All Tables

Table 1: Properties of the five new dwarf novae.
Table 4: The fractional superhump excess of HS 0417 computed from $\epsilon=(\mbox{$P_{\rm sh}$ }-\mbox{$P_{\rm orb}$ })/\mbox{$P_{\rm orb}$ }$ .
Table 5: Sine fits to the ${\rm H\alpha }$ radial velocities of HS 1016, HS,1340, and HS 1857. For HS 2214 a combination of ${\rm H\alpha }$ and ${\rm H\beta }$ radial velocities were fitted, as the September 2000 Calar Alto spectra did not cover ${\rm H\alpha }$ . For HS 1857 and HS 2214, the periods were fixed to their values determined from the photometry.
Table 6: The times of eclipse minima of HS 1857 obtained during the 2002 to 2004 runs.
Table 7: Dwarf novae discovered in the HQS with their subtype, U Gem (UG), SU UMa (SU), Z Cam (ZC), and unclassified (XX). Uncertain classifications are marked by a colon.
Table 2: Log of the observations.
Table 3: Comparison stars used for the differential CCD photometry of HS 0417, HS 1016, HS 1340, HS 1857, and HS 2214, see Fig. 1.