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20032025
most citedObservational Probes of Cosmic Acceleration

1.4k citations · 18.4k across the 169 of their papers we have counts for

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12 papers · 1 filter

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★ 6 cited

Biases in the Gravitational Lens Population Induced by Halo and Galaxy Triaxiality

Eduardo Rozo, Jacqueline Chen, Andrew R. Zentner

The lensing cross section of triaxial halos depends on the relative orientation between a halo's principal axes and its line of sight. Consequently, a lensing subsample of randomly…

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★ 2 cited

Optically-Selected Cluster Catalogs as a Precision Cosmology Tool

Eduardo Rozo, Risa H. Wechsler, Benjamin P. Koester +2

We introduce a framework for describing the halo selection function of optical cluster finders. We treat the problem as being separable into a term that describes the intrinsic gal…