中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Multiwavelength Temporal Variability of the Blazar PKS 1510-089

文献类型:期刊论文

作者Yuan, Q.13,14; Kushwaha, Pankaj11,12; Gupta, Alok C.10,11; Tripathi, Ashutosh8,9; Wiita, Paul J.7; Zhang, M.5,6,14; Liu, X.5,6,14; Lahteenmaki, Anne3,4; Tornikoski, Merja4; Tammi, Joni4
刊名ASTROPHYSICAL JOURNAL
出版日期2023-08-01
卷号953期号:1页码:15
ISSN号0004-637X
DOI10.3847/1538-4357/acdd74
通讯作者Yuan, Q.(yuanqi@xao.ac.cn)
英文摘要We perform correlation and periodicity search analyses on long-term multiband light curves of the flat-spectrum radio quasar PKS 1510-089 observed by the space-based Fermi-Large Area Telescope in & gamma;-rays, the SMARTS and Steward Observatory telescopes in optical and near-infrared (NIR), and the 13.7 m radio telescope in Metsahovi Radio Observatory between 2008 and 2018. The z-transform discrete correlation function method is applied to study the correlation and possible time lags among these multiband light curves. Among all pairs of wavelengths, the & gamma;-ray versus optical/NIR and optical versus NIR correlations show zero time lags; however, both the & gamma;-ray and optical/NIR emissions precede the radio radiation. The generalized Lomb-Scargle periodogram, weighted wavelet z-transform, and REDFIT techniques are employed to investigate the unresolved core emission-dominated 37 GHz light curve and yield evidence for a quasi period around 1540 days, although given the length of the whole data set it cannot be claimed to be significant. We also investigate the optical/NIR color variability and find that this source shows a simple redder-when-brighter behavior over time, even in the low-flux state.
WOS关键词GAMMA-RAY EMISSION ; ACTIVE GALACTIC NUCLEI ; QUASI-PERIODIC OSCILLATIONS ; SPECTRUM RADIO QUASAR ; LARGE-AREA TELESCOPE ; PARSEC-SCALE JETS ; BLACK-HOLE MASS ; OJ 287 ; LIGHT CURVES ; X-RAY
资助项目National Key Ramp;D Intergovernmental Cooperation Program of China[2023YFE0102300] ; National Key Ramp;D Intergovernmental Cooperation Program of China[2022YFE0133700] ; Regional Collaborative Innovation Project of Xinjiang Uyghur Autonomous Region[2022E01013] ; National Natural Science Foundation of China[11873073] ; Chinese Academy of Sciences (CAS) Light of West China Program[2017-XBQNXZ-A-008] ; Chinese Academy of Sciences (CAS) Light of West China Program[2021-XBQNXZ-005] ; Department of Science and Technology (DST), government of India, through the DST-INSPIRE Faculty grant[DST/INSPIRE/04/2020/002586] ; Chinese Academy of Sciences (CAS) President's International Fellowship Initiative (PIFI)[2016VMB073] ; Innovation Program of the Shanghai Municipal Education Commission[2019-01-07-00-07-E00035] ; National Natural Science Foundation of China (NSFC)[11973019] ; Shanghai Pilot Program for Basic Research Chinese Academy of Science, Shanghai Branch[JCYJ-SHFY2021-013] ; China Manned Space Project[CMSCSST-2021-A06]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP Publishing Ltd
WOS记录号WOS:001041266500001
资助机构National Key Ramp;D Intergovernmental Cooperation Program of China ; Regional Collaborative Innovation Project of Xinjiang Uyghur Autonomous Region ; National Natural Science Foundation of China ; Chinese Academy of Sciences (CAS) Light of West China Program ; Department of Science and Technology (DST), government of India, through the DST-INSPIRE Faculty grant ; Chinese Academy of Sciences (CAS) President's International Fellowship Initiative (PIFI) ; Innovation Program of the Shanghai Municipal Education Commission ; National Natural Science Foundation of China (NSFC) ; Shanghai Pilot Program for Basic Research Chinese Academy of Science, Shanghai Branch ; China Manned Space Project
源URL[http://ir.xao.ac.cn/handle/45760611-7/5361]  
专题研究单元未命名
通讯作者Yuan, Q.
作者单位1.Taras Shevchenko Natl Univ Kyiv, Radio Astron & Geodynam Dept CrAO, Kiev, Ukraine
2.Univ Turku, Finnish Ctr Astron ESO FINCA, Vesilinnantie 5, FI-20014 Turku, Finland
3.Aalto Univ, Dept Elect & Nanoengn, POB 15500, FI-00076 Aalto, Finland
4.Aalto Univ, Metsahovi Radio Observ, Metsahovintie 114, FI-02540 Kylmala, Finland
5.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China
6.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Peoples R China
7.Coll New Jersey, Dept Phys, 2000 Pennington Rd, Ewing, NJ 08628 USA
8.Fudan Univ, Ctr Field Theory & Particle Phys, Dept Phys, 2005 Songhu Rd, Shanghai 200438, Peoples R China
9.Southern Methodist Univ, Dept Phys, 3215 Daniel Ave, Dallas, TX 75205 USA
10.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
推荐引用方式
GB/T 7714
Yuan, Q.,Kushwaha, Pankaj,Gupta, Alok C.,et al. Multiwavelength Temporal Variability of the Blazar PKS 1510-089[J]. ASTROPHYSICAL JOURNAL,2023,953(1):15.
APA Yuan, Q..,Kushwaha, Pankaj.,Gupta, Alok C..,Tripathi, Ashutosh.,Wiita, Paul J..,...&Volvach, A. E..(2023).Multiwavelength Temporal Variability of the Blazar PKS 1510-089.ASTROPHYSICAL JOURNAL,953(1),15.
MLA Yuan, Q.,et al."Multiwavelength Temporal Variability of the Blazar PKS 1510-089".ASTROPHYSICAL JOURNAL 953.1(2023):15.

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