Distribution of all KV450 galaxy stellar mass estimates as a function of photo-z. The data is shown as a 2D-histogram with logarithmic scaling. The distribution is fairly consistent with what is expected of a magnitude limited galaxy sample, although the incompleteness at low-z is worth noting. The distribution is fairly uniform above the mass limits (red dashed line). Below the limits we see signs of systematic incompleteness and redshift focussing (caused by the typically noisier data there).