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:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/534/i=1/a=1/pdf
Reference31 articles.
1. A Counts‐in‐Cells Analysis of Lyman‐Break Galaxies at Redshiftz∼ 3
2. Clustering of galaxies at high redshifts
3. The Most Massive Distant Clusters: Determining Ω and σ8
4. Effects of sampling on statistics of large-scale structure
5. How relaxed is the distribution of galaxies?
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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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