We analyze the collisional Penrose process between a particle on the ISCO orbit around an extreme Kerr black hole and a particle impinging from infinity. We consider both cases with non-spinning and spinning particles. We evaluate the maximal efficiency, $\eta_{}=(\text{extracted energy})/()$, for the elastic collision of two massive particles and for the photoemission process, in which the ISCO particle will escape to infinity after the collision with a massless impinging particle. For non-spinning particles, the maximum efficiency is $\eta_{} \approx 2.562\eta_{} \approx 7$ for the photoemission process. While for spinning particles we obtain the maximal efficiency for the elastic collision and for the photoemission process.

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