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A first result of the search for \numu $\rightarrow$ \nue oscillations in theOPERA experiment, located at the Gran Sasso Underground Laboratory, ispresented. The experiment looked for the appearance of \nue in the CNGSneutrino beam using the data collected in 2008 and 2009. Data are compatiblewith the non-oscillation hypothesis in the three-flavour mixing model. Afurther analysis of the same data constrains the non-standard oscillationparameters $\theta_{new}$ and $\Delta m^2_{new}$ suggested by the LSND andMiniBooNE experiments. For large $\Delta m^{2}_{new}$ values ($>$0.1 eV$^{2}$),the OPERA 90% C.L. upper limit on sin$^{2}(2\theta_{new})$ based on a Bayesianstatistical method reaches the value $7.2 \times 10^{-3}$.

Search for $\nu_\mu \rightarrow \nu_e$ oscillations with the OPERA experiment in the CNGS beam