  We report on a search for extremely metal-poor ([Fe/H]<-3.0) turnoff stars in
the Hamburg/ESO objective prism survey (HES). Metal-poor stars are selected by
automatic spectral classification. Extensive simulations show that the
selection efficiency for turnoff stars of [Fe/H]<-3.0 is >25% at B<16.5. Since
the HES is more than 1 mag deeper than the HK survey of Beers et al. (1992),
the HES offers the possibility to efficiently increase the total number of
metal-poor stars by at least a factor of 4.
