Fig. 3.
Panel a: bivariate PDF LK−Mstar: estimated bivariate PDF shown in linear scale (and enlarged in the inset) for the K-band with the stellar masses. Contour lines correspond to levels 0.1, 0.3, 0.5, 0.7, and 0.9. These values correspond to the fraction of the peak value of the BLF that is set to one. Panel b: reconstructed stellar mass function of the HRS sample (red line) shown together with the best fit of the Galactic mass function given by Baldry et al. (2012) for the GAMA survey (blue line).
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