Overview
- JWST’s NIRSpec/PRISM spectroscopy secures MoM‑z14 at z_spec = 14.44, placing its light about 280 million years after the Big Bang and setting a new distance record.
- The redshift is anchored by a sharp Lyman‑alpha break with roughly 3σ detections of five rest‑UV emission lines, providing a robust spectroscopic confirmation.
- MoM‑z14 is luminous (M_UV ≈ −20.2), extremely compact (effective radius ~74 pc) and elongated, with a steep UV slope (β ≈ −2.5) indicating little dust and no dominant AGN.
- Strong nitrogen features with highly super‑solar [N/C] > 1 suggest rapid chemical enrichment reminiscent of patterns in globular clusters, though interpretations remain preliminary.
- The MoM survey infers a number density of bright z ~ 14–15 galaxies over 100× higher than pre‑JWST models, and the spectrum’s lack of a strong damping wing hints at a locally ionized region during reionization, motivating further JWST follow‑up and wider samples from the upcoming Roman telescope.