Are we witnessing the epoch of reionisation at z = 7.1 from the spectrum of J1120+0641?
Name
1606.00441.pdf
Description
Accepted version
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7.02 MB
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Author(s)
Greig, Bradley
Mesinger, Andrei
Haiman, Zoltán
Simcoe, Robert A
Date Issued
2016
Journal
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP)
Version
Author's final manuscript
Abstract
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society We quantify the presence of Lyα damping wing absorption from a partially neutral intergalactic medium (IGM) in the spectrum of the z = 7.08 QSO, ULASJ1120+0641. Using a Bayesian framework, we simultaneously account for uncertainties in: (i) the intrinsic QSO emission spectrum; and (ii) the distribution of cosmic H I patches during the epoch of reionization (EoR). For (i), we use a new intrinsic Lyα emission line reconstruction method, sampling a covariance matrix of emission line properties built from a large data base of moderate-z QSOs. For (ii), we use the Evolution of 21-cm Structure (EOS; Mesinger et al.) simulations, which span a range of physically motivated EoR models. We find strong evidence for the presence of damping wing absorption redward of Lyα (where there is no contamination from the Lyα forest). Our analysis implies that the EoR is not yet complete by z = 7.1, with the volume-weighted IGM neutral fraction constrained to x¯ HI = 0.40+−002119 at 1σ (x¯ HI = 0.40+−004132 at 2σ ). This result is insensitive to the EoR morphology. Our detection of significant neutral H I in the IGM at z = 7.1 is consistent with the latest Planck 2016 measurements of the CMB Thompson scattering optical depth.
MIT Department
MIT Kavli Institute for Astrophysics and Space Research
Massachusetts Institute of Technology. Department of Physics
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DOI of Published Version
https://doi.org/10.1093/MNRAS/STW3351
