ZZ Cyg
Giuricin1981 - Giuricin1981V (Johnson V)
The UBV light curves are from Hall & Cannon (1974). The solutions are from Giuricin et al. (1981) with the temperature of the secondary star reduced from 4310 to 4050 K to better fit the light curves. A solution to the U light curve is also presented here although Giuricin et al. (1981) mention that they could not fit the U light curve in a satisfactory manner.