Left: map of Brγ flux (units given in 10^-16 W m^-2 μm). Right: map of W_Brγ (units given in Å). White contours tracing the K-band stellar continuum, and black circles denoting the black hole locations are overdrawn on both maps. Although the most intense Brγ emission is on the nuclei, the equivalent width here is lowest, suggesting that the K-band light is dominated by an older stellar population. We note that in Sect. 4 we showed that dilution by hot dust emission associated with the AGN cannot play a role in reducing W_Brγ.