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Revisiting Radio Variability of the Blazar 3C 454.3
Tripathi, Ashutosh1,2,3; Gupta, Alok C.4; Smith, Krista Lynne1,3; Wiita, Paul J.5; Aller, Margo F.6; Volvach, Alexandr E.7; Lahteenmaki, Anne8,9; Aller, Hugh D.6; Tornikoski, Merja8; Volvach, Larisa N.7
2024-12-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume977Issue:2Pages:166
Contribution Rank2
AbstractWe examine lengthy radio light curves of the flat spectrum radio galaxy 3C 454.3 for possible quasiperiodic oscillations (QPOs). The data used in this work were collected at five radio frequencies, 4.8, 8.0, 14.5, 22.0, and 37.0 GHz between 1979 and 2013 as observed at the University of Michigan Radio Astronomical Observatory, Crimean Astrophysical Observatory, and Aalto University Mets & auml;hovi Radio Observatory. We employ generalized Lomb-Scargle periodogram and weighted wavelet transform analyses to search for periodicities in these light curves. We confirm a QPO period of similar to 2000 days to be at least 4 sigma significant using both methods at all five radio frequencies between 1979 and 2007, after which a strong flare changed the character of the light curve. We also find a similar to 600 day period, which is at least 4 sigma significant, but only in the 22.0 and 37.0 GHz light curves. We briefly discuss physical mechanisms capable of producing such variations.
DOI10.3847/1538-4357/ad90e3
Indexed BySCI
Language英语
WOS KeywordQUASI-PERIODIC OSCILLATIONS ; GAMMA-RAY FLARE ; SPACE-TELESCOPE OBSERVATIONS ; ACTIVE GALACTIC NUCLEUS ; XMM-NEWTON OBSERVATIONS ; BLACK-HOLE ; LIGHT CURVES ; MULTIWAVELENGTH OBSERVATIONS ; BL LACERTAE ; OJ 287
Funding ProjectNASA[NNX11AO13G] ; NASA[NNX13AP18G] ; NASA[80NSSC22K0741] ; National Science Foundation[AST-0607523] ; National Science Foundation[AST-2407604] ; University of Michigan ; [NNX09AU16G] ; [NNX10AP16G]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001374908300001
PublisherIOP Publishing Ltd
Funding OrganizationNASA ; National Science Foundation ; University of Michigan
Citation statistics
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/7270
Collection射电天文研究室_天体化学研究团组
Corresponding AuthorTripathi, Ashutosh
Affiliation1.Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamental, College Stn, TX 77843 USA
2.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
3.Southern Methodist Univ, Dept Phys, 3215 Daniel Ave, Dallas, TX 75205 USA
4.Aryabhatta Res Inst Observat Sci ARIES, Naini Tal 263001, India
5.Coll New Jersey, Dept Phys, 2000 Pennington Rd, Ewing, NJ 08628 USA
6.Univ Michigan, Dept Astron, 1085 S Univ Ave, Ann Arbor, MI 48109 USA
7.Crimean Astrophys Observ, Radio Astron Lab, Katsiveli, Crimea, Ukraine
8.Aalto Univ, Metsahovi Radio Observ, Metsahovintie 114, Kylmala 02540, Finland
9.Aalto Univ, Dept Elect & Nanoengn, POB 15500, FI-00076 Aalto, Finland
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Tripathi, Ashutosh,Gupta, Alok C.,Smith, Krista Lynne,et al. Revisiting Radio Variability of the Blazar 3C 454.3[J]. ASTROPHYSICAL JOURNAL,2024,977(2):166.
APA Tripathi, Ashutosh.,Gupta, Alok C..,Smith, Krista Lynne.,Wiita, Paul J..,Aller, Margo F..,...&Volvach, Larisa N..(2024).Revisiting Radio Variability of the Blazar 3C 454.3.ASTROPHYSICAL JOURNAL,977(2),166.
MLA Tripathi, Ashutosh,et al."Revisiting Radio Variability of the Blazar 3C 454.3".ASTROPHYSICAL JOURNAL 977.2(2024):166.
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