KMS of Xinjiang Astronomical Observatory, CAS
| Multiwavelength Temporal Variability of the Blazar PKS 1510-089 | |
Yuan, Q.1,2 ; Kushwaha, Pankaj3,4; Gupta, Alok C.4,5; Tripathi, Ashutosh6,7; Wiita, Paul J.8; Zhang, M.1,9,10; Liu, X.1,9,10; Lahteenmaki, Anne11,12; Tornikoski, Merja11; Tammi, Joni11; Ramakrishnan, Venkatessh11,13; Cui, L.1,9,10; Wang, X.1,2; Gu, M. F.5; Bambi, Cosimo7; Volvach, A. E.14
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| 2023-08-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 953Issue:1Pages:47 |
| Contribution Rank | 1 |
| Abstract | 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. |
| DOI | 10.3847/1538-4357/acdd74 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | 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 |
| Funding Project | 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 Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001041266500001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | 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 |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5362 |
| Collection | 中国科学院新疆天文台 |
| Corresponding Author | Yuan, Q. |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Univ Chinese Acad Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China 3.Indian Inst Sci Educ & Res Mohali, Dept Phys Sci, Knowledge City,Sect 8,SAS Nagar, Mohali 140306, Punjab, India 4.Aryabhatta Res Inst Observat Sci ARIES, Naini Tal 263001, India 5.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 6.Southern Methodist Univ, Dept Phys, 3215 Daniel Ave, Dallas, TX 75205 USA 7.Fudan Univ, Ctr Field Theory & Particle Phys, Dept Phys, 2005 Songhu Rd, Shanghai 200438, Peoples R China 8.Coll New Jersey, Dept Phys, 2000 Pennington Rd, Ewing, NJ 08628 USA 9.Chinese Acad Sci, Key Lab Radio Astron, 2 West Beijing Rd, Nanjing 210008, Peoples R China 10.Xinjiang Key Lab Radio Astrophys, Urumqi 830011, Peoples R China 11.Aalto Univ, Metsahovi Radio Observ, Metsahovintie 114, FI-02540 Kylmala, Finland 12.Aalto Univ, Dept Elect & Nanoengn, POB 15500, FI-00076 Aalto, Finland 13.Univ Turku, Finnish Ctr Astron ESO FINCA, Vesilinnantie 5, FI-20014 Turku, Finland 14.Taras Shevchenko Natl Univ Kyiv, Radio Astron & Geodynam Dept CrAO, Kiev, Ukraine |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation 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):47. |
| 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),47. |
| MLA | Yuan, Q.,et al."Multiwavelength Temporal Variability of the Blazar PKS 1510-089".ASTROPHYSICAL JOURNAL 953.1(2023):47. |
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| Yuan-2023-Multiwavel（1721KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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