A summary of all corrector magnet settings used during the SBS GMn run from September 2021 to February 2022. The corrector magnet settings were determined using a TOSCA/OPERA simulation of the SBS magnet for each kinematic configuration, and minimizing both the electron particle trajectories along the beam line and the magnetic field integral from the target pivot towards the beam dump. The calculations are performed for z = 5 m upstream of the target pivot to z = 12 m downstream of the target pivot.