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Yen-Ting Lin et al. 2003 ApJ 591 749 doi:10.1086/375513

Near-Infrared Properties of Galaxy Clusters: Luminosity as a Binding Mass Predictor and the State of Cluster Baryons

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Yen-Ting Lin1, Joseph J. Mohr1,2 and S. Adam Stanford3,4

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Abstract References Cited By
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Simulating the Cooling Flow of Cool-core Clusters

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The Integrated Stellar Content of Dark Matter Halos

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Interpolating Masked Weak-lensing Signal with Karhunen-Loève Analysis

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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

A. Zenteno et al.  The Astrophysical Journal 2011  734 3
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Templates for the Sunyaev-Zel'dovich Angular Power Spectrum

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[9]

Impact of Cluster Physics on the Sunyaev-Zel'dovich Power Spectrum

Laurie D. Shaw et al.  The Astrophysical Journal 2010  725 1452
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The Supernova Delay Time Distribution in Galaxy Clusters and Implications for Type-Ia Progenitors and Metal Enrichment

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Dissipational Versus Dissipationless Galaxy Formation and the Dark Matter Content of Galaxies

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[13]

Constraints on the Relationship between Stellar Mass and Halo Mass at Low and High Redshift

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Galaxy Clusters Identified from the SDSS DR6 and Their Properties

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Combining Semianalytic Models with Simulations of Galaxy Clusters: The Need for Heating from Active Galactic Nuclei

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[16]

Cross-correlation Weak Lensing of SDSS Galaxy Clusters. III. Mass-to-Light Ratios

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[17]

Stellar and Total Baryon Mass Fractions in Groups and Clusters Since Redshift 1

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[18]

Improvement of the Richness Estimates of maxBCG Clusters

Eduardo Rozo et al.  The Astrophysical Journal 2009  703 601
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Sharpening the Precision of the Sunyaev-Zel'dovich Power Spectrum

Laurie D. Shaw et al.  The Astrophysical Journal 2009  702 368
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[20]

Exploring the Energetics of Intracluster Gas with a Simple and Accurate Model

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The Influence of Concentration and Dynamical State on Scatter in the Galaxy Cluster Mass-Temperature Relation

Hsiang-Yi Karen Yang et al.  The Astrophysical Journal 2009  699 315
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Detection of Hot Gas in Galaxy Groups Via the Thermal Sunyaev-Zel'Dovich Effect

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Chandra Studies of the X-Ray Gas Properties of Galaxy Groups

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[26]

Starburst Galaxies in Cluster-feeding Filaments Unveiled by Spitzer

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[27]

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[28]

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The Impact of Halo Properties, Energy Feedback, and Projection Effects on the Mass-SZ Flux Relation

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Thermal Balance in the Intracluster Medium: Is AGN Feedback Necessary?

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Evidence for Line-of-Sight Structure in a Comparison of X-Ray and Optical Observations of the High-Redshift Cluster RCS 043938-2904.7

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Galaxy Orbits for Galaxy Clusters in the Sloan Digital Sky Survey and Two Degree Field Galaxy Redshift Survey

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[33]

Why Do Only Some Galaxy Clusters Have Cool Cores?

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A Fitting Formula for the Merger Timescale of Galaxies in Hierarchical Clustering

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Effects of Baryons and Dissipation on the Matter Power Spectrum

Douglas H. Rudd et al.  The Astrophysical Journal 2008  672 19
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[36]

Radio Sources in Galaxy Clusters: Radial Distribution, and 1.4 GHz and K-band Bivariate Luminosity Function

Yen-Ting Lin and Joseph J. Mohr  The Astrophysical Journal Supplement Series 2007  170 71
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[37]

Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium

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[38]

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Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Luminosity Functions and Density Profiles

Adam Muzzin et al.  The Astrophysical Journal 2007  659 1106
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[48]

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