中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Characterizing Optical Variability of OJ 287 in 2016-2017

文献类型:期刊论文

作者Gupta, Alok C.1,2; Gaur, Haritma1; Wiita, Paul J.3; Pandey, A.1; Kushwaha, P.4; Hu, S. M.5; Kurtanidze, O. M.6,7,8,9; Semkov, E.10,11; Damljanovic, G.12; Goyal, A.13
刊名ASTRONOMICAL JOURNAL
出版日期2019-03-01
卷号157期号:3页码:12
ISSN号0004-6256
关键词BL Lacertae objects: general BL Lacertae objects: individual (OJ 287) techniques: photometric techniques: polarimetric
DOI10.3847/1538-3881/aafe7d
通讯作者Gupta, Alok C.(acgupta30@gmail.com)
英文摘要We report on a recent multiband optical photometric and polarimetric observational campaign of the blazar OJ 287 that was carried out during 2016 September-2017 December. We employed nine telescopes in Bulgaria, China, Georgia, Japan, Serbia, Spain, and the United States. We collected over 1800 photometric image frames in BVRI bands and over 100 polarimetric measurements over similar to 175 nights. In 11 nights with many quasi-simultaneous multiband (V, R, I) observations, we did not detect any genuine intraday variability in flux or color. On longer timescales, multiple flaring events were seen. Large changes in color with respect to time and in a color-magnitude diagram were seen, and while only a weak systematic variability trend was noticed in color with respect to time, the color-magnitude diagram shows a bluer-when-brighter trend. Large changes in the degree of polarization and substantial swings in the polarization angle were detected. The fractional Stokes parameters of the polarization showed a systematic trend with time in the beginning of these observations, followed by chaotic changes and then an apparently systematic variation at the end. These polarization changes coincide with the detection and duration of the source at very high energies as seen by VERITAS. The spectral index shows a systematic variation with time and V-band magnitude. We briefly discuss possible physical mechanisms that could explain the observed flux, color, polarization, and spectral variability.
WOS关键词ACTIVE GALACTIC NUCLEUS ; INTRADAY VARIABILITY ; BL LACERTAE ; BLACK-HOLE ; SPECTRAL VARIABILITY ; RELATIVISTIC JETS ; RADIO OUTBURSTS ; BLAZARS ; MULTIWAVELENGTH ; POLARIZATION
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000457852600001
源URL[http://libir.pmo.ac.cn/handle/332002/18757]  
专题中国科学院紫金山天文台
通讯作者Gupta, Alok C.
作者单位1.Aryabhatta Res Inst Observat Sci ARIES, Naini Tal 263002, India
2.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, Shanghai 200030, Peoples R China
3.Coll New Jersey, Dept Phys, 2000 Pennington Rd, Ewing, NJ 08628 USA
4.Univ Sao Paulo, Dept Astron, IAG USP, BR-05508090 Sao Paulo, Brazil
5.Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Inst Space Sci, Weihai 264209, Peoples R China
6.Abastumani Observ, GE-0301 Mt Kanobili, Abastumani, Rep of Georgia
7.Kazan Fed Univ, Engelhardt Astron Observ, Tatarstan, Russia
8.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
9.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China
10.Bulgarian Acad Sci, Inst Astron, 72 Tsarigradsko Shosse Blvd, Sofia 1784, Bulgaria
推荐引用方式
GB/T 7714
Gupta, Alok C.,Gaur, Haritma,Wiita, Paul J.,et al. Characterizing Optical Variability of OJ 287 in 2016-2017[J]. ASTRONOMICAL JOURNAL,2019,157(3):12.
APA Gupta, Alok C..,Gaur, Haritma.,Wiita, Paul J..,Pandey, A..,Kushwaha, P..,...&Strigachev, A..(2019).Characterizing Optical Variability of OJ 287 in 2016-2017.ASTRONOMICAL JOURNAL,157(3),12.
MLA Gupta, Alok C.,et al."Characterizing Optical Variability of OJ 287 in 2016-2017".ASTRONOMICAL JOURNAL 157.3(2019):12.

入库方式: OAI收割

来源:紫金山天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。