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The clustering and abundance of star-forming and passive galaxies atz∼ 2

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The Nascent Red Sequence at \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 $z\sim 2$ \end{document}

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From Rings to Bulges: Evidence for Rapid Secular Galaxy Evolution atz∼ 2 from Integral Field Spectroscopy in the SINS Survey

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Dynamical Properties ofz∼ 2 Star‐forming Galaxies and a Universal Star Formation Relation

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The Role of the Dust in Primeval Galaxies: A Simple Physical Model for Lyman Break Galaxies and Lyα Emitters

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Multiwavelength Study of Massive Galaxies atz∼2. I. Star Formation and Galaxy Growth

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