99 WZ CANIS MAJORIS (UG) Range: 14.5-18.3V Position: 07 18 49.19 -27 07 43.3 (J2000, from .dat file) Magnitude: V=16.632 B-V=0.639 (Henden, single night) ID RA (2000) DEC X Y N V ERR B-V ERR a) Comparison star sequence 1 07 18 44.3 -27 05 34 -65 129 3 11.772 0.027 1.157 0.023 2 07 19 03.6 -27 12 49 191 -306 2 12.423 0.011 0.424 0.014 3 07 18 58.4 -27 07 08 123 35 3 13.149 0.020 0.812 0.021 4 07 18 50.6 -27 07 48 19 -5 3 13.609 0.016 0.552 0.019 5 07 18 39.0 -27 08 41 -137 -58 3 14.048 0.016 0.516 0.019 6 07 18 38.9 -27 08 18 -138 -34 3 14.489 0.044 1.634 0.073 7 07 18 43.0 -27 07 58 -83 -15 3 15.021 0.022 1.118 0.031 8 07 18 48.3 -27 09 01 -12 -78 3 15.477 0.037 1.000 0.054 9 07 18 43.5 -27 08 33 -76 -50 3 15.970 0.026 0.608 0.045 10 07 18 45.7 -27 07 41 -47 2 3 16.550 0.029 0.668 0.135 11 07 18 49.2 -27 06 48 0 55 2 17.340 0.088 0.611 0.052 b) Wide-colour extension for CCD calibration 07 19 03.4 -27 02 21 190 322 3 12.015 0.011 0.251 0.013 07 18 50.3 -27 11 16 15 -213 3 12.416 0.006 0.261 0.012 07 19 06.5 -27 05 19 231 144 3 11.545 0.051 1.849 0.027 Notes: 1. Two bright stars in this field were not measured during the photometric determination. They both have reliable Tycho-2 magnitudes. One is the bright star very near WZ CMa, being only 25 arcsec northwest of the variable. It has a magnitude of V=10.60+/-0.06. The other bright star is near the east edge of the field and has a magnitude of V=10.28+/-0.05. 2. The magnitude shown here for WZ CMa may not be a quiescent value, but some intermediate magnitude. Henden measured a much bluer magnitude when WZ CMa was at maximum, when the magnitude was measured as V=13.799+/-0.004 and B-V=0.099+/-0.005. Bruce Sumner 15 April 1999 Revised 30 December 2000