“…In our work, we will address this emerging O-K edge prepeak as hole peak (HP). Chemical doping, such as Sr doping in LCO, shifts spectral weight from the upper Hubbard band (UHB) to the HP, thereby introducing holes into the system. − Polarization-dependent XAS provides information on orbital occupation through high energy resolution, ,, but with limited spatial resolution, which is inevitable for characterizing innovative applications like Josephson junctions . EELS bridges this gap, offering atomic-scale characterization of orbital occupation, and the ability to quantify cations and anions, and their physical properties as a function of position by probing different phases.…”