Posterior probability distribution of the parameters σ_sph (the velocity dispersion of the bulge of NGC 3384), σ_r, and v_rot (the radial velocity dispersion and circular velocity of the disk of NGC 3384), and σ_{M 105, Ser} and σ_{M 105, Exp} (the velocity dispersions of the Sérsic and exponential populations in M 105) in the innermost of the five elliptical bins. To illustrate the Gaussian priors on the LOSVD parameters of NGC 3384, which cover a larger range in parameter space, we inserted three additional subplots showing the priors with red solid lines and the posteriors with black histograms, utilising the same binning as the corner plots. The red shaded regions below the Gaussians denote 1σ from the mean. On all plots, the velocities or velocity dispersions are in units of [km s⁻¹].