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Title: Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z~6 Quasars II: A Sample of 19 Quasars

Journal Article · · The Astronomical Journal , vol. 117, N/A, January 6, 2006, pp. 132
DOI:https://doi.org/10.1086/504836· OSTI ID:898445
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We study the evolution of the ionization state of the intergalactic medium (IGM) at the end of the reionization epoch using moderate resolution spectra of a sample of nineteen quasars at 5.74 < z{sub em} < 6.42 discovered in the Sloan Digital Sky Survey. Three methods are used to trace IGM properties: (a) the evolution of the Gunn-Peterson (GP) optical depth in the Ly{alpha}, {beta}, and {gamma} transitions; (b) the distribution of lengths of dark absorption gaps, and (c) the size of HII regions around luminous quasars. Using this large sample, we find that the evolution of the ionization state of the IGM accelerated at z > 5.7: the GP optical depth evolution changes from {tau}{sub GP}{sup eff} {approx} (1 + z){sup 4.3} to (1 + z){sup {approx}> 11}, and the average length of dark gaps with {tau} > 3.5 increases from < 10 to > 80 comoving Mpc. The dispersion of IGM properties along different lines of sight also increases rapidly, implying fluctuations by a factor of {approx}> 4 in the UV background at z > 6, when the mean free path of UV photons is comparable to the correlation length of the star forming galaxies that are thought to have caused reionization. The mean length of dark gaps shows the most dramatic increase at z {approx} 6, as well as the largest line-of-sight variations. We suggest using dark gap statistics as a powerful probe of the ionization state of the IGM at yet higher redshift. The sizes of HII regions around luminous quasars decrease rapidly towards higher redshift, suggesting that the neutral fraction of the IGM has increased by a factor of {approx}> 10 from z = 5.7 to 6.4, consistent with the value derived from the GP optical depth. The mass-averaged neutral fraction is 1-4% at z {approx} 6.2 based on the GP optical depth and HII region size measurements. The observations suggest that z {approx} 6 is the end of the overlapping stage of reionization, and are inconsistent with a mostly neutral IGM at z {approx} 6, as indicated by the finite length of dark absorption gaps.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
898445
Report Number(s):
UCRL-JRNL-220657; TRN: US0701652
Journal Information:
The Astronomical Journal , vol. 117, N/A, January 6, 2006, pp. 132, Journal Name: The Astronomical Journal , vol. 117, N/A, January 6, 2006, pp. 132
Country of Publication:
United States
Language:
English

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71 CLASSICAL AND QUANTUM MECHANICS
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