UU Lyn
Yamasaki1983 - Yamasaki1983B (Johnson B)
The light and radial velocity curves are from Yamasaki et al. (1983). The solutions presented are essentially from their paper as well, but I made modifications to the limb darkening values (I used modern values from Van Hamme’s (1993) tables) and I also had to estimate the temperature difference because it was not specifically given in the paper. There is also room for debate as to whether or not both stars are convective since they give a spectral classification for the primary of F3V that would be convective. However, they treat it as a radiative star and I maintained their designation. The mass ratio is also uncertain, as the radial velocity curve is single-lined.