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ELUCID-EXPLORING THE LOCAL UNIVERSE WITH RECONSTRUCTED INITIAL DENSITY FIELD. III. CONSTRAINED SIMULATION IN THE SDSS VOLUME
Wang, Huiyuan10; Mo, H. J.7,8,9; Yang, Xiaohu5,6; Zhang, Youcai4; Shi, JingJing3,10; Jing, Y. P.5,6; Liu, Chengze6; Li, Shijie6; Kang, Xi2; Gao, Yang1
刊名ASTROPHYSICAL JOURNAL
2016-11-10
卷号831期号:2
关键词Dark Matter Galaxies: Halos Large-scale Structure Of Universe Methods: Statistical
ISSN号0004-637X
DOI10.3847/0004-637X/831/2/164
英文摘要A method we developed recently for the reconstruction of the initial density field in the nearby universe is applied to the Sloan Digital Sky Survey Data Release 7. A high-resolution N-body constrained simulation (CS) of the reconstructed initial conditions, with 3072(3) particles evolved in a 500 h(-1) Mpc box, is carried out and analyzed in terms of the statistical properties of the final density field and its relation with the distribution of Sloan Digital Sky Survey galaxies. We find that the statistical properties of the cosmic web and the halo populations are accurately reproduced in the CS. The galaxy density field is strongly correlated with the CS density field, with a bias that depends on both galaxy luminosity and color. Our further investigations show that the CS provides robust quantities describing the environments within which the observed galaxies and galaxy systems reside. Cosmic variance is greatly reduced in the CS so that the statistical uncertainties can be controlled effectively, even for samples of small volumes.
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000387878200015
内容类型期刊论文
源URL[http://119.78.226.72/handle/331011/32695]  
专题中国科学院上海天文台
通讯作者Wang, Huiyuan
作者单位1.Chinese Acad Sci, Comp Network Informat Ctr, Beijing 100190, Peoples R China
2.Partner Grp MPI Astron, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Jiangsu, Peoples R China
3.SISSA, Via Bonomea 265, I-34136 Trieste, Italy
4.Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Nandan Rd 80, Shanghai 200030, Peoples R China
5.Shanghai Jiao Tong Univ, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China
6.Shanghai Jiao Tong Univ, Ctr Astron & Astrophys, Shanghai 200240, Peoples R China
7.Tsinghua Univ, Ctr Astrophys, Beijing 10084, Peoples R China
8.Tsinghua Univ, Dept Astron, Beijing 10084, Peoples R China
9.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
10.Univ Sci & Technol China, Dept Astron, Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
推荐引用方式
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Wang, Huiyuan,Mo, H. J.,Yang, Xiaohu,et al. ELUCID-EXPLORING THE LOCAL UNIVERSE WITH RECONSTRUCTED INITIAL DENSITY FIELD. III. CONSTRAINED SIMULATION IN THE SDSS VOLUME[J]. ASTROPHYSICAL JOURNAL,2016,831(2).
APA Wang, Huiyuan.,Mo, H. J..,Yang, Xiaohu.,Zhang, Youcai.,Shi, JingJing.,...&Gao, Yang.(2016).ELUCID-EXPLORING THE LOCAL UNIVERSE WITH RECONSTRUCTED INITIAL DENSITY FIELD. III. CONSTRAINED SIMULATION IN THE SDSS VOLUME.ASTROPHYSICAL JOURNAL,831(2).
MLA Wang, Huiyuan,et al."ELUCID-EXPLORING THE LOCAL UNIVERSE WITH RECONSTRUCTED INITIAL DENSITY FIELD. III. CONSTRAINED SIMULATION IN THE SDSS VOLUME".ASTROPHYSICAL JOURNAL 831.2(2016).
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