“…As shown in the Co 2p core‐level spectra (Figure 2a), four typical peaks, 781.6 eV (2p 3/2 ), 786.5 eV (2p 3/2 , satellite), 797.2 eV (2p 1/2 ), and 803.3 eV (2p 1/2 , satellite) present in the Co‐La 50% (w/o H 2 O 2 ), which are assigned to the Co 2+ species [9] . When H 2 O 2 was added (i.e., the Co‐La 50% HTL), the Co 2p core‐level spectra exhibited not only Co 2+ species but also Co 3+ species, which demonstrates the partial oxidation of the Co 2+ species by H 2 O 2 [13a, 17c] . As with the La 3d core‐level spectra (Figure 2b), four typical peaks, 836.0 eV (3d 5/2 ), 839.4 eV (3d 5/2 , satellite), 852.8 eV (3d 3/2 ), and 856.2 eV 3d 3/2 , satellite), ascribed to La 3+ species are observed in the Co‐La 50% (w/o H 2 O 2 ) and there is no significant difference between the spectra of Co‐La 50% (w/o H 2 O 2 ) and Co‐La 50% HTL, revealing that the addition of H 2 O 2 has little effect on the La 3+ precursor [13a, 17c] .…”