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Hi,
While looking at synthesised spectra of hotter stars I'm seeing weird behaviour next to the Balmer break like here (spectrum rebinned by a factor 100)
![image](https://user-images.githubuse…
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I am using pymoogi on the following file types, here is an example of what I am trying to do. I am using the abfind algorithm with the following file types, the atmosphere is in phoenix format. Here…
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Update the documentations with new features and citation links.
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Good afternoon, I need to get evolutionary tracks of star with different masses using this project, how can I do it?
And is it possible to get the names of evolutionary stages such as "Main Sequence"…
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**Submitting author:** @rhdtownsend (Richard Townsend)
**Repository:** https://github.com/rhdtownsend/msg
**Branch with paper.md** (empty if default branch): joss
**Version:** v1.0
**Editor:** @arfon
…
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**Submitting author:** @rhdtownsend (Richard Townsend)
**Repository:** https://github.com/rhdtownsend/msg
**Branch with paper.md** (empty if default branch): joss
**Version:** v1.0
**Editor:** @arfon
…
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**Submitting author:** @rhdtownsend (Richard Townsend)
**Repository:** https://github.com/rhdtownsend/msg-joss.git
**Branch with paper.md** (empty if default branch):
**Version:** v1.0-rc1
**Editor:*…
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Hi,
I am currently working on a project that needs to simulate a stellar population by assuming a star formation history/rate. I have been doing this with the fsps code where we can generate an iso…
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Moving discussion started in #623 here.
> looking forward to seeing this side-to-side with my timelapse photos!
Are they published anywhere? Would be interesting to compare the model with real-w…
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A new feature in MESA is a relaxation of a pre-main-sequence model until it forms a radiative core. This is often a more robust point at which to start changing things like atmospheres, rotation rates…