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Hubble diagram at higher redshifts: model independent calibration of quasars

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成果类型:
期刊论文
作者:
Li, Xiaolei;Keeley, Ryan E.;Shafieloo, Arman;Zheng, Xiaogang;Cao, Shuo;...
通讯作者:
Xiaolei Li<&wdkj&>Ryan E Keeley<&wdkj&>Arman Shafieloo
作者机构:
[Li, Xiaolei] Hebei Normal Univ, Coll Phys, Shijiazhuang 050024, Hebei, Peoples R China.
[Keeley, Ryan E.; Shafieloo, Arman] Korea Astron & Space Sci Inst, Daejeon 34055, South Korea.
[Shafieloo, Arman] Univ Sci & Technol, 217 Gajeong Ro, Daejeon 34113, South Korea.
[Zheng, Xiaogang] Wuhan Polytech Univ, Sch Elect & Elect Engn, Wuhan 430023, Peoples R China.
[Biesiada, Marek; Cao, Shuo; Zhu, Zong-Hong] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China.
通讯机构:
[Xiaolei Li] C
[Ryan E Keeley; Arman Shafieloo] K
Korea Astronomy and Space Science Institute , Daejeon 34055, Korea<&wdkj&>Korea Astronomy and Space Science Institute , Daejeon 34055, Korea<&wdkj&>University of Science and Technology , Yuseong-gu 217 Gajeong-ro, Daejeon 34113, Korea<&wdkj&>College of Physics, Hebei Normal University , Shijiazhuang 050024, China
语种:
英文
关键词:
Cosmology: observations;quasars: general;Methods: statistical
期刊:
Monthly Notices of the Royal Astronomical Society
ISSN:
0035-8711
年:
2021
卷:
507
期:
1
页码:
919-926
基金类别:
National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC) [12003006, 11947091, 12021003, 11690023, 11633001, 11920101003, 11373014]; Hebei NSF [A2020205002]; Korea Institute for Advanced Study (KIAS) - Korea government; Beijing Talents Fund of Organization Department of BeijingMunicipal Committee of the CPC; Strategic Priority Research Program of the Chinese Academy of SciencesChinese Academy of Sciences [XDB23000000]; Interdiscipline Research Funds of Beijing Normal University; Key Foreign Expert Program for the Central Universities [X2018002]; Hebei Normal University [L2020B02]; National Key R&D Program of China [2017YFA0402600]
机构署名:
本校为其他机构
院系归属:
电气与电子工程学院
摘要:
In this paper, we present a model-independent approach to calibrate the largest quasar sample. Calibrating quasar samples is essentially constraining the parameters of the linear relation between the log  of the ultraviolet (UV) and X-ray luminosities. This calibration allows quasars to be used as standardized candles. There is a strong correlation between the parameters characterizing the quasar luminosity relation and the cosmological distances inferred from using quasars as standardized candles. We break this degeneracy by using Gaussian pr...

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