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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5 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 5representative citing papers
The Big Wheel at z~3 has a stellar-to-halo mass ratio of 0.06, higher than expected, implying efficient stellar assembly without major mergers or instabilities.
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.
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.
A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.
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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The galaxy-halo connection and the dynamical evolution of a giant disc in a massive node of the Cosmic Web at z~3
The Big Wheel at z~3 has a stellar-to-halo mass ratio of 0.06, higher than expected, implying efficient stellar assembly without major mergers or instabilities.
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The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
Uncertainties in stellar evolution and IMF lead to stellar mass errors of ~0.3 dex at z~0 and ~0.6 dex at z~2, plus ~0.4 mag uncertainty in K-band luminosity evolution per unit redshift.
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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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Star Formation in the Milky Way and Nearby Galaxies
A review summarizing observations of star formation and gas relations from molecular clouds to entire galaxies, with updated rate calculation prescriptions.