  The notion that the topology of the universe need not be that of the
universal covering space of its geometry has recently received renewed
attention. Generic signatures of cosmological topology have been sought, both
in the distribution of objects in the universe, and especially in the
temperature fluctuations of the cosmic microwave background radiation (CMBR).
One signature identified in the horn topology but hypothesized to be generic is
featureless regions or flat spots in the CMBR sky. We show that typical
observation points within the cusped 3-manifold m003 from the Snappea census
have flat spots with an angular scale of about five degrees for $\Omega_0$=0.3.
We expect that this holds for other small volume cusped manifolds with this
$\Omega_0$ value.
