Chasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly$\alpha$ Forest over $5 < z < 6$
Yongda Zhu, George D. Becker, Sarah E. I. Bosman, Laura C. Keating,, Holly M. Christenson, Eduardo Ba\~nados, Fuyan Bian, Frederick B. Davies,, Valentina D'Odorico, Anna-Christina Eilers, Xiaohui Fan, Martin G. Haehnelt,, Girish Kulkarni, Andrea Pallottini, Yuxiang Qin

TL;DR
This study uses dark gap statistics in the Lyα forest from 55 quasar spectra to investigate the end stages of cosmic reionization, finding evidence that neutral hydrogen persists until at least redshift 5.3.
Contribution
It introduces a new analysis of dark gaps in the Lyα forest to constrain the timeline of cosmic reionization using extensive quasar data and hydrodynamical simulations.
Findings
Long dark gaps persist down to z ≈ 5.3.
The fraction of spectra with gaps >30 h^{-1} Mpc decreases with redshift.
Results are consistent with reionization extending below z=6.
Abstract
We present a new investigation of the intergalactic medium (IGM) near the end of reionization using "dark gaps" in the Lyman-alpha (Ly) forest. Using spectra of 55 QSOs at , including new data from the XQR-30 VLT Large Programme, we identify gaps in the Ly forest where the transmission averaged over 1 comoving bins falls below 5%. Nine ultra-long () dark gaps are identified at . In addition, we quantify the fraction of QSO spectra exhibiting gaps longer than , , as a function of redshift. We measure , 0.6, and 0.15 at , 5.8, and 5.6, respectively, with the last of these long dark gaps persisting down to . Comparing our results with predictions from hydrodynamical simulations, we find that the data are consistent with models wherein…
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