Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
A significant fraction of high redshift star-forming disc galaxies are known to host giant clumps, whose nature and role in galaxy evolution are yet to be understood. In this work, we first present a new method based on neural networks to detect clumps in galaxy images. We use this method to detect clumps in the rest-frame optical and UV images of
Huertas-Company, Marc et al.
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9
2020