Galactic versus Extragalactic Pixel Lensing Events toward M31

A new type of gravitational microlensing experiment toward a field where stars are not resolved is being developed observationally and theoretically: pixel lensing. When the experiment is carried out toward the M31 bulge area, events may be produced both by Massive Compact Halo Objects (MACHOs) in our Galactic halo and by lenses in M31. We estimate that $\sim 10-15\mathrm{\%}$ of the total events are caused by Galactic halo MACHOs assuming an all-MACHO halo. If these Galactic events could be identified, they would provide us with an important constraint on the shape of the halo. We test various observables that can be used for the separation of Galactic halo/M31 events. These observables include the Einstein time scale, the effective duration of an event, and the flux at the maximum amplification, but they cannot be used to separate each population events. However, we find that most high maximum-flux Galactic halo events can be isolated through a satellite-based measurement of the flux difference caused by the parallax effect. For the detection of the flux difference, it is required to monitor events with an exposure time of $\sim 20
{\rm min}$ by a 0.5 m telescope mounted on a satellite. Such observations could be carried out as a minor component of a mission aimed primarily at events seen toward the Galactic bulge and Large Magellanic Cloud. In addition, proper motion can be used to isolate Galactic halo/M31 events, but only for $\sim 5\mathrm{\%}$ of high signal-to-noise ratio M31 events and only 1% of Galactic halo events.