Stellar mass functions in the peaks of the Hyperion protostructure at z~2.5 show a mass-dependent excess relative to the field, with ~10x enhancement at log(M*/M⊙)~11 versus ~3.5x at log(M*/M⊙)~9.5.
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At z=0.9, disk galaxies show a TFR slope of 3.82 and FR slope of 0.44 with moderate TFR and strong FR evolution from z=0, implying higher and less mass-dependent stellar-to-halo mass fractions f_M while f_j remains near 0.8.
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.
citing papers explorer
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The HST-Hyperion Survey: Environmental Imprints on the Stellar-Mass Function at z~2.5
Stellar mass functions in the peaks of the Hyperion protostructure at z~2.5 show a mass-dependent excess relative to the field, with ~10x enhancement at log(M*/M⊙)~11 versus ~3.5x at log(M*/M⊙)~9.5.
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Kinematic scaling relations of disc galaxies from ionised gas at $z\sim1$ and their connection with dark matter haloes
At z=0.9, disk galaxies show a TFR slope of 3.82 and FR slope of 0.44 with moderate TFR and strong FR evolution from z=0, implying higher and less mass-dependent stellar-to-halo mass fractions f_M while f_j remains near 0.8.
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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.