2025/05/29 by Zuyi Chen, Daniel P. Stark, Chen, Zuyi +11
Computer Science · Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Astrophysics of Galaxies (astro-ph.GA) #Computational Physics and Python Applications #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Gamma-ray bursts and supernovae
paper · pdf · doi:10.48550/arxiv.2505.24080
openalex publication_date 2025/05/29 · openalex created_date 2025/10/14 · openalex updated_date 2026/08/02
Lyα spectroscopy with JWST is opening a new window on the sizes of ionized bubbles through the reionization epoch. Theoretical expectations suggest typical bubble radii should be 0.6-1.5 pMpc at z≃ 7, assuming neutral hydrogen fractions of the intergalactic medium in the range x\rm HI=0.5-0.7. Here we investigate this picture using JWST to characterize the environment and Lyα emission of 292 galaxies at 7.0