  We present a search for radio transients in the field of the bright radio
source 3C 286 using archival observations from the Very Large Array. These
observations span 23 years and include 1852 epochs at 1.4 GHz in the C and D
configurations. We find no transients in the field. The sensitivity of the
observations is limited by dynamic range effects in the images. At large flux
densities ($> 0.2$ Jy), single epoch observations provide a strong limit on the
transient surface density. At flux densities near the dynamic range threshold,
we use the requirement that transient sources must appear in consecutive epochs
to be confirmed as real. This sets the sensitivity at low flux densities to
transient durations of $\tau \sim 1$ day, while $\tau > 1$ minute for high flux
densities. At 70 mJy, we find a 1-$\sigma$ limit on the surface density $\Sigma
< 3 \times 10^{-3}$ deg$^{-2}$. At 3 Jy, we find a 1-$\sigma$ limit $\Sigma < 9
\times 10^{-4}$ deg$^{-2}$. A future systematic search of the VLA archives can
provide one to two orders of magnitude more sensitivity to radio transients.
