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## Summary
optimization code for svbrdf crashes with both llvm and cuda variants after hundreds of renders.
## System configuration
OS: Windows-10 …
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With yt > 4.1, add_field no longer accepts the `particle_type` arg. Many aspects of gadget front end break as a result:
```Traceback (most recent call last):
File "/home/s.lower/powderday/powder…
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As part of my PhD project, I am creating X-ray mock observations of galaxy clusters from the Illustris TNG simulation.
I followed the example given in the "X-ray Fields for yt" section of the pyXSI…
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Massive binaries in the high metallicity HMS-HMS grids can reach carbon depletion of the primary star, with the secondary star being stripped. In these binaries, stellar winds are strong enough to str…
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Hi,
When one fits photometry and spectroscopy, how does one force the gas phase metallicity to be identical to the stellar metallicity?
Cheers,
Steve
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**Statement of the problem**
Cosmological hydrodynamical simulations are excellent numerical laboratories to investigate the formation of galaxies and large scale structure. They provide a highly de…
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I imagine I'm missing something here but I wanted to ask about this case in which I thought the total mass of the sampled binaries should be the same as `mass_binaries`. Here's the call:
```
initial…
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I need to find galaxy stellar mass for a set of stellar formation parameters. Could you please clarify the legend for stellar_mass? All the permutations I've tried return an array of length 107. See e…
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Hi!Abdurro'uf
Thank you very much for your timely and accurate reply last time. Through this time of learning and using, the excellent code you have written has given encouraging results. However,…
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```
from scida import load
ds = load(basePath+"/snapdir_099")
data = ds.return_data(subhaloID=42)
```
The above code is taken from the website [https://cbyrohl.github.io/scida/halocatalogs/](…