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Strong and weak lensing united

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Using Weak‐Lensing Dilution to Improve Measurements of the Luminous and Dark Matter in A1689

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Strong and weak lensing united

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Cluster mass profiles from weak lensing: The influence of substructure

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Strong‐Lensing Analysis of A1689 from Deep Advanced Camera Images

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Discovery of diffuse radio emission in the galaxy cluster A1689

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Wide field weak lensing observations of A1689

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Density profiles of galaxy groups and clusters from SDSS galaxy-galaxy weak lensing

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Gravitational lensing

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Combining Strong and Weak Gravitational Lensing in Abell 1689

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THE SERENDIPITOUS OBSERVATION OF A GRAVITATIONALLY LENSED GALAXY ATz= 0.9057 FROM THE BLANCO COSMOLOGY SURVEY: THE ELLIOT ARC

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Resolving the Mass Discrepancy between Strong and Weak Lensing Methods

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A comparison of weak-lensing masses and X-ray properties of galaxy clusters

H. Hoekstra
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ON DARK PEAKS AND MISSING MASS: A WEAK-LENSING MASS RECONSTRUCTION OF THE MERGING CLUSTER SYSTEM A520,

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Effects of asphericity and substructure on the determination of cluster mass with weak gravitational lensing

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A new look at massive clusters: weak lensing constraints on the triaxial dark matter haloes of A1689, A1835 and A2204

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The galaxy cluster concentration–mass scaling relation

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A CFH12k lensing survey of X-ray luminous galaxy clusters

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THE MASS PROFILE OF ABELL 1689 FROM A LENSING ANALYSIS OF DEEP WIDE FIELD SUBARU IMAGES

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Mass and gas profiles in A1689: joint X-ray and lensing analysis

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The observed concentration-mass relation for galaxy clusters

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A CFH12k lensing survey of X-ray luminous galaxy clusters

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The origin of peak-offsets in weak-lensing maps

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Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration

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MEASURING DARK MATTER ELLIPTICITY OF A901/902 USING PARTICLE-BASED LENSING

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Application of anXMM‐NewtonEPIC Monte Carlo Technique to Analysis and Interpretation of Data for the Abell 1689, RX J0658−55, and Centaurus Clusters of Galaxies

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Parametric strong gravitational lensing analysis of Abell 1689

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A HIGH-RESOLUTION MASS MAP OF GALAXY CLUSTER SUBSTRUCTURE: LensPerfect ANALYSIS OF A1689

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INFALL REGIONS AND SCALING RELATIONS OF X-RAY SELECTED GROUPS

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The first detection of weak gravitational shear in infrared observations: Abell 1689

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Complex Structure of Galaxy Cluster A1689: Evidence for a Merger from X‐Ray Data?

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USING WEAK-LENSING DILUTION TO MEASURE LIGHT PROPERTIES OF A1689

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XMM-Newton study of the lensing cluster of galaxies CL 0024+17

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Weak lensing study of dark matter filaments and application to the binary cluster A 222 and A 223

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Spectroscopy of the neighboring massive clusters Abell 222 and Abell 223

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A radial mass profile analysis of the lensing cluster MS 2137.3–2353

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A weak lensing analysis of a STIS dark-lens candidate

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Parameterised models for the lensing cluster Abell 1689

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Wide field weak lensing observations of A1835 and A2204

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Chandra X‐Ray ObservatoryObservation of A1689: New Determination of Mass Distribution and Comparison to Lensing Measurements

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The Sunyaev‐Zeldovich Effect Signature of Excess Entropy in Distant, Massive Clusters

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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

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The ESO Nearby Abell Cluster Survey. XII. The Mass and Mass‐to‐Light Ratio Profiles of Rich Clusters

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New multiply-lensed galaxies identified in ACS/NIC3 observations of Cl0024+1654 using an improved mass model

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Gravitational Lensing: An Astrophysical Tool

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Detailed cluster mass and light profiles of A1703, A370 and RXJ1347−11 from deep Subaru imaging

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The Surprisingly Steep Mass Profile of A1689, from a Lensing Analysis of Subaru Images

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