The addition of hydrogen in the reaction atmosphere is effective in promoting the activity of Ag/alumina and Ag-zeolites on the selective reduction of NO by hydrocarbons (HC-SCR) at low temperatures. The increment of NO conversion over Ag-MFI corresponds to the periodic addition of hydrogen into C 3 H 8 -SCR conditions. The UV-VIS spectra of Ag-MFI have revealed that the addition of hydrogen results in the formation of Ag n d+ clusters due to partial reduction and agglomeration of Ag species . The coincidence of the formation of the Ag n d+ clusters and the increment of NO conversion suggests that Ag n d+ clusters are the highly active species for HC-SCR. From analysis by H 2 -TPR, UV-VIS, and EXAFS, the structure of Ag n d+ clusters on Ag-MFI is identified as being Ag 4 2+ on average. The formation of Ag clusters was strongly affected by the type of zeolites: The major Ag species are Ag + ions for MOR, Ag n d+ clusters for MFI and BEA, and relatively large metallic Ag m particles for Y. The sequence of Ag agglomeration (MOR < MFI < BEA < Y) is in accordance with the strength of the acid sites of zeolites. It can be expected that the interaction between the positive charge of Ag n d+ clusters and acid sites, i.e., the ion-exchange site of zeolites, stabilizes Ag n d+ clusters. The type of Ag species under HC-SCR conditions depends on the concentration of gas-phase oxidants (NO, O 2 ) and reductants (H 2 , HC), and also on the number and strength of the zeolite acid sites.