Published in
American Astronomical Society, Astrophysical Journal Supplement, 2(176), p. 301-330, 2008
DOI: 10.1086/527673
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The Subaru/XMM‐NewtonDeep Survey (SXDS). IV. Evolution of Lyα Emitters from \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 $z=3.1$ \end{document} to 5.7 in the 1 deg2Field: Luminosity Functions and AGN
Journal article published in 2008 by
Masami Ouchi 
,
Kazuhiro Shimasaku,
Masayuki Akiyama,
Chris Simpson,
Tomoki Saito,
Yoshihiro Ueda,
Hisanori Furusawa ,
Kazuhiro Sekiguchi,
Toru Yamada,
Tadayuki Kodama,
Nobunari Kashikawa,
Sadanori Okamura,
Masanori Iye,
Tadafumi Takata ,
Michitoshi Yoshida
and other authors.
,
Kazuhiro Shimasaku,
Masayuki Akiyama,
Chris Simpson,
Tomoki Saito,
Yoshihiro Ueda,
Hisanori Furusawa ,
Kazuhiro Sekiguchi,
Toru Yamada,
Tadayuki Kodama,
Nobunari Kashikawa,
Sadanori Okamura,
Masanori Iye,
Tadafumi Takata ,
Michitoshi Yoshida
and other authors.
This paper was not found in any repository, but could be made available legally by the author.
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