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Starting with on-shell amplitudes compatible with the scattering of Kerrblack holes, we produce the gravitational waveform and memory effect includingspin at their leading post-Minkowskian orders to all orders in the spins ofboth scattering objects. For the memory effect, we present results atnext-to-leading order as well, finding a closed form for all spin orders whenthe spins are anti-aligned and equal in magnitude. Considering insteadgenerically oriented spins, we produce the next-to-leading-order memory tosixth order in spin. Compton-amplitude contact terms up to sixth order in spinare included throughout our analysis.

Leading-order gravitational radiation to all spin orders