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 ${\nu }_{\tau }$ in an almost pure ${\nu }_{\mu }$ beam (the CERN CNGS beam). In five years of physics run the experiment collected $17.97\times {10}^{19}$ p.o.t. The detection of $\tau$s produced in ${\nu }_{\tau }$ 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 ${\nu }_{\mu }\to {\nu }_e$ oscillation channel. In this talk the status of the analysis will be presented together with updated results on both oscillation channels.