  We investigate the behaviour of galaxy clustering on large scales using the
PSCz catalogue. In particular, we ask whether there is any evidence of
large-scale fractal behaviour in this catalogue. We find the correlation
dimension in this survey varies with scale, consistent with other analyses. For
example, our results on small and intermediate scales are consistent those
obtained from the QDOT sample, but the larger PSCz sample allows us to extend
the analysis out to much larger scales. We find firm evidence that the sample
becomes homogeneous at large scales; the correlation dimension of the sample is
D_2=2.992(3) for r>30 h^{-1} Mpc. This provides strong evidence in favour of a
Universe which obeys the Cosmological Principle.
