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dc.creatorRozo, Eduardo
dc.creatorRykoff, Eli S.
dc.creatorKoester, Benjamin P.
dc.creatorMcKay, Timothy
dc.creatorHao, Jiangang
dc.creatorEvrard, August
dc.creatorWechsler, Risa H.
dc.creatorHansen, Sarah
dc.creatorSheldon, Erin
dc.creatorJohnston, David
dc.creatorBecker, Matthew
dc.creatorAnnis, James
dc.creatorBleem, Lindsey
dc.creatorScranton, Ryan
dc.date.accessioned2011-02-02T16:21:57Z
dc.date.available2011-02-02T16:21:57Z
dc.date.issued2009-09-20
dc.identifier.citationEduardo Rozo et al, "Improvement of the Richness Estimates of maxBCG Clusters," The Astrophysical Journal 703, no. 1 (2009), doi:10.1088/0004-637X/703/1/601en_US
dc.identifier.issn1538-4357
dc.identifier.urihttp://hdl.handle.net/1811/47803
dc.description.abstractMinimizing 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 estimator, and test its performance using the maxBCG cluster catalog. Our new estimator significantly reduces the variance in the LX -richness relation, from σ _{ln L_X}^2=(0.86± 0.02)^2 to σ _{ln L_X}^2=(0.69± 0.02)^2. Relative to the maxBCG richness estimate, it also removes the strong redshift dependence of the L_X -richness scaling relations, and is significantly more robust to photometric and redshift errors. These improvements are largely due to the better treatment of galaxy color data. We also demonstrate the scatter in the L_X -richness relation depends on the aperture used to estimate cluster richness, and introduce a novel approach for optimizing said aperture which can easily be generalized to other mass tracers.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Astronomical Societyen_US
dc.subjectcosmology: observationsen_US
dc.subjectmethods: data analysisen_US
dc.titleImprovement of the Richness Estimates of maxBCG Clustersen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-637X/703/1/601


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