The interstellar medium conditions of a strong Lya emitter at z = 8.279 revealed by JWST: a robust LyC leaker candidate at the Epoch of Reionization
Rafael Navarro-Carrera, Karina I. Caputi, Edoardo Iani, Pierluigi, Rinaldi, Vasily Kokorev, Josephine Kerutt

TL;DR
This study uses JWST data to analyze a high-redshift galaxy, GN-z8-LAE, revealing its interstellar medium conditions and strong Lyman continuum leakage, making it a promising candidate for contributing to cosmic reionization.
Contribution
It provides detailed ISM properties and LyC escape fraction estimates for a z=8.279 galaxy, highlighting its role in reionization and identifying it as a robust LyC leaker candidate.
Findings
GN-z8-LAE is a young, low-mass galaxy with high star formation surface density.
The galaxy shows a small Lya velocity offset and a hard ionization field without AGN signatures.
It has a high Lyman continuum escape fraction (>14%), indicating efficient reionization contribution.
Abstract
Making use of JWST NIRSpec and NIRCam data, we conduct a detailed analysis of the spectroscopic and photometric properties of GN-z8-LAE, a strong Lya emitter at z=8.279. Our goal is to investigate the interstellar medium (ISM) physical conditions that enable the Lya detection in this source at the Epoch of Reionization (EoR) and scrutinize GN-z8-LAE as an early reionizer. In broad agreement with previous results, we find that GN-z8-LAE is a young galaxy (age ~ 10 Myr) with a low stellar mass (M* ~ 10^7.66 Msun), significantly lower than those of most Lya emitters known at similarly high redshifts. The derived stellar mass and star formation rate surface densities are 355 Msun/pc^2 and 88 Msun/yr/kpc^2, respectively. Our spectral analysis indicates that: the Lya line peak has a small velocity offset 133+-72 km/s with respect to the galaxy systemic redshift; CIV] / CIII] ~ 3.3; the ISM is…
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Taxonomy
TopicsParticle accelerators and beam dynamics · Atomic and Molecular Physics · Magnetic confinement fusion research
