中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Mass to light ratio of galaxies and gravitational lensing

文献类型:期刊论文

作者Li, Ran; Er, Xin-Zhong; Li, Nan; Li Nan; Li Ran
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2013-09-01
卷号13期号:9页码:1041-1051
关键词Cosmology: Dark Matter Galaxies: Halos Gravitational Lensing
DOI10.1088/1674-4527/13/9/003
英文摘要We investigate the potential of constraining the mass to light ratio of field galaxies using weak lensing shear and flexions. A suite of Monte Carlo simulations are used to generate weak lensing observations with different noise models. Using mock data, we find that the inclusion of flexions can improve the estimate of foreground halo parameters, but the details are strongly dependent on noise in the model. In the intrinsic noise limit, both shear and flexions are promising tools to study the mass to light ratio of galaxies. However, if the noise model of flexions follows the form described by Rowe et al., there is only similar to 5% improvement in the constraints even with next generation lensing observations.
语种英语
WOS记录号WOS:000323757800003
源URL[http://ir.bao.ac.cn/handle/114a11/8893]  
专题国家天文台_射电天文研究部
作者单位Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Li, Ran,Er, Xin-Zhong,Li, Nan,et al. Mass to light ratio of galaxies and gravitational lensing[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2013,13(9):1041-1051.
APA Li, Ran,Er, Xin-Zhong,Li, Nan,Li Nan,&Li Ran.(2013).Mass to light ratio of galaxies and gravitational lensing.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,13(9),1041-1051.
MLA Li, Ran,et al."Mass to light ratio of galaxies and gravitational lensing".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 13.9(2013):1041-1051.

入库方式: OAI收割

来源:国家天文台

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