Constraining the evolution of the ionizing background and the epoch of reionization with z ∼ 6 quasars. II. A sample of 19 quasars

Xiaohui Fan, Michael A. Strauss, Robert H. Becker, Richard L. White, James E. Gunn, Gillian R. Knapp, Gordon T. Richards, Donald P. Schneider, J. Brinkmann, Masataka Fukugita

Research output: Contribution to journalArticle

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Abstract

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 19 quasars at 5.74 < zem < 6.42 discovered in the Sloan Digital Sky Survey. Three methods are used to trace IGM properties: (1) the evolution of the Gunn-Peterson (GP) optical depth in the Lyα, Lyβ, and Lyγ transitions; (2) the distribution of lengths of dark absorption gaps; and (3) the size of H II 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 τ GP eff ∼ (1 + z) 4.3 to (1 + z) ≳11, and the average length of dark gaps with τ > 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 gsim;4 in the UV background at z > 6, when the mean free path of UV photons is comparable to the correlation length of the starforming galaxies that are thought to have caused reionization. The mean length of dark gaps shows the most dramatic increase at z ∼ 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 H II regions around luminous quasars decrease rapidly toward higher redshift, suggesting that the neutral fraction of the IGM has increased by a factor of gsim;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 ∼ 6.2 based on the GP optical depth and H II region size measurements. The observations suggest that z ∼ 6 is the end of the overlapping stage of reionization and are inconsistent with a mostly neutral IGM at z ∼ 6, as indicated by the finite length of the dark absorption gaps.

Original languageEnglish (US)
Pages (from-to)117-136
Number of pages20
JournalAstronomical Journal
Volume132
Issue number1
DOIs
StatePublished - Jul 2006

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intergalactic media
quasars
time measurement
optical depth
optical thickness
H II regions
ionization
line of sight
mean free path
probe
statistics
galaxies
probes
photons

Keywords

  • Cosmology: observations
  • Intergalactic medium
  • Quasars: absorption lines
  • Quasars: general

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Constraining the evolution of the ionizing background and the epoch of reionization with z ∼ 6 quasars. II. A sample of 19 quasars. / Fan, Xiaohui; Strauss, Michael A.; Becker, Robert H.; White, Richard L.; Gunn, James E.; Knapp, Gillian R.; Richards, Gordon T.; Schneider, Donald P.; Brinkmann, J.; Fukugita, Masataka.

In: Astronomical Journal, Vol. 132, No. 1, 07.2006, p. 117-136.

Research output: Contribution to journalArticle

Fan, X, Strauss, MA, Becker, RH, White, RL, Gunn, JE, Knapp, GR, Richards, GT, Schneider, DP, Brinkmann, J & Fukugita, M 2006, 'Constraining the evolution of the ionizing background and the epoch of reionization with z ∼ 6 quasars. II. A sample of 19 quasars', Astronomical Journal, vol. 132, no. 1, pp. 117-136. https://doi.org/10.1086/504836
Fan, Xiaohui ; Strauss, Michael A. ; Becker, Robert H. ; White, Richard L. ; Gunn, James E. ; Knapp, Gillian R. ; Richards, Gordon T. ; Schneider, Donald P. ; Brinkmann, J. ; Fukugita, Masataka. / Constraining the evolution of the ionizing background and the epoch of reionization with z ∼ 6 quasars. II. A sample of 19 quasars. In: Astronomical Journal. 2006 ; Vol. 132, No. 1. pp. 117-136.
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AU - Strauss, Michael A.

AU - Becker, Robert H.

AU - White, Richard L.

AU - Gunn, James E.

AU - Knapp, Gillian R.

AU - Richards, Gordon T.

AU - Schneider, Donald P.

AU - Brinkmann, J.

AU - Fukugita, Masataka

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N2 - 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 19 quasars at 5.74 < zem < 6.42 discovered in the Sloan Digital Sky Survey. Three methods are used to trace IGM properties: (1) the evolution of the Gunn-Peterson (GP) optical depth in the Lyα, Lyβ, and Lyγ transitions; (2) the distribution of lengths of dark absorption gaps; and (3) the size of H II 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 τ GP eff ∼ (1 + z) 4.3 to (1 + z) ≳11, and the average length of dark gaps with τ > 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 gsim;4 in the UV background at z > 6, when the mean free path of UV photons is comparable to the correlation length of the starforming galaxies that are thought to have caused reionization. The mean length of dark gaps shows the most dramatic increase at z ∼ 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 H II regions around luminous quasars decrease rapidly toward higher redshift, suggesting that the neutral fraction of the IGM has increased by a factor of gsim;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 ∼ 6.2 based on the GP optical depth and H II region size measurements. The observations suggest that z ∼ 6 is the end of the overlapping stage of reionization and are inconsistent with a mostly neutral IGM at z ∼ 6, as indicated by the finite length of the dark absorption gaps.

AB - 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 19 quasars at 5.74 < zem < 6.42 discovered in the Sloan Digital Sky Survey. Three methods are used to trace IGM properties: (1) the evolution of the Gunn-Peterson (GP) optical depth in the Lyα, Lyβ, and Lyγ transitions; (2) the distribution of lengths of dark absorption gaps; and (3) the size of H II 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 τ GP eff ∼ (1 + z) 4.3 to (1 + z) ≳11, and the average length of dark gaps with τ > 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 gsim;4 in the UV background at z > 6, when the mean free path of UV photons is comparable to the correlation length of the starforming galaxies that are thought to have caused reionization. The mean length of dark gaps shows the most dramatic increase at z ∼ 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 H II regions around luminous quasars decrease rapidly toward higher redshift, suggesting that the neutral fraction of the IGM has increased by a factor of gsim;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 ∼ 6.2 based on the GP optical depth and H II region size measurements. The observations suggest that z ∼ 6 is the end of the overlapping stage of reionization and are inconsistent with a mostly neutral IGM at z ∼ 6, as indicated by the finite length of the dark absorption gaps.

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