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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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### Observed behaviour
### Expected behaviour
I see the custom system in the view and I can spawn in it.
### Steps to reproduce
1. Put this system file in `data/systems/c…
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Let's make a `gollum` paper!
### Destination and bundling
The `muler` paper is destined to be submitted relatively soon, likely to [JOSS](https://joss.theoj.org) (and possibly part of an affiliate…
gully updated
4 months ago
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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…
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The goal here is to produce a spanning template set using the 30 band SEDs of DC2. @sschmidt23 has provided a set of the Brown et al. templates with a linear interpolation over the strongest emission …
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Compile with
`./configure --enable-cuda`
When executing the line of code
`OMP_NUM_THREADS=8 OMP_STACKSIZE=128M petar -u 1 -b 500 -t 100.0 -o 5.0 input`
in ‘test/sample.sh’ after generated input …
RESBI updated
4 months ago
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Hi all,
I think raising an issue is the best practice to ask about the code. If not please do let me know. I was looking into the SN feedback enrichment of the ISM in galaxies and I see that in the…
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Unfortunately, I don't know whether temperatures measured in like-for-like conditions with MEKAL and APEC are consistent, and unfortunately I don't remember any papers that have a systematic compariso…
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Hello, I found most of the tutorials are about fitting CSP to galaxy spectra (e.g., InteractiveDemo.ipynb). After checking the manuals, I think ssp can be accessed by:
def build_sps(zcontinuous=1, …
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I am using BEAGLE v0.29.2 and am running into an issue where the program cannot seem to find the spectrum when I am trying to do spectro-photometric fitting.
I used the following command to call B…