Notes. Column (1): Name of the galaxy. Note that PGC099188* is actually PGC 047548 (see Section 2.1). Column (2): Number of the Abell cluster. Column (3): 1 – galaxy is a BCG, 2 or higher number – the luminosity rank of the galaxy within its cluster, from the 2nd brightest galaxy to fainter galaxies. Galaxies with number larger than 1 are members of one of the clusters in the SSC (also denoted as non-BCG in the text). Column (4): Distance to the galaxy, as described in Section 2.1. Column (5): Absolute magnitude in K_s band based on the k_m_ext keyword of 2MASS XSC catalogue and the distance from Column (4). Column (6): Richness of the cluster. Column (7): Effective radius in arc seconds, estimated as the mean of j_r_eff, h_r_eff and k_r_eff values from the 2MASS XSC catalog. Column (8): Effective radius in kpc. Column (9): Effective velocity dispersion extracted within the elliptical aperture with semi-major axis equal to R_e. Column (10): λ_Re (uncertainties are less then 0.005). Column (11): Ellipticity of the galaxy within R_e. Column (12): Variation (max-min) of the k₀ coefficient across the FoV. Column (13): Kinematic type based on KINEMETRY analysis, where NRR is ‘non-regular rotator’ and RR is ‘regular rotator’. Column (14): number of the spin reversals visible on the velocity map. “L” indicates the existence of a component rotating around the long-axis. Column (15): Kinematic group (within 1R_e): see Sections 1 and 4.1.2, or (Krajnović et al. 2011). Entries with ^† would be sorted in Group c if the 2R_e region were used for the classification.