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Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. I. The Hβ Broad-line Region Structure and Black Hole Masses of Five Quasars
Li, Yan-Rong1; Hu, Chen1; Yao, Zhu-Heng1,2; Chen, Yong-Jie1,3; Bai, Hua-Rui1,2; Yang, Sen1,2; Du, Pu1; Fang, Feng-Na1,2; Fu, Yi-Xin1,2; Liu, Jun-Rong1,2; Peng, Yue-Chang1,2; Songsheng, Yu-Yang1,3; Wang, Yi-Lin1,2; Xiao, Ming1; Zhai, Shuo1,2; Winkler, Hartmut4; Bai JM(白金明)5; Ho, Luis C.6,7; Petrov, Romain G.8; Aceituno, Jesús9,10; Wang, Jian-Min1,11,12
发表期刊ASTROPHYSICAL JOURNAL
2024-10-01
卷号974期号:1
DOI10.3847/1538-4357/ad6906
产权排序第5完成单位
收录类别SCI
摘要We conduct a reverberation mapping (RM) campaign to spectroscopically monitor a sample of selected bright active galactic nuclei with large anticipated broad-line region (BLR) sizes adequate for spectroastrometric (SA) observations by the GRAVITY instrument on the Very Large Telescope Interferometer. We report the first results for five objects, IC 4329A, Mrk 335, Mrk 509, Mrk 1239, and PDS 456, among which Mrk 1239 and PDS 456 are for the first time spectroscopically monitored. We obtain multiyear monitoring data and perform multicomponent spectral decomposition to extract the broad H beta profiles. We detect significant time lags between the H beta and continuum variations, generally obeying the previously established BLR size-luminosity relation. Velocity-resolved H beta time lags illustrate diverse, possibly evolving, BLR kinematics. We further measure the H beta line widths from mean and rms spectra and the resulting virial products show good consistency among different observing seasons. Adopting a unity virial factor and the FWHM of the broad H beta line from the mean spectra as a measure of velocity, the obtained black hole masses averaged over seasons are log M-center dot/M-circle dot = 8.02(-0.14)(+0.09) ,6.92(-0.12)(+0.12), 8.01(-0.25)(+0.16), 7.44(-0.14)(+0.13), and 8.59(-0.11)(+0.07) for the five objects, respectively. Black hole mass estimations using other line width measures are also reported. For objects with previous RM campaigns, our mass estimates are in agreement with earlier results. In a companion paper, we will employ BLR dynamical modeling to directly infer the black hole mass and thereby determine the virial factors.
资助项目National Key R&D Program of China[11721303]; National Key R&D Program of China[11991052]; National Key R&D Program of China[12011540375]; National Key R&D Program of China[12233001]; National Key R&D Program of China[2022YFF0503401]; National Natural Science Foundation of China (NSFC)[2021YFA1600404]; National Natural Science Foundation of China (NSFC)[2023YFA1607904]; NSFC[11721303]; NSFC[11991052]; NSFC[12011540375]; NSFC[12233001]; NSFC[11833008]; NSFC[11991050]; NSFC[12333003]; NSFC[12273041]; NSFC[NSFC-12122305]; NSFC[NSFC-12022301]; NSFC[11991051]; Youth Innovation Promotion Association CAS; China Manned Space Project[CMS-CSST-2021-A04]; China Manned Space Project[CMS-CSST-2021-A06]; National Science Foundation[12273041]; National Science Foundation[NSFC-12122305]; National Science Foundation[AST-1440341]; National Science Foundation[AST-2034437]
项目资助者National Key R&D Program of China[11721303, 11991052, 12011540375, 12233001, 2022YFF0503401] ; National Natural Science Foundation of China (NSFC)[2021YFA1600404, 2023YFA1607904] ; NSFC[11721303, 11991052, 12011540375, 12233001, 11833008, 11991050, 12333003, 12273041, NSFC-12122305, NSFC-12022301, 11991051] ; Youth Innovation Promotion Association CAS ; China Manned Space Project[CMS-CSST-2021-A04, CMS-CSST-2021-A06] ; National Science Foundation[12273041, NSFC-12122305, AST-1440341, AST-2034437]
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001330603300001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]HIGH ACCRETION RATES ; SEYFERT-GALAXIES ; DYNAMICAL MODELS ; 1ST LIGHT ; X-RAY ; EMISSION ; SPECTRA ; II. ; VARIABILITY ; DISK
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27635
专题南方基地
作者单位1.Key Laboratory for Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, People's Republic of China; [email protected];
2.School of Physics, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
3.Dongguan Neutron Science Center, 1 Zhongziyuan Road, Dongguan 523808, People's Republic of China;
4.Department of Physics, University of Johannesburg, P.O. Box 524, 2006 Auckland Park, Johannesburg, South Africa;
5.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People's Republic of China;
6.The Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China;
7.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People's Republic of China;
8.Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange UMR 7293, Bâtiment H. Fizeau, F-06108 Nice Cedex 2, France;
9.Centro Astronomico Hispano Alemán, Sierra de los filabres sn, 04550 gergal, Almería, Spain;
10.Instituto de Astrofísica de Andalucía, Glorieta de la astronomía sn, 18008 Granada, Spain;
11.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China; [email protected];
12.National Astronomical Observatories of China, Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, People's Republic of China
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Li, Yan-Rong,Hu, Chen,Yao, Zhu-Heng,et al. Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. I. The Hβ Broad-line Region Structure and Black Hole Masses of Five Quasars[J]. ASTROPHYSICAL JOURNAL,2024,974(1).
APA Li, Yan-Rong.,Hu, Chen.,Yao, Zhu-Heng.,Chen, Yong-Jie.,Bai, Hua-Rui.,...&Wang, Jian-Min.(2024).Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. I. The Hβ Broad-line Region Structure and Black Hole Masses of Five Quasars.ASTROPHYSICAL JOURNAL,974(1).
MLA Li, Yan-Rong,et al."Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. I. The Hβ Broad-line Region Structure and Black Hole Masses of Five Quasars".ASTROPHYSICAL JOURNAL 974.1(2024).
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