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Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to z similar to 3
Cao, Shuo1; Zheng, Xiaogang1,2; Biesiada, Marek1,2; Qi, Jingzhao1; Chen, Yun3; Zhu, Zong-Hong1
2017-09-27
发表期刊ASTRONOMY & ASTROPHYSICS
卷号606
摘要Context. Ultra-compact structure in radio sources (especially in quasars that can be observed up to very high redshifts), with milliarcsecond angular sizes measured by very-long-baseline interferometry (VLBI), is becoming an important astrophysical tool for probing both cosmology and the physical properties of AGN.
文章类型Article
关键词Cosmological Parameters Quasars: General Galaxies: Active Radio Continuum: Galaxies
WOS标题词Science & Technology ; Physical Sciences
资助者National Key Research and Development Program of China(2017YFA0402603) ; National Key Research and Development Program of China(2017YFA0402603) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; National Natural Science Foundation of China(11503001 ; National Natural Science Foundation of China(11503001 ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; China Postdoctoral Science Foundation(2015T80052) ; China Postdoctoral Science Foundation(2015T80052) ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; China Scholarship Council ; China Scholarship Council ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Foreign Talent Introducing Project ; Foreign Talent Introducing Project ; Special Fund Support of Foreign Knowledge Introducing Project in China ; Special Fund Support of Foreign Knowledge Introducing Project in China ; 11373014 ; 11373014 ; 11690023) ; 11690023) ; National Key Research and Development Program of China(2017YFA0402603) ; National Key Research and Development Program of China(2017YFA0402603) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; National Natural Science Foundation of China(11503001 ; National Natural Science Foundation of China(11503001 ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; China Postdoctoral Science Foundation(2015T80052) ; China Postdoctoral Science Foundation(2015T80052) ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; China Scholarship Council ; China Scholarship Council ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Foreign Talent Introducing Project ; Foreign Talent Introducing Project ; Special Fund Support of Foreign Knowledge Introducing Project in China ; Special Fund Support of Foreign Knowledge Introducing Project in China ; 11373014 ; 11373014 ; 11690023) ; 11690023)
DOI10.1051/0004-6361/201730551
关键词[WOS]ACTIVE GALACTIC NUCLEI ; SIZE REDSHIFT RELATION ; BARYON ACOUSTIC-OSCILLATIONS ; DISTANCE-DUALITY RELATION ; RELAXED GALAXY CLUSTERS ; SOURCE ANGULAR SIZE ; HUBBLE CONSTANT ; IA SUPERNOVAE ; PARAMETERS ; EXPANSION
收录类别SCI
语种英语
资助者National Key Research and Development Program of China(2017YFA0402603) ; National Key Research and Development Program of China(2017YFA0402603) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; National Natural Science Foundation of China(11503001 ; National Natural Science Foundation of China(11503001 ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; China Postdoctoral Science Foundation(2015T80052) ; China Postdoctoral Science Foundation(2015T80052) ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; China Scholarship Council ; China Scholarship Council ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Foreign Talent Introducing Project ; Foreign Talent Introducing Project ; Special Fund Support of Foreign Knowledge Introducing Project in China ; Special Fund Support of Foreign Knowledge Introducing Project in China ; 11373014 ; 11373014 ; 11690023) ; 11690023) ; National Key Research and Development Program of China(2017YFA0402603) ; National Key Research and Development Program of China(2017YFA0402603) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; Ministry of Science and Technology National Basic Science Program (Project 973)(2014CB845806) ; National Natural Science Foundation of China(11503001 ; National Natural Science Foundation of China(11503001 ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; Fundamental Research Funds for the Central Universities and Scientific Research Foundation of Beijing Normal University ; China Postdoctoral Science Foundation(2015T80052) ; China Postdoctoral Science Foundation(2015T80052) ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; Opening Project of Key Laboratory of Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences ; China Scholarship Council ; China Scholarship Council ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Poland-China Scientific & Technological Cooperation Committee(35-4) ; Foreign Talent Introducing Project ; Foreign Talent Introducing Project ; Special Fund Support of Foreign Knowledge Introducing Project in China ; Special Fund Support of Foreign Knowledge Introducing Project in China ; 11373014 ; 11373014 ; 11690023) ; 11690023)
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000412874100001
引用统计
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/20108
专题太阳物理研究部
作者单位1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
2.Univ Silesia, Inst Phys, Dept Astrophys & Cosmol, Uniwersytecka 4, PL-40007 Katowice, Poland
3.Chinese Acad Sci, Natl Astron Observ, Key Lab Computat Astrophys, Beijing 100012, Peoples R China
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Cao, Shuo,Zheng, Xiaogang,Biesiada, Marek,et al. Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to z similar to 3[J]. ASTRONOMY & ASTROPHYSICS,2017,606.
APA Cao, Shuo,Zheng, Xiaogang,Biesiada, Marek,Qi, Jingzhao,Chen, Yun,&Zhu, Zong-Hong.(2017).Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to z similar to 3.ASTRONOMY & ASTROPHYSICS,606.
MLA Cao, Shuo,et al."Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to z similar to 3".ASTRONOMY & ASTROPHYSICS 606(2017).
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