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WEAK LENSING CALIBRATED M - T SCALING RELATION OF GALAXY GROUPS IN THE COSMOS FIELD
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K ‐band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
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SERENDIPITOUS DISCOVERY OF A MASSIVE cD GALAXY AT z = 1.096: IMPLICATIONS FOR THE EARLY FORMATION AND LATE EVOLUTION OF cD GALAXIES
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JOINT ANALYSIS OF CLUSTER OBSERVATIONS. II. CHANDRA / XMM-NEWTON X-RAY AND WEAK LENSING SCALING RELATIONS FOR A SAMPLE OF 50 RICH CLUSTERS OF GALAXIES
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Growth and Evolution of Thermal Instabilities in Idealized Galaxy Cluster Cores
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Galactic star formation and accretion histories from matching galaxies to dark matter haloes
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Constraints on the Relationship Between Stellar mass and halo mass at low and high Redshift
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Testing X‐Ray Measurements of Galaxy Clusters with Cosmological Simulations
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Galaxy And Mass Assembly (GAMA): testing galaxy formation models through the most massive galaxies in the Universe
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HST /WFC3 CONFIRMATION OF THE INSIDE-OUT GROWTH OF MASSIVE GALAXIES AT 0 < z < 2 AND IDENTIFICATION OF THEIR STAR-FORMING PROGENITORS AT z ∼ 3
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Brightest cluster galaxies in cosmological simulations: achievements and limitations of active galactic nuclei feedback models
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On the Discrepancy Between Theoretical and X-Ray Concentration-Mass Relations for Galaxy Clusters
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CHANDRA STUDIES OF THE X-RAY GAS PROPERTIES OF GALAXY GROUPS
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Publications of the Astronomical Society of the Pacific, Vol. 127, Issue 957
https://doi.org/10.1086/684053
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Intergalactic stars in z 0.25 galaxy clusters: systematic properties from stacking of Sloan Digital Sky Survey imaging data
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