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### Name of software library or topic
Multidimensional Stellar Grids (MSG)
### URL to software repository
https://github.com/rhdtownsend/msg
### Name of person who will give the talk
…
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**Describe the bug**
I noticed that when using something like the following set of options:
./COMPAS -n 1000000 --metallicity-distribution LOGUNIFORM --evolve-unbound-systems FALSE --chemically-ho…
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I've noticed some binaries entering `step_merged` and just ending.
They're tagged as failing binaries, but this is not clear from the `binary.event` nor `binary.state`
Example at solar metallici…
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This is related to #116.
* I think it needs to say where to get the example data. I found it here: https://github.com/OttoStruve/muler_example_data/tree/main/IGRINS/01_IGRINS_test_data
And mention…
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The example works fine, but the real spectrum produces $\chi^2 = 999999.00000000$. Interpolation, smoothing, theoretical spectra give the same result. But the funny thing is that when synthesizing the…
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Get spaxelsleuth working with data from the Hector Galaxy Survey from Gabby's spectral fitting pipeline.
**BIG TO DOs**
- [x] Finalise format for output FITS files
- [ ] Calculate emission lin…
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**Describe the bug**
I am trying to look at a population of supernovae using COMPAS. I noticed that I was getting more supernovae than the number of (single) stars that I evolved, which seemed weird.…
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I am attempting to model some spectroscopic and photometric data using a simple stellar population model template. In the past, I have only done modelling where I had one or the other, but not both. I…
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In some cases, `CC1` or `CC2` occurs twice in the evolutionary pathway, after which the model ends, for example, `ZAMS_CC1_CC1`. This is a result of the model failing in `step_SN` due to the following…
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**Describe the bug**
BSE_Supernovae/Mass_Total@CO(SN) is occasionally zero
**Label the issue**
`urgency_moderate` - This is a moderately urgent issue
`severity_moderate` - This is a moderately s…