Saved in:
| Main Authors: | , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2506.05847 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Table of Contents:
- A statistical analysis of anisotropic quasiperiodic features of the spatial distribution of galaxy clusters obtained on the basis of spectroscopic and photometric redshifts in the interval $0.1 \leq z \leq 0.47$ has been carried out. Based on data from the SDSS~III catalog, we show that the preferential direction previously detected in the northern hemisphere (a narrow cone of directions: $α_0=170^\circ \pm 5^\circ, \ δ_0= 29^\circ \pm 5^\circ$), along which the one-dimensional distribution of projections of the Cartesian coordinates of clusters contains a significant ($\gtrsim (4 - 5) σ$) quasi-periodic component, can also be found using photometric redshifts, achieving a certain accuracy ($Δz \lesssim 0.013$). Based on data from the photometric DES$\times$unWISE catalog, we have analyzed the spatial distribution of clusters in the southern hemisphere, where a cone of close directions was also detected ($α_0=346^\circ \pm 5^\circ,\ δ_0= - 29^\circ \pm 5^\circ $), which are approximately an extention of the directions revealed in the northern hemisphere. The power spectra of one-dimensional distributions along these directions contain significant ($\gtrsim (4 - 5) σ$) features in the same interval of wave numbers $0.04 \lesssim k \lesssim 0.06~h$~Mpc$^{-1}$.