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Up to now, planet search programs have concentrated on main sequence starslater than spectral type F5. However, identifying planets of early type starswould be interesting. For example, the mass loss of planets orbiting early andlate type stars is different because of the differences of the EUV and X-rayradiation of the host stars. As an initial step, we carried out a program toidentify suitable A-stars in the CoRoT fields using spectra taken with theAAOmega spectrograph. In total we identified 562 A-stars in IRa01, LRa01, andLRa02.

Identifying A-stars in the CoRoT-fields IRa01, LRa01 and LRa02