We present a deep R-, I- and Z-band photometric survey of the open clu
ster Praesepe. 26 new photometric candidates have been fund with I > 1
7.8, extending Praesepe's main sequence down to I 21.5. 19 of the new
members are brown dwarf candidates, and two could be binary brown dwar
fs. Praesepe's mass function is derived, and found to be rising into t
he brown dwarf range with alpha greater than or equal to 1.5.