Metals, including Co, Ni, Mn, Fe, Pd, Cr, Zn and Cu, were physically loaded on NDC. The loaded metals were investigated by inductively coupled plasma optical emission spectrometer, and the results were analyzed in Table S1 (Supporting information). All the loaded metals on NDC were detected, and their weight percentage was ~0.5%. The Co, Mn, and Zn loaded NDC were namely Co-NDC, Mn-NDC and Zn-NDC, respectively, and they were selected as typical examples for further investigation using XPS, as shown in
Figs. 1a-
c. There were four peaks observed in the spectrum of the Co 2p orbital (
Fig. 1a). Among them, two peaks at 803.3 and 796.6 eV were attributed to the Co 2p
1/2 satellite and Co 2p
1/2 orbitals, respectively. The other pair at 786.2 and 780.6 eV were assigned to Co 2p
3/2 satellite and Co 2p
3/2 orbitals, respectively. Therefore, Co can be identified as Co(Ⅱ) species [
49,
50]. In the spectrum of the Zn 2p orbital (
Fig. 1b), two distinct peaks were observed at 1044.4 and 1021.7 eV, which were defined as Zn 2p
1/2 and Zn 2p
3/2 orbital, respectively, confirming the presence of the Zn(Ⅱ) species [
51-
54]. Four peaks were assigned from the spectrum of Mn 2p orbitals (
Fig. 1c). Among them, two peaks at 653.5 and 651.9 eV were attributed to the Mn 2p
1/2 satellite and Mn 2p
1/2 orbitals, respectively. The other pair at 645.5 and 641.4 eV were assigned to Mn 2p
3/2 satellite and Mn 2p
3/2 orbitals, respectively. Therefore, Mn can be identified as the mixture of Mn(Ⅱ) and Mn(Ⅲ) species, respectively [
55-
58]. In addition, the C 1s (Fig. S9a in Supporting information) and N 1s (Fig. S9b in Supporting information) spectra were acquired, and the C 1s peaks were presented as similar profile as that without loading any metals. While the N 1s peaks shifted to higher binding energy with respect to that of the pristine NDC. As such, the metal loadings highly affect the nitrogen species [
59]. As a typical example, the Co-NDC was further investigated by transmission electron microscope (TEM). The TEM images, including high-angle annular dark-field (HAADF) images, are presented in Figs. S10a and b (Supporting information), respectively. These images suggest the formation of Co species on the NDC surface resembling a powdery structure. Upon analyzing Fig. S10a, the corresponding particle size analysis of the loaded Co species indicates an average size of approximately 8.46 nm (Fig. S10c in Supporting information). Moreover, high-resolution TEM images in Figs. S10d and e (Supporting information) have shown a lattice spacing of 0.213 nm, corresponding well to the (200) plane of cubic CoO [
60], consistent with the Co 2p XPS results. Furthermore, energy dispersive X-ray spectrometry (EDX) mapping analysis, revealing the homogeneous distribution of Co, C, N, and O elements in
Figs. 1d-
f and Fig. S11 (Supporting information), respectively. This observation further confirmed the uniform anchoring of Co on NDC. In addition, the light absorption of the Co-NDC was investigated by UV–vis DRS, and the absorption spectrum is preserved as the pristine NDC (Fig. S12 in Supporting information), revealing, by such amount loading, metal has minor effect on the light absorption for NDC photocatalysts.