Fig. 3

Construction of the volume-limited galaxy subsamples with different luminosity
(upper panel) and stellar mass (lower panel). In both figures the grey dots
represent the distribution of VUDS galaxies as a function of spectroscopic redshift
z.
At each redshift UV
band, absolute magnitudes and stellar masses are normalized to the characteristic absolute magnitudes or to the
characteristic stellar mass, respectively (see Sect. 2.2). The different colour lines delineate the selection cuts
for selected UV
absolute magnitude and stellar mass subsamples as defined in Tables 2 and
3. The dashed black line represents the evolution of the not corrected characteristic
UV
absolute magnitude
(upper panel) or characteristic stellar mass M*
(lower panel). The grey line indicates the volume limit of the VUDS sample.
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