Constraints on the alignment of galaxies in galaxy clusters from ~14 000 spectroscopic members

Cristóbal Sifón; Henk Hoekstra; Marcello Cacciato; Massimo Viola; Fabian Köhlinger; Remco F. J. van der Burg; David J. Sand; Melissa L. Graham

doi:10.1051/0004-6361/201424435

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Volume 575 (March 2015)

A&A, 575 (2015) A48

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Fig. 1

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Left: redshift distributions of all MENeaCS+CCCP clusters (blue histogram) and clusters used in this study (gray filled histogram). Right: distributions of number of spectroscopic members, N_m (gray filled histogram), and number of spectroscopic members within r₂₀₀, N₂₀₀ (blue histogram). Abell 2142, with N_m = 1052 and N₂₀₀ = 731, is not shown.

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