  We have used the Very Large Array (VLA) to conduct a survey for radio
continuum emission in the sample of 52 Seyfert nuclei selected from the optical
spectroscopic galaxy catalog of Ho, Filippenko, and Sargent. This Seyfert
sample is the most complete and least biased available, and, as such, it will
be useful for a variety of statistical analyses. Here we present the
observations, measurements, and an atlas of radio maps.
  The observations were made at 6 cm in the B-array and at 20 cm in the
A-array, yielding matched angular resolutions of approximately 1". We detected
44 objects (85%) at 6 cm and 37 objects (71%) at 20 cm above a 3-sigma
threshold of 0.12 mJy/beam. The sources have a wide range of radio powers
(10^{18}-10^{25} W/Hz), spectral indices (+0.5 to -1 between 20 and 6 cm), and
linear sizes (from a few tens pc to 15 kpc). The morphology of the radio
emission is predominantly that of a compact core, either unresolved or slightly
resolved, occasionally accompanied by elongated, jet-like features. Linearly
polarized emission was detected at 6 cm in 12 sources, 9 of which were also
detected at 20 cm.
