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We investigate the stellar kinematics of the bulge and disk components in 826 SAMI galaxies. The spatially resolved rotation velocity (V) and velocity dispersion (σ) of bulge and disk components have been simultaneously) of bulge and disk components have been simultaneously estimated using the penalized pixel fitting (PPXF) method with photometrically defined weights for the two components. The spin parameter λR indicates bulges are pressure-dominated systems and disks are supported bydoi:10.5281/zenodo.4721542 fatcat:nkxevedwefecvhywlgn23ga7ce