185 VV PUPPIS (AM) Range: 13.9-18.0V Position: 08 15 06.80 -19 03 17.4 (J2000, from .dat file) Magnitude: V=15.875 B-V=-0.172 (from .dat file) ID RA (2000) DEC X Y N V ERR B-V ERR a) Comparison star sequence 1 08 14 56.1 -19 00 05 -151 192 2 12.288 0.068 0.400 0.021 2 08 15 09.1 -19 02 12 32 66 2 12.964 0.020 0.387 0.033 3 08 15 08.9 -19 04 12 30 -55 2 13.413 0.008 1.065 0.032 4 08 14 56.7 -19 02 13 -143 64 2 13.753 0.024 0.630 0.029 5 08 15 07.0 -19 01 15 3 122 2 14.170 0.012 0.566 0.041 6 08 15 07.0 -19 04 55 3 -98 2 14.722 0.008 0.801 0.035 7 08 14 59.3 -19 02 06 -106 71 2 15.138 0.026 0.820 0.020 8 08 14 57.1 -19 03 30 -137 -13 2 15.514 0.010 0.635 0.040 9 08 15 11.1 -19 03 27 61 -10 2 15.841 0.017 0.947 0.043 10 08 15 09.7 -19 03 10 42 7 2 16.527 0.017 0.892 0.023 11 08 15 05.8 -19 02 35 -14 42 2 17.374 0.046 0.648 0.008 12 08 15 07.2 -19 02 56 6 21 2 18.018 0.065 0.576 0.076 b) Wide-colour extension for CCD calibration 08 15 26.8 -19 04 33 284 -76 2 12.745 0.015 0.271 0.030 08 14 48.7 -19 07 23 -256 -246 2 12.354 0.054 1.554 0.021 Notes: 1. RASNZ chart No. 1016 shows a photoelectric sequence from Karen Meech, PASP, 95, 662, 1983. Four of the magnitudes on that chart are common with this sequence. For the sake of completeness, all Meech's comparison stars are included in the following table, but only those stars with an ID number are part of this new sequence. ID Henden Meech V B-V V B-V 12.107 0.358 12.05 0.43 1 12.288 0.400 12.27 0.42 2 12.964 0.387 12.93 0.39 13.348 0.463 13.34 0.43 4 13.753 0.630 13.76 0.60 13.841 1.104 13.98 1.04 5 14.170 0.566 14.19 0.61 14.694 0.458 14.76 0.27 14.820 0.547 14.83 0.49 2. Meech also measured a bright star in this field that was not measured during the photometric determination. This star is at 08h 14m 50.8s -19d 00' 43" and has a magnitude of V=9.33+/-0.02. Bruce Sumner 30 December 2000