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19922026
most citedSimulating the joint evolution of quasars, galaxies and their large-scale distribution

5.1k citations · 37.8k across the 291 of their papers we have counts for

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68 papers · 1 filter

astro-ph2008★ 81 cited

The Effect of Gas Physics on the Halo Mass Function

R. Stanek, D. Rudd, A. E. Evrard

Cosmological tests based on cluster counts require accurate calibration of the space density of massive halos, but most calibrations to date have ignored complex gas physics associ…

astro-ph2008★ 1 cited

An Improved Cluster Richness Estimator

Eduardo Rozo, Eli S. Rykoff, Benjamin P. Koester +11

Minimizing the scatter between cluster mass and accessible observables is an important goal for cluster cosmology. In this work, we introduce a new matched filter richness estimato…

astro-ph2008★ 158 cited

Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data

Eduardo Rozo, Eli S. Rykoff, August Evrard +10

We measure the logarithmic scatter in mass at fixed richness for clusters in the maxBCG cluster catalog, an optically selected cluster sample drawn from SDSS imaging data. Our meas…

astro-ph2008★ 105 cited

The L_X--M relation of Clusters of Galaxies

E. S. Rykoff, A. E. Evrard, T. A. McKay +8

We present a new measurement of the scaling relation between X-ray luminosity and total mass for 17,000 galaxy clusters in the maxBCG cluster sample. Stacking sub-samples within fi…

astro-ph2007★ 5 cited

Cross-correlation Weak Lensing of SDSS galaxy Clusters II: Cluster Density Profiles and the Mass--Richness Relation

David E. Johnston, Erin S. Sheldon, Risa H. Wechsler +7

We interpret and model the statistical weak lensing measurements around 130,000 groups and clusters of galaxies in the Sloan Digital Sky Survey presented by Sheldon et al. 2007 (Pa…

astro-ph2007★ 84 cited

Measuring the mean and scatter of the X-ray luminosity -- optical richness relation for maxBCG galaxy clusters

E. S. Rykoff, T. A. McKay, M. R. Becker +6

Determining the scaling relations between galaxy cluster observables requires large samples of uniformly observed clusters. We measure the mean X-ray luminosity--optical richness (…