  Motivated by a desire to understand the size distributon of the Kuiper Belt,
an observing program was conducted at the Mount Palomar 5-m telescope from
1994-1996. The observations consisted of follow-up observations of known
objects (in order to improve their very indeterminate orbits), and deep
exposures on a single field to search for small objects below the limiting
magnitudes of other surveys. Eighteen object recoveries were successfully
obtained over the course of the follow-up program. Data reduction of the deep
fields consisted of a software recombination of many fields shifted at
different angular rates in order to detect objects at differing heliocentric
distances. We set an upper limit of <1 object per 0.05 square degrees in the
ecliptic brighter than magnitude R ~ 25. The lack of detected objects in this
work serves to help constrain the number density of Kuiper Belt comets.
