Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30229
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Tang, J.-J. | en_US |
dc.contributor.author | Goto, T. | en_US |
dc.contributor.author | Ohyama, Y. | en_US |
dc.contributor.author | Chen, W.-P. | en_US |
dc.contributor.author | Walter, F. | en_US |
dc.contributor.author | Venemans, B. | en_US |
dc.contributor.author | Chambers, K.C. | en_US |
dc.contributor.author | Banados, E. | en_US |
dc.contributor.author | DECARLI, ROBERTO | en_US |
dc.contributor.author | Fan, X. | en_US |
dc.contributor.author | Farina, E.P. | en_US |
dc.contributor.author | Mazzucchelli, C. | en_US |
dc.contributor.author | Kaiser, N. | en_US |
dc.contributor.author | Magnier, E.A. | en_US |
dc.date.accessioned | 2021-02-08T11:42:40Z | - |
dc.date.available | 2021-02-08T11:42:40Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30229 | - |
dc.description.abstract | Luminous high-redshift quasars can be used to probe of the intergalactic medium in the early universe because their UV light is absorbed by the neutral hydrogen along the line of sight. They help us to measure the neutral hydrogen fraction of the high-z universe, shedding light on the end of reionization epoch. In this paper, we present a discovery of a new quasar (PSO J006.1240+39.2219) at redshift z = 6.61 ± 0.02 from Panoramic Survey Telescope & Rapid Response System 1. Including this quasar, there are nine quasars above z > 6.5 up to date. The estimated continuum brightness is M1450 = -25.96 ± 0.08. PSO J006.1240+39.2219 has a strong Ly α emission compared with typical low-redshift quasars, but the measured near-zone region size is RNZ = 3.2 ± 1.1 proper megaparsecs, which is consistent with other quasars at z ∼ 6. | en_US |
dc.language.iso | eng | en_US |
dc.title | A quasar discovered at redshift 6.6 from Pan-STARRS1 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw3287 | en_US |
dc.identifier.scopus | 2-s2.0-85025462139 | en_US |
dc.identifier.isi | 000402849400058 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/466/4/4568/2712523 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017MNRAS.466.4568T | 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 | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Tang17_stw3287.pdf | Pdf editoriale | 621.46 kB | Adobe PDF | View/Open |
Page view(s)
58
checked on Apr 23, 2024
Download(s)
38
checked on Apr 23, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.