The Magnitude‐Size Relation of Galaxies out to \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 $z\sim 1$ \end{document}
The Astrophysical Journal1999Vol. 519(2), pp. 563–579
Citations Over TimeTop 10% of 1999 papers
Luc Simard, David C. Koo, S. M. Faber, Vicki L. Sarajedini, Nicole P. Vogt, Andrew C. Phillips, Karl Gebhardt, G. D. Illingworth, K. Wu
Abstract
As part of the Deep Extragalactic Evolutionary Probe (DEEP) survey, a sample of 190 field galaxies (I814 ≤ 23.5) in the "Groth Survey Strip" has been used to analyze the magnitude-size relation over the range 0.1 0.7), a handful of luminous, high surface brightness galaxies appears that occupies a region of the magnitude-size plane rarely populated by local galaxies. Their wide range of colors and bulge fractions points to a variety of possible origins.
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