Extended CIII] emission offset from the stars in a z=14.18 galaxy indicates outflows with mass outflow rate ~160 solar masses per year and mass-loading factor 4-15, constraining star-formation efficiency to below 0.08.
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4 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 4years
2026 4representative citing papers
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.
Switching between four common stellar population synthesis models produces systematic offsets of up to 0.6 dex in stellar mass and 0.4 dex in star formation rate for the same galaxies.
AnomalyMatch applied to JWST data identified 58 gravitational lenses, 37 new, graded by experts and spanning redshifts to zphot ~2.1.
citing papers explorer
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Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0
Extended CIII] emission offset from the stars in a z=14.18 galaxy indicates outflows with mass outflow rate ~160 solar masses per year and mass-loading factor 4-15, constraining star-formation efficiency to below 0.08.
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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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Impact of stellar population models on the estimated physical properties of galaxies
Switching between four common stellar population synthesis models produces systematic offsets of up to 0.6 dex in stellar mass and 0.4 dex in star formation rate for the same galaxies.
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High-Redshift Gravitational Lens Discoveries in JWST NIRCam Using AnomalyMatch
AnomalyMatch applied to JWST data identified 58 gravitational lenses, 37 new, graded by experts and spanning redshifts to zphot ~2.1.