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IllustrisTNG vs SIMBA vs Astrid vs Magneticum vs Ramses
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This video shows the spatial distribution of gas density (blue) and gas temperature (red) in 5 different hydrodynamic simulations. All simulations have the same initial conditions but have been run with five different codes. This video illustrates one of the main goals of the CAMELS project: to develop models whose predictions are robust across simulations.
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Astrid vs IllustrisTNG vs SIMBA
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IllustrisTNG vs SIMBA vs Astrid vs Magneticum vs Ramses
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IllustrisTNG vs SIMBA vs Astrid vs Magneticum
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IllustrisTNG vs SIMBA vs Astrid vs Magneticum vs Ramses vs EAGLE
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IllustrisTNG vs Astrid vs Magneticum vs SIMBA
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IllustrisTNG 50 - Formation of a above-average sized galaxy
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Cosmological hydrodynamic simulations: comparison
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CAMELS-IllustrisTNG
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Robust field-level likelihood-free inference with galaxies
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Simulating the formation of Galaxies with TNG50
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AGN Feedback in IllustrisTNG-50 Simulation
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Before real data: pressing graph neural networks to do field-level simulation-based inference w ...
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