While browsing journals for photometric sequences, I have found one for the quasar 3C 232 by Ron Angione (1971 AJ 76, 412). Quite close to the quasar is the bright galaxy NGC 3067. The sequence thus has the additional utility as a comparison set for any supernova that might occur there. Positions from USNO-A1.0 for the stars and the two extragalactic objects are shown below along with Angione's BV photometry. N.B. that for stars C, E, and F the data are less certain than for the remainder. For completeness, Tycho photometry for the bright field star BD+33 1925 is given as well. Name RA (2000) Dec V B-V Remarks NGC 3067 9 58 21.3 +32 22 11 GSC 2502-0767 3C 232 9 58 20.9 +32 24 02 BD+33 1925 9 58 39.3 +32 23 09 9.77 0.50 GSC 2502-0761, Tycho data 3C 232 A 9 58 02.7 +32 29 11 13.07 0.70 GSC 2502-0661 3C 232 B 9 58 01.3 +32 24 03 13.75 0.46 GSC 2502-0750 3C 232 C 9 58 45.0 +32 27 40 13.96: 0.89: GSC 2502-0685 3C 232 D 9 58 38.9 +32 29 44 13.20 0.62 GSC 2502-0645 3C 232 D' 9 58 14.5 +32 23 45 15.15 0.82 GSC 2502-0746 3C 232 E 9 58 24.3 +32 25 13 15.45: 0.96: 3C 232 F 9 58 23.3 +32 23 06 16.18: 0.29: Ton 470 = Case A-F 509 \Brian