On the night of Mar 11/12, 2018, Victor Rau-Sirois and Jen Connelly checked one of the stars in his observing program of suspected variables: NSV 03287.
The main setup was:
Conditions were fair:
The target was NSV 03287 .
RA (J2000) Dec V NSV 03287 06 57 06.2 +44 06 35 A = UCAC4 672-047819 06 57 20.876 +44 14 42.31 10.813 B = UCAC4 672-047806 06 57 07.007 +44 12 42.14 11.102 C = UCAC4 671-048799 06 57 08.550 +44 04 59.11 12.085
The output of our ensemble photometry of stars in this field indicates that the transperency gradually decreased (probably due to the increase in airmass), but one set of clouds moved over the field near the end of the run.
The precision of the photometry was good: in the sigma-vs-mag graph below, note that bright stars have a scatter of about one percent = 0.01 mag.
Last modified 3/1/2018 by MWR.