中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
X-Ray Intraday Variability of the Blazar OJ 287 Observed with XMM-Newton

文献类型:期刊论文

作者Huang, Tao5,6; Gupta, Alok C.4,6; Cui, Lang3,5,6; Tripathi, Ashutosh6; Huang, Yongfeng1,2; Devanand, P. U.4; Liu, Xiang3,6
刊名ASTROPHYSICAL JOURNAL
出版日期2026-02-10
卷号998期号:1页码:14
ISSN号0004-637X
DOI10.3847/1538-4357/ae38b9
通讯作者Gupta, Alok C.(acgupta30@gmail.com)
英文摘要We present X-ray intraday variability, cross-correlated variability, and power spectrum density analysis of the binary black hole blazar candidate OJ 287. The X-ray pointed observations of the source were carried out on eight occasions by the EPIC-pn camera on board the XMM-Newton satellite from 2005 November to 2022 November. The good time intervals range between 3.6 and 24.1 hr. Three energy bands-0.2-2 keV (soft), 2-10 keV (hard), and 0.2-10 keV (total)-have been used to estimate variability. Low amplitude variations are observed in four, five, and six light curves in soft, hard, and total energy bands, respectively. Only two observation IDs have shown variation in the all energy bands. The discrete correlation function of the light curves in soft and hard energy bands peaks at zero lag, suggesting that the emission in both bands was cospatial and came from the same population of leptons. Red noise dominates the power spectral densities of variable light curves. According to our flux and spectrum investigations, both particle acceleration and synchrotron cooling mechanisms contribute significantly to the emission from this blazar.
WOS关键词SPECTRAL ENERGY-DISTRIBUTIONS ; ACTIVE GALACTIC NUCLEI ; LIGHT CURVES ; PKS 2155-304 ; POLARIZATION VARIABILITY ; PARTICLE-ACCELERATION ; PEAKED BLAZARS ; TEV BLAZARS ; 3C 273 ; FLUX
资助项目National Key R&D Program of China[No. 2021YFA0718500] ; CAS 'Light of West China' Program[No. 2021-XBQNXZ-005] ; TianShan Talent training Program[No. 2023TSYCCX0099]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001683683600001
出版者IOP Publishing Ltd
资助机构National Key R&D Program of China ; CAS 'Light of West China' Program ; TianShan Talent training Program
源URL[http://ir.xao.ac.cn/handle/45760611-7/8552]  
专题星系宇宙学研究团组
通讯作者Gupta, Alok C.
作者单位1.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, Peoples R China
2.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
3.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Peoples R China
4.Aryabhatta Res Inst Observat Sci ARIES, Naini Tal 263001, India
5.Univ Chinese Acad Sci, Sch Astron & Space Sci, 1 Yanqihu East Rd, Beijing 101408, Peoples R China
6.Chinese Acad Sci, State Key Lab Radio Astron & Technol, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
推荐引用方式
GB/T 7714
Huang, Tao,Gupta, Alok C.,Cui, Lang,et al. X-Ray Intraday Variability of the Blazar OJ 287 Observed with XMM-Newton[J]. ASTROPHYSICAL JOURNAL,2026,998(1):14.
APA Huang, Tao.,Gupta, Alok C..,Cui, Lang.,Tripathi, Ashutosh.,Huang, Yongfeng.,...&Liu, Xiang.(2026).X-Ray Intraday Variability of the Blazar OJ 287 Observed with XMM-Newton.ASTROPHYSICAL JOURNAL,998(1),14.
MLA Huang, Tao,et al."X-Ray Intraday Variability of the Blazar OJ 287 Observed with XMM-Newton".ASTROPHYSICAL JOURNAL 998.1(2026):14.

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