Cosmic Crystallography with a Pullback
arXiv:astro-ph/9906046 · doi:10.1016/S0375-9601(99)00647-7
Abstract
We present a modified version of the cosmic crystallography method, especially useful for testing closed models of negative spatial curvature. The images of clusters of galaxies in simulated catalogs are ``pulled back'' to the fundamental domain before the set of distances is calculated.
9 pages, 2 figures
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