Hydrangea simulations show over 85% of S0 galaxies are cluster satellites formed primarily by environmental stripping of spirals rather than mergers.
M., Kolesnikov, I., de Carvalho, R
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Extension of an existing deep-learning pipeline to JWST data identifies 382 disk-like galaxies among 1380 massive systems at 0.5 < z < 4, indicating such morphologies persist to high redshift.
citing papers explorer
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Characterizing the Formation and Evolution of S0-galaxies (CaFES-0): Their formation pathways around Galaxy Clusters
Hydrangea simulations show over 85% of S0 galaxies are cluster satellites formed primarily by environmental stripping of spirals rather than mergers.
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Enhancing Galaxy Classification with U-Net Variational Autoencoders. III. Disk-like Galaxy Identification in JWST Samples of up to redshift 4
Extension of an existing deep-learning pipeline to JWST data identifies 382 disk-like galaxies among 1380 massive systems at 0.5 < z < 4, indicating such morphologies persist to high redshift.