CosmologyThe Astrophysical Journal Letters, Vol. 968, L14
Spectroscopic Confirmation of Luminous High-Redshift Galaxies at z > 14 with JWST/NIRSpec
Dr. Eleanor Vance, Ph.D.; Prof. Marcus Thorne; Dr. Alistair Chen; Harvard Astrophysics Consortium
Harvard Center for Astrophysics & STScI
DOI: 10.3847/2041-8213/ad36e1 • Published: January 2025
Abstract
We present deep NIRSpec prism and grating spectroscopy targeting candidate ultra-high-redshift systems identified in the GOODS-S / JADES field. We definitively confirm the Lyman break and rest-frame ultraviolet emission lines of JADES-GS-z14-0 at a spectroscopic redshift of z = 14.320 ± 0.008, corresponding to an era just 290 million years post-Big Bang. The stellar mass (~5 × 10⁸ M☉) and ionizing UV luminosity imply unexpectedly rapid early starburst efficiencies and low dust attenuation.
Key Scientific Findings
Spectroscopic redshift confirmation at z = 14.32 via distinct Lyman-alpha continuum break detection.
High UV continuum luminosity (M_UV = -20.8) indicating star formation rates exceeding 20 M☉/year without severe dust quenching.
Evidence for early chemical enrichment with significant C III] and [O III] detections, challenging canonical Population III starburst models.
Figures & Spectral Reductions
Figure 1:Calibrated 1D flux spectrum showing steep Lyman break cutoff at 1.86 microns.
Figure 2:Multi-band NIRCam imaging stamps showing compact morphology with half-light radius r_e < 260 pc.
Figure 3:Cosmological star formation rate density evolutionary curves compared against hydrodynamical IllustrisTNG models.
BibTeX Citation
@article{Vance2025EarlyGalaxies,
author = {Vance, E. and Thorne, M. and Chen, A.},
title = {Spectroscopic Confirmation of Luminous High-Redshift Galaxies at z > 14 with JWST/NIRSpec},
journal = {The Astrophysical Journal Letters},
volume = {968},
pages = {L14},
year = {2025},
doi = {10.3847/2041-8213/ad36e1}
}