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We compute greybody factors for near extreme Kerr black holes in D=4 and D=5.In D=4 we include four charges so that our solutions can be continuouslydeformed to the BPS limit. In D=5 we include two independent angular momenta soLeft-Right symmetry is incorporated. We discuss the CFT interpretation of ouremission amplitudes, including the overall frequency dependence and thedependence on all black hole parameters. We find that all additional parameterscan be incorporated Kerr/CFT, with central charge independent of U(1) charges.

Greybody Factors and Charges in Kerr/CFT