Multiwavelength Mass Comparisons of the \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} \…
Author(s) -
A. K. Hicks,
E. Ellingson,
Henk Hoekstra,
H. K. C. Yee
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/508138
Subject(s) - physics , astrophysics , hydrostatic equilibrium , galaxy cluster , surface brightness , redshift , cosmology , galaxy , scaling , spectral line , geometry , quantum mechanics , mathematics
Results are presented from a detailed analysis of optical and X-rayobservations of moderate-redshift galaxy clusters from the Canadian Network forObservational Cosmology (CNOC) subsample of the EMSS. The combination ofextensive optical and deep X-ray observations of these clusters make them idealcandidates for multiwavelength mass comparison studies. X-ray surfacebrightness profiles of 14 clusters with 0.17
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