New limits from microlensing on Galactic Black Holes in the mass range $10M_{\odot }<M<1000M_{\odot }$

We have searched for long duration microlensing events originating from intermediate mass Black Holes (BH) in the halo of the Milky Way, using archival data from EROS-2 and MACHO photometric surveys towards the Large Magellanic Cloud. We combined data from these two surveys to create a common database of light curves for 14.1 million objects in LMC, covering a total duration of 10.6 years, with flux series measured through four wide passbands. We have carried out a microlensing search on these light curves, complemented by the light curves of 22.7 million objects, observed by EROS-2 only or MACHO only over about 7 years, with flux series measured through only two passbands. A likelihood analysis, taking into account LMC self lensing and Milky Way disk contributions allows us to conclude that compact objects with masses in the range $10-100M_{\odot }$ cannot make up more than $\sim 15\mathrm{\%}$ of a standard halo total mass (at $95\mathrm{\%}$ confidence level). Our analysis sensitivity weakens for heavier objects, although we still exclude that $\sim 50\mathrm{\%}$ of the halo be made of $\sim 1000M_{\odot }$ BHs. Combined with previous EROS results, an upper limit of $\sim 15\mathrm{\%}$ of the total halo mass can be obtained for the contribution of compact halo objects in the mass range $10^{-6} - 10^2 M_{\odot}$.