“…34-0394), while the peaks for Co . 20 In the O 1s spectrum (Figure 5f), the peaks at 529.4, 530, 531.6, and 532.6 eV, are attributed to Ce−O, Co−O, oxygen defects, and absorbed O, respectively. 37,38 After the OER, the peak of the oxygen vacancy is much stronger than the other peaks, and the peak of the Co−O bond is also significantly enhanced, even stronger than that of the Ce−O bond, which further confirms the formation of CoOOH.…”