Galaxy Protoclusters as Drivers of Cosmic Reionization: II. Te-Based Metallicities of Lyman- alpha Emitters

arXiv:2610.01811 · astro-ph.GA · Submitted 2026-10-01 · Read on arXiv

astro-ph.GA

Submitted: 2026-10-01

Updated: 2026-10-01

Terminology

• Metallicity — 46× in this paper · explained in 3 episodes
• Abundance — 10× in this paper · explained in 1 episode
• Aperture — 8× in this paper · explained in 1 episode
• Aperture Correction — 4× in this paper · explained in 1 episode
• Calibration — 4× in this paper · explained in 7 episodes
• Trace — 3× in this paper · explained in 2 episodes
• Adam — 2× in this paper · explained in 2 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Core — 2× in this paper · explained in 2 episodes
• Dust Attenuation — 2× in this paper · explained in 2 episodes
• Star Formation Rate (SFR) — 2× in this paper · explained in 5 episodes
• alpha — 2× in this paper · explained in 1 episode
• Aperture Photometry — 1× in this paper · explained in 1 episode
• Commentary — 1× in this paper · explained in 2 episodes
• Gravitational Lensing — 1× in this paper · explained in 2 episodes
• Initial Mass Function (IMF) — 1× in this paper · explained in 2 episodes
• JWST Advanced Deep Extragalactic Survey — 1× in this paper
• James Webb Space Telescope — 1× in this paper

Sources

• Ionised gas kinematics and dynamical masses of $z\gtrsim6$ galaxies from JADES/NIRSpec high-resolution spectroscopy
• A Glimpse of the Low-Mass End of the Direct Mass-Metallicity Relation at $z\sim6-8$
• JADES: Physical properties of Ly$\alpha$ and non-Ly$\alpha$ emitters at z ~ 4.8-9.6

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