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Fig. 7

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Comparison of our kinematic profiles with other works. Each diagram shows the rotation curve (upper panel) and the velocity dispersion profile (lower panel). The bottom X-axis is measured in arcseconds and the upper X-axis is measured as a fraction of the effective radius (Reff) of each galaxy in i band (see Sect. 6). For Van Zee et al. (2004) we only present their velocity profiles for MgbI, more similar in wavelength to our data.

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