JWST auroral-line selected galaxies at high redshift show an MZR slope of 0.38 with selection biases favoring high-SFR low-metallicity systems, while stacked non-detections lie closer to the fundamental metallicity relation.
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7 Pith papers cite this work. Polarity classification is still indexing.
7
Pith papers citing it
representative citing papers
Type Ic core-collapse supernovae explode in systematically younger environments than Types II, IIb, and Ib, indicating they arise from more massive progenitors via a distinct channel.
A HeII-based correction method makes UV and optical measurements of electron temperature and O/H metallicity agree within 0.1 dex in three nearby BCD galaxies.
Simulations match observed outflow masses within 0.5 dex but underpredict velocities by an order of magnitude and show face-on galaxies 15-40% more likely to exhibit detectable outflows than edge-on systems.
Chemically decoupled massive galaxies in IllustrisTNG dominate the high end of a present-day habitability proxy by over an order of magnitude due to a trade-off between suppressed planet formation and reduced sterilizing events.
Green Pea and Blueberry galaxies live in isolated low-density environments with the lowest neighbor counts among compared galaxy populations.
A multimodal neural network trained on MPA-JHU references produces SFR, stellar mass, and metallicity estimates for 547 million low-redshift galaxies in DESI LS DR10.
citing papers explorer
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Shape of Direct-Method Mass-Metallicity Relation with JWST: Fast-Track Nitrogen and Helium Enrichment
JWST auroral-line selected galaxies at high redshift show an MZR slope of 0.38 with selection biases favoring high-SFR low-metallicity systems, while stacked non-detections lie closer to the fundamental metallicity relation.
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A statistical study of the environmental age of core-collapse supernovae based on VLT/MUSE integral-field-unit spectroscopy
Type Ic core-collapse supernovae explode in systematically younger environments than Types II, IIb, and Ib, indicating they arise from more massive progenitors via a distinct channel.
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Consistent Gas-Phase Temperatures and Metallicities from UV and Optical Nebular Emission: A Reliable Foundation from z=0 to Cosmic Dawn
A HeII-based correction method makes UV and optical measurements of electron temperature and O/H metallicity agree within 0.1 dex in three nearby BCD galaxies.
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High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
Simulations match observed outflow masses within 0.5 dex but underpredict velocities by an order of magnitude and show face-on galaxies 15-40% more likely to exhibit detectable outflows than edge-on systems.
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The habitability trade-off: Chemical decoupling and quenching in massive galaxies
Chemically decoupled massive galaxies in IllustrisTNG dominate the high end of a present-day habitability proxy by over an order of magnitude due to a trade-off between suppressed planet formation and reduced sterilizing events.
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Blueberry and Green Pea galaxies live in low density environments
Green Pea and Blueberry galaxies live in isolated low-density environments with the lowest neighbor counts among compared galaxy populations.
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A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
A multimodal neural network trained on MPA-JHU references produces SFR, stellar mass, and metallicity estimates for 547 million low-redshift galaxies in DESI LS DR10.