Notes. Column (1): name of the galaxy. Column (2): distances to the galaxies in the sample. The distances found in P13 were taken from Tonry et al. (2001), with corrections by Mei et al. (2007), see P13 for details. Column (3): 1 arcsec expressed in parsecs. Column (4): 1 arcmin expressed in kiloparsecs. Column (5): B-band absolute magnitude (taken from HyperLeda). Column (6): morphological type (taken from P13). Column (7): environment of each galaxy (taken from Arnold et al. (2014); “G” means that the galaxy belongs to a group, “F” is a field galaxy and “C” means that the galaxy belongs to a cluster). Column (8): stellar effective radius (taken from P13, except for the values of NGC 4365 and NGC 4486 that are taken from Kormendy et al. 2009). Column (9): rotational velocity (taken from P13, based on GCs, see their Table 6). Column (10): profile type (“∩” is core, “\” is power law and “?” is unknown due to observational problems, such as obscuration). Column (11): mean isotope shape (“D” indicates disky isophotes, “B” indicates boxy isophotes and “0” indicates pure ellipses). The references for the values found in Cols. (10) and (11) are as follows. (1): Lauer et al. (2007), (2): Spolaor et al. (2008), (3): Lauer et al. (2005), (4): Rest et al. (2001), (5): Emsellem et al. (2007), (6): Nieto et al. (1991), (7): Bender et al. (1989). Column (12): central rotator type (“s” indicates slow and “f” indicates slow rotators); the designations come from Arnold et al. (2014), see their Table 1 and also Emsellem et al. (2007).