I've reduced my CCD frames from last night of this sequence mentioned by Brian Skiff. These frames were taken on a non-photometric night, so the zero points for B and V were set by the published magnitudes/colors for stars A,B,D'. The results are then: Star V B-V pubV pubB-V A 13.060 0.700 13.07 0.70 B 13.765 0.463 13.75 0.46 C 13.976 0.911 13.96: 0.89: D 13.393 0.596 13.20 0.62 D' 15.146 0.817 15.15 0.82 E 15.438 0.922 15.45: 0.96: F 16.378 0.103 16.18: 0.29: Formal Poisson errors are <0.02mag. As you can see, stars D and F are somewhat different from what was given, and star D is definitely not V=15.20. The new V, (B-V) values are not to be considered 'secondary standard' quality. However, since these are CCD measures, the internal accuracy (star-to-star) should be quite good, with just a zero point adjustment to get the sequence on the real Johnson system. (NGC3067 is quite pretty) Arne -------------------------------------------------------------------- Arne Henden Instruments/software/CCDs US Naval Observatory Flagstaff Station Cepheids/photometry/IR P.O. Box 1149 http: ftp.nofs.navy.mil Flagstaff, AZ 86002-1149 Voice: (520)779-5132 aah@nofs.navy.mil FAX: (520)774-3626