Metal ion-linked, self-assembled multilayers on nanocrystalline metal oxide surfaces have recently emerged as an effective strategy for manipulating energy and electron transfer dynamics at organic−inorganic interfaces. The choice of metal ion can have a large impact on the stability, loading concentration, and other properties of the films. Here we report our investigation into the role of the linking ion on the subnanosecond excited state dynamics in the bilayer films (TiO 2 −B−M−RuP). While metal linkers like Cd II , La III , Sn IV , Zn II , and Zr IV are photochemically inert, paramagnetic linking ions such as Cu II , Fe II , and Mn II quench the excited state of the dye with a rate constant on the order of 10 8 s −1 . The absence of new spectral features in the transient absorption spectrum suggests that energy transfer, and not electron transfer, is responsible for the excited state quenching. On TiO 2 , the electron injection rate for TiO 2 −B−M−RuP is an order of magnitude slower (∼1 × 10 9 s −1 ) than for the dye directly on TiO 2 (∼3 × 10 10 s −1 ) due to increased spatial separation and reduced electronic coupling between the dye and the surface. In dye-sensitized solar cells, the TiO 2 −B−M−RuP devices exhibit a notably lower J sc but higher V oc compared to TiO 2 −RuP with even lower photocurrents for Cu II , Fe II , and Mn II bilayers presumably at least in part due to competitive quenching of the excited state by the metal ion. The increases in V oc are offset by the decrease in J sc ; thus, the overall efficiency of the bilayer devices is lower than the that of the parent, monolayer device.