Direct inversion of resonant inelastic x-ray scattering spectra ͑RIXSS͒ has been carried out using a numerical method for solving first-kind Fredholm integral equations. Hereby, the oscillator strength distribution ͑OSD͒, which is proportional to the empty density of states at the absorption edge, has been obtained from the experimental Cu 1s2p RIXSS of CuO. In particular, the inversion of RIXSS measured at incident energies below the K level threshold provides OSD having a better resolution than it can be achieved with one of the customary x-ray absorption near-edge structure spectroscopies. This can be explained by the virtual character of the intermediate states at low energy excitation. By means of the presented method a so-called "hidden electronic excitation" of CuO has been identified as a very weak core excitation. Furthermore, numerical interpretation of polarized spectra has revealed the p y -like character of the excited states in a suitable local reference frame. The obtained results are promising for further applications of the method, preferred in the field of strongly correlated materials. Core excitations into unoccupied levels are sometimes so weak that they apparently do not leave behind visible features in the x-ray absorption near-edge structure ͑XANES͒. However, they can become detectable in the resonant inelastic x-ray scattering spectra ͑RIXSS͒ and in this context the term "hidden electronic excitations" is used.1 The great sensitivity by resonance amplification and the higher energetic resolution as compared with conventional XANES spectroscopies make RIXS spectroscopy a powerful method for investigating unoccupied states in condensed matter, frequently in strongly correlated materials. Among them, divalent CuO with its CuO 4 plaquettes similar to those in the high T c compounds is a good model system toward the understanding of the electronic structure of these materials.Recently, some of the studies on CuO have shown the advantages of RIXS compared to other XANES spectroscopies, but they have also left open questions. In Ref. 2 the existence of a pronounced structure in the Cu 1s2p emission of CuO was discovered for incident energies between 8980 and 8984 eV but without finding a visible counterpart in the corresponding total fluorescence yield ͑TFY͒ XANES. Unfortunately, as the experimental data were obtained from a powder sample, the authors were not able to determine the character and symmetry of the "hidden" excited state. Polarized RIXSS on CuO were measured later by Döring et al. derived oscillator strength distributions ͑OSDs͒ analytically from the experimental 1s2p RIXSS and obtained XANESlike spectra in which the lifetime-broadening ⌫ 1s due to the 1s core hole was suppressed. They compared the spectra with conventional and high-resolution fluorescent excitation ͑HRFE͒ XANES and found that the method revealed weak details in the spectra in the same quality as HRFE. An alternative method to identify even weak spectra structures is based on the interpretation of experimental spec...