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The ab initio SCF calculations were performed using the program HONDO [34]. The non-empirical effective core potentials (ECPs) of Hay and Wadt [35] were used to describe the inner shells of Pd and Rh. These ECPs include mass velocity and Darwin relativistic effects [35]. The 5s, 5p and 4d atomic orbitals of Pd and Rh were explicitly treated using (3s3p4d/2s1p2d) basis sets [13,36]. The charges and orbital populations reported in Table 1 were calculated through a Mulliken population analysis [37], and must be considered only in qualitative terms [38]. For each of the listed clusters, we examined the properties of several possible electronic states taking into consideration different orbital occupancies and spin multiplicities. The values in Table 1 correspond to those observed for the ground state of each cluster.
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5/2 XPS spectrum shows two surface peaks that are 1.0 and 1.45eV toward higher binding energy with respect to the surface peak of Pd(100) [25].
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