“…In addition, two more satellite peaks are observed at 861.1 and 879.3 eV . In contrast, both the deconvoluted Ni 2p high-resolution spectra of binary NH/PIn/MAA and ternary NH/PIn/MAA/Ag heterostructures show a positive shifting in the binding energy of about 0.6–0.8 eV (Figure a), suggesting prominent interactions between NH moieties with the other constituents via reduction of outer electron cloud density. − In the deconvoluted O 1s XPS spectrum of Ni(OH) 2 microflowers, three well-defined peaks at 529.0, 529.9, and 531.2 eV are, respectively, attributed to lattice oxygen (M–O–M, where M = Ni), surface hydroxyl group, and adsorbed water (Figure b). ,, For both NH/PIn/MAA and NH/PIn/MAA/Ag, the O 1s spectrum can be deconvoluted to four distinct XPS peaks, where one peak is associated with the lattice oxygen (M–O–M, where M = Ni), one is for the surface hydroxyl group, and the remaining two are designated for the carboxyl oxygens of the MAA moieties (Figure b) . The peaks for NH/PIn/MAA at 284.3, 285.6, and 286.8 eV and for NH/PIn/MAA/Ag at 284.5, 285.9, and 286.8 eV in the deconvoluted XPS spectra of C 1s (Figure S6a) correspond to CC, C–N/C–S, and O–CO bonds, respectively, suggesting the existence of polymer moieties in both the microspheres.…”