Evidence for Large-Scale Fluctuations in the Metagalactic Ionizing Background Near Redshift Six
arXiv:1803.08932 · doi:10.3847/1538-4357/aacc73
Abstract
The observed scatter in intergalactic Lyman- opacity at requires large-scale fluctuations in the neutral fraction of the intergalactic medium (IGM) after the expected end of reionization. Post-reionization models that explain this scatter invoke fluctuations in either the ionizing ultraviolet background (UVB) or IGM temperature. These models make very different predictions, however, for the relationship between Lyman- opacity and local density. Here we test these models using Lyman- emitting galaxies (LAEs) to trace the density field surrounding the longest and most opaque known Lyman- trough at . Using deep Subaru Hyper Suprime-Cam narrow-band imaging, we find a highly significant deficit of LAEs within 20 Mpc/ of the trough. The results are consistent with a model in which the scatter in Lyman- opacity near is driven by large-scale UVB fluctuations, and disfavor a scenario in which the scatter is primarily driven by variations in IGM temperature. UVB fluctuations at this epoch present a boundary condition for reionization models, and may help shed light on the nature of the ionizing sources.
arXiv comment13 pages, 9 figure, submitted to ApJ, comments welcome
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