We explore the form of extragalactic reddening toward quasars using a sample of 9566 quasars with redshifts 0 0.1, and less than 1% have EB-V > 0.2, where the extinction is relative to quasars with modal colors. Reddening is uncorrelated with the presence of intervening narrow-line absorption systems, but reddened quasars are much more likely to show narrow absorption at the redshift of the quasar than are unreddened quasars. Thus the reddening toward quasars is dominated by SMC-like dust at the quasar redshift.
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