UVJ colors saturate below log(sSFR) ~ -10.5; new UV/MIR color-color diagrams allow more efficient selection of galaxies with substantially lower ongoing star formation.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2019 2verdicts
UNVERDICTED 2representative citing papers
Merger-disturbed cluster galaxies remain bluer than undisturbed ones across all locations and morphologies, possibly because mergers trigger star formation or protect central gas from stripping.
citing papers explorer
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Beyond UVJ: More Efficient Selection of Quiescent Galaxies With UV / Mid-IR Fluxes
UVJ colors saturate below log(sSFR) ~ -10.5; new UV/MIR color-color diagrams allow more efficient selection of galaxies with substantially lower ongoing star formation.
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Impact of Galaxy Mergers on the Colours of Cluster Galaxies
Merger-disturbed cluster galaxies remain bluer than undisturbed ones across all locations and morphologies, possibly because mergers trigger star formation or protect central gas from stripping.