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tokens: We acknowledge partial financial support by contract PRIN/MIUR 2009: ‘Dynamics and Stellar Populations of Superdense Galaxies’ (Code: 2009L2J4MN) and by INAF/PRIN 2011: ‘Galaxy Evolution with the VLT Survey Telescope (VST)’. BV was supported by the World Premier International Research Center Initiative (WPI), MEXT, Japan, and by the Kakenhi Grant-in-Aid for Young Scientists (B)(26870140) from the Japan Society for the Promotion of Science (JSPS).