We present results from a search for gravitational microlensing of sta
rs in the Large Magellanic Cloud by low mass objects in the Galactic H
alo. The search uses the CCD light curves of about 82,000 stars with u
p to 46 measurements per night over a period of 10 months. No light cu
rve exhibits a form that is consistent with a microlensing event of ma
ximum amplification greater than 1.2. This null result makes it unlike
ly that the Halo is dominated by objects in the mass range 5 10(-8)M.
< M < 5 10(-4)M..