussing the design requirements for "gold standard testing" (since this is not necessarily obvious). I wanted to flesh out my own ideas and hear your ideas. As I write this out, I…
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Stargen Fake accretion process.
The other day I was looking at some of the Stargen code. I was looking for the file(s) that refer to the elements that are used in the accretion process, because the o…
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Hi,
I've synthesized a bunch of spectra in the 3000A to 10000A wavelength range using Korg on a logg/teff/feh/alpha grid that I can compare with PHOENIX. One of the features I observe is major diff…
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I use `simCluster` to create synthetic clusters with the $Gaia$ magnitudes using the following lines in the `.yaml` file but I only get the $u, g, r, i, z, J, H,$ and $K$ data.
```
main_sequ…
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@RobeReyes should do a literature search on this object and select some recent papers that he thinks are interesting and relevant.