中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
ELUCID. VI. Cosmic Variance of the Galaxy Distribution in the Local Universe

文献类型:期刊论文

作者Chen, Yangyao1,2; Mo, H. J.1,2,8; Li, Cheng1,2; Wang, Huiyuan3,7; Yang, Xiaohu5,6; Zhou, Huang1,2; Zhang, Youcai4
刊名ASTROPHYSICAL JOURNAL
出版日期2019-02-20
卷号872期号:2页码:16
ISSN号0004-637X
关键词dark matter galaxies: halos large-scale structure of universe methods: statistical
DOI10.3847/1538-4357/ab0208
英文摘要Halo merger trees are constructed from ELUCID, a constrained N-body simulation in the Sloan Digital Sky Survey (SDSS) volume. These merger trees are used to populate dark matter halos with galaxies according to an empirical model of galaxy formation. Mock catalogs in the SDSS sky coverage are constructed, which can be used to study the spatial distribution of galaxies in the low-z universe. These mock catalogs are used to quantify the cosmic variance (CV) in the galaxy stellar mass function (GSMF) measured from the SDSS survey. The GSMF estimated from the SDSS magnitude-limited sample can be affected significantly by the presence of an underdense region at z < 0.03, so that the low-mass end of the function can be underestimated significantly. Several existing methods designed to deal with the effects of the CV in the estimate of the GSMF are tested, and none is found to be able to fully account for the CV. We propose a method based on conditional stellar mass functions in dark matter halos, which can provide an unbiased estimate of the global GSMF. The application of the method to SDSS data shows that the GSMF has a significant upturn at M-* < 10(9.5) h(-1) M-circle dot, which has been missed in many earlier measurements of the local GSMF.
资助项目National Key R&D Program of China[2018YFA0404503] ; National Key R&D Program of China[2018YFA0404502] ; National Key Basic Research Program of China[2015CB857002] ; National Key Basic Research Program of China[2015CB857004] ; National Science Foundation of China[11233005] ; National Science Foundation of China[11621303] ; National Science Foundation of China[11522324] ; National Science Foundation of China[11421303] ; National Science Foundation of China[11503065] ; National Science Foundation of China[11673015] ; National Science Foundation of China[11733004] ; National Science Foundation of China[11320101002] ; NSF[AST-1517528]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000460814000003
源URL[http://119.78.226.72/handle/331011/31891]  
专题中国科学院上海天文台
通讯作者Chen, Yangyao
作者单位1.Tsinghua Univ, Phys Dept, Beijing 100084, Peoples R China
2.Tsinghua Univ, Ctr Astrophys, Beijing 100084, Peoples R China
3.Univ Sci & Technol China, Dept Astron, Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
4.Shanghai Astron Observ, Shanghai 200030, Peoples R China
5.Shanghai Jiao Tong Univ, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China
6.Shanghai Jiao Tong Univ, Dept Astron, Shanghai 200240, Peoples R China
7.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
8.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
推荐引用方式
GB/T 7714
Chen, Yangyao,Mo, H. J.,Li, Cheng,et al. ELUCID. VI. Cosmic Variance of the Galaxy Distribution in the Local Universe[J]. ASTROPHYSICAL JOURNAL,2019,872(2):16.
APA Chen, Yangyao.,Mo, H. J..,Li, Cheng.,Wang, Huiyuan.,Yang, Xiaohu.,...&Zhang, Youcai.(2019).ELUCID. VI. Cosmic Variance of the Galaxy Distribution in the Local Universe.ASTROPHYSICAL JOURNAL,872(2),16.
MLA Chen, Yangyao,et al."ELUCID. VI. Cosmic Variance of the Galaxy Distribution in the Local Universe".ASTROPHYSICAL JOURNAL 872.2(2019):16.

入库方式: OAI收割

来源:上海天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。