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Published online by Cambridge University Press: 25 May 2016
The maturity of all-sky surveys hold great promise for galactic structure studies. Surveys such as the APS Catalog of POSS I allow large scale studies of stellar distributions where the data is very complete to a reasonably faint magnitude, uniformly reduced, and independently calibrated. The APS data covers a large portion of the sky, allowing studies where the primary source of uncertainty is no longer small-number statistics.