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Dynamical Masses of RCS Galaxy Clusters

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arxiv astro-ph/0404314 v1 pith:RCDYSCUS submitted 2004-04-15 astro-ph

K. Blindert , H. K. C. Yee , E. Ellingson , M. D. Gladders This is my paper · ORCID
classification astro-ph
keywords clusterssurveyclustergalaxymasschosencompletedcorrelation
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A multi-object spectroscopy follow-up survey of galaxy clusters selected from the Red-sequence Cluster Survey (RCS) is being completed. About forty clusters were chosen with redshifts from 0.15 to 0.6, and in a wide range of richnesses. One of the main science drivers of this survey is a study of internal dynamics of clusters. We present some preliminary results for a subset of the clusters, including the correlation of optical richness with mass, and the mass-to-light ratio as a function of cluster mass.

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