  We present a new sample of 4634 eclipsing binary stars in the Large
Magellanic Cloud (LMC), expanding on a previous sample of 611 objects and a new
sample of 1509 eclipsing binary stars in the Small Magellanic Cloud (SMC), that
were identified in the light curve database of the MACHO project. We perform a
cross correlation with the OGLE-II LMC sample, finding 1236 matches. A cross
correlation with the OGLE-II SMC sample finds 698 matches. We then compare the
LMC subsamples corresponding to center and the periphery of the LMC and find
only minor differences between the two populations. These samples are
sufficiently large and complete that statistical studies of the binary star
populations are possible.
