An accurate sequence and chart are now available for this variable star thanks to field photometry acquired by Arne Henden. The chart, courtesy of Mike Simonsen, is available at: http://joevp.20m.com/cgi-bin/i/charts/hscharts/South_up/ The full field photometry file, including R&I measures, is at: http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/dwcnc.dat Bruce Sumner ----------------------- 208 DW CANCRI (UG) Range: 14.1v-17.5p Position: 07 58 53.04 +16 16 45.5 (J2000, from .dat file) Magnitude: V=14.915 B-V=0.023 (.dat file) ID RA (2000) DEC X Y N V ERR B-V ERR a) Comparison star sequence 1 07 59 12.1 +16 13 28 275 -197 2 12.331 0.019 0.506 0.031 2 07 58 43.0 +16 17 24 -144 39 2 12.688 0.010 0.465 0.005 3 07 59 06.8 +16 18 22 199 97 2 13.437 0.006 0.525 0.008 4 07 58 35.6 +16 13 47 -251 -178 2 13.757 0.032 0.765 0.008 5 07 59 04.6 +16 14 38 167 -127 2 14.074 0.008 0.528 0.002 6 07 58 50.9 +16 14 45 -30 -120 2 14.539 0.012 0.916 0.008 7 07 59 10.1 +16 15 42 247 -63 2 14.907 0.006 0.739 0.013 8 07 59 00.5 +16 16 47 108 2 2 15.198 0.010 0.687 0.013 9 07 58 38.5 +16 19 55 -209 190 2 15.495 0.017 0.781 0.013 10 07 58 55.8 +16 17 11 40 26 2 16.093 0.008 0.944 0.019 11 07 58 50.1 +16 16 50 -41 5 2 17.221 0.011 0.597 0.017 12 07 58 54.4 +16 15 57 20 -48 2 18.701 0.055 0.704 0.151 b) Wide-colour extension for CCD calibration 07 58 38.9 +16 11 30 -203 -315 2 12.938 0.012 0.197 0.004 07 58 34.8 +16 11 11 -262 -334 2 15.703 0.016 1.374 0.020 Notes: 1. This sequence is created from field photometry acquired by Arne Henden on two separate nights. Apart from the faintest star, this sequence is quite reliable and is not expected to change when extra nights are added to a later date to refine the errors. The star #4 has a large error and may be a low amplitude variable. Bruce Sumner 22 March 2001