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Figure 5
(a) MS XANES calculations at the Sm L3-edge versus the oxygen vacancy in different shells. The inset shows both the intensity and linewidth of peak A as a function of oxygen vacancies in the first shell. (b) PDOS of each atomic species of SmOFeAs. (c) PDOS of the Sm-d state versus oxygen vacancy in the first shell. The Fermi level is set to 0 eV.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
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