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JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe

Nakane, Minami et al.
arXiv (All) · Papers
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astrophysics-of-galaxies
We investigate UV absorption lines tracing cool gas in eight bright ($-21.9 < M_\mathrm{UV} < -20.5$) galaxies at $z=7.2-10.6$ using deep archival JWST/NIRSpec medium-resolution spectra. The eight galaxies were homogeneously selected based on wavelength coverage and data quality from 362 galaxies at
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