  We combine new results from the search for microlensing towards the Large
Magellanic Cloud (LMC) by EROS2 (Experience de Recherche d'Objets Sombres) with
limits previously reported by EROS1 and EROS2 towards both Magellanic Clouds.
The derived upper limit on the abundance of stellar mass MACHOs rules out such
objects as an important component of the Galactic halo if their mass is smaller
than 1 solar mass.
