We present the statistical properties of large scale galaxy distributi
on in the LEDA redshift database. This catalog contains more than 40,0
00 redshifts over all the sky We find that LEDA, although seriously af
fected by incompleteness, shows quite stable statistical properties. I
n particular, we have considered the behavior of the two points correl
ation function and of the power spectrum of the density fluctuations,
and we have done several tests to check whether the incompleteness of
the catalog affect these statistical quantities. Our conclusion is tha
t galaxy distribution in this catalog has fractal properties up to the
distance similar to 200h(-1)Mpc with D = 2.1+/-0.2, with no sign towa
rds homogeneity: this result is statistically stable. Finally, we comp
are these results with those obtained in other redshift surveys, findi
ng that this sample well reproduces the properties of galaxy distribut
ion found in the different catalogs.