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Affiliation:, Hosei University, National Astronomical Observatory of Japan
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Over a third of high-equivalent-width narrow-band emitters harbor active galactic nuclei, pinpointing an elusive population of sub-solar metallicity accretion systems that fall outside standard diagnostic classifications.
Massive early galaxies exhibit boosted Ly$\alpha$ visibility despite possessing properties that typically quench it, proving that dense cosmic neighborhoods carved out the primary ionized bubbles driving late-stage reionization.
Spectroscopic confirmation of four $z \sim 3.4$ protoclusters validates that deep learning can accurately direct targeted telescope follow-up to unearth chemically diverse, extreme cosmic structures.
