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Fig. 4


Relation between SFR and stellar mass for 416 CALIFA galaxies, color coded by Hubble type. A linear fit to the points of Sc galaxies is shown as a gray-blue dashed line. Different panels show the results obtained considering different selection criteria imposed upon the individual xy spaxels included in the computation of the galaxy’s total SFR = ∑ xySFRxy: Only xY> 3.4% (left), WHα> 3 Å (middle), and WHα> 6 Å (right).

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