Since most of the stars in this sequence are reddened, I've revised it to
exclude the known variables and suspects, and replaced the bluer stars with new
12th mag stars that are all similar reddish B-Vs to the rest of the comparison
stars.

I've retained the nearby 131 for ID purposes when the variable is faint. I'm not
married to this idea. It has a relatively high error also, probably due to
crowding.

I'd appreciate feedback from visual observers as to the 'improvements'. I can't
observe until I'm well again.

AUID label U (err) B (err) V (err)


000-BCF-097 117 14.234 (0.030)10 13.011 (0.013)10 11.687 (0.010)10

000-BJP-393 120 16.532 (0.019)10 14.068 (0.013)10 12.024 (0.006)10

000-BJP-394 123 16.462 (0.017)10 14.183 (0.010)10 12.253 (0.005)10

000-BJP-396 126 16.671 (0.021)10 14.496 (0.009)10 12.574 (0.008)10

000-BJP-397 128 15.472 (0.035)10 14.243 (0.008)10 12.763 (0.005)10

000-BCF-093 131 14.096 (0.123)10 14.055 (0.121)10 13.093 (0.120)10

000-BJP-398 132 17.575 (0.084)10 15.289 (0.083)10 13.232 (0.083)10

000-BCF-084 136 16.308 (0.025)10 15.058 (0.011)10 13.622 (0.009)10


Mike Simonsen