  We have studied the photometric variability of ten SMC Be/X-ray pulsars using
MACHO and OGLE-II data. For some of these systems we have found periodic
behavior, including orbital outbursts and/or nonradial pulsations (NRP) of the
Be star. For others we were unable to identify any clear photometric
periodicity, although their longterm light curves show significant structure.
We present periodograms, phase dispersion minimization (PDM) variances, and
folded light curves for the systems which exhibit periodic photometric
variability.
