  The first multicolor observations and light curve solutions of the stars
1SWASP J130111.22+420214.0 and 1SWASP J231839.72+352848.2 are presented. The
estimated physical parameters of 1SWASP J130111.22+420214.0 are
$M_1=1.0M_{\odot}$, $M_2=1.63M_{\odot}$, $R_1=0.77R_{\odot}$,
$R_2=0.91R_{\odot}$, $L_1=0.59L_{\odot}$, and $L_2=0.68L_{\odot}$. While a
binary model could not be fitted to the light curve of 1SWASP
J231839.72+352848.2, its Fourier series representation indicates that this
system could well be a rotating ellipsoidal variable. The components of 1SWASP
J130111.22+420214.0 are also compared to other well--known binary systems and
their position in mass--radius plane and the Hertzsprung--Russel diagram are
argued and possible evolutionary statuses are discussed.
