Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0

We present the spectroscopic discovery of 69 quasars at 5.8 < z < 7.0, drawn from the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) imaging survey data. This is the 16th publication from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, and it completes identi...

Descripción completa

Detalles Bibliográficos
Autores: Matsuoka, Yoshiki, Iwasawa, Kazushi, Onoue, Masafusa, Izumi, Takuma, Kashikawa, Nobunari, Strauss, Michael A., Imanishi, Masatoshi, Nagao, Tohru, Akiyama, Masayuki, Silverman, John D., Asami, Naoko, Bosch, Jaime, Furusawa, Hisanori, Goto, Tomotsugu, Gunn, James E., Harikane, Yuichi, Ikeda, Hiroyuki, Ishimoto, Rikako, Kawaguchi, Toshihiro, Kato, Nanako, Kikuta, Satoshi, Kohno, Kotaro, Komiyama, Yutaka, Lee, Chien-Hsiu, Lupton, Robert H., Minezaki, Takeo, Miyazaki, Satoshi, Murayama, Hitoshi, Nishizawa, Atsushi J., Oguri, Masamune, Ono, Yoshiaki, Ouchi, Masami, Price, Paul A., Sameshima, Hiroaki, Sugiyama, N., Tait, Philip J., Takada, Masahiro, Takahashi, Ayumi, Tanaka, Masayuki, Toba, Yoshiki, Utsumi, Yousuke, Wang, Shiang-Yu, Yamashita, Takuji
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2022
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:dnet:digitalcsic_::6886be027343c1f260bd10fc196870a3
Acceso en línea:http://hdl.handle.net/10261/277875
Access Level:acceso abierto
Palabra clave:Reionization
Quasars
Supermassive black holes
High-redshift galaxies
id ES_b527cd4e4e0c717a1d30c20143d4851c
oai_identifier_str oai:dnet:digitalcsic_::6886be027343c1f260bd10fc196870a3
network_acronym_str ES
network_name_str España
repository_id_str
spelling Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0Matsuoka, YoshikiIwasawa, KazushiOnoue, MasafusaIzumi, TakumaKashikawa, NobunariStrauss, Michael A.Imanishi, MasatoshiNagao, TohruAkiyama, MasayukiSilverman, John D.Asami, NaokoBosch, JaimeFurusawa, HisanoriGoto, TomotsuguGunn, James E.Harikane, YuichiIkeda, HiroyukiIshimoto, RikakoKawaguchi, ToshihiroKato, NanakoKikuta, SatoshiKohno, KotaroKomiyama, YutakaLee, Chien-HsiuLupton, Robert H.Minezaki, TakeoMiyazaki, SatoshiMurayama, HitoshiNishizawa, Atsushi J.Oguri, MasamuneOno, YoshiakiOuchi, MasamiPrice, Paul A.Sameshima, HiroakiSugiyama, N.Tait, Philip J.Takada, MasahiroTakahashi, AyumiTanaka, MasayukiToba, YoshikiUtsumi, YousukeWang, Shiang-YuYamashita, TakujiReionizationQuasarsSupermassive black holesHigh-redshift galaxiesWe present the spectroscopic discovery of 69 quasars at 5.8 < z < 7.0, drawn from the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) imaging survey data. This is the 16th publication from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, and it completes identification of all but the faintest candidates (i.e., i-band dropouts with z AB < 24 and y-band detections, and z-band dropouts with y AB < 24) with Bayesian quasar probability PQB>0.1 in the HSC-SSP third public data release (PDR3). The sample reported here also includes three quasars with PQB<0.1 at z ∼6.6, which we selected in an effort to completely cover the reddest point sources with simple color cuts. The number of high-z quasars discovered in SHELLQs has now grown to 162, including 23 type II quasar candidates. This paper also presents identification of seven galaxies at 5.6 < z < 6.7, an [O iii] emitter at z = 0.954, and 31 Galactic cool stars and brown dwarfs. High-z quasars and galaxies compose 75% and 16%, respectively, of all the spectroscopic SHELLQs objects that pass our latest selection algorithm with the PDR3 photometry. That is, a total of 91% of the objects lie at z > 5.6. This demonstrates that the algorithm has very high efficiency, even though we are probing an unprecedentedly low luminosity population down to M 1450 ∼-21 mag.Y.M. was supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI grant No. JP17H04830, No. 21H04494, and the Mitsubishi Foundation grant No. 30140. K.I. acknowledges support by the Spanish MCIN under grant PID2019-105510GB-C33/AEI/10.13039/501100011033 and "Unit of excellence María de Maeztu 2020-2023" awarded to ICCUB (CEX2019-000918-M).IOP PublishingJapan Society for the Promotion of ScienceMitsubishi International CorporationMinisterio de Ciencia e Innovación (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2022202220222022info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/277875reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105510GB-C33http://doi.org/10.3847/1538-4365/ac3d31Síinfo:eu-repo/semantics/openAccessoai:dnet:digitalcsic_::6886be027343c1f260bd10fc196870a32026-05-22T06:33:51Z
dc.title.none.fl_str_mv Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
title Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
spellingShingle Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
Matsuoka, Yoshiki
Reionization
Quasars
Supermassive black holes
High-redshift galaxies
title_short Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
title_full Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
title_fullStr Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
title_full_unstemmed Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
title_sort Subaru High- z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0
dc.creator.none.fl_str_mv Matsuoka, Yoshiki
Iwasawa, Kazushi
Onoue, Masafusa
Izumi, Takuma
Kashikawa, Nobunari
Strauss, Michael A.
Imanishi, Masatoshi
Nagao, Tohru
Akiyama, Masayuki
Silverman, John D.
Asami, Naoko
Bosch, Jaime
Furusawa, Hisanori
Goto, Tomotsugu
Gunn, James E.
Harikane, Yuichi
Ikeda, Hiroyuki
Ishimoto, Rikako
Kawaguchi, Toshihiro
Kato, Nanako
Kikuta, Satoshi
Kohno, Kotaro
Komiyama, Yutaka
Lee, Chien-Hsiu
Lupton, Robert H.
Minezaki, Takeo
Miyazaki, Satoshi
Murayama, Hitoshi
Nishizawa, Atsushi J.
Oguri, Masamune
Ono, Yoshiaki
Ouchi, Masami
Price, Paul A.
Sameshima, Hiroaki
Sugiyama, N.
Tait, Philip J.
Takada, Masahiro
Takahashi, Ayumi
Tanaka, Masayuki
Toba, Yoshiki
Utsumi, Yousuke
Wang, Shiang-Yu
Yamashita, Takuji
author Matsuoka, Yoshiki
author_facet Matsuoka, Yoshiki
Iwasawa, Kazushi
Onoue, Masafusa
Izumi, Takuma
Kashikawa, Nobunari
Strauss, Michael A.
Imanishi, Masatoshi
Nagao, Tohru
Akiyama, Masayuki
Silverman, John D.
Asami, Naoko
Bosch, Jaime
Furusawa, Hisanori
Goto, Tomotsugu
Gunn, James E.
Harikane, Yuichi
Ikeda, Hiroyuki
Ishimoto, Rikako
Kawaguchi, Toshihiro
Kato, Nanako
Kikuta, Satoshi
Kohno, Kotaro
Komiyama, Yutaka
Lee, Chien-Hsiu
Lupton, Robert H.
Minezaki, Takeo
Miyazaki, Satoshi
Murayama, Hitoshi
Nishizawa, Atsushi J.
Oguri, Masamune
Ono, Yoshiaki
Ouchi, Masami
Price, Paul A.
Sameshima, Hiroaki
Sugiyama, N.
Tait, Philip J.
Takada, Masahiro
Takahashi, Ayumi
Tanaka, Masayuki
Toba, Yoshiki
Utsumi, Yousuke
Wang, Shiang-Yu
Yamashita, Takuji
author_role author
author2 Iwasawa, Kazushi
Onoue, Masafusa
Izumi, Takuma
Kashikawa, Nobunari
Strauss, Michael A.
Imanishi, Masatoshi
Nagao, Tohru
Akiyama, Masayuki
Silverman, John D.
Asami, Naoko
Bosch, Jaime
Furusawa, Hisanori
Goto, Tomotsugu
Gunn, James E.
Harikane, Yuichi
Ikeda, Hiroyuki
Ishimoto, Rikako
Kawaguchi, Toshihiro
Kato, Nanako
Kikuta, Satoshi
Kohno, Kotaro
Komiyama, Yutaka
Lee, Chien-Hsiu
Lupton, Robert H.
Minezaki, Takeo
Miyazaki, Satoshi
Murayama, Hitoshi
Nishizawa, Atsushi J.
Oguri, Masamune
Ono, Yoshiaki
Ouchi, Masami
Price, Paul A.
Sameshima, Hiroaki
Sugiyama, N.
Tait, Philip J.
Takada, Masahiro
Takahashi, Ayumi
Tanaka, Masayuki
Toba, Yoshiki
Utsumi, Yousuke
Wang, Shiang-Yu
Yamashita, Takuji
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Japan Society for the Promotion of Science
Mitsubishi International Corporation
Ministerio de Ciencia e Innovación (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Reionization
Quasars
Supermassive black holes
High-redshift galaxies
topic Reionization
Quasars
Supermassive black holes
High-redshift galaxies
description We present the spectroscopic discovery of 69 quasars at 5.8 < z < 7.0, drawn from the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) imaging survey data. This is the 16th publication from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, and it completes identification of all but the faintest candidates (i.e., i-band dropouts with z AB < 24 and y-band detections, and z-band dropouts with y AB < 24) with Bayesian quasar probability PQB>0.1 in the HSC-SSP third public data release (PDR3). The sample reported here also includes three quasars with PQB<0.1 at z ∼6.6, which we selected in an effort to completely cover the reddest point sources with simple color cuts. The number of high-z quasars discovered in SHELLQs has now grown to 162, including 23 type II quasar candidates. This paper also presents identification of seven galaxies at 5.6 < z < 6.7, an [O iii] emitter at z = 0.954, and 31 Galactic cool stars and brown dwarfs. High-z quasars and galaxies compose 75% and 16%, respectively, of all the spectroscopic SHELLQs objects that pass our latest selection algorithm with the PDR3 photometry. That is, a total of 91% of the objects lie at z > 5.6. This demonstrates that the algorithm has very high efficiency, even though we are probing an unprecedentedly low luminosity population down to M 1450 ∼-21 mag.
publishDate 2022
dc.date.none.fl_str_mv 2022
2022
2022
2022
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/277875
url http://hdl.handle.net/10261/277875
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105510GB-C33
http://doi.org/10.3847/1538-4365/ac3d31

dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869417320015724544
score 15.81155