中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Is BZB J1450+5201 the most distant gamma-ray BL Lacertae object?

文献类型:期刊论文

作者Liao NH(廖能惠)1,2,3; Bai JM(白金明)1,2; Wang JG(王建国)1,2; Liu HT(刘洪涛)1,2; Zhang JJ(张居甲)1,2,3; Jiang, N4,5; Yuan ZL(袁尊里)1,2; Chen, L6
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2015-03
卷号15期号:3页码:313-326
ISSN号1674-4527
关键词galaxies: active BL Lacertae objects: individual (BZB J1450+5201) gamma rays: galaxies radiation mechanisms: non-thermal
通讯作者Liao, NH (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
产权排序第一完成单位
英文摘要BL Lacertae (BL Lac) objects at high redshifts (z >= 2) are rarely detected. Through careful analysis of its Sloan Digital Sky Survey spectrum, BZB J1450+5201 is confirmed to be a high-z BL Lac object with z >= 2.471 by identifying the Ly alpha 1216 and CIV 1548/1550 absorption lines. This indicates that BZB J1450+5201 is the most distant BL Lac object discovered to date. Careful analysis of the five-year Fermi-LAT data of 2FGL J1451.0+5159 shows that its gamma-ray emission is robust with a confidence level of 6.2 sigma at 1-3 GeV and 6.7 sigma at 3-10 GeV. This analysis with the five-year data overcomes confusion with its bright neighbor, which is a problem when analyzing the two-year data. In addition, 2FGL J1451.0+5159 is confirmed to be associated with BZB J1450+5201 using the five-year data. The analysis of multiwavelength data, from radio to gamma-ray energies, indicates that BZB J1450+5201 is an intermediate synchrotron peaked (ISP) source. Its multiwavelength properties are consistent with distributions of other ISP sources at lower redshifts in the second Fermi-LAT AGN catalog. The pure synchrotron self-Compton (SSC) model seems to be disfavored, but the scattering of weak external emission plus the SSC process can provide a satisfactory description of the broadband emission.
学科主题Astronomy & Astrophysics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]LARGE-AREA TELESCOPE ; DIGITAL SKY SURVEY ; INFRARED-SURVEY-EXPLORER ; EXTRAGALACTIC BACKGROUND LIGHT ; ACTIVE GALACTIC NUCLEI ; BLAZAR S5 0716+714 ; DATA RELEASE ; MULTIWAVELENGTH OBSERVATIONS ; OPTICAL SPECTROSCOPY ; DETECTED BLAZARS
收录类别SCI
原文出处http://iopscience.iop.org/article/10.1088/1674-4527/15/3/002/meta
语种英语
WOS记录号WOS:000350680800002
源URL[http://ir.ynao.ac.cn/handle/114a53/5470]  
专题云南天文台_丽江天文观测站(南方基地)
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
3.University of Chinese Academy of Sciences, Beijing 100049, China
4.Key Laboratory for Research in Galaxies and Cosmology, University of Science and Technology of China, Chinese Academy of Sciences, Hefei 230026, China
5.Department of Astronomy, University of Science and Technology of China, Hefei 230026, China
6.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China
推荐引用方式
GB/T 7714
Liao NH,Bai JM,Wang JG,et al. Is BZB J1450+5201 the most distant gamma-ray BL Lacertae object?[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2015,15(3):313-326.
APA Liao NH.,Bai JM.,Wang JG.,Liu HT.,Zhang JJ.,...&Chen, L.(2015).Is BZB J1450+5201 the most distant gamma-ray BL Lacertae object?.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,15(3),313-326.
MLA Liao NH,et al."Is BZB J1450+5201 the most distant gamma-ray BL Lacertae object?".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 15.3(2015):313-326.

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来源:云南天文台

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