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Caustic and Weak-Lensing Estimators of Galaxy Cluster Masses

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Published 2005 July 19 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Antonaldo Diaferio et al 2005 ApJ 628 L97 DOI 10.1086/432880

1538-4357/628/2/L97

Abstract

There are only two methods for estimating the mass distribution in the outer regions of galaxy clusters, where virial equilibrium does not hold: weak gravitational lensing and identification of caustics in redshift space. For the first time, we apply both methods to three clusters: Abell 2390, MS 1358.4+6245, and Cl 0024+1654. The two measures are in remarkably good agreement out to ~2 h-1 Mpc from the cluster centers. This result demonstrates that the caustic technique is a valuable complement to weak lensing. With a few tens of redshifts per square comoving megaparsec within the cluster, the caustic method is applicable for any z ≲ 0.5.

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10.1086/432880