R. Ansari et al., OBSERVATIONAL LIMITS ON THE CONTRIBUTION OF SUB-STELLAR AND STELLAR OBJECTS TO THE GALACTIC HALO, Astronomy and astrophysics, 314(1), 1996, pp. 94-103
EROS (Experience de Recherche d'Objets Sombres) has been monitoring th
e luminosity of 4 million stars in the Large Magellanic Cloud in order
to search for gravitational microlensing by unseen objects in the gal
actic halo. We present here the results from 3 years of EROS Schmidt p
lates data. Two stars exhibit light curves that are consistent with a
sizeable microlensing effect. CCD data obtained later on revealed that
one of these stars is an eclipsing binary system. Combining Schmidt p
lates data and the published results from our 16 CCD camera, we set up
per limits on the number of unseen objects in the halo in the mass ran
ge [10(-7), 1]M..