  We report R- and V-band photometry derived from CCD imaging for objects in
nine fields in and around the Draco dwarf spheroidal galaxy. The most distant
fields are about 1.3 degrees from the center. We use these data to search for
Draco stars outside of its measured tidal boundary. The search involves three
methods: 1) Plotting color-magnitude diagrams for individual fields, for
sections of fields, and for combined fields and sections. A color-magnitude
diagram can reveal a population of Draco stars by the presence of the expected
principal sequences. 2) Measuring field-to-field fluctuations and 3) measuring
intra-field fluctuations in the surface density of objects located near the
Draco principal sequences in the color-magnitude diagram. We find evidence for
the presence of Draco stars immediately beyond the measured tidal boundary of
Draco and place an upper limit on the number of such stars in more distant
fields that lie close to the extension of its major axis. The best evidence is
the presence of the Draco principal sequences in the color-magnitude diagram
for some combined fields and sections of fields. The measurements of the
field-to-field fluctuations in the stellar surface density confirm this result.
