  I report on recent results from the POINT-AGAPE pixel-lensing experiment,
which is engaged in a search towards the Andromeda galaxy (M31) for
gravitational microlensing signatures from massive compact halo objects
(Machos). An analysis of two years of data reveals over 360 light-curves
compatible with microlensing. The third year of data, currently being analysed,
will be crucial in determining how many of these candidates are long-period
variables rather than microlensing. Within the dataset we have isolated a
subset of four high signal-to-noise ratio, short duration events which are
compelling microlensing candidates. The properties and possible origins of
these events are discussed.
