The nature of giant clumps in high-z discs: a deep-learning comparison of simulations and observations
We use deep learning to explore the nature of observed giant clumps in high-redshift disc galaxies, based on their identification and classification in cosmological simulations. Simulated clumps are detected using the 3D gas and stellar densities in the VELA zoom-in cosmological simulation suite, with ${\sim}25\ \rm {pc}$ maximum resolution
Ginzburg, Omri et al.
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2021