Modelling the redshift-space three-point correlation function in SDSS-III
文献类型：期刊论文
| 作者 | Guo, Hong1 ; Zheng, Zheng1; Jing, Y. P.2,3; Zehavi, Idit4; Li, Cheng5,6; Weinberg, David H.7,8; Skibba, Ramin A.9; Nichol, Robert C.10; Rossi, Graziano11,12; Sabiu, Cristiano G.13
|
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2015-05-01 |
| 卷号 | 449期号:1页码:L95-L99 |
| 关键词 | galaxies: distances and redshifts galaxies: haloes galaxies: statistics cosmology: observations cosmology: theory large-scale structure of Universe |
| 英文摘要 | We present the measurements of the redshift-space three-point correlation function (3PCF) for z similar to 0.5 luminous red galaxies of the CMASS sample in the Sloan Digital Sky Survey-III Baryon Oscillation Spectroscopic Survey Data Release 11. The 3PCF measurements are interpreted within the halo occupation distribution framework using high-resolution N-body simulations, and the model successfully reproduces the 3PCF on scales larger than 1 h(-1) Mpc. As with the case for the redshift-space two-point correlation functions, we find that the redshift-space 3PCF measurements also favour the inclusion of galaxy velocity bias in the model. In particular, the central galaxy in a halo is on average in motion with respect to the core of the halo. We discuss the potential of the small-scale 3PCF to tighten the constraints on the relation between galaxies and dark matter haloes and on the phase-space distribution of galaxies. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | DIGITAL SKY SURVEY ; OSCILLATION SPECTROSCOPIC SURVEY ; HALO OCCUPATION DISTRIBUTION ; PAIRWISE VELOCITY DISPERSION ; GALAXY CORRELATION-FUNCTION ; LUMINOUS RED GALAXIES ; LARGE-SCALE STRUCTURE ; COLOR DEPENDENCE ; BIAS ; UNIVERSE |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000353555000021 |
| 公开日期 | 2015-08-18 |
| 源URL | [http://119.78.226.72/handle/331011/18232]  |
| 专题 | 上海天文台_星系宇宙学重点实验室 |
| 作者单位 | 1.Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA 2.Shanghai Jiao Tong Univ, Dept Phys & Astron, Ctr Astron & Astrophys, Shanghai 200240, Peoples R China 3.Shanghai Jiao Tong Univ, IFSA Collaborat Innovat Ctr, Shanghai 200240, Peoples R China 4.Case Western Reserve Univ, Dept Astron, Cleveland, OH 44106 USA 5.Chinese Acad Sci, Shanghai Astron Observ, Max Planck Inst Astrophys, Partner Grp, Shanghai 200030, Peoples R China 6.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China 7.Ohio State Univ, Dept Astron, Columbus, OH 43210 USA 8.Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA 9.Univ Calif San Diego, Ctr Astrophys & Space Sci, San Diego, CA 92093 USA 10.Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England |
| 推荐引用方式 GB/T 7714 | Guo, Hong,Zheng, Zheng,Jing, Y. P.,et al. Modelling the redshift-space three-point correlation function in SDSS-III[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2015,449(1):L95-L99. |
| APA | Guo, Hong.,Zheng, Zheng.,Jing, Y. P..,Zehavi, Idit.,Li, Cheng.,...&McBride, Cameron K..(2015).Modelling the redshift-space three-point correlation function in SDSS-III.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,449(1),L95-L99. |
| MLA | Guo, Hong,et al."Modelling the redshift-space three-point correlation function in SDSS-III".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 449.1(2015):L95-L99. |
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。