  The EROS-2 collaboration has conducted a survey of the Magellanic Clouds
between July 1996 and February 2003 (6.7 years), in order to search for
microlensing phenomena due to putative machos (massive astronomical compact
halo objects). About 55 million stars were monitored over 100 deg^2, typically
with 400 to 500 measurements per star, simultaneously in two wide passbands.
The full EROS-2 Magellanic Cloud data set was processed using the same program
chain, and a photometric database was constructed. The lightcurves of the
brightest 33 million stars were then searched for the characteristic signature
of microlensing phenomena, in the wide timescale range of 1 to 1000 days
(corresponding to macho masses ranging from about 0.01 solar mass to a few
hundred solar masses). The sensitivity of this new analysis is better by a
factor 4. The new EROS-2 microlensing candidates towards the LMC and the
corresponding (preliminary) final limits from EROS-2 on the macho content of
the halo are presented; they are by far not numerous enough to account for the
galactic dark matter. We have also followed, whenever possible, the
microlensing candidates that were previously published by the EROS and MACHO
collaborations. 1 MACHO and 2 EROS LMC candidates have shown subsequent
variability and cannot be considered to be serious candidates.
