We present the results of a six-square-degree Pleiades survey in I and Z, w
hich is photometrically complete to approximately I-KP = 19.2 (I-Cou = 19.6
in the Pleiades). We remove non-cluster contamination on the basis of prop
er motions and infrared photometry, and present 339 candidate cluster membe
rs, 30 of which are fainter than I-KP = 17.5, and are thus strong brown-dwa
rf candidates.