Fig. 1
Characterisation of the sample of galaxies under analysis in this work (red) compared to the CALIFA DR3 sample of galaxies limited to spiral systems (grey). Left-hand panel: distribution is indicated of the morphological types according to the T parameter from Walcher et al. (2014). Middle panel: distribution is indicated of stellar masses from Walcher et al. (2014). Right-hand panel: distribution is indicated of the galaxies in the (u − z) – Mz colour magnitude diagram.
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