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In the sixth of the series of papers reporting on a large reverberationmapping (RM) campaign of active galactic nuclei (AGNs) with high accretionrates, we present velocity-resolved time lags of H$\beta$ emission lines fornine objects observed in the campaign during 2012$-$2013. In order to correctthe line-broadening caused by seeing and instruments before the analysis ofvelocity-resolved RM, we adopt Richardson-Lucy deconvolution to reconstructtheir H$\beta$ profiles. The validity and effectiveness of the deconvolutionare checked out by Monte Carlo simulation. Five among the nine objects showclear dependence of time delay on velocity. Mrk 335 and Mrk 486 show signaturesof gas inflow whereas the clouds in the broad-line regions (BLRs) of Mrk 142and MCG +06-26-012 tend to be radial outflowing. Mrk 1044 is consistent withthe case of virialized motions. The lags of the rest four are notvelocity-resolvable. The velocity-resolved RM of super-Eddington accretingmassive black holes (SEAMBHs) shows that they have diversity of the kinematicsin their BLRs. Comparing with the AGNs with sub-Eddington accretion rates, wedo not find significant differences in the BLR kinematics of SEAMBHs.

Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. VI. Velocity-resolved Reverberation Mapping of H$\beta$ Line