Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31267
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Wang, Feige | en_US |
dc.contributor.author | Davies, Frederick B. | en_US |
dc.contributor.author | Yang, Jinyi | en_US |
dc.contributor.author | Hennawi, Joseph F. | en_US |
dc.contributor.author | Fan, Xiaohui | en_US |
dc.contributor.author | Barth, Aaron J. | en_US |
dc.contributor.author | Jiang, Linhua | en_US |
dc.contributor.author | Wu, Xue-Bing | en_US |
dc.contributor.author | Mudd, Dale M. | en_US |
dc.contributor.author | Bañados, Eduardo | en_US |
dc.contributor.author | Bian, Fuyan | en_US |
dc.contributor.author | DECARLI, ROBERTO | en_US |
dc.contributor.author | Eilers, Anna-Christina | en_US |
dc.contributor.author | Farina, Emanuele Paolo | en_US |
dc.contributor.author | Venemans, Bram | en_US |
dc.contributor.author | Walter, Fabian | en_US |
dc.contributor.author | Yue, Minghao | en_US |
dc.date.accessioned | 2021-12-28T10:49:12Z | - |
dc.date.available | 2021-12-28T10:49:12Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31267 | - |
dc.description.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 λ<SUB>Edd</SUB> = 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. | en_US |
dc.language.iso | eng | en_US |
dc.title | A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Quasar J0252-0503 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/ab8c45 | en_US |
dc.identifier.scopus | 2-s2.0-85090245387 | en_US |
dc.identifier.isi | WOS:000541828400001 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/ab8c45 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85090245387 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 896 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 23 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2020ApJ...896...23W | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-2662-8803 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
2004.10877.pdf | preprint | 1.94 MB | Adobe PDF | View/Open |
Wang_2020_ApJ_896_23.pdf | [Administrators only] | 2.49 MB | Adobe PDF |
Page view(s)
37
checked on Apr 19, 2024
Download(s)
18
checked on Apr 19, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.