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Based on the reflections from Bug #414 , we will thoroughly inspect the calculations and implementations of the code up to now.
## emission spectrum comparison with PetitRadtrans, which was perfor…
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Sorry for the long list here, I think that by trying to push everything under Measure, this section got rather complicated.
We may need to tackle these in waves as we hit the cases in implementation.…
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I was using the latest commit for COSMIC-POP and noticed that the memory occupied by the program is steadily increasing and is later terminated by the OS as soon as the RAM and swap is filled.
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[adding_bse_flag_to_cosmic.txt](https://github.com/COSMIC-PopSynth/COSMIC/files/5856918/adding_bse_flag_to_cosmic.txt)
[show_bse_flag_change.txt](https://github.com/COSMIC-PopSynth/COSMIC/files/58569…
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Do we include stellar parameter info inferred from photometry in Paper 1 about the candidate sample? My gut says "yes" since it seems like it is fairly easy for @timothydmorton to run on a sample with…
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Either Pysynphot reads the wrong PHOENIX spectra, interpolates them incorrectly, or there is something wrong with PHOENIX itself. The spectra do not match what is expected at the given temperatures. T…
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Reopening this issue with the preliminary results of running DESI on BOSS shown in
https://desi.lbl.gov/trac/wiki/DataSystems/Telecons/2017-02-28
Possible areas of improvements
- use several e…
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**Describe the bug**
At Z = 0.001, for fiducial pythonSubmit, stars with MZAMS [15-30] have WR winds as their dominant Mass loss rate when they pass the VINK_MASS_LOSS_MINIMUM_TEMP on their way to b…
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With RAMSES datasets, the outcome of some fields depend on previous fields having been accessed or not.
For example, the following script yields two different results depending on whether the line …
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Eventually the Sonora-Bobcat models will have metallicity, C/O ratio, and possibly other dimensions like `f_sed`. We want to be able to read in those future metallicity grids, while maintaining suppo…
gully updated
4 months ago