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The Sloan Digital Sky Survey (SDSS) was revolutionary because of theextraordinary breadth and ambition of its optical imaging and spectroscopy. Weargue that a 'sub-millimeter SDSS' - a sensitive large-areaimaging+spectroscopic survey in the sub-mm window - will revolutionize ourunderstanding of galaxy evolution in the early Universe. By detecting thethermal dust continuum emission and atomic and molecular line emission ofgalaxies out to z~10 it will be possible to measure the redshifts, starformation rates, dust and gas content of hundreds of thousands of high-zgalaxies down to ~L*. Many of these galaxies will have counterparts visible inthe deep optical imaging of the Large Synoptic Survey Telescope. This 3D map ofgalaxy evolution will span the peak epoch of galaxy formation all the way backto cosmic dawn, measuring the co-evolution of the star formation rate densityand molecular gas content of galaxies, tracking the production of metals andcharting the growth of large-scale structure.

The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z~10