First-star imprints in a metal-poor galaxy overdensity near the end of reionization
astro-ph.GA
Submitted: 2026-06-30
Updated: 2026-09-08
Comments: Submitted to Nature Astronomy. Comments are welcome
Code: https://github.com/XQR-30/Metal-catalogue
Project page: https://eiger-jwst.github.io/data.html
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GLIMPSE-D: An Exotic Balmer-Jump Object at z=6.20? Revisiting Photometric Selection and the Cosmic Abundance of Pop III Galaxies
- Hunting for the First Explosions at the High-Redshift Frontier
- An Ultra-Faint, Chemically Primitive Galaxy Forming in the Reionization Era
- Novel $z\sim~10$ auroral line measurements extend the gradual offset of the FMR deep into the first Gyr of cosmic time
- Pristine Massive Star Formation Caught at the Break of Cosmic Dawn
- The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6
- GA-NIFS and JADES: Confirmation of pristine gas near GN-z11
- The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars
- Catching the Nebular Needle in a Polluted Haystack: Line-emission Signatures from Population III-forming Pockets around Massive Galaxies at the End of Reionization
- EIGER VIII: First stars signatures in the connection between OI absorption and Galaxies in the Epoch of Reionization
- EIGER VII. The evolving relationship between galaxies and the intergalactic medium in the final stages of reionization
- A Cosmic Archipelago of lensed metal-poor galaxies at $z\sim6$
- JWST ASPIRE: How Did Galaxies Complete Reionization? Evidence for Excess IGM Transmission around ${\rm [O\,{\scriptstyle III}]}$ Emitters during Reionization
- How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background
- The THESAN-ZOOM project: The Hidden Neighbours of OI Absorbers during Reionization
- The galaxy-IGM connection in THESAN: observability and information content of the galaxy-Lyman-$\alpha$ cross-correlation at z$\geq$6
- Rapid, out of equilibrium metal enrichment indicated by a flat mass-metallicity relation at z~6 from NIRCam grism spectroscopy
- SpectRes: A Fast Spectral Resampling Tool in Python
- The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10
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