We present 1.4 GHz VLA observations of the variability of radio sources in
the Lockman Hole region at the level of > 100 uJy on timescales of 17 months
and 19 days. These data indicate that the areal density of highly variable
sources at this level is < 0.005 arcmin^{-2}. We set an upper limit of 2% to
the fraction of 50 to 100uJy sources that are highly variable (> 50%). These
results imply a lower limit to the beaming angle for GRBs of 1deg, and give a
lower limit of 200 arcmin^2 to the area that can be safely searched for GRB
radio afterglows before confusion might become an issue.Comment: aastex 2 postscript figures. to appear in the Astrophysical Journa