18 =NSVS 6427464/6496597 (Gettel et al. 2006, Cat. J/AJ/131/621)
1770 =NSVS 8932555/8825959 (Gettel et al. 2006, Cat. J/AJ/131/621)
  18 =ASAS 014035+2806.8 (Pojmanski 2002, Cat. II/264)
 180 =ASAS 044223+2803.7 (Pojmanski 2002, Cat. II/264)
 814 =ASAS 180615+2801.2 (Pojmanski 2002, Cat. II/264)
1767 =ASAS 221736+2806.9 (Pojmanski 2002, Cat. II/264)
1770 =ASAS 222153+2802.8. (Pojmanski 2002, Cat. II/264)
 390 =ASAS 061833+2802.2 (Pojmanski 2002, Cat. II/264)
 598 =ASAS 073451+2805.7 (Pojmanski 2002, Cat. II/264)
1478 =ASAS 200540+2805.2. (Pojmanski 2002, Cat. II/264)
 162 =NSVS 6767121 (Wozniak et al. 2004, Cat. J/AJ/128/2965)
1677 =NSVS 8606023 (Wozniak et al. 2004, Cat. J/AJ/128/2965)
1730 =NSVS 8766925 (Wozniak et al. 2004, Cat. J/AJ/128/2965)
 713 =ROTSE1 J150337.75+280334.1 (Akerlof et al. 2000, Cat. J/AJ/119/1901)
 814 =ROTSE1 J180616.31+280109.1, reported on in Wetterer et al.  (2004IBVS.5515....1W)
1529 =NSV 13070 (Kukarkin et al. 1982, Cat. II/140)
1115 =NSV 24717 (Kukarkin et al. 1982, Cat. II/140)
 999 =NSV 24643 (Kukarkin et al. 1982, Cat. II/140)
1007 =NSV 24652 (Kukarkin et al. 1982, Cat. II/140)
 756 unexplained 0.3mag offset between AFA and CTI V magnitudes in Table 5
1649 completely blended with neighbor. The V magnitudes are for an individual star ~0.31 fainter than listed in Table 5
1176 possible EW with twice period
1718 possible EW with twice period
1670 possible DSCT with half period