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with these settings
 before applying on my own Gadget simulation.
However, r…
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E(B-V) is now determined using the `analysis.attenuation` modules. It is implemented in a number of functions and other modules. However, it has not been fully integrated within MSC.
Here are the…
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This is related to Issue #4 but a separate problem, I think. When I run `get_mags()` without any `tage` option it gives me an array of mags at each isochrone age, as expected. But I'm finding that whe…
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**Describe the bug**
Mistake in radius evolution on AGB for stars with masses M_HeF - 0.2 < M < M_HeF. Stars end up too cold (and so too large) during the AGB phase.
**Label the issue**
`urgency_…
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The code (commit 47d034d532d28d101251104bd1551eb820b6b1c4) crashes on ada-0-00 with the following input:
`python3 run_system.py --configuration "fully nested" --masses 1.10 0.90 0.15 --metallicitie…
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Hi! a quick update on the emcee convergence issue. I have the following situation:
1) I am working with flux-calibrated data
2) I have a stellar model with flux computed at the surface of the star
…
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@katiebreivik could you check out this binary and why it gives NaNs?
The condition that gives a Nan
```
kstar_1,kstar_2,mass_1,mass_2,porb,ecc,metallicity,tphysf,mass0_1,mass0_2,rad_1,rad_2,lu…
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COMPAS finally succeeded in breaking through the speed of light barrier! It can create binaries with orbital velocities of >10^{10} km/s, and separations of