Constraining the galaxy-halo connection at z>10 using the neighbors of UV-bright galaxies

arXiv:2609.33817 · astro-ph.GA, astro-ph.CO · Submitted 2026-09-27 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-09-27

Updated: 2026-09-27

Terminology

• Clustering — 62× in this paper · explained in 2 episodes
• Adam — 16× in this paper · explained in 2 episodes
• Abundance — 15× in this paper · explained in 1 episode
• AGN — 8× in this paper · explained in 1 episode
• Trace — 8× in this paper · explained in 2 episodes
• Degeneracy — 4× in this paper · explained in 3 episodes
• Dust Attenuation — 3× in this paper · explained in 2 episodes
• N-body simulations — 2× in this paper · explained in 2 episodes
• Interpretability — 1× in this paper · explained in 15 episodes
• Matter Power Spectrum — 1× in this paper · explained in 2 episodes
• Metallicity — 1× in this paper · explained in 3 episodes
• Simulation-Based Inference (SBI) — 1× in this paper · explained in 3 episodes
• Simulation-based Inference — 1× in this paper · explained in 2 episodes
• Wide Field Instrument — 1× in this paper

Sources

• Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0
• SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$
• SPURS: Massive Stars, Dense Gas, and Ly alpha Escape in GN-z11 at z = 10.6
• A UV-Luminous Galaxy at z=11 with Surprisingly Weak Star Formation Activity
• Stochastic star formation and the abundance of $z>10$ UV-bright galaxies
• BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies
• Think inside the box: cosmic variance and large-scale conformity of high-redshift massive galaxies in the FLAMINGO simulations
• The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6
• A search for the first galaxies across $>0.6$ deg$^2$ of JWST imaging: new evidence for a rapid decline in star-formation activity at $z>12$
• Roman Observations Time Allocation Committee: Final Report and Recommendations
• An Improved Fit for Linear Halo Bias at High Redshift
• JADES: Dynamical Measurements of Dark Matter Halo Masses at z about 7 Using Galaxy Pairs

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