“…In comparison of these two spectra, however, the data of Cu-IO@SiO 2 NPs exhibit more narrowed linewidth than that of IO@SiO 2 NPs, also giving us a greater satellite peak of Fe 2p 3/2 located at 718.5 eV, indicative of the presence of Fe 3+ . Two separated peaks at 709.5 eV and 711.2 eV in Fe 2p 3/2 may be attributed to Fe 3+ from Fe 3 O 4 phase and Fe 2 O 3 phase [20,21] as in FTIR spectra. Cu 2p, O 1s, and survey spectra can be found in Figure S1 in the Supplementary Materials.…”