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Hello, thank you very much for your packages. It is very useful.
I would like to know if it is normal that for FeH < -2, the isochrone seems to be truncated respect to the -2 case. I have tested fo…
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**Describe the bug**
When using the latest version of COMPAS (version 03.07.00), I encountered an issue where the data for 'Mass_Core@CO(SN)' is NaN for some binaries.
**Label the issue**
urgency…
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In V1, it was possible to evolve a binary from an arbitrary state, but in V2 you can only start a binary on a grid.
For example, the system in the tutorial NS+H-rich_core-h-burning can start on the C…
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whenever I hit run test i get errors in my terminal. I know the data is good because I used old data that has been processed through hops already and worked but now doesnt work aswell as all the new t…
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There are several different values for the solar metallicity still in common use in the astrophysical literature (yes, it's silly but true).
We should find a way to allow the user to set their own…
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In `fit.py`, when the 1D PDFs are getting initialized, the number of bins is increased by 1 for the metallicity. The comment says it's temp code. Should it be removed, or is the comment out of date?…
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Temperature, Energy.
And for star particles: age, chemical composition (metallicity).
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Parametric histories in particular are defined in SFR space, so to get the current stellar mass requires an assumed recycling fraction. This will be SPS model dependent.
We could provide a few comm…
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Hello, can I use this package to analyze XMM x-ray data from clusters? Can I generate radial profiles and maps of temperature, pressure, metallicity and entropy? Could you help me configure the packag…
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For systems with state=NS and SN_Type=WD, no mass is present in the MODELxx.
Is this expected behaviour for the models, when the state and SN type do not match?
Should we recalculate the mass with…