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We propose a stress tensor for the Kerr black hole written in theBoyer-Lindquist coordinate. To achieve this, we use the dictionary of theFlat/CCFT correspondence and take the flat-space limit from the quasi-localstress tensor of the four-dimensional Kerr-AdS black hole. The proposed stresstensor yields the correct values for the mass and angular momentum of the Kerrblack hole at spatial infinity. We also calculate some components of the energymomentum tensor of the three dimensional CCFT and show that they are consistentwith the holographic calculation of the Kerr black hole. The calculation wepresent in this paper is another confirmation for the Flat/CCFT proposal.

Flat-Space Holography and Stress Tensor of Kerr Black Hole