Year: 2015
Type: article
Abstract: We report the discovery of an extremely long (∼110 Mpc h−1) and dark (τeff ≳ 7) Lyα trough extending down to z ≃ 5.5 towards the zem ≃ 6.0 quasar ULAS J0148+0600. We use these new data in combination with Lyα forest measurements from 42 quasars at 4.5 ≤ zem ≤ 6.4 to conduct an updated analysis of the line-of-sight variance in the intergalactic Lyα opacity over 4 ≤ z ≤ 6. We find that the scatter in transmission among lines of sight near z ∼ 6 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 z ≃ 5.6–5.8, 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 z ≃ 5.6, however, a large fraction of the data are consistent with a uniform UVB, and by z ∼ 5 the data are fully consistent with opacity fluctuations arising solely from the density field. This suggests that while reionization may be ongoing at z ∼ 6, it has fully completed by z ∼ 5.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Awards: Astronomy & Astrophysics at Nottingham, THE STUDY OF THE FORMATION, MERGING HISTORY, AND ENVIRONMENTAL IMPACT OF THE MASSIVE BLACK HOLES (MBHS) THAT ARE UBIQUITOUS IN THE NUCLEI OF LUMINOUS, Nottingham Astronomy Rolling Grant 2011 - 2016, Astronomy Observation and Theory Consolidated Grant 2012, The COSMOS Consortium: Fundamental Cosmology, Dark Energy and the Cosmic Microwave Sky, The Structure of the Universe: Cosmology, Exoplanets and Lattice QCD, DiRAC SMP Facility: Revealing the Structure of the Universe, Collaborative Research: CDI- Type II: Towards Analyzing Complex Petascale Datasets: The Milky Way Laboratory
OpenAlex ID: W2325917856
