Glimpsing through the high redshift neutral hydrogen fog
S. Gallerani, A. Ferrara, X. Fan, T. R. Choudhury

TL;DR
This study uses high-redshift quasar spectra to refine constraints on the neutral hydrogen fraction during reionization, revealing smooth evolution and evidence of local ionization effects, including the first detection of a transverse proximity effect.
Contribution
It provides new measurements of the neutral hydrogen fraction at z~6 and reports the first detection of a transverse proximity effect in the Lyalpha forest.
Findings
Neutral hydrogen fraction decreases smoothly from 10^{-4.4} to 10^{-4.2} between z=5.3 and 5.6.
Upper limit of xHI<0.36 at z=6.3 constrains reionization timeline.
First detection of transverse proximity effect indicating local radiation enhancement.
Abstract
We analyze the transmitted flux in a sample of 17 QSOs spectra at 5.74<zem<6.42 to obtain tighter constraints on the volume-averaged neutral hydrogen fraction, xHI, at z~6. We study separately the narrow transmission windows (peaks) and the wide dark portions (gaps) in the observed absorption spectra. By comparing the statistics of these spectral features with Lyalpha forest simulations, we conclude that xHI evolves smoothly from 10^{-4.4} at z=5.3 to 10^{-4.2} at z=5.6, with a robust upper limit xHI<0.36 at z=6.3. The frequency and physical sizes of the peaks imply an origin in cosmic underdense regions and/or in HII regions around faint quasars or galaxies. In one case (the intervening HII region of the faint quasar RD J1148+5253 at z=5.70 along the LOS of SDSS J1148+5251 at z=6.42) the increase of the peak spectral density is explained by the first-ever detected transverse proximity…
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