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Why are there basically no red galaxies in IllustrisTNG at cosmic noon? It's tempting to think that there might be something wrong about SFRs, but what about dust...
arxiv.org/abs/2501.12008
Why are there basically no red galaxies in IllustrisTNG at cosmic noon? It's tempting to think that there might be something wrong about SFRs, but what about dust...
arxiv.org/abs/2501.12008
The issue: the accretion rate is key for the properties of cluster halos, but we have no reliable observational proxies. So we decided to use ML to look for "optimal" info in realistic X-ray/SZ maps from MTNG.
The issue: the accretion rate is key for the properties of cluster halos, but we have no reliable observational proxies. So we decided to use ML to look for "optimal" info in realistic X-ray/SZ maps from MTNG.
colossus.astro.umd.edu
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colossus.astro.umd.edu
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