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Clustering of Submillimeter‐selected Galaxies
Accurate Spectral Energy Distributions and Selection Effects for High‐Redshift Dusty Galaxies: A New Hot Population to Discover with theSpitzer Space Telescope?
A multiply imaged, submillimetre-selected ultraluminous infrared galaxy in a galaxy group atz∼ 2.5
A Filamentary Structure of Massive Star-forming Galaxies Associated with an X-Ray-absorbed QSO atz=1.8
Near-Infrared Colors of Submillimeter-selected Galaxies
Deep Near-Infrared Imaging of Submillimeter Selected Galaxies
Deep infrared imaging around ultraluminous high-redshift galaxies
AnHSTmorphological survey of faint extremely red objects
ChandraDetections of SCUBA Galaxies around High‐zRadio Sources
A Wide‐FieldHubble Space TelescopeStudy of the Cluster Cl 0024+1654 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 $z=0.4$ \end{document} . II. The Cluster Mass Distribution
The morphology-density relation in the Sloan Digital Sky Survey
Extended X‐Ray Emission around 4C 41.17 atz= 3.8
INGRID: A near-infrared camera for the William Herschel Telescope
The formation of cluster elliptical galaxies as revealed by extensive star formation
Erratum: "The Transformation of Galaxies within the Large-Scale Structure around az= 0.41 Cluster" ([URL ADDRESS="/cgi-bin/resolve?2001ApJ...562L...9K" STATUS="OKAY"]ApJ, 562, L9 [2001][/URL])
Thez=2.51 Extremely Red Submillimeter Galaxy SMM J04431+0210
A Wide‐FieldHubble Space TelescopeStudy of the Cluster Cl 0024+16 atz= 0.4. I. Morphological Distributions to 5 Mpc Radius
Measuring 8 with Cluster Lensing: Biases from Unrelaxed Clusters
A median redshift of 2.4 for galaxies bright at submillimetre wavelengths
Data analysis method for XMM-Newton observations of extended sources and application to bright massive clusters of galaxies at z=0.2
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