Discovery of an overdense 'Cosmic Archipelago' of young metal-poor star-forming galaxies at z~6.14 with one detailed example showing high Lyman-continuum escape fraction suggesting significant contribution to cosmic reionization.
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5 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 5representative citing papers
A massive galaxy at z=9.3 shows bursty star formation with a recent downturn and sits in a small ionized bubble in a neutral IGM.
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.
Simulations show observationally selected protocluster candidates at z ≳ 5 include significant interlopers, undergo 2-6 major mergers, and exhibit stronger clustering than observed, requiring total galaxy mass within 10 cMpc for reliable progenitor identification.
A review summarizing recent advances in strong gravitational lensing applications and near-future prospects with the James Webb Space Telescope.
citing papers explorer
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A Cosmic Archipelago of lensed metal-poor galaxies at $z\sim6$
Discovery of an overdense 'Cosmic Archipelago' of young metal-poor star-forming galaxies at z~6.14 with one detailed example showing high Lyman-continuum escape fraction suggesting significant contribution to cosmic reionization.
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SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$
A massive galaxy at z=9.3 shows bursty star formation with a recent downturn and sits in a small ionized bubble in a neutral IGM.
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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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On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$
Simulations show observationally selected protocluster candidates at z ≳ 5 include significant interlopers, undergo 2-6 major mergers, and exhibit stronger clustering than observed, requiring total galaxy mass within 10 cMpc for reliable progenitor identification.