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Six objects with broad emission lines and redshifts from 0.48 to 2.07 werediscovered among 736 extragalactic objects in the Canada-France Redshift Survey(CFRS). Although the luminosities of half of the objects are such that they arein the Seyfert regime (M_B > -23), all would be designated as quasars intraditional surveys. Since the only selection criterion was that 17.5 < I_{AB}< 22.5, or approximately B < 23 (assuming a continuum power-law slope of alpha= -0.5), these quasars represent an unbiased, flux-limited sample. Althoughuncertain, the implied surface density, 200^{+120}_{-80} deg^{-2} is thehighest yet measured, and is in good agreement with extrapolations from otherfaint surveys and the evolving luminosity function models of Boyle (1991). Thedistributions of the continuum properties, emission-line strengths, etc., ofthe quasars do not differ significantly from those of quasars selected by othermeans, and therefore they would have been detected in most traditional surveys.Three of the quasars may be associated with clusters or large structures ofgalaxies at z > 1.

Canada-France Redshift Survey -- X. The quasar sample