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Correlation Analysis between OJ 287 Radio Jet Observables
Yuan, Q.1,2; Zhang, M.1,3,4; Liu, X.1,3,4; Jiang, P. F.1,2; Kokhirova, G. I.5
2023-05-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume949Issue:1Pages:20
Contribution Rank1
AbstractWe collected the archival data of blazar OJ 287 from heterogeneous very long baseline interferometry monitoring programs at 2.3, 8.6, 15, and 43 GHz. The data reduction and observable extraction of those multiband, multiepoch observations are batch-processed consistently with our automated pipeline. We present the multivariate correlation analysis on the observables at each band. We employ the cross-correlation function to search the correlations and the Monte Carlo technique to verify the certainty of correlations. Several correlations are found. The foremost findings are the correlations between the core flux density and the jet position angles on different scales, which validated the plausible predictions of the jet with precession characteristics. Meanwhile, there is a variation in the offset between the core electric vector position angle and the inner-jet position angle over time at 15 and 43 GHz.
DOI10.3847/1538-4357/acc5ec
Indexed BySCI
Language英语
WOS KeywordACTIVE GALACTIC NUCLEI ; LINEAR-POLARIZATION PROPERTIES ; INNER JET ; AGN JETS ; RELATIVISTIC JETS ; PRECESSING JET ; VLBA ; RAY ; KINEMATICS ; BLAZARS
Funding ProjectNational Key R&D Intergovernmental Cooperation Program of China[2022YFE0133700] ; Regional Collaborative Innovation Project of Xinjiang Uyghur Autonomous Region[2022E01013] ; National Natural Science Foundation of China[12173078] ; National Natural Science Foundation of China[11773062] ; Light of West China Program of the Chinese Academy of Sciences[2017-XBQNXZ-A-008] ; NASA through the Fermi Guest Investigator Program
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000993098500001
PublisherIOP Publishing Ltd
Funding OrganizationNational Key R&D Intergovernmental Cooperation Program of China ; Regional Collaborative Innovation Project of Xinjiang Uyghur Autonomous Region ; National Natural Science Foundation of China ; Light of West China Program of the Chinese Academy of Sciences ; NASA through the Fermi Guest Investigator Program
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Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5487
Collection射电天文研究室_星系宇宙学研究团组
射电天文研究室
Corresponding AuthorZhang, M.
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
2.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Peoples R China
4.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Peoples R China
5.Natl Acad Sci Tajikistan, Inst Astrophys, 22 Bukhoro St, Dushanbe 734042, Tajikistan
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Yuan, Q.,Zhang, M.,Liu, X.,et al. Correlation Analysis between OJ 287 Radio Jet Observables[J]. ASTROPHYSICAL JOURNAL,2023,949(1):20.
APA Yuan, Q.,Zhang, M.,Liu, X.,Jiang, P. F.,&Kokhirova, G. I..(2023).Correlation Analysis between OJ 287 Radio Jet Observables.ASTROPHYSICAL JOURNAL,949(1),20.
MLA Yuan, Q.,et al."Correlation Analysis between OJ 287 Radio Jet Observables".ASTROPHYSICAL JOURNAL 949.1(2023):20.
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