A.A. Borisov, A.A. Agapov, I.K. Rozgacheva, I.A. Pozdneev, O.A. Shchetinina
The statistical analysis and spherical wavelet transformation of the SDSS DR7-quasars distribution and of the WMAP-CMB anisotropy are performed. The qualitative agreement between the angular power spectrum of CMB and the angular power spectrum of the quasar distribution are revealed. The large quasar groups are discovered and they form the fractal set: the relation between the number of quasar groups and the angular size is characterized by the power-law.