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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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.