Chasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly

Yongda Zhu, George D. Becker, Sarah E.I. Bosman, Laura C. Keating, Holly M. Christenson, Eduardo Bañados, Fuyan Bian, Frederick B. Davies, Valentina D’Odorico, Anna Christina Eilers, Xiaohui Fan, Martin G. Haehnelt, Girish Kulkarni, Andrea Pallottini, Yuxiang Qin, Feige Wang, Jinyi Yang

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

Abstract

We present a new investigation of the intergalactic medium (IGM) near the end of reionization using “dark gaps” in the Lyα forest. Using spectra of 55 QSOs at z em > 5.5, including new data from the XQR-30 VLT Large Programme, we identify gaps in the Lyα forest where the transmission averaged over 1 comoving h −1 Mpc bins falls below 5%. Nine ultralong (L > 80 h −1 Mpc) dark gaps are identified at z < 6. In addition, we quantify the fraction of QSO spectra exhibiting gaps longer than 30 h −1 Mpc, F 30, as a function of redshift. We measure F 30 ≃ 0.9, 0.6, and 0.15 at z = 6.0, 5.8, and 5.6, respectively, with the last of these long dark gaps persisting down to z ≃5.3. Comparing our results with predictions from hydrodynamical simulations, we find that the data are consistent with models wherein reionization extends significantly below redshift six. Models wherein the IGM is essentially fully reionized that retain large-scale fluctuations in the ionizing UV background at z ≲6 are also potentially consistent with the data. Overall, our results suggest that signatures of reionization in the form of islands of neutral hydrogen and/or large-scale fluctuations in the ionizing background remain present in the IGM until at least z ≃ 5.3.

Original languageEnglish (US)
Article number223
JournalAstrophysical Journal
Volume923
Issue number2
DOIs
StatePublished - Dec 20 2021
Externally publishedYes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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