N=ap=owaw=a`enakaulua: a close quasar pair at cosmic dawn in the Aether survey

arXiv:2609.31835 · astro-ph.GA, astro-ph.CO · Submitted 2026-09-25 · Read on arXiv

astro-ph.GA, astro-ph.CO

Submitted: 2026-09-25

Updated: 2026-09-25

Terminology

• Calibration — 13× in this paper · explained in 7 episodes
• Clustering — 11× in this paper · explained in 2 episodes
• Aperture — 8× in this paper · explained in 1 episode
• Trace — 6× in this paper · explained in 2 episodes
• Microlensing — 4× in this paper · explained in 2 episodes
• Elias — 3× in this paper · explained in 2 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Dust Attenuation — 2× in this paper · explained in 2 episodes
• Aperture Correction — 1× in this paper · explained in 1 episode
• Core — 1× in this paper · explained in 2 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Hubble Space Telescope — 1× in this paper
• James Webb Space Telescope — 1× in this paper
• Narrow Line Region — 1× in this paper

Sources

• The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at Redshift around 6
• Clustering of z~6.6 Quasars and [O III] Emitters Constrains Host Halo Masses and Duty Cycles in 25 ASPIRE Fields
• A JWST/NIRSpec Integral Field Unit Survey of Luminous Quasars at z ~ 5-6 (Q-IFU): Rest-frame Optical Nuclear Properties and Extended Nebulae
• Aether-SHELLQs: JWST integral-field spectroscopy of candidate obscured quasars at z ~ 6
• Rapid growth in a dual AGN during a gas-rich merger at z~4.5
• ASPIRE: The Environments and Dark Matter Halos of Luminous Quasars in the Epoch of Reionization

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