Nearest neighbor vector analysis of sdss dr5 galaxy distribution
  We present the Nearest Neighbor Distance (NND) analysis of SDSS DR5 galaxies.
We give NND results for observed, mock and random sample, and discuss the
differences. We find that the observed sample gives us a significantly stronger
aggregation characteristic than the random samples. Moreover, we investigate
the direction of NND and find that the direction has close relation with the
size of the NND for the observed sample.
