Stellar velocity dispersion results, which are calculated from the CaT and CO (2-0) absorption features. Some of sources are not still observed for our entire sample, therefore, the sources for which our sample includes both σ_CaT and σ_CO(2-0) estimates are compared. The red solid line represents 1:1 line, whereas the blue solid line shows the offset between the σ_CaT and σ_CO(2-0) estimates of our data. The LLAMA AGNs and inactive galaxies are presented as black and purple, respectively.