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c Ce 3d core level, and d O 2p core level for the CeO2 sample after UV irradiation.
Open image in new window Fig. 3 a Ce 3d core level, and b O 2p core level for the CeO2 sample before UV irradiation.
The quantitative Ag/C atomic ratios of the samples were determined using the peak area ratio of the corresponding XPS core levels and the sensitivity factor (SF) of each element in XPS. Figure 4 shows high-resolution XPS spectra of the C(1 s) core level for the AgNPs.
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The peak height ratios of the Ta 4f7/2, Ta 4f5/2, and Ta2O5 4f5/2 core levels for the w/o Ti samples with respect to the Ta2O5 4f7/2 peak height were 0.03, 0.03, and 0.77, respectively, while those for the w/ Ti samples were 0.27, 0.16, and 0.77, respectively.
The binding energy of the Ag 3d5/ 2) core level for Ag, Ag2O, and AgO is 368.5, 368.3, and 367.7 eV, respectively.
The XP spectra of Ru 3d core level for various samples are presented in Fig. 4.
The XP spectra of Ce 3d core level for various samples are presented in Figure S2 (Supporting Information).
Experimental and fitted XPS spectra of Ni 2p (d), Fe 2p (e), and Co 2p (f) core level for Ti0.97TM0.03O2 films.
Fig. 2 (Color online) XPS analysis of O 1s core level for Hf-Ti-O/IL/Si stack.
High-resolution XPS spectra of Ni 2p (a), Fe 2p (b), and Co 2p (c) core level for TM-doped TiO2 films.
The binding energies of the core-level spectra were determined with respect to the binding energy (E B = 84.0 eV) of the clean Au 4f core-level for the same photon energy.
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