We present the results of a six-square-degree Pleiades survey in I and Z, which is photometrically complete to approximately I_KP_=19.2mag (I_C_=19.6 in the Pleiades). We remove non-cluster contamination on the basis of proper motions and infrared photometry, and present 339 candidate cluster members, 30 of which are fainter than I_KP_=17.5, and are thus strong brown-dwarf candidates.
Cone search capability for table J/MNRAS/313/347/tablea2 (Burrell Pleiades (BPl) candidates.)
Cone search capability for table J/MNRAS/313/347/tablea5 (BPl brown dwarf candidates)