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Fig. 5.

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Observed galaxies in the Wide survey (colors) compared to the parent catalog from 3D-HST (Momcheva et al. 2016 contours at 250, 500, and 1000 sources) in our three primary redshift bins. Across all redshift and mass ranges, Wide is sampling galaxies across the full range of SFRs from 3D-HST, including those that lie below the “main sequence” (overplotted at ±1-σ as dashed lines at z = 1, 2, and 3, respectively; Speagle et al. 2014).

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