Lightcurve results for USNO 1395-0370184.
USNO 1395-0370184 is a 14.7 magnitude star in the constellation Cygnus. I discovered it to be variable on images taken on 22 October, 2010. Further observations were made in 2014 and 2015. The lightcurve is typical of a W UMa eclipsing binary and the period derived was 6.0257 hours. However the lightcurves from each year did not match up very well when combined with those from different years as can be seen in the graph below. Further observations are planned during 2016 to see if the period is changing. The amplitude was 0.35 magnitude