Large Scale Distribution of Galaxies in The Field HS 47.5-22. II.
  Observational Data Analysis
  The results of the study of the large-scale distribution of galaxies up to z
~0.8 in the field HS 47.5-22 on the basis of photometric data of the 1-meter
Schmidt telescope of the BAO NAS Armenia are presented. The full sample
contains 28,398 galaxies. Candidates for large-scale structures were determined
using two independent methods for reconstructing density contrast maps in 57
narrow slices of the three-dimensional distribution of galaxies: adaptive
aperture algorithm with smoothing and 2D Voronoi tessellation. We have
identified more than 250 statistically significant overdense structures. The
obtained results demonstrate a wide range of overdense structures over the full
range of redshifts up to z ~0.8.
