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  5. A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Quasar J0252-0503
 

A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Quasar J0252-0503

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2020
Author(s)
Wang, Feige
•
Davies, Frederick B.
•
Yang, Jinyi
•
Hennawi, Joseph F.
•
Fan, Xiaohui
•
Barth, Aaron J.
•
Jiang, Linhua
•
Wu, Xue-Bing
•
Mudd, Dale M.
•
Bañados, Eduardo
•
Bian, Fuyan
•
DECARLI, ROBERTO  
•
Eilers, Anna-Christina
•
Farina, Emanuele Paolo
•
Venemans, Bram
•
Walter, Fabian
•
Yue, Minghao
DOI
10.3847/1538-4357/ab8c45
Abstract
Luminous z ≥ 7 quasars provide direct probes of the evolution of supermassive black holes (SMBHs) and the intergalactic medium (IGM) during the epoch of reionization (EoR). The Lyα damping wing absorption imprinted by neutral hydrogen in the IGM can be detected in a single EoR quasar spectrum, allowing the measurement of the IGM neutral fraction toward that line of sight. However, damping wing features have only been detected in two z > 7 quasars in previous studies. In this paper, we present new high-quality optical and near-infrared spectroscopy of the z = 7.00 quasar DES J025216.64-050331.8 obtained with Keck/Near-Infrared Echellette Spectrometer and Gemini/GMOS. By using the Mg II single-epoch virial method, we find that it hosts a $(1.39\pm 0.16)\times {10}^{9}\,{M}_{\odot }$ SMBH accreting at an Eddington ratio of λEdd = 0.7 ± 0.1, consistent with the values seen in other luminous z ∼ 7 quasars. Furthermore, the Lyα region of the spectrum exhibits a strong damping wing absorption feature. The lack of associated metal absorption in the quasar spectrum indicates that this absorption is imprinted by a neutral IGM. Using a state-of-the-art model developed by Davies et al., we measure a volume-averaged neutral hydrogen fraction at z = 7 of $\langle {X}_{{\rm{H}}{\rm{I}}}\rangle ={0.70}_{-0.23}^{+0.20}{(}_{-0.48}^{+0.28})$ within 68% (95%) confidence intervals when marginalizing over quasar lifetimes of ${10}^{3}\leqslant {t}_{{\rm{Q}}}\leqslant {10}^{8}\,\mathrm{yr}$ . This is the highest IGM neutral fraction yet measured using reionization-era quasar spectra.
Volume
896
Issue
1
Start page
23
Uri
http://hdl.handle.net/20.500.12386/31267
Url
https://iopscience.iop.org/article/10.3847/1538-4357/ab8c45
https://api.elsevier.com/content/abstract/scopus_id/85090245387
Issn Identifier
0004-637X
Ads BibCode
2020ApJ...896...23W
Rights
open.access
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