  We study the angular correlations of various galaxy catalogs (CfA1, SSRS1,
Perseus-Pisces, APM Bright Galaxies and Zwicky). We find that the angular
correlation exponent is $\gamma_a= 0.1 \pm 0.1$ rather than $\gamma_a=0.7$ as
usually found by the standard correlation function $\omega(\theta)$. We
identify the problem in the artificial decay of $\omega(\theta)$. Moreover we
find that no characteristic angular scale is present in any of the analyzed
catalogs. Finally we show that all the available data are consistent with each
other and the angular distribution of galaxies is quite naturally compatible
with a fractal structure with $D \approx 2$.
