  The French collaboration EROS and the American-Australian collaboration MACHO
have reported the observation of altogether $\sim$ 10 microlensing events by
monitoring during several years the brightness of millions of stars in the
Large Magellanic Cloud. In particular the MACHO team announced the discovery of
8 microlensing candidates by analysing their first 2 years of observations.
This would imply that the halo dark matter fraction in form of MACHOs (Massive
Astrophysical Compact Halo Objects) is of the order of 45-50%. The most
accurate way to get information on the mass of the MACHOs is to use the method
of mass moments. For the microlensing events detected so far by the MACHO
collaboration in the Large Magellanic Cloud the average mass turns out to be
0.27$M_{\odot}$.
