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Redshifts of Distant Blazars Limited by Fermi and VHE gamma-Ray Observations
Yang JP(杨建平)1,2,3; Wang JC(王建成)1,2; Yang, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
2010
卷号62期号:4页码:L23-L26
DOI10.1093/pasj/62.4.L23
产权排序第1完成单位
收录类别SCI ; EI
关键词Diffuse Radiation Bl Lacertae Objects: Individual (Pg 1553+113 Gamma-rays: Observations 3c 66a Pks 1424+240)
摘要Our goal is to limit the redshifts of three blazars, PG 1553+113, 3C 66A, and PKS 1424+240, through an investigation of their Fermi and VHE (very high energy) gamma-ray observations. We assume that the intrinsic spectra of PG 1553+113, 3C 66A, and PKS 1424+240 have no cutoff across the Fermi and VHE gamma-ray energy ranges. The intrinsic spectra of VHE gamma-rays are obtained through extrapolation of the Fermi spectra. Comparing the measured and intrinsic VHE spectra due to extragalactic background light (EBL) absorption, we give the redshift upper limits of three blazars, while assuming a specific EBL model. The redshift upper limits of PG 1553+113, 3C 66A, and PKS 1424+240 are 0.78, 0.58, and 1.19, respectively. Near to the TeV energy the optical depth of VHE gamma photons might be overestimated by the Franceschini EBL model (Franceschini et al. 2008, A&A, 487, 837), or the second emission component might be present in the VHE spectra and lead the intrinsic photon index to be harder than the Fermi ones.
项目资助者National Natural Science Foundation of China [10673028, 10778702] ; National Basic Research Program of China [2009CB824800] ; Chinese Academy of Sciences [KJCX2-YW-T24]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0004-6264
URL查看原文
归档日期2010-08-06
WOS记录号WOS:000282485100009
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]BL LACERTAE OBJECTS ; EXTRAGALACTIC BACKGROUND LIGHT ; ACTIVE GALACTIC NUCLEI ; HIGH-ENERGY RADIATION ; GEV EMISSION ; PG 1553+113 ; OPTICAL SPECTROSCOPY ; LAC OBJECTS ; 3C 66A ; X-RAY
EI入藏号20215211380724
EI主题词Gamma rays
EI分类号723.1.1 Computer Programming Languages - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics
引用统计
被引频次:15[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5002
专题高能天体物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Yang, JP (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories, Yunnan Observatory, 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.Yunnan Agricultural University, Kunming 650201, China
第一作者单位中国科学院云南天文台
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Yang JP,Wang JC,Yang, JP . Redshifts of Distant Blazars Limited by Fermi and VHE gamma-Ray Observations[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2010,62(4):L23-L26.
APA Yang JP,Wang JC,&Yang, JP .(2010).Redshifts of Distant Blazars Limited by Fermi and VHE gamma-Ray Observations.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,62(4),L23-L26.
MLA Yang JP,et al."Redshifts of Distant Blazars Limited by Fermi and VHE gamma-Ray Observations".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 62.4(2010):L23-L26.
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