American Astronomical Society, Astrophysical Journal, 2(776), p. 91, 2013
DOI: 10.1088/0004-637x/776/2/91
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We provide a new observational test for a key prediction of the ΛCDM cosmological model: the contributions of mergers with different halo-to-main-cluster mass ratios to cluster-sized halo growth. We perform this test by dynamically analyzing 7 galaxy clusters, spanning the redshift range 0.13