Mass to light ratio of galaxies and gravitational lensing
文献类型:期刊论文
作者 | Li, Ran![]() ![]() ![]() ![]() |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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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 |
DOI | 10.1088/1674-4527/13/9/003 |
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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