Abstract
Beginning with an unbiased sample of unobscured QSOs (type 1 within AGN unification), we identify regions in the WISE color space that harbor the putative population of obscured type 2 counterparts. For the first time, we can predict the relation of their number vs. flux limits of a survey, applying knowledge from the CLUMPY torus models. This proceedings contribution is a preview of a forthcoming pair of papers (Nikkuta et al. 2014a,b).
