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Super-Large-Scale Structures in the Sloan Digital Sky Survey
引用本文:Xin-Fa Deng~1 Yi-Qing Chen~2 Qun Zhang~1 and Ji-Zhou He~1 1 Mathematics and Physics College,Nanchang University,Jiangxi 330047, 2 Management College,Nanchang University,Nanchang 330047. Super-Large-Scale Structures in the Sloan Digital Sky Survey[J]. 中国天文和天体物理学报, 2006, 6(1): 35-42
作者姓名:Xin-Fa Deng~1 Yi-Qing Chen~2 Qun Zhang~1 and Ji-Zhou He~1 1 Mathematics and Physics College  Nanchang University  Jiangxi 330047   2 Management College  Nanchang University  Nanchang 330047
作者单位:Xin-Fa Deng~1 Yi-Qing Chen~2 Qun Zhang~1 and Ji-Zhou He~1 1 Mathematics and Physics College,Nanchang University,Jiangxi 330047; 2 Management College,Nanchang University,Nanchang 330047
基金项目:Supported by the National Natural Science Foundation of China
摘    要:We study the super-large-scale structures in the Sloan Digital Sky Survey by cluster analysis,and examine the geometry and the properties of the member galaxies.Two subsamples are selected from the SDSS,Subsample 1 at the celestial equator and Subsample 2 further north.In Subsample 1 we discover two compact super-large-scale structures:the Sloan Great Wall and the CfA Great Wall.The Sloan Great Wall,located at a median redshift of z=0.07804,has a total length of about 433 Mpc and a mean galaxy density of about six times that of the whole sample. Most of its member galaxies are of medium size and brightness.The CfA Great Wall, located at a median redshift of z=0.03058,has a total length of about 251 Mpc and includes large percentages of faint and small galaxies and relatively fewer early-type galaxies.

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Super-Large-Scale Structures in the Sloan Digital Sky Survey
Xin-Fa Deng,Yi-Qing Chen,Qun Zhang,Ji-Zhou He. Super-Large-Scale Structures in the Sloan Digital Sky Survey[J]. Chinese Journal of Astronomy and Astrophysics, 2006, 6(1): 35-42
Authors:Xin-Fa Deng  Yi-Qing Chen  Qun Zhang  Ji-Zhou He
Affiliation:[1]Mathematics and Physics College, Nanchang University, Jiangxi 330047 [2]Management Collegel Nanchang University,Nanchang 330047
Abstract:We study the super-large-scale structures in the Sloan Digital Sky Survey by cluster analysis,and examine the geometry and the properties of the member galaxies.Two subsamples are selected from the SDSS,Subsample 1 at the celestial equator and Subsample 2 further north.In Subsample 1 we discover two compact super-large-scale structures:the Sloan Great Wall and the CfA Great Wall.The Sloan Great Wall,located at a median redshift of z=0.07804,has a total length of about 433 Mpc and a mean galaxy density of about six times that of the whole sample. Most of its member galaxies are of medium size and brightness.The CfA Great Wall, located at a median redshift of z=0.03058,has a total length of about 251 Mpc and includes large percentages of faint and small galaxies and relatively fewer early-type galaxies.
Keywords:galaxy  distances and redshifts-large-scale structure of universe
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