Top: Distribution of spectroscopically identified galaxies in our parent sample as a function of spectroscopic survey (SDSS-II Legacy, SDSS-III BOSS, PRIMUS, VIPERs, GAMA, and Wiggle-Z). Middle: Fractional contribution of a given spectroscopic survey to our parent galaxy sample as a function of redshift for all galaxies within our parent sample, and for the star-forming galaxy sample after applying the UVJ cut shown in figure 3. Bottom: Spectroscopic sample as a function of i-band magnitude. (Color online)