中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Monitoring AGNs with H beta Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars

文献类型:期刊论文

AuthorBao, Dong-Wei21,22; Brotherton, Michael S.20; Du, Pu22; McLane, Jacob N.20; Zastrocky, T. E.19,20; Olson, Kianna A.20; Fang, Feng-Na21,22; Zhai, Shuo21,22; Huang, Zheng-Peng22; Wang, Kai22
SourceASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Issued Date2022-09-01
Volume262Issue:1
ISSN0067-0049
DOI10.3847/1538-4365/ac7beb
Rank第6完成单位
SubtypeArticle
English Abstract

In this third paper of the series reporting on the reverberation mapping campaign of active galactic nuclei with asymmetric H beta emission-line profiles, we present results for 15 Palomar-Green quasars using spectra obtained between the end of 2016-2021 May. This campaign combines long time spans with relatively high cadence. For eight objects, both the time lags obtained from the entire light curves and the measurements from individual observing seasons are provided. Reverberation mapping of nine of our targets has been attempted for the first time, while the results for six others can be compared with previous campaigns. We measure the H beta time lags over periods of years and estimate their black hole masses. The long duration of the campaign enables us to investigate their broad-line region (BLR) geometry and kinematics for different years by using velocity-resolved lags, which demonstrate signatures of diverse BLR geometry and kinematics. The BLR geometry and kinematics of individual objects are discussed. In this sample, the BLR kinematics of Keplerian/virialized motion and inflow is more common than that of outflow.

Subject天文学 ; 星系与宇宙学
URL查看原文
Publish PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
Funding ProjectCAS ; Peoples Government of Yunnan Province ; National Science Foundation of China[NSFC-12022301] ; National Science Foundation of China[NSFC-11991051] ; National Science Foundation of China[NSFC-11991054] ; National Science Foundation of China[NSFC-11873048] ; National Science Foundation of China[NSFC-11833008] ; National Key R&D Program of China[2016YFA0400701] ; National Key R&D Program of China[11721303] ; National Key R&D Program of China[11991052] ; National Key R&D Program of China[2016YFA0400702] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH007] ; Strategic Priority Research Program of CAS[XDB23010400] ; International Partnership Program of CAS[113111KYSB20200014] ; Chinese Academy of Sciences Presidents International Fellowship Initiative[2018VMA0005] ; National Natural Science Foundation of China[NSFC-11922304] ; Youth Innovation Promotion Association CAS ; University of Wyoming Science Initiative Faculty Innovation Seed grant ; National Science Foundation under REU grant[AST 1852289] ; NSF grant[1005444I] ; National Science Foundation[AST-1440341] ; Caltech ; IPAC ; Weizmann Institute for Science ; Oskar Klein Center at Stockholm University ; University of Maryland ; University of Washington ; Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories ; TANGO Consortium of Taiwan ; University of Wisconsin at Milwaukee ; Lawrence Berkeley National Laboratories ; Gordon and Betty Moore Foundation[GBMF5490] ; NSF grants[AST-1515927] ; NSF grants[AST-1908570] ; NSF grants[AST-0908816] ; Mt. Cuba Astronomical Foundation ; Center for Cosmology and AstroParticle Physics at the Ohio State University ; Chinese Academy of Sciences South America Center for Astronomy (CAS- SACA) ; Villum Foundation ; George Skestos ; [NSFC-12122305]
WOS KeywordBROAD-LINE REGION ; ACTIVE GALACTIC NUCLEI ; SUPERMASSIVE BLACK-HOLES ; HIGH ACCRETION RATES ; VELOCITY-DELAY MAPS ; EMISSION-LINES ; SPECTRAL VARIABILITY ; SEYFERT-GALAXIES ; COMPLETE SAMPLE ; PROJECT
WOS Research AreaAstronomy & Astrophysics
Language英语
PublisherIOP Publishing Ltd
WOS IDWOS:000842723400001
Funding OrganizationCAS ; Peoples Government of Yunnan Province ; National Science Foundation of China[NSFC-12022301, NSFC-11991051, NSFC-11991054, NSFC-11873048, NSFC-11833008] ; National Key R&D Program of China[2016YFA0400701, 11721303, 11991052, 2016YFA0400702] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH007] ; Strategic Priority Research Program of CAS[XDB23010400] ; International Partnership Program of CAS[113111KYSB20200014] ; Chinese Academy of Sciences Presidents International Fellowship Initiative[2018VMA0005] ; National Natural Science Foundation of China[NSFC-11922304] ; Youth Innovation Promotion Association CAS ; University of Wyoming Science Initiative Faculty Innovation Seed grant ; National Science Foundation under REU grant[AST 1852289] ; NSF grant[1005444I] ; National Science Foundation[AST-1440341] ; Caltech ; IPAC ; Weizmann Institute for Science ; Oskar Klein Center at Stockholm University ; University of Maryland ; University of Washington ; Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories ; TANGO Consortium of Taiwan ; University of Wisconsin at Milwaukee ; Lawrence Berkeley National Laboratories ; Gordon and Betty Moore Foundation[GBMF5490] ; NSF grants[AST-1515927, AST-1908570, AST-0908816] ; Mt. Cuba Astronomical Foundation ; Center for Cosmology and AstroParticle Physics at the Ohio State University ; Chinese Academy of Sciences South America Center for Astronomy (CAS- SACA) ; Villum Foundation ; George Skestos ; [NSFC-12122305]
Version出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/25544]  
Collection云南天文台_丽江天文观测站(南方基地)
Corresponding AuthorBao, Dong-Wei
Affiliation1.National Astronomical Observatories of China, Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, People's Republic of China
2.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People's Republic of China;
3.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China;
4.Instituto de Astrofísica de Andalucía (CSIC), Glorieta de la astronomía sn, E-18008 Granada, Spain;
5.Centro Astronomico Hispano Alemán, Sierra de los filabres sn, E-04550 Gergal, Almería, Spain;
6.Center for Theoretical Physics, Polish Academy of Sciences, Al. Lotnikow 32/46, 02-668 Warsaw, Poland;
7.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China;
8.Dipartimento di Fisica & Astronomia
9.Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Padova, I-35122 Padova, Italy;
10.Department of Physics, University of Johannesburg, P.O. Box 524, 2006 Auckland Park, South Africa;
Recommended Citation
GB/T 7714
Bao, Dong-Wei,Brotherton, Michael S.,Du, Pu,et al. Monitoring AGNs with H beta Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2022,262(1).
APA Bao, Dong-Wei.,Brotherton, Michael S..,Du, Pu.,McLane, Jacob N..,Zastrocky, T. E..,...&Wang, Jian-Min.(2022).Monitoring AGNs with H beta Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,262(1).
MLA Bao, Dong-Wei,et al."Monitoring AGNs with H beta Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 262.1(2022).

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来源:云南天文台

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