High‐Redshift Galaxy Clustering and \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\Omega _{0}$ \end{document}

Author:

Saslaw William C.,Edgar James H.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Fluctuations of non-point mass galaxy distribution;Astrophysics and Space Science;2010-07-10

2. THE SPATIAL DISTRIBUTION FUNCTION OF GALAXIES AT HIGH REDSHIFT;The Astrophysical Journal;2009-04-07

3. The Galaxy Distribution Function from the 2MASS Survey;The Astrophysical Journal;2005-06-20

4. Gravitational Binding, Virialization, and the Peculiar Velocity Distribution of the Galaxies;The Astrophysical Journal;2004-06-20

5. Atomic and molecular processes in the early Universe;Journal of Physics B: Atomic, Molecular and Optical Physics;2002-05-09

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