Evidence of patchy hydrogen reionization from an extreme Ly trough below redshift six
arXiv:1407.4850 · doi:10.1093/mnras/stu2646
Abstract
We report the discovery of an extremely long (110 Mpc/) and dark () Ly trough extending down to towards the quasar ULAS J0148+0600. We use these new data in combination with Ly forest measurements from 42 quasars at to conduct an updated analysis of the line-of-sight variance in the intergalactic Ly opacity over . We find that the scatter in transmission among lines of sight near significantly exceeds theoretical expectations for either a uniform ultraviolet background (UVB) or simple fluctuating UVB models in which the mean free path to ionizing photons is spatially invariant. The data, particularly near -5.8, instead require fluctuations in the volume-weighted hydrogen neutral fraction that are a factor of 3 or more beyond those expected from density variations alone. We argue that these fluctuations are most likely driven by large-scale variations in the mean free path, consistent with expectations for the final stages of inhomogeneous hydrogen reionization. Even by , however, a large fraction of the data are consistent with a uniform UVB, and by the data are fully consistent with opacity fluctuations arising solely from the density field. This suggests that while reionization may be ongoing at , it has fully completed by .
19 pages, 20 figures, MNRAS, in press
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