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Fig. 2

image

Top and middle panels: distribution of our sample of 300 galaxies (orange circles) in redshift, isophotal diameter (Aiso), and absolute r-band petrosian magnitude (Mr,p). For reference, the CALIFA mother sample is shown with black dots. The vertical lines indicate the limits in absolute magnitude in which the CALIFA mother sample is representative. Bottom panel: comparison of the luminosity functions of the SDSS (Blanton et al. 2003, thick dashed line), CALIFA mother sample (dark blue circles), and the kinematic sample presented here (orange circles).

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