Hi Berto et al.,Yeah, CD Ind is a long-term project, following the synchronization of that wayward white dwarf. Your early-season data specifies the phase pretty well; a rush of late-season data, and a couple of mid-season points sprinkled in there, will do the job nicely. But VY Aqr in a July superoutburst, now that's just too delicious to resist... or even to be restrained about.
Thanks for the calibration homework. joe
The following comparison stars (for C or K) can be adviced.With Loneos photometry:VY Aqr 15 21 12 10.2 -08 49 03 h 5772-0390 13.91 0.86 0.54 VY Aqr 16 21 12 11.2 -08 49 59 h 5772-0074 13.82 0.75 0.42 VY Aqr 1v 21 12 11.3 -08 53 08 G 5772-0143 10.97 0.55From the latter we can derive an R magnitude of 10.65 for unfiltered reference. For the others subtract the third column values (V-R) from the first column (which is V).Good luck to the campaign! Berto Monard / CBA Pretoria