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19992009
most citedCross-correlation Weak Lensing of SDSS galaxy Clusters II: Cluster Density Profiles and the Mass--Richness Relation

5 citations · 10 across the 5 of their papers we have counts for

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astro-ph20081 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-ph20075 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-ph20072 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…

astro-ph20072 cited

Cosmological Constraints from SDSS maxBCG Cluster Abundances

Eduardo Rozo, Risa H. Wechsler, Benjamin P. Koester +6

We perform a maximum likelihood analysis of the cluster abundance measured in the SDSS using the maxBCG cluster finding algorithm. Our analysis is aimed at constraining the power s…

astro-ph2002

Discovery of the CV ROTSE3 J015118.59-022300.1

D. A. Smith, C. Akerlof, M. C. B. Ashley +11

We report on the discovery of an outburst from a previously unknown high- latitude CV we designate ROTSE3 J015118.59-022300.1. The object was first detected on 2001 Oct 13.291 at m…

astro-ph2001

Early-type galaxies in the SDSS

M. Bernardi, R. K. Sheth, J. Annis +28

A sample of nearly 9000 early-type galaxies, in the redshift range 0.01<z<0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. The sample…