SED fitting with flexible delayed, NonParametric, and extended Regulator SFH models on CEERS/MIRI galaxies shows MIRI boosts QGC counts by up to 45% and finds 13% of QGCs have AV > 0.5 regardless of SFH.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2025 2representative citing papers
J-PLUS DR3 yields Schechter-function stellar mass functions for quiescent and star-forming galaxies at 0.05 <= z <= 0.2 that match prior work, with quiescent galaxies showing higher characteristic mass and flatter faint-end slope.
citing papers explorer
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Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry
SED fitting with flexible delayed, NonParametric, and extended Regulator SFH models on CEERS/MIRI galaxies shows MIRI boosts QGC counts by up to 45% and finds 13% of QGCs have AV > 0.5 regardless of SFH.
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J-PLUS: The stellar mass function of quiescent and star-forming galaxies at 0.05 <= z <= 0.2
J-PLUS DR3 yields Schechter-function stellar mass functions for quiescent and star-forming galaxies at 0.05 <= z <= 0.2 that match prior work, with quiescent galaxies showing higher characteristic mass and flatter faint-end slope.