Rapid evolution and transformation into quiescence?: ALMA view on z > 6 low-luminosity quasars

Takuma Izumi; Masafusa Onoue; Yoshiki Matsuoka; Tohru Nagao; Michael A. Strauss; Masatoshi Imanishi; Nobunari Kashikawa; Seiji Fujimoto; Kotaro Kohno; Yoshiki Toba; Hideki Umehata; Tomotsugu Goto; Yoshihiro Ueda; Hikari Shirakata; John D. Silverman; Jenny E. Greene; Yuichi Harikane; Yasuhiro Hashimoto; Soh Ikarashi; Daisuke Iono; Kazushi Iwasawa; Chien Hsiu Lee; Takeo Minezaki; Kouichiro Nakanishi; Yoichi Tamura; Ji Jia Tang; Akio Taniguchi

doi:10.1017/S1743921319009487

Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars

Takuma Izumi
, Masafusa Onoue
, Yoshiki Matsuoka
, Tohru Nagao
, Michael A. Strauss
, Masatoshi Imanishi
, Nobunari Kashikawa
, Seiji Fujimoto
, Kotaro Kohno
, Yoshiki Toba
, Hideki Umehata
, Tomotsugu Goto
, Yoshihiro Ueda
, Hikari Shirakata
, John D. Silverman
, Jenny E. Greene
, Yuichi Harikane
, Yasuhiro Hashimoto
, Soh Ikarashi
, Daisuke Iono

Kazushi Iwasawa, Chien Hsiu Lee, Takeo Minezaki, Kouichiro Nakanishi, Yoichi Tamura, Ji Jia Tang, Akio Taniguchi

地球科學系(含海洋環境研究所)

研究成果: 書貢獻/報告類型 › 會議論文篇章

摘要

We present ALMA [CII] line and far-infrared (FIR) continuum observations of seven z > 6 low-luminosity quasars (M1450 > −25 mag) discovered by our on-going Subaru Hyper Suprime-Cam survey. The [CII] line was detected in all targets with luminosities of ∼ (2 − 10) × 10⁸ L, about one order of magnitude smaller than optically luminous quasars. Also found was a wide scatter of FIR continuum luminosity, ranging from LFIR < 10¹¹ L to ∼ 2 × 10¹² L. With the [CII]-based dynamical mass, we suggest that a significant fraction of low-luminosity quasars are located on or even below the local Magorrian relation, particularly at the massive end of the galaxy mass distribution. This is a clear contrast to the previous finding that luminous quasars tend to have overmassive black holes relative to the relation. Our result is expected to show a less-biased nature of the early co-evolution of black holes and their host galaxies.

原文	英語
主出版物標題	Proceedings of the International Astronomical Union
編輯	Elisabete da Cunha, Elisabete da Cunha, Jacqueline Hodge, Jose Afonso, Laura Pentericci, David Sobral
發行者	Cambridge University Press
頁面	139-143
頁數	5
版本	352
ISBN（電子）	9781108492133
DOIs	https://doi.org/10.1017/S1743921319009487
出版狀態	已發佈 - 2020
事件	352nd Symposium of the International Astronomical Union on Uncovering Early Galaxy Evolution in the ALMA and JWST Era - Viana do Castelo, 葡萄牙持續時間: 2019 6月 3 → 2019 6月 7

出版系列

名字	Proceedings of the International Astronomical Union
號碼	352
卷	15
ISSN（列印）	1743-9213
ISSN（電子）	1743-9221

會議

會議	352nd Symposium of the International Astronomical Union on Uncovering Early Galaxy Evolution in the ALMA and JWST Era
國家/地區	葡萄牙
城市	Viana do Castelo
期間	2019/06/03 → 2019/06/07

ASJC Scopus subject areas

天文和天體物理學
空間與行星科學

存取文件

10.1017/S1743921319009487

其它文件與鏈接

引用此

Izumi, T., Onoue, M., Matsuoka, Y., Nagao, T., Strauss, M. A., Imanishi, M., Kashikawa, N., Fujimoto, S., Kohno, K., Toba, Y., Umehata, H., Goto, T., Ueda, Y., Shirakata, H., Silverman, J. D., Greene, J. E., Harikane, Y., Hashimoto, Y., Ikarashi, S., ... Taniguchi, A. (2020). Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars. 於 E. da Cunha, E. da Cunha, J. Hodge, J. Afonso, L. Pentericci, & D. Sobral (編輯), Proceedings of the International Astronomical Union (352 編輯, 頁 139-143). (Proceedings of the International Astronomical Union; 卷 15, 編號 352). Cambridge University Press. https://doi.org/10.1017/S1743921319009487

Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars. / Izumi, Takuma; Onoue, Masafusa; Matsuoka, Yoshiki 等.
Proceedings of the International Astronomical Union. 編輯 / Elisabete da Cunha; Elisabete da Cunha; Jacqueline Hodge; Jose Afonso; Laura Pentericci; David Sobral. 352. 編輯 Cambridge University Press, 2020. p. 139-143 (Proceedings of the International Astronomical Union; 卷 15, 編號 352).

研究成果: 書貢獻/報告類型 › 會議論文篇章

Izumi, T, Onoue, M, Matsuoka, Y, Nagao, T, Strauss, MA, Imanishi, M, Kashikawa, N, Fujimoto, S, Kohno, K, Toba, Y, Umehata, H, Goto, T, Ueda, Y, Shirakata, H, Silverman, JD, Greene, JE, Harikane, Y, Hashimoto, Y, Ikarashi, S, Iono, D, Iwasawa, K, Lee, CH, Minezaki, T, Nakanishi, K, Tamura, Y, Tang, JJ & Taniguchi, A 2020, Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars. 於 E da Cunha, E da Cunha, J Hodge, J Afonso, L Pentericci & D Sobral (編輯), Proceedings of the International Astronomical Union. 352 edn, Proceedings of the International Astronomical Union, 編號 352, 卷 15, Cambridge University Press, 頁 139-143, 352nd Symposium of the International Astronomical Union on Uncovering Early Galaxy Evolution in the ALMA and JWST Era, Viana do Castelo, 葡萄牙, 2019/06/03. https://doi.org/10.1017/S1743921319009487

Izumi T, Onoue M, Matsuoka Y, Nagao T, Strauss MA, Imanishi M 等. Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars. 於 da Cunha E, da Cunha E, Hodge J, Afonso J, Pentericci L, Sobral D, 編輯, Proceedings of the International Astronomical Union. 352 編輯 Cambridge University Press. 2020. p. 139-143. (Proceedings of the International Astronomical Union; 352). doi: 10.1017/S1743921319009487

Izumi, Takuma ; Onoue, Masafusa ; Matsuoka, Yoshiki 等. / Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars. Proceedings of the International Astronomical Union. 編輯 / Elisabete da Cunha ; Elisabete da Cunha ; Jacqueline Hodge ; Jose Afonso ; Laura Pentericci ; David Sobral. 352. 編輯 Cambridge University Press, 2020. 頁 139-143 (Proceedings of the International Astronomical Union; 352).

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title = "Rapid evolution and transformation into quiescence?: ALMA view on z > 6 low-luminosity quasars",

abstract = "We present ALMA [CII] line and far-infrared (FIR) continuum observations of seven z > 6 low-luminosity quasars (M1450 > −25 mag) discovered by our on-going Subaru Hyper Suprime-Cam survey. The [CII] line was detected in all targets with luminosities of ∼ (2 − 10) × 108 L, about one order of magnitude smaller than optically luminous quasars. Also found was a wide scatter of FIR continuum luminosity, ranging from LFIR < 1011 L to ∼ 2 × 1012 L. With the [CII]-based dynamical mass, we suggest that a significant fraction of low-luminosity quasars are located on or even below the local Magorrian relation, particularly at the massive end of the galaxy mass distribution. This is a clear contrast to the previous finding that luminous quasars tend to have overmassive black holes relative to the relation. Our result is expected to show a less-biased nature of the early co-evolution of black holes and their host galaxies.",

keywords = "galaxies: evolution, galaxies: high-redshift, quasars: general",

author = "Takuma Izumi and Masafusa Onoue and Yoshiki Matsuoka and Tohru Nagao and Strauss, \{Michael A.\} and Masatoshi Imanishi and Nobunari Kashikawa and Seiji Fujimoto and Kotaro Kohno and Yoshiki Toba and Hideki Umehata and Tomotsugu Goto and Yoshihiro Ueda and Hikari Shirakata and Silverman, \{John D.\} and Greene, \{Jenny E.\} and Yuichi Harikane and Yasuhiro Hashimoto and Soh Ikarashi and Daisuke Iono and Kazushi Iwasawa and Lee, \{Chien Hsiu\} and Takeo Minezaki and Kouichiro Nakanishi and Yoichi Tamura and Tang, \{Ji Jia\} and Akio Taniguchi",

note = "Publisher Copyright: {\textcopyright} International Astronomical Union 2020.; 352nd Symposium of the International Astronomical Union on Uncovering Early Galaxy Evolution in the ALMA and JWST Era ; Conference date: 03-06-2019 Through 07-06-2019",

year = "2020",

doi = "10.1017/S1743921319009487",

language = "English",

series = "Proceedings of the International Astronomical Union",

publisher = "Cambridge University Press",

number = "352",

pages = "139--143",

editor = "\{da Cunha\}, Elisabete and \{da Cunha\}, Elisabete and Jacqueline Hodge and Jose Afonso and Laura Pentericci and David Sobral",

booktitle = "Proceedings of the International Astronomical Union",

address = "United Kingdom",

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T1 - Rapid evolution and transformation into quiescence?

T2 - 352nd Symposium of the International Astronomical Union on Uncovering Early Galaxy Evolution in the ALMA and JWST Era

AU - Izumi, Takuma

AU - Onoue, Masafusa

AU - Matsuoka, Yoshiki

AU - Nagao, Tohru

AU - Strauss, Michael A.

AU - Imanishi, Masatoshi

AU - Kashikawa, Nobunari

AU - Fujimoto, Seiji

AU - Kohno, Kotaro

AU - Toba, Yoshiki

AU - Umehata, Hideki

AU - Goto, Tomotsugu

AU - Ueda, Yoshihiro

AU - Shirakata, Hikari

AU - Silverman, John D.

AU - Greene, Jenny E.

AU - Harikane, Yuichi

AU - Hashimoto, Yasuhiro

AU - Ikarashi, Soh

AU - Iono, Daisuke

AU - Iwasawa, Kazushi

AU - Lee, Chien Hsiu

AU - Minezaki, Takeo

AU - Nakanishi, Kouichiro

AU - Tamura, Yoichi

AU - Tang, Ji Jia

AU - Taniguchi, Akio

PY - 2020

Y1 - 2020

N2 - We present ALMA [CII] line and far-infrared (FIR) continuum observations of seven z > 6 low-luminosity quasars (M1450 > −25 mag) discovered by our on-going Subaru Hyper Suprime-Cam survey. The [CII] line was detected in all targets with luminosities of ∼ (2 − 10) × 108 L, about one order of magnitude smaller than optically luminous quasars. Also found was a wide scatter of FIR continuum luminosity, ranging from LFIR < 1011 L to ∼ 2 × 1012 L. With the [CII]-based dynamical mass, we suggest that a significant fraction of low-luminosity quasars are located on or even below the local Magorrian relation, particularly at the massive end of the galaxy mass distribution. This is a clear contrast to the previous finding that luminous quasars tend to have overmassive black holes relative to the relation. Our result is expected to show a less-biased nature of the early co-evolution of black holes and their host galaxies.

AB - We present ALMA [CII] line and far-infrared (FIR) continuum observations of seven z > 6 low-luminosity quasars (M1450 > −25 mag) discovered by our on-going Subaru Hyper Suprime-Cam survey. The [CII] line was detected in all targets with luminosities of ∼ (2 − 10) × 108 L, about one order of magnitude smaller than optically luminous quasars. Also found was a wide scatter of FIR continuum luminosity, ranging from LFIR < 1011 L to ∼ 2 × 1012 L. With the [CII]-based dynamical mass, we suggest that a significant fraction of low-luminosity quasars are located on or even below the local Magorrian relation, particularly at the massive end of the galaxy mass distribution. This is a clear contrast to the previous finding that luminous quasars tend to have overmassive black holes relative to the relation. Our result is expected to show a less-biased nature of the early co-evolution of black holes and their host galaxies.

KW - galaxies: evolution

KW - galaxies: high-redshift

KW - quasars: general

UR - https://www.scopus.com/pages/publications/85091311798

UR - https://www.scopus.com/pages/publications/85091311798#tab=citedBy

U2 - 10.1017/S1743921319009487

DO - 10.1017/S1743921319009487

M3 - Conference contribution

AN - SCOPUS:85091311798

T3 - Proceedings of the International Astronomical Union

SP - 139

EP - 143

BT - Proceedings of the International Astronomical Union

A2 - da Cunha, Elisabete

A2 - Hodge, Jacqueline

A2 - Afonso, Jose

A2 - Pentericci, Laura

A2 - Sobral, David

PB - Cambridge University Press

Y2 - 3 June 2019 through 7 June 2019

ER -

Rapid evolution and transformation into quiescence? ALMA view on z > 6 low-luminosity quasars

摘要

出版系列

會議

ASJC Scopus subject areas

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