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Fig. 3

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Stellar mass as a function of redshift (small grey dots). Also shown are ℳlim (intermediate size dark dots) and ℳmin (big black circles and lines) at 95% of the ℳ/L completeness level (see text): upper panel for the total population, middle and lower panel for SED-ETGs and SED-LTGs, respectively, defined by their photometric type. Also shown with a dashed black line is the ℳ threshold (corresponding to 95% of the completeness level for the global GSMF) derived using mock Millenium samples by Meneux et al. (2009).

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