Fig. 15
Evolution of the number densities in three bins of M∗, for the global (black), SF (blue), and Q (red) populations. The corresponding shaded area shows the systematic uncertainty that is due to the SF/Q selection around our reference measurement (stars). The measurements of Moustakas et al. (2013, triangles) and Matsuoka & Kawara (2010, pentagons) are plotted for comparison.
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