distribution of stellar orbits, in particular to constrain the amount of stars on radially extended orbits. One galaxy (NGC5516) out of the original 10-galaxy sample is omitted here since its kinematical data reach only out to $r_\mathrm{max} \lesssim 12 \, {r_b}$ and the orbital structure in the core is less constrained than in the other galaxies ($r_\mathrm{max} > 20 \, {r_b}$). To this sample of nine galaxies we add two additional high-$\sigma$ galaxies that we also observed with SINFONI: NGC307 and NGC1332. The data for NGC1332 were already published in @Rusli11; the new data for NGC307 are described in Erwin et al. (in preparation). Both new galaxies have been analyzed following the same data reduction/modeling scheme as described in @Rusli13a. To constrain the spatial distribution of the stars we use a combination of [[*HST*]{}]{} images, ground-based images, and our SINFONI data [@Rusli13a].

Six out of the 11 galaxies are core galaxies, while five do not have a detectable core at the limit of [[*HST*]{}]{} resolution [@Rusli13b]. Cores in the observed galaxies were identified and measured using core-S[é]{}rsic model [@Graham03; @Trujillo04] fits to surface brightness profiles that extend out to large radii, typically more than twice the half-light radius of the 