Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six
We report the discovery of an extremely long (∼110 Mpc/h) 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-si...
| Main Authors: | , , , , , |
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| Format: | Article |
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Oxford University Press
2015
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| Online Access: | https://eprints.nottingham.ac.uk/34605/ |
| _version_ | 1848794892454592512 |
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| author | Becker, George D. Bolton, James S. Madau, Piero Pettini, Max Ryan-Weber, Emma V. Venemans, Bram P. |
| author_facet | Becker, George D. Bolton, James S. Madau, Piero Pettini, Max Ryan-Weber, Emma V. Venemans, Bram P. |
| author_sort | Becker, George D. |
| building | Nottingham Research Data Repository |
| collection | Online Access |
| description | We report the discovery of an extremely long (∼110 Mpc/h) 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. |
| first_indexed | 2025-11-14T19:23:25Z |
| format | Article |
| id | nottingham-34605 |
| institution | University of Nottingham Malaysia Campus |
| institution_category | Local University |
| last_indexed | 2025-11-14T19:23:25Z |
| publishDate | 2015 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | nottingham-346052020-05-04T17:04:46Z https://eprints.nottingham.ac.uk/34605/ Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six Becker, George D. Bolton, James S. Madau, Piero Pettini, Max Ryan-Weber, Emma V. Venemans, Bram P. We report the discovery of an extremely long (∼110 Mpc/h) 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. Oxford University Press 2015-03-11 Article PeerReviewed Becker, George D., Bolton, James S., Madau, Piero, Pettini, Max, Ryan-Weber, Emma V. and Venemans, Bram P. (2015) Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six. Monthly Notices of the Royal Astronomical Society, 447 (4). pp. 3402-3419. ISSN 1365-2966 Intergalactic Medium Quasars Absorption Lines Cosmology Observations Dark Ages Reionization First Stars Large-scale Structure of the Universe http://mnras.oxfordjournals.org/content/447/4/3402 doi:10.1093/mnras/stu2646 doi:10.1093/mnras/stu2646 |
| spellingShingle | Intergalactic Medium Quasars Absorption Lines Cosmology Observations Dark Ages Reionization First Stars Large-scale Structure of the Universe Becker, George D. Bolton, James S. Madau, Piero Pettini, Max Ryan-Weber, Emma V. Venemans, Bram P. Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six |
| title | Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six |
| title_full | Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six |
| title_fullStr | Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six |
| title_full_unstemmed | Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six |
| title_short | Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six |
| title_sort | evidence of patchy hydrogen reionization from an extreme lyα trough below redshift six |
| topic | Intergalactic Medium Quasars Absorption Lines Cosmology Observations Dark Ages Reionization First Stars Large-scale Structure of the Universe |
| url | https://eprints.nottingham.ac.uk/34605/ https://eprints.nottingham.ac.uk/34605/ https://eprints.nottingham.ac.uk/34605/ |