  Galaxy peculiar velocity data provide important dynamical clues to the
structures obscured by the Zone of Avoidance (hereafter, ZOA) with resolution
>~ 500km/s. This indirect probe complements the very challenging approach of
directly mapping of the distribution of galaxies behind the Milky Way. In this
work, the Wiener filter method is applied to reconstruct the 3D density and
velocity distributions of the universe, within ~8000km/s, using SEcat the
largest peculiar velocity catalog yet. This catalog is a combination of the SFI
spiral galaxy peculiar velocity catalog and the newly completed nearby
early-type galaxy peculiar velocity catalog, ENEAR. The recovered density is
smoothed with 900km/s Gaussian. The main reconstructed structures are
consistent with those extracted from the IRAS 1.2-Jy redshift galaxy catalogs.
The revealed structures are identified and their robustness and significance
are discussed.
