  We present the results of VLA A-array 8.46 GHz continuum imaging of 55
Seyfert galaxies (19 Seyfert 1's and 36 Seyfert 2's). These galaxies are part
of a larger sample of 88 Seyfert galaxies, selected from mostly isotropic
properties, the flux at 60 mum and warm infrared 25 mum to 60 mum colors. These
images are used to study the structure of the radio continuum emission of these
galaxies and their position angles, in the case of extended sources. These
data, combined with information from broad-band B and I observations, have been
used to study the orientation of radio jets relative to the plane of their host
galaxies (Kinney et al. 2000).
