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   <subfield code="a">The statistical properties of elements of the large-scale structure of the Universe are studied using the SDSS DR7 galaxy catalog and a dark-matter halo catalog obtained via numerical modeling using MultiDark Run1. The minimum spanning tree technique is used to distinguish the large-scale structure, and the Core Sampling method is used to analyze its properties. As a result, the SDSS DR7 and MultiDark Run1 catalogs are divided into subcatalogs of two-dimensonal walls and one-dimensional filaments. Some statistical properties of these subcatalogs are compared with theoretical predictions. The mean separation between the walls is measured using both the observations and numerical modeling results (50-60 Mpc/h) and the distribution of the wall surface density is derived. The fraction of the SDSS DR7 galaxy clusters thought to have been distorted by the observational effect called &quot;fingers of God” is estimated. Dense clusters for which this effect is most appreciable constitute ∼15% of the analyzed clusters. The influence of these clusters on the final result is eliminated by fitting the orientation of test cylinders in the Core Sampling method.</subfield>
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