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Figure 3
Spin-averaged and spin-polarized XAFS spectra of EuS at the Eu LII,III-edges in the ferromagnetic phase. The SP-XAFS spectrum is a direct difference of two consecutive scans recorded with opposite photon helicity. |
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Figure 3
Spin-averaged and spin-polarized XAFS spectra of EuS at the Eu LII,III-edges in the ferromagnetic phase. The SP-XAFS spectrum is a direct difference of two consecutive scans recorded with opposite photon helicity. |