Recent results of the OPERA experiment

The OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of ν_τ in an almost pure ν_μ beam (the CERN CNGS beam). In five years of physics run the experiment collected 17.97 × 10¹⁹ p.o.t. The detection of τS produced in ν_τ CC interactions and of their decays is accomplished exploiting the high spatial resolution of nuclear emulsions. Furthermore OPERA has good capabilities in detecting electron neutrino interactions, setting limits on the ν_μ → ν_ℯ oscillation channel. In this talk the status of the analysis will be presented together with updated results on both oscillation channels.