  We present the analysis of the first two years of a search for microlensing
of stars in the Small Magellanic Cloud with the EROS (Exp\'erience de Recherche
d'Objets Sombres) project. A single event is detected, already present in the
first year analysis. This low event rate allows us to put new constraints on
the fraction of the Galactic Halo mass due to compact objects in the mass range
[10^-2, 1] Msol. These limits, along with the fact that the two SMC events
observed so far are probably due to SMC deflectors, suggest that LMC and SMC
self-lensing may dominate the event rate.
