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SDSS J094635.06+101706.1: a redshift one, very radio-loud, gamma-ray emitting narrow-line Seyfert 1 galaxy
Yao, Su1,2; Komossa, S.3; Liu, Wen-Juan4,5; Yi, Weimin4,5,6; Yuan, Weimin7; Zhou, Hongyan8,9; Wu, Xue-Bing1,10
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2019-07-01
卷号487期号:1页码:L40-L45
关键词accretion, accretion discs galaxies: active galaxies: jets galaxies: nuclei galaxies: Seyfert
ISSN号0035-8711
DOI10.1093/mnrasl/slz071
英文摘要As hybrids of narrow-line Seyfert 1 (NLS1) galaxies and blazars, gamma-ray emitting NLS1s are important probes of jet physics in the high Eddington-ratio regime. Only very few of them are known to date; the majority of them below redshift z = 0.5. Here, we present the identification of the gamma-ray emitting AGN TXS 0943+105 (SDSS J094635.06+101706.1) as a high-redshift NLS1 galaxy. It turns out to be one of the radio-loudest NLS1s known, highly variable at all wavelengths, and shows widely extended radio emission at a (projected) >100 kpc scale. It is a known strong gamma-ray emitter with a luminous flare reported previously. At redshift z = 1.004, this is the most distant gamma-NLS1 known to date.
资助项目KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Chinese Academy of Sciences ; Natural Science Foundation of China (NSFC)[11703079] ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; NSFC[11703076] ; NSFC[11721303] ; NSFC[11533001] ; West Light Foundation of the Chinese Academy of Sciences[Y6XB016001] ; Ministry of Science and Technology of China[2016YFA0400703]
WOS关键词BLACK-HOLE MASSES ; ALL-SKY SURVEY ; EMISSION ; SPECTRUM ; QUASARS ; CATALOG ; VIEW ; JET
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000482695900008
资助机构KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Chinese Academy of Sciences ; KIAACAS Fellowship - Chinese Academy of Sciences ; Natural Science Foundation of China (NSFC) ; Natural Science Foundation of China (NSFC) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; NSFC ; NSFC ; West Light Foundation of the Chinese Academy of Sciences ; West Light Foundation of the Chinese Academy of Sciences ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Chinese Academy of Sciences ; KIAACAS Fellowship - Chinese Academy of Sciences ; Natural Science Foundation of China (NSFC) ; Natural Science Foundation of China (NSFC) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; NSFC ; NSFC ; West Light Foundation of the Chinese Academy of Sciences ; West Light Foundation of the Chinese Academy of Sciences ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Chinese Academy of Sciences ; KIAACAS Fellowship - Chinese Academy of Sciences ; Natural Science Foundation of China (NSFC) ; Natural Science Foundation of China (NSFC) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; NSFC ; NSFC ; West Light Foundation of the Chinese Academy of Sciences ; West Light Foundation of the Chinese Academy of Sciences ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Peking University ; KIAACAS Fellowship - Chinese Academy of Sciences ; KIAACAS Fellowship - Chinese Academy of Sciences ; Natural Science Foundation of China (NSFC) ; Natural Science Foundation of China (NSFC) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; "Light of West China" Programme of Chinese Academy of Sciences (CAS) ; NSFC ; NSFC ; West Light Foundation of the Chinese Academy of Sciences ; West Light Foundation of the Chinese Academy of Sciences ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/27653]  
专题中国科学院国家天文台
通讯作者Yao, Su
作者单位1.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
4.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Yunnan, Peoples R China
5.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Yunnan, Peoples R China
6.Penn State Univ, Dept Astron & Astrophys, 525 Davey Lab, University Pk, PA 16802 USA
7.Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, Beijing 100012, Peoples R China
8.USTC, CAS Key Lab Res Galaxies & Cosmol, Dept Astron, Hefei 230026, Anhui, Peoples R China
9.Polar Res Inst China, SOA Key Lab Polar Sci, 451 Jinqiao Rd, Shanghai 200136, Peoples R China
10.Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China
推荐引用方式
GB/T 7714
Yao, Su,Komossa, S.,Liu, Wen-Juan,et al. SDSS J094635.06+101706.1: a redshift one, very radio-loud, gamma-ray emitting narrow-line Seyfert 1 galaxy[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,487(1):L40-L45.
APA Yao, Su.,Komossa, S..,Liu, Wen-Juan.,Yi, Weimin.,Yuan, Weimin.,...&Wu, Xue-Bing.(2019).SDSS J094635.06+101706.1: a redshift one, very radio-loud, gamma-ray emitting narrow-line Seyfert 1 galaxy.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,487(1),L40-L45.
MLA Yao, Su,et al."SDSS J094635.06+101706.1: a redshift one, very radio-loud, gamma-ray emitting narrow-line Seyfert 1 galaxy".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 487.1(2019):L40-L45.
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