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We report on observations of the nova-like cataclysmic variable AE Aqrperformed by MAGIC. The observations were part of a quasi-simultaneousmulti-wavelength campaign carried out between 2012 May and June covering theoptical, UV, X-ray and gamma-ray ranges. MAGIC conducted the campaign andobserved the source during 12 hours. The other instruments involved were KVA,Skinakas, and Vidojevica in the optic and Swift in the X-ray. We also usedoptical data from the AAVSO. The goals were to: monitor the variability of thesource at different wavelengths, perform gamma-ray studies coincident with thehighest states of the source at the other wavelengths, and confirm or rule outprevious claims of detection of very-high-energy emission from this object. Wereport on a search for steady TeV emission during the whole observation, forvariable TeV emission coincident with the highest optical and X-ray states andperiodic TeV emission at the 33.08 s rotation period (30.23 mHz rotationfrequency) of the white dwarf and its first harmonic (60.46 mHz rotationfrequency). These are the first observations under good weather conditionsperformed by the present generation of IACTs for this object.

Search for TeV $\gamma$-ray emission from AE Aqr coincident with high optical and X-ray states with the MAGIC telescopes