Direct detection of ionizing photons from z~6 faint galaxies yields escape fraction ~0.8 and log ξ_ion^true = 25.86, implying higher IGM transparency and that young low-metallicity stars in such galaxies can reionize the universe.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
TECHNICOLOR DAWN simulations reveal an inside-out-middle reionization topology where CGM remains more neutral than IGM at z=5.5, and PDLA column density depends primarily on halo mass rather than neutral fraction.
citing papers explorer
-
The Great Escape of ionizing photons during Cosmic Morning
Direct detection of ionizing photons from z~6 faint galaxies yields escape fraction ~0.8 and log ξ_ion^true = 25.86, implying higher IGM transparency and that young low-metallicity stars in such galaxies can reionize the universe.
-
Galaxy Proximate Damped Lyman-Alpha Systems and HI Reionization Topology in TECHNICOLOR DAWN
TECHNICOLOR DAWN simulations reveal an inside-out-middle reionization topology where CGM remains more neutral than IGM at z=5.5, and PDLA column density depends primarily on halo mass rather than neutral fraction.