  As the 2dF Galaxy Redshift Survey and Sloan Digital Sky Survey move toward
completion, it is time to ask what the next generation of survey of large-scale
structure should be. I discuss some of the cosmological justifications for such
surveys and conclude that surveys at z=3 offer a critical advantage in their
ability to access linear-regime clustering at scales smaller than any current
survey and even the CMB. I discuss a possible implementation of such a survey
and highlight some of the potential science return.
