2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/5682As 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.Proceedings from Wide-Field Multi-Object Spectroscopy conference at NOAO in October 2001, to be published by the ASP Conference Series. 8 pages, LaTex, 1 figureAstrophysicstext