论文标题
HS 47.5-22中星系的大规模分布。 ii。观察数据分析
Large Scale Distribution of Galaxies in The Field HS 47.5-22. II. Observational Data Analysis
论文作者
论文摘要
根据1米的Schmidt望远镜的光度数据，在Bao Nas Armenia的1米Schmidt望远镜的光度数据基础上，在田间HS 47.5-22中高达Z〜0.8的大型星系的研究结果。完整的样本包含28,398个星系。使用两种独立的方法确定了大规模结构的候选物，用于重建星系三维分布的57个狭窄切片中的密度对比度图：具有平滑性和2D Voronoi Tessellation的自适应孔径算法。我们已经确定了250多个具有统计学意义的过重结构。获得的结果表明，在Z〜0.8的整个红移范围内，各种过度密度结构。
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.
