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Dwarf novae in the Hamburg quasar survey : rarer than expected

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Figure

Table 1. Properties of the five new dwarf novae.
Fig. 4.Sample filterless light curves of HS 1016 obtained at theKryoneri observatory.
Fig. 5. Sample light curves of HS 1340. Top panel: R-band data ob-tained at the Kryoneri observatory
Fig. 9. The Scargle periodogram of the radial velocities of HS 1016,HS 1340, HS 1857, and HS 2214
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