“…As shown in Figure C,D, the disappearance of the shake-up Cu 2+ satellite peak located at 937–948 eV and the simultaneous shift of the Cu 2p 3/2 peak toward lower BEs in all of the reduced catalysts indicated the reduction of Cu 2+ to Cu 0 or Cu + . ,,, The Cu LMM XAES spectra were performed to distinguish Cu + and Cu 0 species (Figure S13, SI). For the reduced CZA, the peaks at 918.1 and 916.0 eV were attributed to Cu 0 and Cu + species, respectively. ,,, While for the CZAS@SA catalysts, the peaks for Cu 0 and Cu + species appeared at about 918.5 and 914.3 eV, respectively, in good agreement with our previous study . Interestingly, the Zn 2p 3/2 peak in the reduced CZA catalyst was at about 1022.4 eV, which was much higher than that in calcined CZA (1020.0 eV) (Figure B,D).…”