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Each peak was deconvoluted with a single Gaussian distribution. When we used the Voigt profile, the peak position and the trend of the linewidth changes were the same. The energy separation of the spin-orbit split in the Ge 3 d5/2-3/2, Sb 4 d5/2-3/2, Te 4 d5/2-3/2, and In 4 d5/2-3/2 orbitals was 0.6, 1.25, 1.5, and 0.65 eV, respectively.
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