  We summarise results for the predicted density and peculiar velocity fields
from the PSCz survey. We have used a generalisation of the Path Interchange
Zeldovich Approximation to determine the velocity field; the most remarkable
feature being a coherent large-scale flow along the baseline connecting the
Local Supercluster, Centaurus and the Shapley Concentration. Comparison of the
predicted and observed bulk flows gives a value of beta = 0.50+-0.1.
  We re-examine the PSCz dipole, with improved redshift completeness at
low-latitudes and using PIZA to estimate real-space distances. We find the
dipole to be stable between 80 and 180 hMpc, although there appears to be a
significant contribution to the dipole around 200 hMpc. The overall
misalignment with the CMB dipole remains at 20degrees. The implied value of
beta is in the range 0.40-0.55 with statistical error +-0.1. We also present
the density field and a preliminary dipole analysis from the almost completed
Behind The Plane survey, which extends the PSCz to cover 93% of the sky
including the proposed core of the Great Attractor. We find a density peak at
(325,-5,3500km/s), about half as massive as Centaurus or Pavo-Indus, and
forming part of a continuous filament linking them across the Plane. We also
find evidence for a much larger `Greater Attractor' directly behind the GA, at
a distance of 125 hMpc, and more massive than the Shapley concentration.
  At large distances the dipole direction is in much improved agreement with
the CMB: at 250-300hMpc, the misalignment is only 5-10 degrees, though this
depends on the incompleteness corrections made. The dipole amplitude implies a
value for the parameter beta of 0.44+-0.1.
