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Near-Infrared Properties of Moderate-Redshift Galaxy Clusters. II. Halo Occupation Number, Mass-to-Light Ratios, and Ωm

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Adam Muzzin1, H. K. C. Yee1, Patrick B. Hall2,4 and H. Lin3,4

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[1]

Lensing Magnification: A Novel Method to Weigh High-redshift Clusters and its Application to SpARCS

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XMM-Newton/Sloan Digital Sky Survey: Star Formation Efficiency in Galaxy Clusters and Constraints on the Matter-density Parameter

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A Multiband Study of the Galaxy Populations of the First Four Sunyaev-Zel'dovich Effect Selected Galaxy Clusters

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[4]

Spectroscopic Confirmation of Three Red-sequence Selected Galaxy Clusters at z = 0.87, 1.16, and 1.21 from the SpARCS Survey

Ricardo Demarco et al.  The Astrophysical Journal 2010  711 1185
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[5]

Mapping The Dark Side with DEIMOS: Globular Clusters, X-Ray Gas, and Dark Matter in the NGC 1407 Group

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Erin S. Sheldon et al.  The Astrophysical Journal 2009  703 2232
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Improvement of the Richness Estimates of maxBCG Clusters

Eduardo Rozo et al.  The Astrophysical Journal 2009  703 601
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[8]

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Spectroscopic Confirmation of a Massive Red-Sequence-Selected Galaxy Cluster at z = 1.34 in the SpARCS-South Cluster Survey

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[10]

Spectroscopic Confirmation of Two Massive Red-Sequence-Selected Galaxy Clusters at z ~ 1.2 in the SpARCS-North Cluster Survey

Adam Muzzin et al.  The Astrophysical Journal 2009  698 1934
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[11]

The Evolution of Dusty Star Formation and Stellar Mass Assembly in Clusters: Results from the IRAC 3.6, 4.5, 5.8, and 8.0 μm Cluster Luminosity Functions

Adam Muzzin et al.  The Astrophysical Journal 2008  686 966
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  1. Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Luminosity Functions and Density Profiles
  2. K-Band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution, and Halo Occupation Number

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