  We report proper motion measurements for 25 very-low mass (VLM) star and
brown dwarf (BD) candidates of the Pleiades cluster previously identified by
Bouvier et al. (1998). Proper motions are measured with an accuracy of 9
mas/yr, compared to an expected tangential motion of about 50 mas/yr for
Pleiades members. Of the 25 candidates, 15 have a membership probability of 95%
or more and 7 are rejected as being field dwarfs. The 3 remaining candidates
exhibit independent evidence for membership (lithium absorption or long-term
proper motion). From the firm identification of Pleiades VLM and BD members,
the cluster's substellar mass function is revised to dN/dM \propto M^{-0.5} in
the mass range from 0.04 to 0.3 M_solar.
