  We present the first catalogue of eclipsing binaries in two MOA fields
towards the Galactic bulge, in which over 8,000 candidates, mostly contact and
semi-detached binaries of periods < 1 d, were identified. In this paper, the
light curves of a small number of interesting candidates including eccentric
binaries, binaries with noteworthy phase modulations and eclipsing RS CVn type
stars are shown as examples. In addition, we identified three triple object
candidates by detecting the light-travel-time effect in their eclipse time
variation curves.
