  We analyze quasi-2-dimensional slices of the SDSS EDR. Gaussian smoothing
with weighting by the inverse of the selection function provides 2D density
fields across the full survey depth. Superclusters (SC) are characterized by a
percolation algorithm in the large-scale smoothed field. Group candidates are
identified with density maxima in the small-scale smoothed field. The group
mass function depends on the SC environmental density. We derive the
shape-dependent 3-point correlation function and the void size distribution.
These are well reproduced by the galaxies identified in high-resolution
$\Lambda$CDM simulations.
