Direct Te-based metallicities at z≈10 are 3× lower than at z=0-3, extending the gradual FMR offset and pointing to pristine gas inflows during early galaxy assembly.
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3 Pith papers cite this work, alongside 6 external citations. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
JWST data show the A2744-z7p9OD protocluster at z=7.88 as the most extreme evolved overdensity yet seen at z>7, with a dusty massive core in a synchronized lulling phase and high neutral hydrogen columns.
A source 660 million years after the Big Bang is interpreted as a black hole star with a dust-free dense gas atmosphere, implying Little Red Dots have black hole masses overestimated by orders of magnitude.
citing papers explorer
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Novel $z\sim~10$ auroral line measurements extend the gradual offset of the FMR deep into the first Gyr of cosmic time
Direct Te-based metallicities at z≈10 are 3× lower than at z=0-3, extending the gradual FMR offset and pointing to pristine gas inflows during early galaxy assembly.
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Before its time: a remarkably evolved protocluster core at z=7.88
JWST data show the A2744-z7p9OD protocluster at z=7.88 as the most extreme evolved overdensity yet seen at z>7, with a dusty massive core in a synchronized lulling phase and high neutral hydrogen columns.
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A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots
A source 660 million years after the Big Bang is interpreted as a black hole star with a dust-free dense gas atmosphere, implying Little Red Dots have black hole masses overestimated by orders of magnitude.